K |
| Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
| k1 |
catwise_2020, catwise_prelim |
WISE |
W1 photometry usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) |
int |
4 |
|
|
|
| k2 |
catwise_2020, catwise_prelim |
WISE |
W2 photometry usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) |
int |
4 |
|
|
|
| k_2mrat |
twomass_scn |
TWOMASS |
Ks-band average 2nd image moment ratio. |
real |
4 |
|
|
stat.fit.param |
| k_2mrat |
twomass_sixx2_scn |
TWOMASS |
K band average 2nd image moment ratio for scan |
real |
4 |
|
|
|
| k_5sig_ba |
twomass_xsc |
TWOMASS |
K minor/major axis ratio fit to the 5-sigma isophote. |
real |
4 |
|
|
phys.size.axisRatio |
| k_5sig_phi |
twomass_xsc |
TWOMASS |
K angle to 5-sigma major axis (E of N). |
smallint |
2 |
degrees |
|
stat.error |
| k_5surf |
twomass_xsc |
TWOMASS |
K central surface brightness (r<=5). |
real |
4 |
mag |
|
phot.mag.sb |
| k_ba |
twomass_sixx2_xsc |
TWOMASS |
K minor/major axis ratio fit to the 3-sigma isophote |
real |
4 |
|
|
|
| k_ba |
twomass_xsc |
TWOMASS |
K minor/major axis ratio fit to the 3-sigma isophote. |
real |
4 |
|
|
phys.size.axisRatio |
| k_back |
twomass_xsc |
TWOMASS |
K coadd median background. |
real |
4 |
|
|
meta.code |
| k_bisym_chi |
twomass_xsc |
TWOMASS |
K bi-symmetric cross-correlation chi. |
real |
4 |
|
|
stat.fit.param |
| k_bisym_rat |
twomass_xsc |
TWOMASS |
K bi-symmetric flux ratio. |
real |
4 |
|
|
phot.flux;arith.ratio |
| k_bndg_amp |
twomass_xsc |
TWOMASS |
K banding maximum FT amplitude on this side of coadd. |
real |
4 |
DN |
|
stat.fit.param |
| k_bndg_per |
twomass_xsc |
TWOMASS |
K banding Fourier Transf. period on this side of coadd. |
int |
4 |
arcsec |
|
stat.fit.param |
| k_chif_ellf |
twomass_xsc |
TWOMASS |
K % chi-fraction for elliptical fit to 3-sig isophote. |
real |
4 |
|
|
stat.fit.param |
| k_cmsig |
twomass_psc |
TWOMASS |
Corrected photometric uncertainty for the default Ks-band magnitude. |
real |
4 |
mag |
Ks-band |
phot.flux |
| k_con_indx |
twomass_xsc |
TWOMASS |
K concentration index r_75%/r_25%. |
real |
4 |
|
|
phys.size;arith.ratio |
| k_d_area |
twomass_xsc |
TWOMASS |
K 5-sigma to 3-sigma differential area. |
smallint |
2 |
|
|
stat.fit.residual |
| k_flg_10 |
twomass_xsc |
TWOMASS |
K confusion flag for 10 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_15 |
twomass_xsc |
TWOMASS |
K confusion flag for 15 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_20 |
twomass_xsc |
TWOMASS |
K confusion flag for 20 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_25 |
twomass_xsc |
TWOMASS |
K confusion flag for 25 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_30 |
twomass_xsc |
TWOMASS |
K confusion flag for 30 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_40 |
twomass_xsc |
TWOMASS |
K confusion flag for 40 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_5 |
twomass_xsc |
TWOMASS |
K confusion flag for 5 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_50 |
twomass_xsc |
TWOMASS |
K confusion flag for 50 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_60 |
twomass_xsc |
TWOMASS |
K confusion flag for 60 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_7 |
twomass_sixx2_xsc |
TWOMASS |
K confusion flag for 7 arcsec circular ap. mag |
smallint |
2 |
|
|
|
| k_flg_7 |
twomass_xsc |
TWOMASS |
K confusion flag for 7 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_70 |
twomass_xsc |
TWOMASS |
K confusion flag for 70 arcsec circular ap. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_c |
twomass_xsc |
TWOMASS |
K confusion flag for Kron circular mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_e |
twomass_xsc |
TWOMASS |
K confusion flag for Kron elliptical mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_fc |
twomass_xsc |
TWOMASS |
K confusion flag for fiducial Kron circ. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_fe |
twomass_xsc |
TWOMASS |
K confusion flag for fiducial Kron ell. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_i20c |
twomass_xsc |
TWOMASS |
K confusion flag for 20mag/sq." iso. circ. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_i20e |
twomass_xsc |
TWOMASS |
K confusion flag for 20mag/sq." iso. ell. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_i21c |
twomass_xsc |
TWOMASS |
K confusion flag for 21mag/sq." iso. circ. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_i21e |
twomass_xsc |
TWOMASS |
K confusion flag for 21mag/sq." iso. ell. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_j21fc |
twomass_xsc |
TWOMASS |
K confusion flag for 21mag/sq." iso. fid. circ. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_j21fe |
twomass_xsc |
TWOMASS |
K confusion flag for 21mag/sq." iso. fid. ell. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_k20fc |
twomass_xsc |
TWOMASS |
K confusion flag for 20mag/sq." iso. fid. circ. mag. |
smallint |
2 |
|
|
meta.code |
| k_flg_k20fe |
twomass_sixx2_xsc |
TWOMASS |
K confusion flag for 20mag/sq.″ iso. fid. ell. mag |
smallint |
2 |
|
|
|
| k_flg_k20fe |
twomass_xsc |
TWOMASS |
K confusion flag for 20mag/sq." iso. fid. ell. mag. |
smallint |
2 |
|
|
meta.code |
| k_m |
twomass_psc |
TWOMASS |
Default Ks-band magnitude |
real |
4 |
mag |
|
phot.flux |
| k_m |
twomass_sixx2_psc |
TWOMASS |
K selected "default" magnitude |
real |
4 |
mag |
|
|
| k_m_10 |
twomass_xsc |
TWOMASS |
K 10 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_15 |
twomass_xsc |
TWOMASS |
K 15 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_20 |
twomass_xsc |
TWOMASS |
K 20 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_25 |
twomass_xsc |
TWOMASS |
K 25 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_2mass |
allwise_sc |
WISE |
2MASS Ks-band magnitude of the associated 2MASS PSC source. This column is "null" if there is no associated 2MASS PSC source or if the 2MASS PSC Ks-band magnitude entry is "null". |
float |
8 |
mag |
|
|
| k_m_2mass |
wise_allskysc |
WISE |
2MASS Ks-band magnitude or magnitude upper limit of the associated 2MASS PSC source. This column is default if there is no associated 2MASS PSC source or if the 2MASS PSC Ks-band magnitude entry is default. |
real |
4 |
mag |
-0.9999995e9 |
|
| k_m_2mass |
wise_prelimsc |
WISE |
2MASS Ks-band magnitude or magnitude upper limit of the associated 2MASS PSC source This column is default if there is no associated 2MASS PSC source or if the 2MASS PSC Ks-band magnitude entry is default |
real |
4 |
mag |
-0.9999995e9 |
|
| k_m_30 |
twomass_xsc |
TWOMASS |
K 30 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_40 |
twomass_xsc |
TWOMASS |
K 40 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_5 |
twomass_xsc |
TWOMASS |
K 5 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_50 |
twomass_xsc |
TWOMASS |
K 50 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_60 |
twomass_xsc |
TWOMASS |
K 60 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_7 |
twomass_sixx2_xsc |
TWOMASS |
K 7 arcsec radius circular aperture magnitude |
real |
4 |
mag |
|
|
| k_m_7 |
twomass_xsc |
TWOMASS |
K 7 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_70 |
twomass_xsc |
TWOMASS |
K 70 arcsec radius circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_c |
twomass_xsc |
TWOMASS |
K Kron circular aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_e |
twomass_xsc |
TWOMASS |
K Kron elliptical aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_ext |
twomass_sixx2_xsc |
TWOMASS |
K mag from fit extrapolation |
real |
4 |
mag |
|
|
| k_m_ext |
twomass_xsc |
TWOMASS |
K mag from fit extrapolation. |
real |
4 |
mag |
|
phot.flux |
| k_m_fc |
twomass_xsc |
TWOMASS |
K fiducial Kron circular magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_fe |
twomass_xsc |
TWOMASS |
K fiducial Kron ell. mag aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_i20c |
twomass_xsc |
TWOMASS |
K 20mag/sq." isophotal circular ap. magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_i20e |
twomass_xsc |
TWOMASS |
K 20mag/sq." isophotal elliptical ap. magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_i21c |
twomass_xsc |
TWOMASS |
K 21mag/sq." isophotal circular ap. magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_i21e |
twomass_xsc |
TWOMASS |
K 21mag/sq." isophotal elliptical ap. magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_j21fc |
twomass_xsc |
TWOMASS |
K 21mag/sq." isophotal fiducial circ. ap. mag. |
real |
4 |
mag |
|
phot.flux |
| k_m_j21fe |
twomass_xsc |
TWOMASS |
K 21mag/sq." isophotal fiducial ell. ap. magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_k20fc |
twomass_xsc |
TWOMASS |
K 20mag/sq." isophotal fiducial circ. ap. mag. |
real |
4 |
mag |
|
phot.flux |
| k_m_k20fe |
twomass_sixx2_xsc |
TWOMASS |
K 20mag/sq.″ isophotal fiducial ell. ap. magnitude |
real |
4 |
mag |
|
|
| k_m_k20fe |
twomass_xsc |
TWOMASS |
K 20mag/sq." isophotal fiducial ell. ap. magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_stdap |
twomass_psc |
TWOMASS |
Ks-band "standard" aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_m_sys |
twomass_xsc |
TWOMASS |
K system photometry magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_mnsurfb_eff |
twomass_xsc |
TWOMASS |
K mean surface brightness at the half-light radius. |
real |
4 |
mag |
|
phot.mag.sb |
| k_msig |
twomass_sixx2_psc |
TWOMASS |
K "default" mag uncertainty |
real |
4 |
mag |
|
|
| k_msig_10 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 10 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_15 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 15 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_20 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 20 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_25 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 25 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_2mass |
allwise_sc |
WISE |
2MASS Ks-band corrected photometric uncertainty of the associated 2MASS PSC source. This column is "null" if there is no associated 2MASS PSC source or if the 2MASS PSC Ks-band uncertainty entry is "null". |
float |
8 |
mag |
|
|
| k_msig_2mass |
wise_allskysc |
WISE |
2MASS Ks-band corrected photometric uncertainty of the associated 2MASS PSC source. This column is default if there is no associated 2MASS PSC source or if the 2MASS PSC Ks-band uncertainty entry is default. |
real |
4 |
mag |
-0.9999995e9 |
|
| k_msig_2mass |
wise_prelimsc |
WISE |
2MASS Ks-band corrected photometric uncertainty of the associated 2MASS PSC source This column is default if there is no associated 2MASS PSC source or if the 2MASS PSC Ks-band uncertainty entry is default |
real |
4 |
mag |
-0.9999995e9 |
|
| k_msig_30 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 30 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_40 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 40 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_5 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 5 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_50 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 50 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_60 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 60 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_7 |
twomass_sixx2_xsc |
TWOMASS |
K 1-sigma uncertainty in 7 arcsec circular ap. mag |
real |
4 |
mag |
|
|
| k_msig_7 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 7 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_70 |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 70 arcsec circular ap. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_c |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in Kron circular mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_e |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in Kron elliptical mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_ext |
twomass_sixx2_xsc |
TWOMASS |
K 1-sigma uncertainty in mag from fit extrapolation |
real |
4 |
mag |
|
|
| k_msig_ext |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in mag from fit extrapolation. |
real |
4 |
mag |
|
stat.error |
| k_msig_fc |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in fiducial Kron circ. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_fe |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in fiducial Kron ell. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_i20c |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 20mag/sq." iso. circ. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_i20e |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 20mag/sq." iso. ell. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_i21c |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 21mag/sq." iso. circ. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_i21e |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 21mag/sq." iso. ell. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_j21fc |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 21mag/sq." iso.fid.circ.mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_j21fe |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 21mag/sq." iso.fid.ell.mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_k20fc |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 20mag/sq." iso.fid.circ. mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_k20fe |
twomass_sixx2_xsc |
TWOMASS |
K 1-sigma uncertainty in 20mag/sq.″ iso.fid.ell.mag |
real |
4 |
mag |
|
|
| k_msig_k20fe |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in 20mag/sq." iso.fid.ell.mag. |
real |
4 |
mag |
|
stat.error |
| k_msig_stdap |
twomass_psc |
TWOMASS |
Uncertainty in the Ks-band standard aperture magnitude. |
real |
4 |
mag |
|
phot.flux |
| k_msig_sys |
twomass_xsc |
TWOMASS |
K 1-sigma uncertainty in system photometry mag. |
real |
4 |
mag |
|
stat.error |
| k_msigcom |
twomass_psc |
TWOMASS |
Combined, or total photometric uncertainty for the default Ks-band magnitude. |
real |
4 |
mag |
Ks-band |
phot.flux |
| k_msigcom |
twomass_sixx2_psc |
TWOMASS |
combined (total) K band photometric uncertainty |
real |
4 |
mag |
|
|
| k_msnr10 |
twomass_scn |
TWOMASS |
The estimated Ks-band magnitude at which SNR=10 is achieved for this scan. |
real |
4 |
mag |
|
phot.flux |
| k_msnr10 |
twomass_sixx2_scn |
TWOMASS |
K mag at which SNR=10 is achieved, from k_psp and k_zp_ap |
real |
4 |
mag |
|
|
| k_n_snr10 |
twomass_scn |
TWOMASS |
Number of point sources at Ks-band with SNR>10 (instrumental mag <=14.3) |
int |
4 |
|
|
meta.number |
| k_n_snr10 |
twomass_sixx2_scn |
TWOMASS |
number of K point sources with SNR>10 (instrumental m<=14.3) |
int |
4 |
|
|
|
| k_pchi |
twomass_xsc |
TWOMASS |
K chi^2 of fit to rad. profile (LCSB: alpha scale len). |
real |
4 |
|
|
stat.fit.param |
| k_peak |
twomass_xsc |
TWOMASS |
K peak pixel brightness. |
real |
4 |
mag |
|
phot.mag.sb |
| k_perc_darea |
twomass_xsc |
TWOMASS |
K 5-sigma to 3-sigma percent area change. |
smallint |
2 |
|
|
FIT_PARAM |
| k_phi |
twomass_sixx2_xsc |
TWOMASS |
K angle to 3-sigma major axis (E of N) |
smallint |
2 |
deg |
|
|
| k_phi |
twomass_xsc |
TWOMASS |
K angle to 3-sigma major axis (E of N). |
smallint |
2 |
degrees |
|
pos.posAng |
| k_psfchi |
twomass_psc |
TWOMASS |
Reduced chi-squared goodness-of-fit value for the Ks-band profile-fit photometry made on the 1.3 s "Read_2" exposures. |
real |
4 |
|
|
stat.fit.param |
| k_psp |
twomass_scn |
TWOMASS |
Ks-band photometric sensitivity paramater (PSP). |
real |
4 |
|
|
instr.sensitivity |
| k_psp |
twomass_sixx2_scn |
TWOMASS |
K photometric sensitivity param: k_shape_avg*(k_fbg_avg^.29) |
real |
4 |
|
|
|
| k_pts_noise |
twomass_scn |
TWOMASS |
Base-10 logarithm of the mode of the noise distribution for all point source detections in the scan, where the noise is estimated from the measured Ks-band photometric errors and is expressed in units of mJy. |
real |
4 |
|
|
instr.det.noise |
| k_pts_noise |
twomass_sixx2_scn |
TWOMASS |
log10 of K band modal point src noise estimate |
real |
4 |
logmJy |
|
|
| k_r_c |
twomass_xsc |
TWOMASS |
K Kron circular aperture radius. |
real |
4 |
arcsec |
|
phys.angSize;src |
| k_r_e |
twomass_xsc |
TWOMASS |
K Kron elliptical aperture semi-major axis. |
real |
4 |
arcsec |
|
phys.angSize;src |
| k_r_eff |
twomass_xsc |
TWOMASS |
K half-light (integrated half-flux point) radius. |
real |
4 |
arcsec |
|
phys.angSize;src |
| k_r_i20c |
twomass_xsc |
TWOMASS |
K 20mag/sq." isophotal circular aperture radius. |
real |
4 |
arcsec |
|
phys.angSize;src |
| k_r_i20e |
twomass_xsc |
TWOMASS |
K 20mag/sq." isophotal elliptical ap. semi-major axis. |
real |
4 |
arcsec |
|
phys.angSize;src |
| k_r_i21c |
twomass_xsc |
TWOMASS |
K 21mag/sq." isophotal circular aperture radius. |
real |
4 |
arcsec |
|
phys.angSize;src |
| k_r_i21e |
twomass_xsc |
TWOMASS |
K 21mag/sq." isophotal elliptical ap. semi-major axis. |
real |
4 |
arcsec |
|
phys.angSize;src |
| k_resid_ann |
twomass_xsc |
TWOMASS |
K residual annulus background median. |
real |
4 |
DN |
|
meta.code |
| k_sc_1mm |
twomass_xsc |
TWOMASS |
K 1st moment (score) (LCSB: super blk 2,4,8 SNR). |
real |
4 |
|
|
meta.code |
| k_sc_2mm |
twomass_xsc |
TWOMASS |
K 2nd moment (score) (LCSB: SNRMAX - super SNR max). |
real |
4 |
|
|
meta.code |
| k_sc_msh |
twomass_xsc |
TWOMASS |
K median shape score. |
real |
4 |
|
|
meta.code |
| k_sc_mxdn |
twomass_xsc |
TWOMASS |
K mxdn (score) (LCSB: BSNR - block/smoothed SNR). |
real |
4 |
|
|
meta.code |
| k_sc_r1 |
twomass_xsc |
TWOMASS |
K r1 (score). |
real |
4 |
|
|
meta.code |
| k_sc_r23 |
twomass_xsc |
TWOMASS |
K r23 (score) (LCSB: TSNR - integrated SNR for r=15). |
real |
4 |
|
|
meta.code |
| k_sc_sh |
twomass_xsc |
TWOMASS |
K shape (score). |
real |
4 |
|
|
meta.code |
| k_sc_vint |
twomass_xsc |
TWOMASS |
K vint (score). |
real |
4 |
|
|
meta.code |
| k_sc_wsh |
twomass_xsc |
TWOMASS |
K wsh (score) (LCSB: PSNR - peak raw SNR). |
real |
4 |
|
|
meta.code |
| k_seetrack |
twomass_xsc |
TWOMASS |
K band seetracking score. |
real |
4 |
|
|
meta.code |
| k_sh0 |
twomass_xsc |
TWOMASS |
K ridge shape (LCSB: BSNR limit). |
real |
4 |
|
|
FIT_PARAM |
| k_shape_avg |
twomass_scn |
TWOMASS |
Ks-band average seeing shape for scan. |
real |
4 |
|
|
instr.obsty.seeing |
| k_shape_avg |
twomass_sixx2_scn |
TWOMASS |
K band average seeing shape for scan |
real |
4 |
|
|
|
| k_shape_rms |
twomass_scn |
TWOMASS |
RMS-error of Ks-band average seeing shape. |
real |
4 |
|
|
instr.obsty.seeing |
| k_shape_rms |
twomass_sixx2_scn |
TWOMASS |
rms of K band avg seeing shape for scan |
real |
4 |
|
|
|
| k_sig_sh0 |
twomass_xsc |
TWOMASS |
K ridge shape sigma (LCSB: B2SNR limit). |
real |
4 |
|
|
FIT_PARAM |
| k_snr |
twomass_psc |
TWOMASS |
Ks-band "scan" signal-to-noise ratio. |
real |
4 |
mag |
|
instr.det.noise |
| k_snr |
twomass_sixx2_psc |
TWOMASS |
K band "scan" signal-to-noise ratio |
real |
4 |
|
|
|
| k_subst2 |
twomass_xsc |
TWOMASS |
K residual background #2 (score). |
real |
4 |
|
|
meta.code |
| k_zp_ap |
twomass_scn |
TWOMASS |
Photometric zero-point for Ks-band aperture photometry. |
real |
4 |
mag |
|
phot.mag;arith.zp |
| k_zp_ap |
twomass_sixx2_scn |
TWOMASS |
K band ap. calibration photometric zero-point for scan |
real |
4 |
mag |
|
|
| k_zperr_ap |
twomass_scn |
TWOMASS |
RMS-error of zero-point for Ks-band aperture photometry |
real |
4 |
mag |
|
stat.error |
| k_zperr_ap |
twomass_sixx2_scn |
TWOMASS |
K band ap. calibration rms error of zero-point for scan |
real |
4 |
mag |
|
|
| ka |
catwise_2020, catwise_prelim |
WISE |
astrometry usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) |
int |
4 |
|
|
|
| kABMagLim |
allSkyNIRFrameSetInfo |
VULCANiDR |
AB magnitude limit of pointing in K/Ks band |
float |
8 |
mag |
|
|
| kAllAperMag3 |
allSkyNIRSource |
VULCANiDR |
Default point source K/Ks aperture corrected mag (2.0 arcsec aperture diameter) using All Sky calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kAllAperMag3Err |
allSkyNIRSource |
VULCANiDR |
Error in default point/extended source K/Ks mag (2.0 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kAllAperMag4 |
allSkyNIRSource |
VULCANiDR |
Point source K/Ks aperture corrected mag (2.8 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kAllAperMag4Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source K/Ks mag (2.8 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kAllAperMag6 |
allSkyNIRSource |
VULCANiDR |
Point source K/Ks aperture corrected mag (5.7 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kAllAperMag6Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source K/Ks mag (5.7 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kAllAperMagNoAperCorr3 |
allSkyNIRSource |
VULCANiDR |
Default extended source K/Ks aperture mag (2.0 arcsec aperture diameter) using All Sky calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kAllAperMagNoAperCorr4 |
allSkyNIRSource |
VULCANiDR |
Extended source K/Ks aperture mag (2.8 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kAllAperMagNoAperCorr6 |
allSkyNIRSource |
VULCANiDR |
Extended source K/Ks aperture mag (5.7 arcsec aperture diameter) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kAllPetroMag |
allSkyNIRSource |
VULCANiDR |
Extended source K/Ks mag (Petrosian) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kAllPetroMagErr |
allSkyNIRSource |
VULCANiDR |
Error in extended source K/Ks mag (Petrosian) using All Sky calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kClass |
allSkyNIRSource |
VULCANiDR |
discrete image classification flag in K/Ks |
smallint |
2 |
|
-9999 |
src.class&MagUCD& |
| kClassStat |
allSkyNIRSource |
VULCANiDR |
N(0,1) stellarness-of-profile statistic/SExtractor STAR_CLASS in K/Ks |
real |
4 |
|
-0.9999995e9 |
stat&MagUCD& |
| kEll |
allSkyNIRSource |
VULCANiDR |
1-b/a, where a/b=semi-major/minor axes in K/Ks |
real |
4 |
|
-0.9999995e9 |
src.ellipticity&MagUCD& |
| keNum |
allSkyNIRFrameSetInfo |
VULCANiDR |
the extension number of this K/Ks frame |
tinyint |
1 |
|
|
meta.number;em.IR.K |
| kErrBits |
allSkyNIRSource |
VULCANiDR |
processing warning/error bitwise flags in K/Ks |
int |
4 |
|
-99999999 |
meta.code&MagUCD& |
| Apparently not actually an error bit flag, but a count of the number of zero confidence pixels in the default (2 arcsec diameter) aperture. |
| kEta |
allSkyNIRSource |
VULCANiDR |
Offset of K/Ks detection from master position (+north/-south) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.dec;arith.diff&MagUCD& |
| When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 2.0 (UKIDSS LAS and GPS; UHS; also non-survey programmes) or 1.0 (UKIDSS GPS, DXS and UDS) arcseconds is used, the higher value enabling pairing of moving sources when epoch separations may be several years. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the LAS, you might wish to insist that the offsets in the selected sample are all below 1 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |
| kGausig |
allSkyNIRSource |
VULCANiDR |
RMS of axes of ellipse fit in K/Ks |
real |
4 |
pixels |
-0.9999995e9 |
src.morph.param&MagUCD& |
| kHlCorSMjRadAs |
allSkyNIRSource |
VULCANiDR |
Seeing corrected half-light, semi-major axis in K/Ks band |
real |
4 |
arcsec |
-0.9999995e9 |
phys.angSize;em.opt.I |
| km |
catwise_2020, catwise_prelim |
WISE |
proper motion usage code (0: neither the ascending nor the descending scan provided a solution; 1: only the ascending scan provided a solution; 2: only the descending scan provided a solution; 3: both scans provided solutions which were combined in the relevant way) |
int |
4 |
|
|
|
| kmfID |
allSkyNIRFrameSetInfo |
VULCANiDR |
the UID of the relevant K/Ks multiframe |
bigint |
8 |
|
|
meta.id;obs.field;em.IR.K |
| kMjd |
allSkyNIRSource |
VULCANiDR |
Modified Julian Day in K/Ks band |
float |
8 |
days |
-0.9999995e9 |
time.epoch&MagUCD& |
| kNEpochs |
allSkyNIRFrameSetInfo |
VULCANiDR |
Number of epochs in K/Ks band (0 if no measurements) |
int |
4 |
|
|
|
| kObs |
allSkyNIRSource |
VULCANiDR |
There are pixels at this position in the K/Ks-band |
tinyint |
1 |
|
0 |
meta.flag |
| kPA |
allSkyNIRSource |
VULCANiDR |
ellipse fit celestial orientation in K/Ks |
real |
4 |
Degrees |
-0.9999995e9 |
pos.posAng&MagUCD& |
| kppErrBits |
allSkyNIRSource |
VULCANiDR |
additional WFAU post-processing error bits in K/Ks |
int |
4 |
|
0 |
meta.code&MagUCD& |
Post-processing error quality bit flags assigned (NB: from UKIDSS DR2 release onwards) in the WSA curation procedure for survey data. From least to most significant byte in the 4-byte integer attribute byte 0 (bits 0 to 7) corresponds to information on generally innocuous conditions that are nonetheless potentially significant as regards the integrity of that detection; byte 1 (bits 8 to 15) corresponds to warnings; byte 2 (bits 16 to 23) corresponds to important warnings; and finally byte 3 (bits 24 to 31) corresponds to severe warnings: | Byte | Bit | Detection quality issue | Threshold or bit mask | Applies to | | | | Decimal | Hexadecimal | | | 0 | 4 | Deblended | 16 | 0x00000010 | All VDFS catalogues | | 0 | 6 | Bad pixel(s) in default aperture | 64 | 0x00000040 | All VDFS catalogues | | 1 | 15 | Source in poor flat field region | 32768 | 0x00008000 | All but mosaics | | 2 | 16 | Close to saturated | 65536 | 0x00010000 | All VDFS catalogues (though deeps excluded prior to DR8) | | 2 | 17 | Photometric calibration probably subject to systematic error | 131072 | 0x00020000 | GPS only | | 2 | 19 | Possible crosstalk artefact/contamination | 524288 | 0x00080000 | All but GPS | | 2 | 22 | Lies within a dither offset of the stacked frame boundary | 4194304 | 0x00400000 | All but mosaics | In this way, the higher the error quality bit flag value, the more likely it is that the detection is spurious. The decimal threshold (column 4) gives the minimum value of the quality flag for a detection having the given condition (since other bits in the flag may be set also; the corresponding hexadecimal value, where each digit corresponds to 4 bits in the flag, can be easier to compute when writing SQL queries to test for a given condition). For example, to exclude all K band sources in the LAS having any error quality condition other than informational ones, include a predicate ... AND kppErrBits ≤ 255. See the SQL Cookbook and other online pages for further information. |
| kronFlux |
Detection |
PS1DR2 |
Kron (1980) flux. |
real |
4 |
Janskys |
-999 |
|
| kronFluxErr |
Detection |
PS1DR2 |
Error on Kron (1980) flux. |
real |
4 |
Janskys |
-999 |
|
| kronRad |
Detection |
PS1DR2 |
Kron (1980) radius. |
real |
4 |
arcsec |
-999 |
|
| kSeeing |
allSkyNIRFrameSetInfo |
VULCANiDR |
Ks band seeing |
float |
8 |
arcsec |
|
|
| kSeqNum |
allSkyNIRSource |
VULCANiDR |
the running number of the K/Ks detection |
int |
4 |
|
-99999999 |
meta.number&MagUCD& |
| kTelAperMag3 |
allSkyNIRSource |
VULCANiDR |
Default point source K/Ks aperture corrected mag (2.0 arcsec aperture diameter) using original calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kTelAperMag3Err |
allSkyNIRSource |
VULCANiDR |
Error in default point/extended source K/Ks mag (2.0 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kTelAperMag4 |
allSkyNIRSource |
VULCANiDR |
Point source K/Ks aperture corrected mag (2.8 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kTelAperMag4Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source K/Ks mag (2.8 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kTelAperMag6 |
allSkyNIRSource |
VULCANiDR |
Point source K/Ks aperture corrected mag (5.7 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kTelAperMag6Err |
allSkyNIRSource |
VULCANiDR |
Error in point/extended source K/Ks mag (5.7 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kTelAperMagNoAperCorr3 |
allSkyNIRSource |
VULCANiDR |
Default extended source K/Ks aperture mag (2.0 arcsec aperture diameter) using original calibration If in doubt use this flux estimator |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kTelAperMagNoAperCorr4 |
allSkyNIRSource |
VULCANiDR |
Extended source K/Ks aperture mag (2.8 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kTelAperMagNoAperCorr6 |
allSkyNIRSource |
VULCANiDR |
Extended source K/Ks aperture mag (5.7 arcsec aperture diameter) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kTelPetroMag |
allSkyNIRSource |
VULCANiDR |
Extended source K/Ks mag (Petrosian) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
phot.mag&MagUCD& |
| kTelPetroMagErr |
allSkyNIRSource |
VULCANiDR |
Error in extended source K/Ks mag (Petrosian) using original calibration |
real |
4 |
mag |
-0.9999995e9 |
stat.error;phot.mag&MagUCD& |
| kXi |
allSkyNIRSource |
VULCANiDR |
Offset of K/Ks detection from master position (+east/-west) |
real |
4 |
arcsec |
-0.9999995e9 |
pos.eq.ra;arith.diff&MagUCD& |
| When associating individual passband detections into merged sources, a generous (in terms of the positional uncertainties) pairing radius of 2.0 (UKIDSS LAS and GPS; UHS; also non-survey programmes) or 1.0 (UKIDSS GPS, DXS and UDS) arcseconds is used, the higher value enabling pairing of moving sources when epoch separations may be several years. Such a large association criterion can of course lead to spurious pairings in the merged sources lists (although note that between passband pairs, handshake pairing is done: both passbands must agree that the candidate pair is their nearest neighbour for the pair to propagate through into the merged source table). In order to help filter spurious pairings out, and assuming that large positional offsets between the different passband detections are not expected (e.g. because of source motion, or larger than usual positional uncertainties) then the attributes Xi and Eta can be used to filter any pairings with suspiciously large offsets in one or more bands. For example, for a clean sample of QSOs from the LAS, you might wish to insist that the offsets in the selected sample are all below 1 arcsecond: simply add WHERE clauses into the SQL sample selection script to exclude all Xi and Eta values larger than the threshold you want. NB: the master position is the position of the detection in the shortest passband in the set, rather than the ra/dec of the source as stored in source attributes of the same name. The former is used in the pairing process, while the latter is generally the optimally weighted mean position from an astrometric solution or other combinatorial process of all individual detection positions across the available passbands. |