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Glossary of OSA attributes |
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This Glossary alphabetically lists all attributes used in the OSAv20230621 database(s) held in the OSA. If you would like to have more information about the schema tables please use the OSAv20230621 Schema Browser (other Browser versions). |
| A | B | C | D | E | F | G | H | I | J | K | L | M |
| N | O | P | Q | R | S | T | U | V | W | X | Y | Z |
A | ||||||||
|---|---|---|---|---|---|---|---|---|
| Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
| a | twomass_psc | TWOMASS | Catalog identifier of an optical source from either the Tycho 2 or USNO-A2.0 catalog that falls within ~5" of the TWOMASS source position. | varchar | 1 | meta.id | ||
| A1 | mgcGalaxyStruct | MGC | Asymmetry index (background corrected) alpha=1 | real | 4 | 99.99 | ||
| A2 | mgcGalaxyStruct | MGC | Asymmetry index (background corrected) alpha=2 | real | 4 | 99.99 | ||
| A3 | mgcGalaxyStruct | MGC | Asymmetry index (background corrected) alpha=3 | real | 4 | 99.99 | ||
| A4 | mgcGalaxyStruct | MGC | Asymmetry index (background corrected) alpha=4 | real | 4 | 99.99 | ||
| a_g_percentile_lower | gaia_source | GAIADR2 | Lower uncertainty on A_G | real | 4 | mag | phys.absorption.gal;stat.min | |
| a_g_percentile_upper | gaia_source | GAIADR2 | Upper uncertainty on A_G | real | 4 | mag | phys.absorption.gal;stat.max | |
| a_g_val | gaia_source | GAIADR2 | Line-of-sight extinction in the G band, A_G | real | 4 | mag | phys.absorption.gal | |
| A_IMAGE | mgcDetection | MGC | Flux rms along major axis | real | 4 | pixel | ||
| ab_flags | catwise_2020, catwise_prelim | WISE | Two character (W1 W2) artifact flag | varchar | 9 | |||
| abbe | phot_variable_time_series_g_fov_statistical_parameters | GAIADR1 | Abbe value of the G-band time series values | float | 8 | stat.value | ||
| abMagLim | MultiframeDetector | ATLASDR1 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | ATLASDR2 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | ATLASDR3 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | ATLASDR4 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | ATLASDR5 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | ATLASv20131127 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | ATLASv20160425 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | ATLASv20180209 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | VPHASDR3 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | VPHASv20160112 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| abMagLim | MultiframeDetector | VPHASv20170222 | 5-sigma limiting AB magnitude for point sources {catalogue extension keyword: ABMAGLIM} | real | 4 | mag | -0.9999995e9 | |
| ABS_CSB_BULGE | mgcGalaxyStruct | MGC | Absolute Central Surface Brightness of Bulge | real | 4 | Vega mag/sq arcsec | 99.99 | |
| ABS_CSB_DISK | mgcGalaxyStruct | MGC | Absolute Central Surface Brightness of Disk | real | 4 | Vega mag/sq arcsec | 99.99 | |
| ABS_ESB_BULGE | mgcGalaxyStruct | MGC | Absolute Effective Surface Brightness of Bulge | real | 4 | Vega mag/sq arcsec | 99.99 | |
| ABS_ESB_DISK | mgcGalaxyStruct | MGC | Absolute Effective Surface Brightness of Disk | real | 4 | Vega mag/sq arcsec | 99.99 | |
| ABS_HLRSB_BULG | mgcGalaxyStruct | MGC | Absolute Surface Brightness at Re | real | 4 | Vega mag/sq arcsec | 99.99 | |
| ABS_HLRSB_DISK | mgcGalaxyStruct | MGC | Absolute Surface Brightness at 1.678alpha | real | 4 | Vega mag/sq arcsec | 99.99 | |
| ABS_MAG_GIM2D | mgcGalaxyStruct | MGC | GIM2D B Absolute Disk mag, dust and K & E-corrected | real | 4 | Vega mag | 99.99 | |
| ABS_MAG_GIM2DB | mgcGalaxyStruct | MGC | GIM2D B Absolute mag, dust and K & E-corrected | real | 4 | Vega mag | 99.99 | |
| ABS_MAG_GIM2DD | mgcGalaxyStruct | MGC | GIM2D B Absolute Bulge mag, dust and K & E-corrected | real | 4 | Vega mag | 99.99 | |
| ABS_SB_B | mgcGalaxyStruct | MGC | MGC B Absolute KRON SB, dust K & E-corrected | real | 4 | Vega mag | -99.000 | |
| ABS_SB_g | mgcGalaxyStruct | MGC | SDSS g Absolute PET SB, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| ABS_SB_i | mgcGalaxyStruct | MGC | SDSS i Absolute PET SB, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| ABS_SB_r | mgcGalaxyStruct | MGC | SDSS r Absolute PET SB, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| ABS_SB_u | mgcGalaxyStruct | MGC | SDSS u Absolute PET SB, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| ABS_SB_z | mgcGalaxyStruct | MGC | SDSS z Absolute PET SB, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| abSatMag | MultiframeDetector | ATLASDR1 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | ATLASDR2 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | ATLASDR3 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | ATLASDR4 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | ATLASDR5 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | ATLASv20131127 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | ATLASv20160425 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | ATLASv20180209 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | VPHASDR3 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | VPHASv20160112 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| abSatMag | MultiframeDetector | VPHASv20170222 | Saturation limit for point sources (AB magnitude) {catalogue extension keyword: ABMAGSAT} | real | 4 | mag | -0.9999995e9 | |
| absMagPsf_g | mgcGalaxyStruct | MGC | SDSS g Absolute PSF mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPsf_i | mgcGalaxyStruct | MGC | SDSS i Absolute PSF mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPsf_r | mgcGalaxyStruct | MGC | SDSS r Absolute PSF mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPsf_u | mgcGalaxyStruct | MGC | SDSS u Absolute PSF mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPsf_z | mgcGalaxyStruct | MGC | SDSS z Absolute PSF mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPt_B | mgcGalaxyStruct | MGC | MGC B Absolute KRON mag, dust K & E-corrected | real | 4 | Vega mag | -99.000 | |
| absMagPt_g | mgcGalaxyStruct | MGC | SDSS g Absolute PET mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPt_i | mgcGalaxyStruct | MGC | SDSS i Absolute PET mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPt_r | mgcGalaxyStruct | MGC | SDSS r Absolute PET mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPt_u | mgcGalaxyStruct | MGC | SDSS u Absolute PET mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| absMagPt_z | mgcGalaxyStruct | MGC | SDSS z Absolute PET mag, dust K & E-corrected | real | 4 | AB mag | -99.000 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASDR1 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASDR2 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASDR3 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASDR4 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASDR5 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASv20131127 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASv20160425 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | ATLASv20180209 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | VPHASDR3 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | VPHASv20160112 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotEnd | MultiframeEsoKeys | VPHASv20170222 | Abs rot angle at exp end {image primary HDU keyword: HIERARCH ESO ADA ABSROT END} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotPpos | MultiframeEsoKeys | ATLASDR1 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | ATLASDR2 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | ATLASDR3 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | ATLASDR4 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | ATLASDR5 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | ATLASv20131127 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | ATLASv20160425 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | ATLASv20180209 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | VPHASDR3 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | VPHASv20160112 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotPpos | MultiframeEsoKeys | VPHASv20170222 | sign of probe position {image primary HDU keyword: HIERARCH ESO ADA ABSROT PPOS} | varchar | 4 | NONE | ||
| adaAbsrotStart | MultiframeEsoKeys | ATLASDR1 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | ATLASDR2 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | ATLASDR3 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | ATLASDR4 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | ATLASDR5 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | ATLASv20131127 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | ATLASv20160425 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | ATLASv20180209 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | VPHASDR3 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | VPHASv20160112 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaAbsrotStart | MultiframeEsoKeys | VPHASv20170222 | Abs rot angle at exp start {image primary HDU keyword: HIERARCH ESO ADA ABSROT START} | real | 4 | deg | -9.999995e+08 | |
| adaGuidStatus | MultiframeEsoKeys | ATLASDR1 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | ATLASDR2 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | ATLASDR3 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | ATLASDR4 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | ATLASDR5 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | ATLASv20131127 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | ATLASv20160425 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | ATLASv20180209 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | VPHASDR3 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | VPHASv20160112 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaGuidStatus | MultiframeEsoKeys | VPHASv20170222 | Status of autoguider {image primary HDU keyword: HIERARCH ESO ADA GUID STATUS} | varchar | 4 | NONE | ||
| adaPosang | MultiframeEsoKeys | ATLASDR1 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | ATLASDR2 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | ATLASDR3 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | ATLASDR4 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | ATLASDR5 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | ATLASv20131127 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | ATLASv20160425 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | ATLASv20180209 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | VPHASDR3 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | VPHASv20160112 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adaPosang | MultiframeEsoKeys | VPHASv20170222 | Position angle at start {image primary HDU keyword: HIERARCH ESO ADA POSANG} | real | 4 | -9.999995e+08 | ||
| adjacentFrameTolerance | Programme | ATLASDR1 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | ATLASDR2 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | ATLASDR3 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | ATLASDR4 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | ATLASDR5 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | ATLASv20131127 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | ATLASv20160425 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | ATLASv20180209 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | VPHASDR3 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | VPHASv20160112 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| adjacentFrameTolerance | Programme | VPHASv20170222 | The match tolerance for adjacent frames in the survey | real | 4 | Degrees | ?? | |
| aebv | Filter | ATLASDR2 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | ATLASDR3 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | ATLASDR4 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | ATLASDR5 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | ATLASv20131127 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | ATLASv20160425 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | ATLASv20180209 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | VPHASDR3 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | VPHASv20160112 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter | VPHASv20170222 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aebv | Filter, FilterSections | ATLASDR1 | The constant to multiply the Schlegel map E(B-V) by to get the total galactic extinction. | real | 4 | -0.9999995e9 | ||
| aG | atlasSource | ATLASDR1 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aG | atlasSource | ATLASDR2 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aG | atlasSource | ATLASDR3 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aG | atlasSource | ATLASDR4 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aG | atlasSource | ATLASDR5 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aG | atlasSource | ATLASv20131127 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aG | atlasSource | ATLASv20160425 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aG | atlasSource | ATLASv20180209 | The galactic extinction correction in the G band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aI | atlasSource | ATLASDR1 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aI | atlasSource | ATLASDR2 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aI | atlasSource | ATLASDR3 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aI | atlasSource | ATLASDR4 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aI | atlasSource | ATLASDR5 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aI | atlasSource | ATLASv20131127 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aI | atlasSource | ATLASv20160425 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aI | atlasSource | ATLASv20180209 | The galactic extinction correction in the I band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| air_temp | twomass_scn | TWOMASS | Air temperature at beginning of scan. | real | 4 | degC | phys.temperature | |
| air_temp | twomass_sixx2_scn | TWOMASS | air temperature (deg C) at beginning of scan | real | 4 | degC | ||
| airm | twomass_scn | TWOMASS | Airmass at beginning of scan. | real | 4 | obs.airMass | ||
| airm | twomass_sixx2_scn | TWOMASS | beginning airmass of scan | real | 4 | |||
| Al | ravedr5Source | RAVE | [Al/H] abundance of Al | real | 4 | dex | phys.abund.Z | |
| Al_N | ravedr5Source | RAVE | Number of used spectral lines in calc. of [Al/H] | smallint | 2 | meta.number | ||
| Algo_Conv_K | ravedr5Source | RAVE | Quality Flag for Stellar Parameter pipeline,[0..4] | int | 4 | meta.code.qual | ||
| Alpha_c | ravedr5Source | RAVE | [Alpha/Fe] [Chemical pipeline] (Note 2) | real | 4 | dex | phys.abund | |
| amEnd | Multiframe | ATLASDR1 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | ATLASDR2 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | ATLASDR3 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | ATLASDR4 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | ATLASDR5 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | ATLASv20131127 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | ATLASv20160425 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | ATLASv20180209 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | VPHASDR3 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | VPHASv20160112 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amEnd | Multiframe | VPHASv20170222 | Airmass at end of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM END} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASDR1 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASDR2 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASDR3 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASDR4 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASDR5 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASv20131127 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASv20160425 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | ATLASv20180209 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | VPHASDR3 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | VPHASv20160112 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| amStart | Multiframe | VPHASv20170222 | Airmass at start of observation {image primary HDU keyword: HIERARCH ESO TEL AIRM START} | real | 4 | -0.9999995e9 | obs.airMass | |
| ANCHOR_PARITY | mgcGalaxyStruct | MGC | 0=OK, 1=Inverted, 2=LSB BULGE | tinyint | 1 | 9 (FIX) | ||
| ANCHOR_POINT | mgcGalaxyStruct | MGC | Radius at which MU_BULGE=MU_DISK | real | 4 | kpc | 9 | |
| ANCHOR_SB | mgcGalaxyStruct | MGC | Surface brightness at Anchor Point | real | 4 | Vega mag/sq arcsec | 99.99 | |
| anom | twomass_scn | TWOMASS | Special flag indicating whether or not an unusual problem was found in the Atlas Images for this scan. | smallint | 2 | meta.code | ||
| anom | twomass_sixx2_scn | TWOMASS | entry in coadd anomaly table (0:not found|1:found) | smallint | 2 | |||
| Ap35mag_I | denisDR3Source | DENIS | Magnitude in I band from 3.5" aperture | float | 8 | mag | ||
| Ap35mag_J | denisDR3Source | DENIS | Magnitude in J band from 3.5" aperture | float | 8 | mag | ||
| Ap35mag_K | denisDR3Source | DENIS | Magnitude in K band from 3.5" aperture | float | 8 | mag | ||
| Ap45mag_I | denisDR3Source | DENIS | Magnitude in I band from 4.5" aperture | float | 8 | mag | ||
| Ap45mag_J | denisDR3Source | DENIS | Magnitude in J band from 4.5" aperture | float | 8 | mag | ||
| Ap45mag_K | denisDR3Source | DENIS | Magnitude in K band from 4.5" aperture | float | 8 | mag | ||
| Ap55mag_I | denisDR3Source | DENIS | Magnitude in I band from 5.5" aperture | float | 8 | mag | ||
| Ap55mag_J | denisDR3Source | DENIS | Magnitude in J band from 5.5" aperture | float | 8 | mag | ||
| Ap55mag_K | denisDR3Source | DENIS | Magnitude in K band from 5.5" aperture | float | 8 | mag | ||
| apassZPCat | MultiframeDetector | ATLASDR2 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | ATLASDR3 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | ATLASDR4 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | ATLASDR5 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | ATLASv20160425 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | ATLASv20180209 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | VPHASDR3 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | VPHASv20160112 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | MultiframeDetector | VPHASv20170222 | APASS zero point (AB) for default extinction {catalogue extension keyword: APASSZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPCat | PreviousMFDZP | ATLASDR4 | Photometric zeropoint for APASS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| apassZPCat | PreviousMFDZP | ATLASDR5 | Photometric zeropoint for APASS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| apassZPErrCat | MultiframeDetector | ATLASDR2 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | ATLASDR3 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | ATLASDR4 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | ATLASDR5 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | ATLASv20160425 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | ATLASv20180209 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | VPHASDR3 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | VPHASv20160112 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | MultiframeDetector | VPHASv20170222 | APASS zero point error {catalogue extension keyword: APASSZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| apassZPErrCat | PreviousMFDZP | ATLASDR4 | Photometric zeropoint error for APASS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| apassZPErrCat | PreviousMFDZP | ATLASDR5 | Photometric zeropoint error for APASS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| apassZPNum | MultiframeDetector | ATLASDR2 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | ATLASDR3 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | ATLASDR4 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | ATLASDR5 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | ATLASv20160425 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | ATLASv20180209 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | VPHASDR3 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | VPHASv20160112 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| apassZPNum | MultiframeDetector | VPHASv20170222 | Number of APASS standards used {catalogue extension keyword: APASSNUM} | int | 4 | -99999999 | ||
| Apc15mag_I | denisDR3Source | DENIS | I band Magnitude in 1.5" corr. aperture | float | 8 | mag | ||
| Apc15mag_J | denisDR3Source | DENIS | J band Magnitude in 1.5" corr. aperture | float | 8 | mag | ||
| Apc15mag_K | denisDR3Source | DENIS | K band Magnitude in 1.5" corr. aperture | float | 8 | mag | ||
| Apc25mag_I | denisDR3Source | DENIS | I band Magnitude in 2.5" corr. aperture | float | 8 | mag | ||
| Apc25mag_J | denisDR3Source | DENIS | J band Magnitude in 2.5" corr. aperture | float | 8 | mag | ||
| Apc25mag_K | denisDR3Source | DENIS | K band Magnitude in 2.5" corr. aperture | float | 8 | mag | ||
| Apc35mag_I | denisDR3Source | DENIS | I band Magnitude in 3.5" corr. aperture | float | 8 | mag | ||
| Apc35mag_J | denisDR3Source | DENIS | J band Magnitude in 3.5" corr. aperture | float | 8 | mag | ||
| Apc35mag_K | denisDR3Source | DENIS | K band Magnitude in 3.5" corr. aperture | float | 8 | mag | ||
| aperCor1 | MultiframeDetector | ATLASDR1 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | ATLASDR2 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | ATLASDR3 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | ATLASDR4 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | ATLASDR5 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | VPHASDR3 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor1 | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: 1⁄2 × core flux {catalogue extension keyword: APCOR1} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASDR1 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASDR2 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASDR3 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASDR4 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASDR5 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | VPHASDR3 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor2 | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: 1⁄√2 core flux {catalogue extension keyword: APCOR2} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASDR1 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASDR2 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASDR3 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASDR4 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASDR5 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | VPHASDR3 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor3 | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: core flux {catalogue extension keyword: APCOR3} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASDR1 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASDR2 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASDR3 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASDR4 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASDR5 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | VPHASDR3 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor4 | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: √2 × core flux {catalogue extension keyword: APCOR4} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASDR1 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASDR2 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASDR3 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASDR4 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASDR5 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | VPHASDR3 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor5 | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: 2 × core flux {catalogue extension keyword: APCOR5} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASDR1 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASDR2 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASDR3 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASDR4 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASDR5 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | VPHASDR3 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor6 | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: 2√2 × core flux {catalogue extension keyword: APCOR6} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASDR1 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASDR2 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASDR3 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASDR4 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASDR5 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | VPHASDR3 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCor7 | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: 4 × core flux {catalogue extension keyword: APCOR7} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASDR1 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASDR2 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASDR3 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASDR4 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASDR5 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASv20131127 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASv20160425 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | ATLASv20180209 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | VPHASDR3 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | VPHASv20160112 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperCorPeak | MultiframeDetector | VPHASv20170222 | Stellar aperture correction: peak height {catalogue extension keyword: APCORPK} corrected photometry = 2.5×log10(flux) + aperCor + skyCorr |
real | 4 | -0.9999995e9 | ?? | |
| Aperture corrections in magnitudes needed to correct the assorted aperture-like measures produced in the catalogues onto the equivalent of a total flux stellar system. These constitute the components of a curve-of-growth analysis contained within the catalogues with radii defined in the previous table. They also work well as a first order seeing correction for faint galaxies. Larger aperture corrections are not included. | ||||||||
| aperFlux1 | atlasDetection | ATLASDR1 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | atlasDetection | ATLASDR3 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | atlasDetection | ATLASDR4 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | atlasDetection | ATLASDR5 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | atlasDetection | ATLASv20131127 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | atlasDetection | ATLASv20160425 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | atlasDetection | ATLASv20180209 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | vphasDetection | VPHASv20160112 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | vphasDetection | VPHASv20170222 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux1 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Default aperture flux counts 1 {catalogue TType keyword: Aper_flux_1} 1/2 × rcore |
real | 4 | ADU | phot.count;em.opt | |
| These are a series of different radii soft-edged apertures designed to adequately sample the curve-of-growth of the majority of images and to provide fixed-sized aperture fluxes for all images. The scale size for these apertures is selected by defining a scale radius ≈<FWHM> for site+instrument. The "core" radius (rcore) has been fixed at 1.0 arcsec for convenience in inter-comparison with other datasets. A 1.0 arcsec radius is equivalent to 3.0 pixels for non-interleaved data, 6.0 pixels for 2×2 interleaved data, and 9.0 pixels for 3×3 interleaved data. In ≈1 arcsec seeing an rcore-radius aperture contains roughly 2/3 of the total flux of stellar images. [In general the rcore parameter is user specifiable and hence is recorded in the output catalogue FITS header.] The aperture fluxes are sky-corrected integrals (summations) with a soft-edge (ie. pro-rata flux division for boundary pixels). However, for overlapping images they are more subtle than this since they are in practice simultaneously fitted top-hat functions, to minimise the effects of crowding. Images external to the blend are also flagged and not included in the large radius summations. Extras for generalised galaxy photometry further spaced in radius to ensure reasonable sampling further out. Note these are all corrected for pixels from overlapping neighbouring images. The aperture fluxes can be combined with later-derived aperture corrections for general purpose photometry and together with pHeight (the peak flux) give a simple curve-of-growth measurement which forms the basis of the morphological classification scheme. | ||||||||
| aperFlux10 | atlasDetection | ATLASDR1 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | atlasDetection | ATLASDR3 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | atlasDetection | ATLASDR4 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | atlasDetection | ATLASDR5 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | atlasDetection | ATLASv20131127 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | atlasDetection | ATLASv20160425 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | atlasDetection | ATLASv20180209 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | vphasDetection | VPHASv20160112 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | vphasDetection | VPHASv20170222 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 10 {catalogue TType keyword: Aper_flux_10} 7 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux10err | atlasDetection | ATLASDR1 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | atlasDetection | ATLASDR3 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | atlasDetection | ATLASDR4 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | atlasDetection | ATLASDR5 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | atlasDetection | ATLASv20131127 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | atlasDetection | ATLASv20160425 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | atlasDetection | ATLASv20180209 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | vphasDetection | VPHASv20160112 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | vphasDetection | VPHASv20170222 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux10err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 10 {catalogue TType keyword: Aper_flux_10_err} | real | 4 | ADU | stat.error | |
| aperFlux11 | atlasDetection | ATLASDR1 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | atlasDetection | ATLASDR3 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | atlasDetection | ATLASDR4 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | atlasDetection | ATLASDR5 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | atlasDetection | ATLASv20131127 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | atlasDetection | ATLASv20160425 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | atlasDetection | ATLASv20180209 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | vphasDetection | VPHASv20160112 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | vphasDetection | VPHASv20170222 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 11 {catalogue TType keyword: Aper_flux_11} 8 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux11err | atlasDetection | ATLASDR1 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | atlasDetection | ATLASDR3 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | atlasDetection | ATLASDR4 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | atlasDetection | ATLASDR5 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | atlasDetection | ATLASv20131127 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | atlasDetection | ATLASv20160425 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | atlasDetection | ATLASv20180209 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | vphasDetection | VPHASv20160112 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | vphasDetection | VPHASv20170222 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux11err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 11 {catalogue TType keyword: Aper_flux_11_err} | real | 4 | ADU | stat.error | |
| aperFlux12 | atlasDetection | ATLASDR1 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | atlasDetection | ATLASDR3 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | atlasDetection | ATLASDR4 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | atlasDetection | ATLASDR5 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | atlasDetection | ATLASv20131127 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | atlasDetection | ATLASv20160425 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | atlasDetection | ATLASv20180209 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | vphasDetection | VPHASv20160112 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | vphasDetection | VPHASv20170222 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 12 {catalogue TType keyword: Aper_flux_12} 10 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux12err | atlasDetection | ATLASDR1 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | atlasDetection | ATLASDR3 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | atlasDetection | ATLASDR4 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | atlasDetection | ATLASDR5 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | atlasDetection | ATLASv20131127 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | atlasDetection | ATLASv20160425 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | atlasDetection | ATLASv20180209 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | vphasDetection | VPHASv20160112 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | vphasDetection | VPHASv20170222 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux12err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 12 {catalogue TType keyword: Aper_flux_12_err} | real | 4 | ADU | stat.error | |
| aperFlux13 | atlasDetection | ATLASDR1 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | atlasDetection | ATLASDR3 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | atlasDetection | ATLASDR4 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | atlasDetection | ATLASDR5 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | atlasDetection | ATLASv20131127 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | atlasDetection | ATLASv20160425 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | atlasDetection | ATLASv20180209 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | vphasDetection | VPHASv20160112 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | vphasDetection | VPHASv20170222 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 13 {catalogue TType keyword: Aper_flux_13} 12 × rcore ie. ≈24 arcsec diameter. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux13err | atlasDetection | ATLASDR1 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | atlasDetection | ATLASDR3 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | atlasDetection | ATLASDR4 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | atlasDetection | ATLASDR5 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | atlasDetection | ATLASv20131127 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | atlasDetection | ATLASv20160425 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | atlasDetection | ATLASv20180209 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | vphasDetection | VPHASv20160112 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | vphasDetection | VPHASv20170222 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux13err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 13 {catalogue TType keyword: Aper_flux_13_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection | ATLASDR1 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection | ATLASDR3 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection | ATLASDR4 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection | ATLASDR5 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection | ATLASv20131127 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection | ATLASv20160425 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection | ATLASv20180209 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | vphasDetection | VPHASv20160112 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | vphasDetection | VPHASv20170222 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux1err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux counts 1 {catalogue TType keyword: Aper_flux_1_err} | real | 4 | ADU | stat.error | |
| aperFlux2 | atlasDetection | ATLASDR1 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | atlasDetection | ATLASDR3 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | atlasDetection | ATLASDR4 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | atlasDetection | ATLASDR5 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | atlasDetection | ATLASv20131127 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | atlasDetection | ATLASv20160425 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | atlasDetection | ATLASv20180209 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | vphasDetection | VPHASv20160112 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | vphasDetection | VPHASv20170222 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Default aperture flux 2 {catalogue TType keyword: Aper_flux_2} 1/√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | phot.count;em.opt | |
| aperFlux2err | atlasDetection | ATLASDR1 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | atlasDetection | ATLASDR3 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | atlasDetection | ATLASDR4 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | atlasDetection | ATLASDR5 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | atlasDetection | ATLASv20131127 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | atlasDetection | ATLASv20160425 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | atlasDetection | ATLASv20180209 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | vphasDetection | VPHASv20160112 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | vphasDetection | VPHASv20170222 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux2err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 2 {catalogue TType keyword: Aper_flux_2_err} | real | 4 | ADU | stat.error | |
| aperFlux3 | atlasDetection | ATLASDR1 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | atlasDetection | ATLASDR3 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | atlasDetection | ATLASDR4 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | atlasDetection | ATLASDR5 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | atlasDetection | ATLASv20131127 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | atlasDetection | ATLASv20160425 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | atlasDetection | ATLASv20180209 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | vphasDetection | VPHASv20160112 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | vphasDetection | VPHASv20170222 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 3 {catalogue TType keyword: Aper_flux_3} rcore; recommended if a single number is required to represent the flux for ALL images. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux3err | atlasDetection | ATLASDR1 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | atlasDetection | ATLASDR3 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | atlasDetection | ATLASDR4 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | atlasDetection | ATLASDR5 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | atlasDetection | ATLASv20131127 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | atlasDetection | ATLASv20160425 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | atlasDetection | ATLASv20180209 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | vphasDetection | VPHASv20160112 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | vphasDetection | VPHASv20170222 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux3err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 3 {catalogue TType keyword: Aper_flux_3_err} | real | 4 | ADU | stat.error | |
| aperFlux4 | atlasDetection | ATLASDR1 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | atlasDetection | ATLASDR3 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | atlasDetection | ATLASDR4 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | atlasDetection | ATLASDR5 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | atlasDetection | ATLASv20131127 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | atlasDetection | ATLASv20160425 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | atlasDetection | ATLASv20180209 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | vphasDetection | VPHASv20160112 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | vphasDetection | VPHASv20170222 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 4 {catalogue TType keyword: Aper_flux_4} √2 × rcore; ensures ∼99% of PSF flux. (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux4err | atlasDetection | ATLASDR1 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | atlasDetection | ATLASDR3 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | atlasDetection | ATLASDR4 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | atlasDetection | ATLASDR5 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | atlasDetection | ATLASv20131127 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | atlasDetection | ATLASv20160425 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | atlasDetection | ATLASv20180209 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | vphasDetection | VPHASv20160112 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | vphasDetection | VPHASv20170222 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux4err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 4 {catalogue TType keyword: Aper_flux_4_err} | real | 4 | ADU | stat.error | |
| aperFlux5 | atlasDetection | ATLASDR1 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | atlasDetection | ATLASDR3 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | atlasDetection | ATLASDR4 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | atlasDetection | ATLASDR5 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | atlasDetection | ATLASv20131127 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | atlasDetection | ATLASv20160425 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | atlasDetection | ATLASv20180209 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | vphasDetection | VPHASv20160112 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | vphasDetection | VPHASv20170222 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 5 {catalogue TType keyword: Aper_flux_5} 2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux5err | atlasDetection | ATLASDR1 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | atlasDetection | ATLASDR3 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | atlasDetection | ATLASDR4 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | atlasDetection | ATLASDR5 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | atlasDetection | ATLASv20131127 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | atlasDetection | ATLASv20160425 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | atlasDetection | ATLASv20180209 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | vphasDetection | VPHASv20160112 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | vphasDetection | VPHASv20170222 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux5err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 5 {catalogue TType keyword: Aper_flux_5_err} | real | 4 | ADU | stat.error | |
| aperFlux6 | atlasDetection | ATLASDR1 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | atlasDetection | ATLASDR3 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | atlasDetection | ATLASDR4 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | atlasDetection | ATLASDR5 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | atlasDetection | ATLASv20131127 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | atlasDetection | ATLASv20160425 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | atlasDetection | ATLASv20180209 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | vphasDetection | VPHASv20160112 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | vphasDetection | VPHASv20170222 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 6 {catalogue TType keyword: Aper_flux_6} 2√2 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux6err | atlasDetection | ATLASDR1 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | atlasDetection | ATLASDR3 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | atlasDetection | ATLASDR4 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | atlasDetection | ATLASDR5 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | atlasDetection | ATLASv20131127 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | atlasDetection | ATLASv20160425 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | atlasDetection | ATLASv20180209 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | vphasDetection | VPHASv20160112 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | vphasDetection | VPHASv20170222 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux6err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 6 {catalogue TType keyword: Aper_flux_6_err} | real | 4 | ADU | stat.error | |
| aperFlux7 | atlasDetection | ATLASDR1 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | atlasDetection | ATLASDR3 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | atlasDetection | ATLASDR4 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | atlasDetection | ATLASDR5 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | atlasDetection | ATLASv20131127 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | atlasDetection | ATLASv20160425 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | atlasDetection | ATLASv20180209 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | vphasDetection | VPHASv20160112 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | vphasDetection | VPHASv20170222 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 7 {catalogue TType keyword: Aper_flux_7} 4 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux7err | atlasDetection | ATLASDR1 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | atlasDetection | ATLASDR3 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | atlasDetection | ATLASDR4 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | atlasDetection | ATLASDR5 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | atlasDetection | ATLASv20131127 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | atlasDetection | ATLASv20160425 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | atlasDetection | ATLASv20180209 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | vphasDetection | VPHASv20160112 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | vphasDetection | VPHASv20170222 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux7err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 7 {catalogue TType keyword: Aper_flux_7_err} | real | 4 | ADU | stat.error | |
| aperFlux8 | atlasDetection | ATLASDR1 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | atlasDetection | ATLASDR3 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | atlasDetection | ATLASDR4 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | atlasDetection | ATLASDR5 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | atlasDetection | ATLASv20131127 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | atlasDetection | ATLASv20160425 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | atlasDetection | ATLASv20180209 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | vphasDetection | VPHASv20160112 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | vphasDetection | VPHASv20170222 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 8 {catalogue TType keyword: Aper_flux_8} 5 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux8err | atlasDetection | ATLASDR1 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | atlasDetection | ATLASDR3 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | atlasDetection | ATLASDR4 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | atlasDetection | ATLASDR5 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | atlasDetection | ATLASv20131127 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | atlasDetection | ATLASv20160425 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | atlasDetection | ATLASv20180209 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | vphasDetection | VPHASv20160112 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | vphasDetection | VPHASv20170222 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux8err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 8 {catalogue TType keyword: Aper_flux_8_err} | real | 4 | ADU | stat.error | |
| aperFlux9 | atlasDetection | ATLASDR1 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | atlasDetection | ATLASDR3 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | atlasDetection | ATLASDR4 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | atlasDetection | ATLASDR5 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | atlasDetection | ATLASv20131127 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | atlasDetection | ATLASv20160425 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | atlasDetection | ATLASv20180209 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | vphasDetection | VPHASv20160112 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | vphasDetection | VPHASv20170222 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | default aperture flux 9 {catalogue TType keyword: Aper_flux_9} 6 × rcore (see glossary entry for aperFlux1) |
real | 4 | ADU | aperture | phot.count;em.opt |
| aperFlux9err | atlasDetection | ATLASDR1 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | atlasDetection | ATLASDR3 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | atlasDetection | ATLASDR4 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | atlasDetection | ATLASDR5 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | atlasDetection | ATLASv20131127 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | atlasDetection | ATLASv20160425 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | atlasDetection | ATLASv20180209 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | vphasDetection | VPHASv20160112 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | vphasDetection | VPHASv20170222 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperFlux9err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in aperture flux 9 {catalogue TType keyword: Aper_flux_9_err} | real | 4 | ADU | stat.error | |
| aperMag1 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag1 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 10. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag10err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag10err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 10 | real | 4 | mag | stat.error | |
| aperMag11 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 11. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag11err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag11err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 11 | real | 4 | mag | stat.error | |
| aperMag12 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 12. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag12err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag12err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 12 | real | 4 | mag | stat.error | |
| aperMag13 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 13. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag13err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag13err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 13 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag1err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 1 | real | 4 | mag | stat.error | |
| aperMag2 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 2 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag2err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag2err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 2 | real | 4 | mag | stat.error | |
| aperMag3 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 3. aperMag3 has also a saturation correction applied for saturated stars. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag3err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag3err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 3 | real | 4 | mag | stat.error | |
| aperMag4 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 4 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag4err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag4err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 4 | real | 4 | mag | stat.error | |
| aperMag5 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 5 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag5err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag5err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 5 | real | 4 | mag | stat.error | |
| aperMag6 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 6 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag6err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag6err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 6 | real | 4 | mag | stat.error | |
| aperMag7 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 7 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag7err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag7err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 7 | real | 4 | mag | stat.error | |
| aperMag8 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 8. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag8err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag8err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 8 | real | 4 | mag | stat.error | |
| aperMag9 | atlasDetection | ATLASDR1 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | atlasDetection | ATLASDR3 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | atlasDetection | ATLASDR4 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | atlasDetection | ATLASDR5 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | atlasDetection | ATLASv20131127 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | atlasDetection | ATLASv20160425 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | atlasDetection | ATLASv20180209 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | vphasDetection | VPHASv20160112 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | vphasDetection | VPHASv20170222 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and corrected aperture magnitude 9. No aperture correction applied since it is 0. | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMag9err | atlasDetection | ATLASDR1 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | atlasDetection | ATLASDR3 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | atlasDetection | ATLASDR4 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | atlasDetection | ATLASDR5 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | atlasDetection | ATLASv20131127 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | atlasDetection | ATLASv20160425 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | atlasDetection | ATLASv20180209 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | vphasDetection | VPHASv20160112 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | vphasDetection | VPHASv20170222 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMag9err | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Error in calibrated aperture magnitude 9 | real | 4 | mag | stat.error | |
| aperMagNoAperCorr1 | atlasDetection | ATLASDR1 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | atlasDetection | ATLASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | atlasDetection | ATLASDR4 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | atlasDetection | ATLASDR5 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | atlasDetection | ATLASv20131127 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | atlasDetection | ATLASv20160425 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | atlasDetection | ATLASv20180209 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | vphasDetection | VPHASv20160112 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | vphasDetection | VPHASv20170222 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr1 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection | ATLASDR1 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection | ATLASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection | ATLASDR4 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection | ATLASDR5 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection | ATLASv20131127 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection | ATLASv20160425 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection | ATLASv20180209 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | vphasDetection | VPHASv20160112 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | vphasDetection | VPHASv20170222 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr2 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection | ATLASDR1 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection | ATLASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection | ATLASDR4 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection | ATLASDR5 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection | ATLASv20131127 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection | ATLASv20160425 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection | ATLASv20180209 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | vphasDetection | VPHASv20160112 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | vphasDetection | VPHASv20170222 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr3 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection | ATLASDR1 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection | ATLASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection | ATLASDR4 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection | ATLASDR5 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection | ATLASv20131127 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection | ATLASv20160425 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection | ATLASv20180209 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | vphasDetection | VPHASv20160112 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | vphasDetection | VPHASv20170222 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr4 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection | ATLASDR1 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection | ATLASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection | ATLASDR4 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection | ATLASDR5 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection | ATLASv20131127 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection | ATLASv20160425 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection | ATLASv20180209 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | vphasDetection | VPHASv20160112 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | vphasDetection | VPHASv20170222 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr5 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection | ATLASDR1 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection | ATLASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection | ATLASDR4 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection | ATLASDR5 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection | ATLASv20131127 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection | ATLASv20160425 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection | ATLASv20180209 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | vphasDetection | VPHASv20160112 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | vphasDetection | VPHASv20170222 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr6 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection | ATLASDR1 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection | ATLASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection | ATLASDR4 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection | ATLASDR5 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection | ATLASv20131127 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection | ATLASv20160425 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection | ATLASv20180209 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | vphasDetection | VPHASv20160112 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | vphasDetection | VPHASv20170222 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperMagNoAperCorr7 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | Calibrated and standard corrected (but no aperture correction applied) aperture magnitude 1 | real | 4 | mag | phot.mag | |
| The aperture magnitudes are calculated from the given aperFlux values. The following standard corrections have been applied: zero points, extinction, exposure time, distortion, and illumination. Additionally aperMag3 has a saturation correction applied in case that: sky*peakHeight > 0.9*saturate. aperMag values also have the apermag corrections applied opposed to the AperMagNoAperCorr values. Since the apermag corrections for aperMags8 to 13 are 0, no apermag corrections (or a zero correction) have been applied to these values. | ||||||||
| aperture | RequiredListDrivenProduct | ATLASDR1 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | ATLASDR2 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | ATLASDR3 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | ATLASDR4 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | ATLASDR5 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | ATLASv20131127 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | ATLASv20160425 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | ATLASv20180209 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | VPHASDR3 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | VPHASv20160112 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aperture | RequiredListDrivenProduct | VPHASv20170222 | CASU list-driven photometry tool option specifying the fixed radius to be used for photometry | real | 4 | pixels | ?? | |
| aProf1 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf1 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 1 (can be non-integer for deblends) {catalogue TType keyword: Areal_1_profile} | real | 4 | pixels | meta.number | |
| Number of pixels above a series of threshold levels relative to local sky. Levels are set at T, 2T, 4T, 8T … 128T where T is the threshold. These can be thought of as a sort of poor man's radial profile. Note that for now deblended, ie. overlapping images, only the first areal profile is computed and the rest are set to -1 flagging the difficulty of computing accurate profiles. For blended images this parameter is used to flag the start of the sequence of the deblended components by setting the first in the sequence to 0. | ||||||||
| aProf2 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf2 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 2 {catalogue TType keyword: Areal_2_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf3 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 3 {catalogue TType keyword: Areal_3_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf4 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 4 {catalogue TType keyword: Areal_4_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf5 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 5 {catalogue TType keyword: Areal_5_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf6 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 6 {catalogue TType keyword: Areal_6_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf7 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 7 {catalogue TType keyword: Areal_7_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection | ATLASDR1 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection | ATLASDR3 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection | ATLASDR4 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection | ATLASDR5 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection | ATLASv20131127 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection | ATLASv20160425 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection | ATLASv20180209 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | atlasDetection, atlasDetectionUncorr | ATLASDR2 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | vphasDetection | VPHASv20160112 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | vphasDetection | VPHASv20170222 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aProf8 | vphasDetection, vphasDetectionUncorr | VPHASDR3 | No. of pixels above rethreshold 8 {catalogue TType keyword: Areal_8_profile} (see glossary entry for aProf1) |
int | 4 | pixels | meta.number | |
| aR | atlasSource | ATLASDR1 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aR | atlasSource | ATLASDR2 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aR | atlasSource | ATLASDR3 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aR | atlasSource | ATLASDR4 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aR | atlasSource | ATLASDR5 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aR | atlasSource | ATLASv20131127 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aR | atlasSource | ATLASv20160425 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aR | atlasSource | ATLASv20180209 | The galactic extinction correction in the R band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| arcfile | Multiframe | ATLASDR1 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | ATLASDR2 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | ATLASDR3 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | ATLASDR4 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | ATLASDR5 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | ATLASv20131127 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | ATLASv20160425 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | ATLASv20180209 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | VPHASDR3 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | VPHASv20160112 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| arcfile | Multiframe | VPHASv20170222 | Archive File Name {image primary HDU keyword: ARCFILE} | varchar | 64 | NONE | ||
| astrometric_chi2_al | gaia_source | GAIADR2 | Along-Scan chi-square value | real | 4 | stat.fit.chi2 | ||
| astrometric_delta_q | gaia_source, tgas_source | GAIADR1 | Hipparcos/Gaia data discrepancy (Hipparcos subset of TGAS only) | real | 4 | stat.value | ||
| astrometric_excess_noise | gaia_source | GAIADR2 | Excess noise of the source | float | 8 | milliarcsec | stat.value | |
| astrometric_excess_noise | gaia_source, tgas_source | GAIADR1 | Excess noise of the source | float | 8 | milliarcsec | stat.value | |
| astrometric_excess_noise_sig | gaia_source | GAIADR2 | Significance of the excess noise | float | 8 | stat.value | ||
| astrometric_excess_noise_sig | gaia_source, tgas_source | GAIADR1 | Significance of the excess noise | float | 8 | stat.value | ||
| astrometric_gof_al | gaia_source | GAIADR2 | Goodness of fit statistic of model wrt Along-Scan observations | real | 4 | stat.fit.goodness | ||
| astrometric_matched_observations | gaia_source | GAIADR2 | Matched FoV transits used in the AGIS solution | smallint | 2 | meta.number | ||
| astrometric_n_bad_obs_ac | gaia_source, tgas_source | GAIADR1 | Number of bad observations in the Across-Scan direction | int | 4 | meta.number | ||
| astrometric_n_bad_obs_al | gaia_source | GAIADR2 | Number of bad observations in the Along-Scan direction | int | 4 | meta.number | ||
| astrometric_n_bad_obs_al | gaia_source, tgas_source | GAIADR1 | Number of bad observations in the Along-Scan direction | int | 4 | meta.number | ||
| astrometric_n_good_obs_ac | gaia_source, tgas_source | GAIADR1 | Number of good observations in the Across-Scan direction | int | 4 | meta.number | ||
| astrometric_n_good_obs_al | gaia_source | GAIADR2 | Number of good observations in the Along-Scan direction | int | 4 | meta.number | ||
| astrometric_n_good_obs_al | gaia_source, tgas_source | GAIADR1 | Number of good observations in the Along-Scan direction | int | 4 | meta.number | ||
| astrometric_n_obs_ac | gaia_source | GAIADR2 | Total number of observations in the Across-Scan direction | int | 4 | meta.number | ||
| astrometric_n_obs_ac | gaia_source, tgas_source | GAIADR1 | Total number of observations in the Across-Scan direction | int | 4 | meta.number | ||
| astrometric_n_obs_al | gaia_source | GAIADR2 | Total number of observations in the Along-Scan direction | int | 4 | meta.number | ||
| astrometric_n_obs_al | gaia_source, tgas_source | GAIADR1 | Total number of observations in the Along-Scan direction | int | 4 | meta.number | ||
| astrometric_params_solved | gaia_source | GAIADR2 | Which parameters have been solved for? | tinyint | 1 | meta.number | ||
| astrometric_primary_flag | gaia_source | GAIADR2 | Primary or secondary | tinyint | 1 | meta.code.status | ||
| astrometric_primary_flag | gaia_source, tgas_source | GAIADR1 | Primary or secondary | bit | 1 | meta.code | ||
| astrometric_priors_used | aux_qso_icrf2_match | GAIADR1 | Type of prior used in the astrometric solution | int | 4 | meta.number | ||
| astrometric_priors_used | gaia_source, tgas_source | GAIADR1 | Type of prior used in the astrometric solution | int | 4 | |||
| astrometric_pseudo_colour | gaia_source | GAIADR2 | Astrometrically determined pseudocolour of the source | real | 4 | micron^-1 | em.wavenumber | |
| astrometric_pseudo_colour_error | gaia_source | GAIADR2 | STandard error of the pseudocolour of the source | real | 4 | micron^-1 | em.wavenumber | |
| astrometric_relegation_factor | gaia_source, tgas_source | GAIADR1 | Relegation factor | real | 4 | arith.factor | ||
| astrometric_sigma_5d_max | gaia_source | GAIADR2 | The longest semi-major axis of the 5d error ellipsoid | real | 4 | mas | pos.errorEllipse;stat.max | |
| astrometric_weight_ac | gaia_source, tgas_source | GAIADR1 | Mean astrometric weight of the source Across-Scan | real | 4 | stat.weight;stat.mean | ||
| astrometric_weight_al | gaia_source | GAIADR2 | Mean astrometric weight of the source Along-Scan | real | 4 | mas^-2 | stat.weight;stat.mean | |
| astrometric_weight_al | gaia_source, tgas_source | GAIADR1 | Mean astrometric weight of the source Along-Scan | real | 4 | stat.weight;stat.mean | ||
| atlasZPCat | MultiframeDetector | ATLASDR4 | Final ATLAS zero point (AB) for default extinction, calculated by ATLAS team using GaiaDR2 + photometry {catalogue extension keyword: ATLASZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| atlasZPCat | MultiframeDetector | ATLASDR5 | Final ATLAS zero point (AB) for default extinction, calculated by ATLAS team using GaiaDR2 + photometry {catalogue extension keyword: ATLASZPT} | real | 4 | mags | -0.9999995e9 | ?? |
| atlasZPCat | PreviousMFDZP | ATLASDR4 | Photometric zeropoint for final ATLAS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| atlasZPCat | PreviousMFDZP | ATLASDR5 | Photometric zeropoint for final ATLAS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| atlasZPErrCat | MultiframeDetector | ATLASDR4 | ATLAS zero point error {catalogue extension keyword: ATLASZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| atlasZPErrCat | MultiframeDetector | ATLASDR5 | ATLAS zero point error {catalogue extension keyword: ATLASZRR} | real | 4 | mags | -0.9999995e9 | ?? |
| atlasZPErrCat | PreviousMFDZP | ATLASDR4 | Photometric zeropoint error for final ATLAS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| atlasZPErrCat | PreviousMFDZP | ATLASDR5 | Photometric zeropoint error for final ATLAS (AB) in catalogue header | real | 4 | mag | -0.9999995e9 | |
| aU | atlasSource | ATLASDR1 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aU | atlasSource | ATLASDR2 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aU | atlasSource | ATLASDR3 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aU | atlasSource | ATLASDR4 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aU | atlasSource | ATLASDR5 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aU | atlasSource | ATLASv20131127 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aU | atlasSource | ATLASv20160425 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aU | atlasSource | ATLASv20180209 | The galactic extinction correction in the U band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aux_epc | igsl_source | GAIADR1 | Flag indicating presence in Ecliptic Poles Catalogue (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_gsc23 | igsl_source | GAIADR1 | Flag indicating presence in GSC2.3 (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_hip | igsl_source | GAIADR1 | Flag indicating presence in Hipparcos (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_lqrf | igsl_source | GAIADR1 | Flag indicating presence in LQRF (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_ogle | igsl_source | GAIADR1 | Flag indicating presence in OGLE (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_ppmxl | igsl_source | GAIADR1 | Flag indicating presence in PPMXL (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_sdss | igsl_source | GAIADR1 | Flag indicating presence in SDSS (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_tmass | igsl_source | GAIADR1 | Flag indicating presence in 2MASS PSC (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_tycho | igsl_source | GAIADR1 | Flag indicating presence in Tycho (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| aux_ucac | igsl_source | GAIADR1 | Flag indicating presence in UCAC (0 = no; 1 = yes) | bit | 1 | meta.id;meta.dataset | ||
| AV_Schlegel | ravedr5Source | RAVE | float | 8 | mag Total Extinction in V-band from Schlegel et al. (1998) | phys.absorption | ||
| averageConf | atlasDetection | ATLASDR1 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | atlasDetection | ATLASDR3 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | atlasDetection | ATLASDR4 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | atlasDetection | ATLASDR5 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | atlasDetection | ATLASv20131127 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | atlasDetection | ATLASv20160425 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | atlasDetection | ATLASv20180209 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | atlasDetection, atlasDetectionUncorr | ATLASDR2 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | vphasDetection | VPHASv20160112 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | vphasDetection | VPHASv20170222 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| averageConf | vphasDetection, vphasDetectionUncorr | VPHASDR3 | The average confidence level in the default 2 arcsec diameter aperture (aper3). {catalogue TType keyword: Av_conf} | real | 4 | -99999999 | meta.code | |
| avSaturLevel | MultiframeDetector | ATLASDR1 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | ATLASDR2 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | ATLASDR3 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | ATLASDR4 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | ATLASDR5 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | ATLASv20131127 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | ATLASv20160425 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | ATLASv20180209 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | VPHASDR3 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | VPHASv20160112 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avSaturLevel | MultiframeDetector | VPHASv20170222 | Average saturation level in frame {catalogue extension keyword: SATURATE} | real | 4 | -9.999995e+08 | ||
| avStellarEll | MultiframeDetector | ATLASDR1 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | ATLASDR2 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | ATLASDR3 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | ATLASDR4 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | ATLASDR5 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | ATLASv20131127 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | ATLASv20160425 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | ATLASv20180209 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | VPHASDR3 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | VPHASv20160112 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| avStellarEll | MultiframeDetector | VPHASv20170222 | Average stellar ellipticity (1-b/a) {catalogue extension keyword: ELLIPTIC} Should not average much above 0.15 for "normal" frames |
real | 4 | -0.9999995e9 | src.ellipticity | |
| axis1Length | MultiframeDetector | ATLASDR1 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | ATLASDR2 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | ATLASDR3 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | ATLASDR4 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | ATLASDR5 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | ATLASv20131127 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | ATLASv20160425 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | ATLASv20180209 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | VPHASDR3 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | VPHASv20160112 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis1Length | MultiframeDetector | VPHASv20170222 | length of data axis 1 (X-axis size) {image extension keyword: (Z)NAXIS1} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASDR1 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASDR2 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASDR3 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASDR4 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASDR5 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASv20131127 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASv20160425 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | ATLASv20180209 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | VPHASDR3 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | VPHASv20160112 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| axis2Length | MultiframeDetector | VPHASv20170222 | length of data axis 2 (Y-axis size) {image extension keyword: (Z)NAXIS2} | int | 4 | -99999999 | meta.number | |
| aZ | atlasSource | ATLASDR1 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aZ | atlasSource | ATLASDR2 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aZ | atlasSource | ATLASDR3 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aZ | atlasSource | ATLASDR4 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aZ | atlasSource | ATLASDR5 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aZ | atlasSource | ATLASv20131127 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | |
| aZ | atlasSource | ATLASv20160425 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |
| aZ | atlasSource | ATLASv20180209 | The galactic extinction correction in the Z band for extragalactic objects | real | 4 | mag | -0.9999995e9 | phys.absorption.gal |