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Glossary of OSA attributes
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

W
Name	Schema Table	Database	Description	Type	Length	Unit	Default Value	Unified Content Descriptor
w1ab_map	catwise_2020, catwise_prelim	WISE	w1 artifact code value	int	4
w1ab_map_str	catwise_2020, catwise_prelim	WISE	w1 artifact string	varchar	13
w1ba	allwise_sc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W1.	float	8	arcsec
w1ba	wise_allskysc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W1.	real	4	arcsec	-0.9999995e9
w1ba	wise_prelimsc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W1	real	4	arcsec	-0.9999995e9
w1cc_map	allwise_sc	WISE	Contamination and confusion map for this source in W1. This column contains the integer equivalent of the 9-bit binary number that specifies if the W1 measurement is believed to be contaminated by or a spurious detection of an image artifact.	int	4
			The elements of the binary array are: S 0 0 0 O H 0 P D. The leftmost bit, S, differentiates whether the band-detection is believed to be a real detection contaminated by an artifact ("0") or a spurious detection of an artifact ("1"). The remaining bits are set to "1" to denote contamination by different types of artifacts according to the letters: D - Diffraction spike. Source may be a spurious detection of or contaminated by a diffraction spike of a nearby bright star on the same image. P - Persistence. Source may be a spurious detection of or contaminated by a short-term latent (persistence) image left by a bright source. H - Halo. Source may be a spurious detection of or contaminated by the scattered light halo associated with a bright star. O (letter "o") - Optical ghost. Source may be a spurious detection of or contaminated by an optical ghost image caused by a nearby bright source on the same image. For example, a measurement that is believed to be a spurious detection of a diffraction spike and scattered light halo has a binary bit map value of "100001001" and w?cc_map=265.
w1cc_map	catwise_2020, catwise_prelim	WISE	worst case w1cc_map from AllWISE	int	4
w1cc_map	wise_allskysc	WISE	Contamination and confusion map for this source in W1. This column contains the integer equivalent of the 9-bit binary number that specifies if the W1 measurement is believed to be contaminated by or a spurious detection of an image artifact.	smallint	2
w1cc_map	wise_prelimsc	WISE	Contamination and confusion map for this source in W1 This column contains the integer equivalent of the 9-bit binary number that specifies if the W1 measurement is believed to be contaminated by or a spurious detection of an image artifact	smallint	2
w1cc_map_str	allwise_sc	WISE	Contamination and confusion string. This column is a character string that denotes all artifacts that may contaminate the W1 measurement of this source, in the priority order D,P,H,O,d,p,h,o. Lower-case letters denote cases where the source detection in this band is believed to be real but the measurement may be contaminated by the artifact. upper-case letters denote cases where the source detection in this band may be a spurious detection of an artifact. This string is "null" if there are no artifacts that affect the measurement in this band. The value that appears in first element of the cc_flags string is the left-most character in w1cc_map_str. If w1cc_map_str is "null", then the corresponding cc_flags entry is "0".	varchar	9
			For example, a real detection that is contaminated by a diffraction spike and a latent (persistent) image has a w?cc_map_str="dp". A spurious detection of a diffraction spike that is also contaminated by a latent image has w?cc_map_str="Dp".
w1cc_map_str	catwise_2020, catwise_prelim	WISE	worst case w1cc_map_str from AllWISE	varchar	20
w1cc_map_str	wise_allskysc	WISE	Contamination and confusion string in W1. This column is a character string that denotes all artifacts that may contaminate the W1 measurement of this source, in the priority order D,P,H,O,d,p,h,o.	char	9
w1cc_map_str	wise_prelimsc	WISE	Contamination and confusion string in W1 This column is a character string that denotes all artifacts that may contaminate the W1 measurement of this source, in the priority order D,P,H,O	char	9
w1conf	allwise_sc	WISE	Estimated confusion noise in the W1 sky background annulus, in digital numbers. This number is the difference between the measured noise in the sky background w1sigsk and the noise measured in the same region on the Atlas Uncertainty Maps.	float	8	dn
w1conf	catwise_2020, catwise_prelim	WISE	frame sky confusion based on the UNC images	real	4	dn
w1conf	wise_allskysc	WISE	Estimated confusion noise in the W1 sky background annulus, in digital numbers. This number is the difference between the measured noise in the sky background w1sigsk and the noise measured in the same region on the Atlas Uncertainty Maps.	float	8	ADU	-0.9999995e9
w1conf	wise_prelimsc	WISE	Estimated confusion noise in the W1 sky background annulus, in digital numbers This number is the difference between the measured noise in the sky background w1sigsk and the noise measured in the same region on the Atlas Uncertainty Maps	float	8	ADU	-0.9999995e9
w1Cov	catwise_2020, catwise_prelim	WISE	mean coverage depth, band-1	real	4
w1cov	allwise_sc	WISE	Mean pixel coverage in W1. This column gives the mean pixel value from the W1 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source.	float	8
			W1cov may differ from the integer frame coverage value given in w1m for two reasons. First, individual pixels in the measurement area may be masked or otherwise unusable, reducing the effective pixel count and thus the mean coverage value. Second, the effective sky area sampled by a pixels in single-exposure image varies across the focal plane because of field distortion. Distortion is corrected when coadding to generate the Atlas Images. Therefore, the effective number of pixels contributing to a pixel in the Atlas Coverage Map may be slightly smaller or larger than expected if there was no distortion. Third, the values of w1m may be artificially reduced for sources that are covered by saturated 3-Band Cryo single-exposures.
w1cov	wise_allskysc	WISE	Mean pixel coverage in W1. This column gives the mean pixel value from the W1 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source.	real	4		-0.9999995e9
w1cov	wise_prelimsc	WISE	Mean pixel coverage in W1 This column gives the mean pixel value from the W1 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source.	real	4		-0.9999995e9
w1dmag	wise_allskysc	WISE	Difference between maximum and minimum magnitude of the source from all usable single-exposure frames, W1. Single-exposure measurements with w1rchi2 values greater than 3.0 times the median are rejected from this computation.	real	4	mag	-0.9999995e9
w1fitr	catwise_2020, catwise_prelim	WISE	fitting radius, band-1 (clipped at 999.99)	real	4	asec
w1flg	allwise_sc	WISE	W1 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg	catwise_2020, catwise_prelim	WISE	standard aperture flag, band-1	int	4
			Standard aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise ususable pixels, or is an upper limit. The flag value is the integer sum of any of following values which correspond to different conditions: 0 - nominal: no contamination 1 - source confusion: another source falls within the measurement aperture/li> 2 - bad or fatal pixels: presence of bad pixels in the measurement aperture (bit 2 or 18 set) 4 - non-zero bit flag tripped (other than 2 or 18) 8 - corruption: all pixels are flagged as unusable, or the aperture flux is negative; in the former case, the aperture magnitude is "null"; in the latter case, the aperture magnitude is a 95% confidence upper limit 16 - saturation: here are one or more saturated pixels in the measurement aperture 32 - upper limit: the magnitude is a 95% confidence upper limit Note about upper limits: threshold = 2 * RMS if ( f < threshold) then if (f < 0) then upper_limit = threshold else upper_limit = f + threshold where f is the flux of the source, RMS is the source flux uncertainty. The upper limit is reported in the WPRO and standard aperture MAG columns; the reported uncertainty is set to 9.99 mag.
w1flg	wise_allskysc	WISE	W1 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	smallint	2		-9999
w1flg	wise_prelimsc	WISE	W1 "standard" aperture measurement quality flag This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit	smallint	2		-9999
w1flg_1	allwise_sc	WISE	W1 5.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_1	catwise_2020, catwise_prelim	WISE	Aper 1 (5.50 arcsec), aperture flag, band-1	int	4
w1flg_1	wise_allskysc	WISE	W1 5.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_1	wise_prelimsc	WISE	W1 5.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flg_2	allwise_sc	WISE	W1 8.25" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_2	catwise_2020, catwise_prelim	WISE	Aper 2 (8.25 arcsec), aperture flag, band-1	int	4
w1flg_2	wise_allskysc	WISE	W1 8.25" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_2	wise_prelimsc	WISE	W1 8.25" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flg_3	allwise_sc	WISE	W1 11.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_3	catwise_2020, catwise_prelim	WISE	Aper 3 (11.00 arcsec), aperture flag, band-1	int	4
w1flg_3	wise_allskysc	WISE	W1 11.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_3	wise_prelimsc	WISE	W1 11.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flg_4	allwise_sc	WISE	W1 13.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_4	catwise_2020, catwise_prelim	WISE	Aper 4 (13.75 arcsec), aperture flag, band-1	int	4
w1flg_4	wise_allskysc	WISE	W1 13.75" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_4	wise_prelimsc	WISE	W1 13.75" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flg_5	allwise_sc	WISE	W1 16.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_5	catwise_2020, catwise_prelim	WISE	Aper 5 (16.50 arcsec), aperture flag, band-1	int	4
w1flg_5	wise_allskysc	WISE	W1 16.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_5	wise_prelimsc	WISE	W1 16.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flg_6	allwise_sc	WISE	W1 19.25" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_6	catwise_2020, catwise_prelim	WISE	Aper 6 (19.25 arcsec), aperture flag, band-1	int	4
w1flg_6	wise_allskysc	WISE	W1 19.25" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_6	wise_prelimsc	WISE	W1 19.25" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flg_7	allwise_sc	WISE	W1 22.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_7	catwise_2020, catwise_prelim	WISE	Aper 7 (22.00 arcsec), aperture flag, band-1	int	4
w1flg_7	wise_allskysc	WISE	W1 22.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_7	wise_prelimsc	WISE	W1 22.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flg_8	allwise_sc	WISE	W1 24.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1flg_8	catwise_2020, catwise_prelim	WISE	Aper 8 (24.75 arcsec), aperture flag, band-1	int	4
w1flg_8	wise_allskysc	WISE	W1 24.75" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w1flg_8	wise_prelimsc	WISE	W1 24.75" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w1flux	allwise_sc	WISE	The "raw" W1 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w1flux	catwise_2020, catwise_prelim	WISE	WPRO raw flux, band-1	real	4	dn
w1flux	wise_allskysc	WISE	The "raw" W1 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w1flux	wise_prelimsc	WISE	The "raw" W1 source flux measured in profile-fit photometry in units of digital numbers This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w1flux_pm	catwise_2020, catwise_prelim	WISE	WPRO raw flux, band-1	real	4	dn
w1frl	wise_prelimsc	WISE	Fraction of W1 pixels affected by latents This column gives the fraction of all W1 pixels in the stack of individual W1 exposures used to characterize this source that may be affected by the presence of a latent image produced by a bright source	real	4		-0.9999995e9
w1frtr	wise_allskysc	WISE	Fraction of W1 pixels affected by transients. This column gives the fraction of all W1 pixels in the stack of individual W1 exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 7.25", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.	real	4		-0.9999995e9
w1gerr	allwise_sc	WISE	Uncertainty in the W1 magnitude of source measured in elliptical aperture. CAUTION: A w1gerr value of 9.999 indicates that the measurement uncertainty is very large, or the uncertainty could not be computed. In either case, the w1gmag measurement should be considered highly suspect.	float	8	mag
w1gerr	wise_allskysc	WISE	Uncertainty in the W1 magnitude of source measured in elliptical aperture.	real	4	mag	-0.9999995e9
w1gerr	wise_prelimsc	WISE	Uncertainty in the W1 magnitude of source measured in elliptical aperture	real	4	mag	-0.9999995e9
w1gflg	allwise_sc	WISE	W1 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w1gflg	wise_allskysc	WISE	W1 elliptical aperture measurement quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag, w1mflg.	smallint	2		-9999
w1gflg	wise_prelimsc	WISE	W1 elliptical aperture measurement quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag	smallint	2		-9999
w1gmag	allwise_sc	WISE	W1 magnitude of source measured in the elliptical aperture described by w1rsemi, w1ba, and w1pa.	float	8	mag
w1gmag	wise_allskysc	WISE	W1 magnitude of source measured in the elliptical aperture described by w1rsemi, w1ba, and w1pa.	real	4	mag	-0.9999995e9
w1gmag	wise_prelimsc	WISE	W1 magnitude of source measured in the elliptical aperture described by w1rsemi, w1ba, and w1pa	real	4	mag	-0.9999995e9
w1k	allwise_sc	WISE	Stetson K variability index (Stetson, P. 1996, PASP, 108, 851) computed using the W1 profile-fit fluxes measured on the individual single-exposure images. This column is null if there are <3 single-exposure measurements available in W1.	float	8
w1k	catwise_2020, catwise_prelim	WISE	Stetson k index for variability; band-1	real	4
w1M	catwise_2020, catwise_prelim	WISE	WPRO, M , band-1 M == number of flux measurements for a given source	int	4
w1m	allwise_sc	WISE	Integer frame coverage. This column gives the number of individual 7.7s W1 exposures on which a profile-fit measurement of this source was possible. This number can differ between the four bands because band-dependent criteria are used to select individual frames for inclusion in the coadded Atlas Images. This column is null if there is no frame coverage in this band at the position of this source. CAUTION: The value of w1m may be lower than expected for sources that were covered by saturated 3-Band Cryo single-exposures. A sign of this is if w1m differs significantly from w1cov.	int	4
w1m	wise_allskysc	WISE	Integer frame coverage in W1. This column gives the number of individual 7.7s W1 exposures on which a profile-fit measurement of this source was possible.	bigint	8		-99999999
w1m	wise_prelimsc	WISE	Integer frame coverage in W1 This column gives the number of individual 7.7s W1 exposures on which a profile-fit measurement of this source was possible	bigint	8		-99999999
w1mag	allwise_sc	WISE	W1 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w1mcor. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag	catwise_2020, catwise_prelim	WISE	standard aperture mag w/ correction applied	real	4	mag
w1mag	wise_allskysc	WISE	W1 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness.	real	4	mag	-0.9999995e9
w1mag	wise_prelimsc	WISE	W1 "standard" aperture magnitude This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness	real	4	mag	-0.9999995e9
w1mag_1	allwise_sc	WISE	W1 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8
w1mag_1	catwise_2020, catwise_prelim	WISE	Aper 1 (5.50 arcsec), aperture mag, band-1	real	4	mag
w1mag_1	wise_allskysc	WISE	W1 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_1	wise_prelimsc	WISE	W1 5.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
w1mag_2	allwise_sc	WISE	W1 8.25" radius aperture magnitude. This is the calibrated source brightness measured in a 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag_2	catwise_2020, catwise_prelim	WISE	Aper 2 (8.25 arcsec), aperture mag, band-1	real	4	mag
w1mag_2	wise_allskysc	WISE	W1 8.25" radius aperture magnitude. This is the calibrated source brightness measured in a 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_2	wise_prelimsc	WISE	W1 8.25" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
w1mag_3	allwise_sc	WISE	W1 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag_3	catwise_2020, catwise_prelim	WISE	Aper 3 (11.00 arcsec), aperture mag, band-1	real	4	mag
w1mag_3	wise_allskysc	WISE	W1 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_3	wise_prelimsc	WISE	W1 11.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
w1mag_4	allwise_sc	WISE	W1 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag_4	catwise_2020, catwise_prelim	WISE	Aper 4 (13.75 arcsec), aperture mag, band-1	real	4	mag
w1mag_4	wise_allskysc	WISE	W1 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_4	wise_prelimsc	WISE	W1 13.75" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
w1mag_5	allwise_sc	WISE	W1 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag_5	catwise_2020, catwise_prelim	WISE	Aper 5 (16.50 arcsec), aperture mag, band-1	real	4	mag
w1mag_5	wise_allskysc	WISE	W1 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_5	wise_prelimsc	WISE	W1 16.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
w1mag_6	allwise_sc	WISE	W1 19.25" radius aperture magnitude. This is the calibrated source brightness measured in a 19.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag_6	catwise_2020, catwise_prelim	WISE	Aper 6 (19.25 arcsec), aperture mag, band-1	real	4	mag
w1mag_6	wise_allskysc	WISE	W1 19.25" radius aperture magnitude. This is the calibrated source brightness measured in a 19.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_6	wise_prelimsc	WISE	W1 19.25" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
w1mag_7	allwise_sc	WISE	W1 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag_7	catwise_2020, catwise_prelim	WISE	Aper 7 (22.00 arcsec), aperture mag, band-1	real	4	mag
w1mag_7	wise_allskysc	WISE	W1 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_7	wise_prelimsc	WISE	W1 22.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
w1mag_8	allwise_sc	WISE	W1 24.75" radius aperture magnitude. This is the calibrated source brightness measured in a 24.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W1.	float	8	mag
w1mag_8	catwise_2020, catwise_prelim	WISE	Aper 8 (24.75 arcsec), aperture mag, band-1	real	4	mag
w1mag_8	wise_allskysc	WISE	W1 24.75" radius aperture magnitude. This is the calibrated source brightness measured in a 24.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W1.	real	4	mag	-0.9999995e9
w1mag_8	wise_prelimsc	WISE	W1 24.75" radius aperture magnitude This column is default if this aperture measurement was not possible in W1	real	4	mag	-0.9999995e9
W1mag_ALLWISE	ravedr5Source	RAVE	W1 magnitude from ALLWISE	real	4	mag		phot.mag;em.opt
w1magP	catwise_2020, catwise_prelim	WISE	WPRO repeatability mag; band-1	real	4	mag
w1magp	allwise_sc	WISE	Magnitude computed from the inverse-variance-weighted mean of the profile-fit flux measurements on the w1m individual W1 frames covering this source. This differs from w1mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w1mpro is computed by fitting all W1 frames simultaneously and incorporating a robust error model. This column is "null" if w1m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w1mpro for the optimal flux measurement for point sources.	float	8	mag
w1magp	wise_allskysc	WISE	Inverse-variance-weighted mean W1 magnitude computed from profile-fit measurements on the w1m individual frames covering this source. This differs from w1mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w1mpro is computed by fitting all W1 frames simultaneously and incorporating a robust error model. This column is default if w1m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w1mpro for the optimal flux measurement for point sources.	real	4	mag	-0.9999995e9
w1magp	wise_prelimsc	WISE	Inverse-variance-weighted mean W1 magnitude computed from profile-fit measurements on the w1m individual frames covering this source This differs from w1mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w1mpro is computed by fitting all W1 frames simultaneously and incorporating a robust error model. This column is default if w1m=0, the mean flux is negative or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w1mcor	allwise_sc	WISE	W1 aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness, w1mag_2, to give the "standard-aperture" magnitude.	float	8	mag
w1mcor	wise_allskysc	WISE	W1 aperture curve-of-growth correction. This correction is subtracted from the nominal 8.25" aperture photometry brightness, w1mag_2, to give the "standard-aperture" magnitude.	real	4	mag	-0.9999995e9
w1mcor	wise_prelimsc	WISE	W1 aperture curve-of-growth correction This correction is subtracted from the nominal 8.25" aperture photometry brightness, w1mag_2, to give the "standard-aperture" magnitude	real	4	mag	-0.9999995e9
w1mCorr	twompzPhotoz	TWOMPZ	WISE w1mpro measurement corrected for Galactic dust extinction {image primary HDU keyword: W1mCorr}	real	4		-0.9999995e9
w1mCorrErr	twompzPhotoz	TWOMPZ	W1 profile fit photometric measurement uncertainty {image primary HDU keyword: w1sigmpro}	real	4	mag	-0.9999995e9
w1mJDmax	catwise_2020, catwise_prelim	WISE	maximum mJD; band-1	float	8
w1mjdmax	allwise_sc, wise_allskysc	WISE	The latest modified Julian Date (mJD) of the W1 single-exposures covering the source.	float	8
w1mJDmea	catwise_2020, catwise_prelim	WISE	mean mJD; band-1	float	8
w1mjdmean	allwise_sc, wise_allskysc	WISE	The average modified Julian Date (mJD) of the W1 single-exposures covering the source.	float	8
w1mJDmin	catwise_2020, catwise_prelim	WISE	minimum mJD; band-1	float	8
w1mjdmin	allwise_sc, wise_allskysc	WISE	The earliest modified Julian Date (mJD) of the W1 single-exposures covering the source.	float	8
w1mLQ	catwise_2020, catwise_prelim	WISE	-log(Q), Q = 1-P(chi-square); band-1	real	4
w1mlq	allwise_sc	WISE	Probability measure that the source is variable in W1 flux. The value is -ln(Q), where Q = 1 - P(χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	float	8
			The Q value is the fraction of all cases to be at least as large as that observed if the null hypothesis is true. The null hypothesis is that the flux is emitted by a non-variable astrophysical object. It may be false because the object is a true variable. It may also be false because the flux measurement is corrupted by artifacts such as cosmic rays, scattered light, etc. The smaller the Q value, the more implausible the null hypothesis, i.e., the more likely it is that the flux is either variable or corrupted or both.
w1mlq	wise_allskysc	WISE	Probability measure that the source is variable in W1 flux. The value is -log10(Q), where Q = 1 - P(Χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	int	4		-99999999
w1mpro	allwise_sc	WISE	W1 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W1 flux measurement has SNR<2. This column is null if the source is nominally detected in W1, but no useful brightness estimate could be made.	float	8	mag
			NOTE: A special exception to the upper limit conditions described above applies if the W1 value of ph_qual is "Z" (e.g. ph_qual LIKE 'Z%'). In these cases, the value of w1mpro corresponds to the actual flux measurement, w1flux, or is null if w1flux is negative. This occurs for 106,140 sources in the AllWISE Catalog and 54,900 sources in the Reject Table, all of which are confined to a narrow strip of ecliptic longitude.
w1mpro	catwise_2020, catwise_prelim	WISE	WPRO flux in mag units, band-1	real	4	mag
w1mpro	wise_allskysc	WISE	W1 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W1 flux measurement has SNR<2. This column is default if the source is nominally detected in W1, but no useful brightness estimate could be made.	real	4	mag	-0.9999995e9
w1mpro	wise_prelimsc	WISE	W1 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W1 flux measurement has SNR<2 This column is default if the source is nominally detected in W1, but no useful brightness estimate could be made	real	4	mag	-0.9999995e9
w1mpro_pm	catwise_2020, catwise_prelim	WISE	WPRO flux in mag units, band-1	real	4	mag
w1Ndf	catwise_2020, catwise_prelim	WISE	No. degrees of freedom in var chi-square; band-1	int	4
w1ndf	allwise_sc	WISE	Number of degrees of freedom in the flux variability chi-square, W1.	int	4
w1ndf	wise_allskysc	WISE	Number of degrees of freedom in the flux variability chi-square, W1.	bigint	8		-99999999
w1NM	catwise_2020, catwise_prelim	WISE	WPRO, N (of M), band-1 M == number of flux measurements for a given source; N == number of M sources that have SNR >= 3	int	4
w1nm	allwise_sc	WISE	Integer frame detection count. This column gives the number of individual 7.7s exposures on which this source was detected with SNR>3 in the W1 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	int	4
w1nm	wise_allskysc	WISE	Integer frame detection count in W1. This column gives the number of individual 7.7s exposures on which this source was detected with SNR>3 in the W1 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	bigint	8		-99999999
w1nm	wise_prelimsc	WISE	Integer frame detection count in W1 This column gives the number of individual 7.7s exposures on which this source was detected with SNR>3 in the W1 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures	bigint	8		-99999999
w1pa	allwise_sc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W1.	float	8	deg
w1pa	wise_allskysc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W1.	real	4	degrees	-0.9999995e9
w1pa	wise_prelimsc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W1	real	4	degrees	-0.9999995e9
w1rchi2	allwise_sc	WISE	Reduced χ2 of the W1 profile-fit photometry measurement. This column is null if the W1 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4
w1rchi2	catwise_2020, catwise_prelim	WISE	WPRO reduced chi^2, band-1	real	4
w1rchi2	wise_allskysc	WISE	Reduced chi-squared of the W1 profile-fit photometry measurement. This column is default if the W1 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4		-0.9999995e9
w1rchi2	wise_prelimsc	WISE	Reduced chi-squared of the W1 profile-fit photometry measurement This column is default if the W1 magnitude is a 95% confidence upper limit (i.e. the source is not detected)	real	4		-0.9999995e9
w1rchi2_pm	allwise_sc	WISE	Reduced χ2 of the W1 profile-fit photometry measurement including motion estimation. This column is null if the source is not detected in W1, or if the motion fit failed to converge or was not attempted.	real	4
w1rchi2_pm	catwise_2020, catwise_prelim	WISE	WPRO reduced chi^2, band-1	real	4
w1rsemi	allwise_sc	WISE	Semi-major axis of the elliptical aperture used to measure source in W1.	float	8	arcsec
w1rsemi	wise_allskysc	WISE	Semi-major axis of the elliptical aperture used to measure source in W1.	real	4	arcsec	-0.9999995e9
w1rsemi	wise_prelimsc	WISE	Semi-major axis of the elliptical aperture used to measure source in W1	real	4	arcsec	-0.9999995e9
w1Sat	catwise_2020, catwise_prelim	WISE	fraction of pixels saturated, band-1	real	4
w1sat	allwise_sc	WISE	Saturated pixel fraction, W1. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W1]~8 mag. Saturation may occur in fainter sources because of charged particle strikes, or if the source is covered by 3-Band Cryo single-exposures that began to saturate because of rising temperatures.	float	8
w1sat	wise_allskysc	WISE	Saturated pixel fraction, W1. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W1]∼8 mag. Saturation may occur in fainter sources because of a charged particle strike.	real	4		-0.9999995e9
w1sat	wise_prelimsc	WISE	Saturated pixel fraction, W1 The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation	real	4		-0.9999995e9
w1sigflux	allwise_sc	WISE	Uncertainty in the "raw" W1 source flux measurement in profile-fit photometry in units of digital numbers. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w1sigflux	catwise_2020, catwise_prelim	WISE	WPRO raw flux uncertainty, band-1	real	4	dn
w1sigflux	wise_allskysc	WISE	Uncertainty in the "raw" W1 source flux measurement in profile-fit photometry in units of digital numbers This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	ADU	-0.9999995e9
w1sigflux	wise_prelimsc	WISE	Uncertainty in the "raw" W1 source flux measurement in profile-fit photometry in units of digital numbers This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w1sigflux_pm	catwise_2020, catwise_prelim	WISE	WPRO raw flux uncertainty, band-1	real	4	dn
w1sigm	allwise_sc	WISE	Uncertainty in the W1 "standard" aperture magnitude. This column is null if the W1 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm	catwise_2020, catwise_prelim	WISE	standard aperture mag uncertainty, band-1	real	4	mag
w1sigm	wise_allskysc	WISE	Uncertainty in the W1 "standard" aperture magnitude. This column is default if the W1 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm	wise_prelimsc	WISE	Uncertainty in the W1 "standard" aperture magnitude This column is default if the W1 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_1	allwise_sc	WISE	Uncertainty in the W1 5.5" radius aperture magnitude. This column is null if the the 5.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_1	catwise_2020, catwise_prelim	WISE	Aper 1 (5.50 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_1	wise_allskysc	WISE	Uncertainty in the W1 5.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_1	wise_prelimsc	WISE	Uncertainty in the W1 5.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_2	allwise_sc	WISE	Uncertainty in the W1 8.25" radius aperture magnitude. This column is null if the the 8.25" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_2	catwise_2020, catwise_prelim	WISE	Aper 2 (8.25 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_2	wise_allskysc	WISE	Uncertainty in the W1 8.25" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_2	wise_prelimsc	WISE	Uncertainty in the W1 8.25" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_3	allwise_sc	WISE	Uncertainty in the W1 11.0" radius aperture magnitude. This column is null if the the 11.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_3	catwise_2020, catwise_prelim	WISE	Aper 3 (11.00 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_3	wise_allskysc	WISE	Uncertainty in the W1 11.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_3	wise_prelimsc	WISE	Uncertainty in the W1 11.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_4	allwise_sc	WISE	Uncertainty in the W1 13.75" radius aperture magnitude. This column is null if the the 13.75" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_4	catwise_2020, catwise_prelim	WISE	Aper 4 (13.75 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_4	wise_allskysc	WISE	Uncertainty in the W1 13.75" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_4	wise_prelimsc	WISE	Uncertainty in the W1 13.75" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_5	allwise_sc	WISE	Uncertainty in the W1 16.5" radius aperture magnitude. This column is null if the the 16.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_5	catwise_2020, catwise_prelim	WISE	Aper 5 (16.50 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_5	wise_allskysc	WISE	Uncertainty in the W1 16.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_5	wise_prelimsc	WISE	Uncertainty in the W1 16.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_6	allwise_sc	WISE	Uncertainty in the W1 19.25" radius aperture magnitude. This column is null if the the 19.25" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_6	catwise_2020, catwise_prelim	WISE	Aper 6 (19.25 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_6	wise_allskysc	WISE	Uncertainty in the W1 19.25" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_6	wise_prelimsc	WISE	Uncertainty in the W1 19.25" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_7	allwise_sc	WISE	Uncertainty in the W1 22.0" radius aperture magnitude. This column is null if the the 22.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_7	catwise_2020, catwise_prelim	WISE	Aper 7 (22.00 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_7	wise_allskysc	WISE	Uncertainty in the W1 22.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_7	wise_prelimsc	WISE	Uncertainty in the W1 22.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigm_8	allwise_sc	WISE	Uncertainty in the W1 24.75" radius aperture magnitude. This column is null if the the 24.75" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w1sigm_8	catwise_2020, catwise_prelim	WISE	Aper 8 (24.75 arcsec), aperture mag uncertainty, band-1	real	4	mag
w1sigm_8	wise_allskysc	WISE	Uncertainty in the W1 24.75" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w1sigm_8	wise_prelimsc	WISE	Uncertainty in the W1 24.75" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w1sigmpro	allwise_sc	WISE	W1 profile-fit photometric measurement uncertainty in mag units. This column is null if the W1 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	float	8	mag
			Note - In a small number of cases where the W1 value of ph_qual is "Z" (e.g. ph_qual LIKE 'Z%'), the W1 source flux uncertainty was not measurable because of the presence of a large number of saturated pixels from 3-Band Cryo frames covered the source. In these cases, this column is null, but the w1mpro column will correspond either to the actual source flux, w1flux, rather than the 95% confidence upper limit, or will be null if w1flux is negative.
w1sigmpro	catwise_2020, catwise_prelim	WISE	WPRO flux uncertainty in mag units, band-1	real	4	mag
w1sigmpro	wise_allskysc	WISE	W1 profile-fit photometric measurement uncertainty. This column is default if the W1 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	real	4	mag	-0.9999995e9
w1sigmpro	wise_prelimsc	WISE	W1 profile-fit photometric measurement uncertainty This column is default if the W1 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable	real	4	mag	-0.9999995e9
w1sigmpro_pm	catwise_2020, catwise_prelim	WISE	WPRO flux uncertainty in mag units, band-1	real	4	mag
w1sigP1	catwise_2020, catwise_prelim	WISE	WPRO mag population sigma; band-1	real	4	mag
w1sigp1	allwise_sc	WISE	Standard deviation of the population of W1 fluxes measured on the w1m individual frames covering this source, in magnitudes. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is "null" if w1m<2 or if no individual frame measurements are possible.	float	8	mag
w1sigp1	wise_allskysc	WISE	Standard deviation of the population of W1 fluxes measured on the w1m individual frames covering this source. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w1m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w1sigp1	wise_prelimsc	WISE	Standard deviation of the population of W1 fluxes measured on the w1m individual frames covering this source This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w1m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w1sigP2	catwise_2020, catwise_prelim	WISE	WPRO mag uncertainty of the mean; band-1	real	4	mag
w1sigp2	allwise_sc	WISE	Standard deviation of the mean of the distribution of W1 fluxes (w1magp) computed from profile-fit measurements on the w1m individual frames covering this source, in magnitudes. This is equivalent to w1sigp1/sqrt(w1m). This column is "null" if w1m<2 or if no individual frame measurements are possible.	float	8	mag
w1sigp2	wise_allskysc	WISE	Standard deviation of the mean of the distribution of W1 fluxes (w1magp) computed from profile-fit measurements on the w1m individual frames covering this source. This column is default if w1m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w1sigp2	wise_prelimsc	WISE	Standard deviation of the mean of the distribution of W1 fluxes (w1magp) computed from profile-fit measurements on the w1m individual frames covering this source This column is default if w1m<2 or if no individual frame measurements are possible	real	4	mag	-0.9999995e9
w1sigsk	allwise_sc	WISE	The uncertainty in the W1 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70".	float	8	dn
w1sigsk	catwise_2020, catwise_prelim	WISE	frame sky background value uncertainty, band-1	real	4	dn
w1sigsk	wise_allskysc	WISE	The uncertainty in the W1 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70".	real	4	ADU	-0.9999995e9
w1sigsk	wise_prelimsc	WISE	The uncertainty in the W1 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70"	real	4	ADU	-0.9999995e9
w1sky	allwise_sc	WISE	The trimmed average of the W1 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	dn
			For profile-fit photometry, the sky background is measured on the individual single-exposure images that are used for source characterization. For aperture photometry, the sky background is measured on the Atlas Image.
w1sky	catwise_2020, catwise_prelim	WISE	frame sky background value, band-1	real	4	dn
w1sky	wise_allskysc	WISE	The trimmed average of the W1 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	ADU	-0.9999995e9
w1sky	wise_prelimsc	WISE	The trimmed average of the W1 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70" Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value	float	8	ADU	-0.9999995e9
w1snr	allwise_sc	WISE	W1 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w1flux) to flux uncertainty (w1sigflux)in the W1 profile-fit photometry measurement. This column is null if w1flux is negative, or if w1flux or w1sigflux are null.	float	8
w1snr	catwise_2020, catwise_prelim	WISE	S/N ratio, band-1	real	4
w1snr	wise_allskysc	WISE	W1 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w1flux) to flux uncertainty (w1sigflux) in the W1 profile-fit photometry measurement. This column is default if w1flux is negative, or if w1flux or w1sigflux are default.	real	4		-0.9999995e9
w1snr	wise_prelimsc	WISE	W1 profile-fit measurement signal-to-noise ratio This value is the ratio of the flux (w1flux) to flux uncertainty (w1sigflux)in the W1 profile-fit photometry measurement. This column is default if w1flux is negative, or if w1flux or w1sigflux are default.	real	4		-0.9999995e9
w1snr_pm	catwise_2020, catwise_prelim	WISE	flux S/N ratio, band-1	real	4
w2ab_map	catwise_2020, catwise_prelim	WISE	w2 artifact code value	int	4
w2ab_map_str	catwise_2020, catwise_prelim	WISE	w2 artifact string	varchar	13
w2ba	allwise_sc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W2.	float	8	arcsec
w2ba	wise_allskysc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W2.	real	4	arcsec	-0.9999995e9
w2ba	wise_prelimsc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W2	real	4	arcsec	-0.9999995e9
w2cc_map	allwise_sc	WISE	Contamination and confusion map for this source in W2. This column contains the integer equivalent of the 9-bit binary number that specifies if the W2 measurement is believed to be contaminated by or a spurious detection of an image artifact.	int	4
			The elements of the binary array are: S 0 0 0 O H 0 P D. The leftmost bit, S, differentiates whether the band-detection is believed to be a real detection contaminated by an artifact ("0") or a spurious detection of an artifact ("1"). The remaining bits are set to "1" to denote contamination by different types of artifacts according to the letters: D - Diffraction spike. Source may be a spurious detection of or contaminated by a diffraction spike of a nearby bright star on the same image. P - Persistence. Source may be a spurious detection of or contaminated by a short-term latent (persistence) image left by a bright source. H - Halo. Source may be a spurious detection of or contaminated by the scattered light halo associated with a bright star. O (letter "o") - Optical ghost. Source may be a spurious detection of or contaminated by an optical ghost image caused by a nearby bright source on the same image. For example, a measurement that is believed to be a spurious detection of a diffraction spike and scattered light halo has a binary bit map value of "100001001" and w?cc_map=265.
w2cc_map	catwise_2020, catwise_prelim	WISE	worst case w2cc_map from AllWISE	int	4
w2cc_map	wise_allskysc	WISE	Contamination and confusion map for this source in W2. This column contains the integer equivalent of the 9-bit binary number that specifies if the W2 measurement is believed to be contaminated by or a spurious detection of an image artifact.	smallint	2
w2cc_map	wise_prelimsc	WISE	Contamination and confusion map for this source in W2 This column contains the integer equivalent of the 9-bit binary number that specifies if the W2 measurement is believed to be contaminated by or a spurious detection of an image artifact	smallint	2
w2cc_map_str	allwise_sc	WISE	Contamination and confusion string. This column is a character string that denotes all artifacts that may contaminate the W2 measurement of this source, in the priority order D,P,H,O,d,p,h,o. Lower-case letters denote cases where the source detection in this band is believed to be real but the measurement may be contaminated by the artifact. Upper-case letters denote cases where the source detection in this band may be a spurious detection of an artifact. This string is "null" if there are no artifacts that affect the measurement in this band. The value that appears in second element of the cc_flags string is the left-most character in w2cc_map_str. If w2cc_map_str is "null", then the corresponding cc_flags entry is "0".	varchar	9
			For example, a real detection that is contaminated by a diffraction spike and a latent (persistent) image has a w?cc_map_str="dp". A spurious detection of a diffraction spike that is also contaminated by a latent image has w?cc_map_str="Dp".
w2cc_map_str	catwise_2020, catwise_prelim	WISE	worst case w2cc_map_str from AllWISE	varchar	20
w2cc_map_str	wise_allskysc	WISE	Contamination and confusion string in W2. This column is a character string that denotes all artifacts that may contaminate the W2 measurement of this source, in the priority order D,P,H,O,d,p,h,o.	char	9
w2cc_map_str	wise_prelimsc	WISE	Contamination and confusion string in W2 This column is a character string that denotes all artifacts that may contaminate the W2 measurement of this source, in the priority order D,P,H,O	char	9
w2conf	allwise_sc	WISE	Estimated confusion noise in the W2 sky background annulus, in digital numbers. This number is the difference between the measured noise in the sky background w2sigsk and the noise measured in the same region on the Atlas Uncertainty Maps.	float	8	dn
w2conf	catwise_2020, catwise_prelim	WISE	frame sky confusion based on the UNC images	real	4	dn
w2conf	wise_allskysc	WISE	Estimated confusion noise in the W2 sky background annulus, in digital numbers. This number is the difference between the measured noise in the sky background w2sigsk and the noise measured in the same region on the Atlas Uncertainty Maps.	float	8	ADU	-0.9999995e9
w2conf	wise_prelimsc	WISE	Estimated confusion noise in the W2 sky background annulus, in digital numbers This number is the difference between the measured noise in the sky background w2sigsk and the noise measured in the same region on the Atlas Uncertainty Maps	float	8	ADU	-0.9999995e9
w2Cov	catwise_2020, catwise_prelim	WISE	mean coverage depth, band-2	real	4
w2cov	allwise_sc	WISE	Mean pixel coverage in W2. This column gives the mean pixel value from the W2 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source.	float	8
			W2cov may differ from the integer frame coverage value given in w2m for two reasons. First, individual pixels in the measurement area may be masked or otherwise unusable, reducing the effective pixel count and thus the mean coverage value. Second, the effective sky area sampled by a pixels in single-exposure image varies across the focal plane because of field distortion. Distortion is corrected when coadding to generate the Atlas Images. Therefore, the effective number of pixels contributing to a pixel in the Atlas Coverage Map may be slightly smaller or larger than expected if there was no distortion.
w2cov	wise_allskysc	WISE	Mean pixel coverage in W2. This column gives the mean pixel value from the W2 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source.	real	4		-0.9999995e9
w2cov	wise_prelimsc	WISE	Mean pixel coverage in W2 This column gives the mean pixel value from the W2 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source	real	4		-0.9999995e9
w2dmag	wise_allskysc	WISE	Difference between maximum and minimum magnitude of the source from all usable single-exposure frames, W2. Single-exposure measurements with w2rchi2 values greater than 3.0 times the median are rejected from this computation.	real	4	mag	-0.9999995e9
w2fitr	catwise_2020, catwise_prelim	WISE	fitting radius, band-2 (clipped at 999.99)	real	4	asec
w2flg	allwise_sc	WISE	W2 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg	catwise_2020, catwise_prelim	WISE	standard aperture flag, band-2	int	4
w2flg	wise_allskysc	WISE	W2 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	smallint	2		-9999
w2flg	wise_prelimsc	WISE	W2 "standard" aperture measurement quality flag This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit	smallint	2		-9999
w2flg_1	allwise_sc	WISE	W2 5.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_1	catwise_2020, catwise_prelim	WISE	Aper 1 (5.50 arcsec), aperture flag, band-2	int	4
w2flg_1	wise_allskysc	WISE	W2 5.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_1	wise_prelimsc	WISE	W2 5.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flg_2	allwise_sc	WISE	W2 8.25" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_2	catwise_2020, catwise_prelim	WISE	Aper 2 (8.25 arcsec), aperture flag, band-2	int	4
w2flg_2	wise_allskysc	WISE	W2 8.25" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_2	wise_prelimsc	WISE	W2 8.25" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flg_3	allwise_sc	WISE	W2 11.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_3	catwise_2020, catwise_prelim	WISE	Aper 3 (11.00 arcsec), aperture flag, band-2	int	4
w2flg_3	wise_allskysc	WISE	W2 11.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_3	wise_prelimsc	WISE	W2 11.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flg_4	allwise_sc	WISE	W2 13.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_4	catwise_2020, catwise_prelim	WISE	Aper 4 (13.75 arcsec), aperture flag, band-2	int	4
w2flg_4	wise_allskysc	WISE	W2 13.75" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_4	wise_prelimsc	WISE	W2 13.75" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flg_5	allwise_sc	WISE	W2 16.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_5	catwise_2020, catwise_prelim	WISE	Aper 5 (16.50 arcsec), aperture flag, band-2	int	4
w2flg_5	wise_allskysc	WISE	W2 16.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_5	wise_prelimsc	WISE	W2 16.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flg_6	allwise_sc	WISE	W2 19.25" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_6	catwise_2020, catwise_prelim	WISE	Aper 6 (19.25 arcsec), aperture flag, band-2	int	4
w2flg_6	wise_allskysc	WISE	W2 19.25" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_6	wise_prelimsc	WISE	W2 19.25" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flg_7	allwise_sc	WISE	W2 22.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_7	catwise_2020, catwise_prelim	WISE	Aper 7 (22.00 arcsec), aperture flag, band-2	int	4
w2flg_7	wise_allskysc	WISE	W2 22.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_7	wise_prelimsc	WISE	W2 22.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flg_8	allwise_sc	WISE	W2 24.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2flg_8	catwise_2020, catwise_prelim	WISE	Aper 8 (24.75 arcsec), aperture flag, band-2	int	4
w2flg_8	wise_allskysc	WISE	W2 24.75" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w2flg_8	wise_prelimsc	WISE	W2 24.75" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w2flux	allwise_sc	WISE	The "raw" W2 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w2flux	catwise_2020, catwise_prelim	WISE	WPRO raw flux, band-2	real	4	dn
w2flux	wise_allskysc	WISE	The "raw" W2 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	ADU	-0.9999995e9
w2flux	wise_prelimsc	WISE	The "raw" W2 source flux measured in profile-fit photometry in units of digital numbers This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w2flux_pm	catwise_2020, catwise_prelim	WISE	WPRO raw flux, band-2	real	4	dn
w2frl	wise_prelimsc	WISE	Fraction of W2 pixels affected by latents This column gives the fraction of all W2 pixels in the stack of individual W2 exposures used to characterize this source that may be affected by the presence of a latent image produced by a bright source	real	4		-0.9999995e9
w2frtr	wise_allskysc	WISE	Fraction of W2 pixels affected by transients. This column gives the fraction of all W2 pixels in the stack of individual W2 exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 7.25", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.	real	4		-0.9999995e9
w2gerr	allwise_sc	WISE	Uncertainty in the W2 magnitude of source measured in elliptical aperture. CAUTION: A w2gerr value of 9.999 indicates that the measurement uncertainty is very large, or the uncertainty could not be computed. In either case, the w2gmag measurement should be considered highly suspect.	float	8	mag
w2gerr	wise_allskysc	WISE	Uncertainty in the W2 magnitude of source measured in elliptical aperture.	real	4	mag	-0.9999995e9
w2gerr	wise_prelimsc	WISE	Uncertainty in the W2 magnitude of source measured in elliptical aperture	real	4	mag	-0.9999995e9
w2gflg	allwise_sc	WISE	W2 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w2gflg	wise_allskysc	WISE	W2 elliptical aperture measurement quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag, w2mflg.	smallint	2		-9999
w2gflg	wise_prelimsc	WISE	W2 elliptical aperture measurement quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag	smallint	2		-9999
w2gmag	allwise_sc	WISE	W2 magnitude of source measured in the elliptical aperture described by w2rsemi, w2ba, and w2pa.	float	8	mag
w2gmag	wise_allskysc	WISE	W2 magnitude of source measured in the elliptical aperture described by w2rsemi, w2ba, and w2pa.	real	4	mag	-0.9999995e9
w2gmag	wise_prelimsc	WISE	W2 magnitude of source measured in the elliptical aperture described by w2rsemi, w2ba, and w2pa	real	4	mag	-0.9999995e9
w2k	allwise_sc	WISE	Stetson K variability index (Stetson, P. 1996, PASP, 108, 851) computed using the W2 profile-fit fluxes measured on the individual single-exposure images. This column is null if there are <3 single-exposure measurements available in W2.	float	8
w2k	catwise_2020, catwise_prelim	WISE	Stetson k index for variability; band-2	real	4
w2M	catwise_2020, catwise_prelim	WISE	WPRO, M , band-2 M == number of flux measurements for a given source	int	4
w2m	allwise_sc	WISE	Integer frame coverage. This column gives the number of individual 7.7s W2 exposures on which a profile-fit measurement of this source was possible. This number can differ between the four bands because band-dependent criteria are used to select individual frames for inclusion in the coadded Atlas Images. This column is null if there is no frame coverage in this band at the position of this source.	int	4
w2m	wise_allskysc	WISE	Integer frame coverage in W2. This column gives the number of individual 7.7s W2 exposures on which a profile-fit measurement of this source was possible.	bigint	8		-99999999
w2m	wise_prelimsc	WISE	Integer frame coverage in W2 This column gives the number of individual 7.7s W2 exposures on which a profile-fit measurement of this source was possible	bigint	8		-99999999
w2mag	allwise_sc	WISE	W2 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w2mcor. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag	catwise_2020, catwise_prelim	WISE	standard aperture mag w/ correction applied	real	4	mag
w2mag	wise_allskysc	WISE	W2 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness.	real	4	mag	-0.9999995e9
w2mag	wise_prelimsc	WISE	W2 "standard" aperture magnitude This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness	real	4	mag	-0.9999995e9
w2mag_1	allwise_sc	WISE	W2 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_1	catwise_2020, catwise_prelim	WISE	Aper 1 (5.50 arcsec), aperture mag, band-2	real	4	mag
w2mag_1	wise_allskysc	WISE	W2 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag	-0.9999995e9
w2mag_1	wise_prelimsc	WISE	W2 5.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
w2mag_2	allwise_sc	WISE	W2 8.25" radius aperture magnitude. This is the calibrated source brightness measured in a 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_2	catwise_2020, catwise_prelim	WISE	Aper 2 (8.25 arcsec), aperture mag, band-2	real	4	mag
w2mag_2	wise_allskysc	WISE	W2 8.25" radius aperture magnitude. This is the calibrated source brightness measured in a 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag	-0.9999995e9
w2mag_2	wise_prelimsc	WISE	W2 8.25" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
w2mag_3	allwise_sc	WISE	W2 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_3	catwise_2020, catwise_prelim	WISE	Aper 3 (11.00 arcsec), aperture mag, band-2	real	4	mag
w2mag_3	wise_allskysc	WISE	W2 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag	-0.9999995e9
w2mag_3	wise_prelimsc	WISE	W2 11.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
w2mag_4	allwise_sc	WISE	W2 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_4	catwise_2020, catwise_prelim	WISE	Aper 4 (13.75 arcsec), aperture mag, band-2	real	4	mag
w2mag_4	wise_allskysc	WISE	W2 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag	-0.9999995e9
w2mag_4	wise_prelimsc	WISE	W2 13.75" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
w2mag_5	allwise_sc	WISE	W2 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_5	catwise_2020, catwise_prelim	WISE	Aper 5 (16.50 arcsec), aperture mag, band-2	real	4	mag
w2mag_5	wise_allskysc	WISE	W2 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag	-0.9999995e9
w2mag_5	wise_prelimsc	WISE	W2 16.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
w2mag_6	allwise_sc	WISE	W2 19.25" radius aperture magnitude. This is the calibrated source brightness measured in a 19.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_6	catwise_2020, catwise_prelim	WISE	Aper 6 (19.25 arcsec), aperture mag, band-2	real	4	mag
w2mag_6	wise_allskysc	WISE	W2 19.25" radius aperture magnitude This is the calibrated source brightness measured in a 19.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag.	-0.9999995e9
w2mag_6	wise_prelimsc	WISE	W2 19.25" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
w2mag_7	allwise_sc	WISE	W2 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_7	catwise_2020, catwise_prelim	WISE	Aper 7 (22.00 arcsec), aperture mag, band-2	real	4	mag
w2mag_7	wise_allskysc	WISE	W2 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag	-0.9999995e9
w2mag_7	wise_prelimsc	WISE	W2 22.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
w2mag_8	allwise_sc	WISE	W2 24.75" radius aperture magnitude. This is the calibrated source brightness measured in a 24.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W2.	float	8	mag
w2mag_8	catwise_2020, catwise_prelim	WISE	Aper 8 (24.75 arcsec), aperture mag, band-2	real	4	mag
w2mag_8	wise_allskysc	WISE	W2 24.75" radius aperture magnitude. This is the calibrated source brightness measured in a 24.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W2.	real	4	mag	-0.9999995e9
w2mag_8	wise_prelimsc	WISE	W2 24.75" radius aperture magnitude This column is default if this aperture measurement was not possible in W2	real	4	mag	-0.9999995e9
W2mag_ALLWISE	ravedr5Source	RAVE	W2 magnitude from ALLWISE	real	4	mag		phot.mag;em.opt
w2magP	catwise_2020, catwise_prelim	WISE	WPRO repeatability mag; band-2	real	4	mag
w2magp	allwise_sc	WISE	Magnitude computed from the inverse-variance-weighted mean of the profile-fit flux measurements on the w2m individual W2 frames covering this source. This differs from w2mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w2mpro is computed by fitting all W2 frames simultaneously and incorporating a robust error model. This column is "null" if w2m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w2mpro for the optimal flux measurement for point sources.	float	8	mag
w2magp	wise_allskysc	WISE	Inverse-variance-weighted mean W2 magnitude computed from profile-fit measurements on the w2m individual frames covering this source. This differs from w2mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w2mpro is computed by fitting all W2 frames simultaneously and incorporating a robust error model. This column is default if w2m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w2mpro for the optimal flux measurement for point sources.	real	4	mag	-0.9999995e9
w2magp	wise_prelimsc	WISE	Inverse-variance-weighted mean W2 magnitude computed from profile-fit measurements on the w2m individual frames covering this source This differs from w2mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w2mpro is computed by fitting all W2 frames simultaneously and incorporating a robust error model. This column is default if w2m=0, the mean flux is negative or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w2mcor	allwise_sc	WISE	W2 aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness, w2mag_2, to give the "standard-aperture" magnitude.	float	8	mag
w2mcor	wise_allskysc	WISE	W2 aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness, w2mag_2, to give the "standard-aperture" magnitude.	real	4	mag	-0.9999995e9
w2mcor	wise_prelimsc	WISE	W2 aperture curve-of-growth correction, in magnitudes This correction is subtracted from the nominal 8.25" aperture photometry brightness, w2mag_2, to give the "standard-aperture" magnitude	real	4	mag	-0.9999995e9
w2mCorr	twompzPhotoz	TWOMPZ	WISE w2mpro measurement corrected for Galactic dust extinction {image primary HDU keyword: W2mCorr}	real	4	mag	-0.9999995e9
w2mCorrErr	twompzPhotoz	TWOMPZ	W2 profile fit photometric measurement uncertainty {image primary HDU keyword: w2sigmpro}	real	4	mag	-0.9999995e9
w2mJDmax	catwise_2020, catwise_prelim	WISE	maximum mJD; band-2	float	8
w2mjdmax	allwise_sc, wise_allskysc	WISE	The latest modified Julian Date (mJD) of the W2 single-exposures covering the source.	float	8
w2mJDmean	catwise_2020, catwise_prelim	WISE	mean mJD; band-2	float	8
w2mjdmean	allwise_sc, wise_allskysc	WISE	The average modified Julian Date (mJD) of the W2 single-exposures covering the source.	float	8
w2mJDmin	catwise_2020, catwise_prelim	WISE	minimum mJD; band-2	float	8
w2mjdmin	allwise_sc, wise_allskysc	WISE	The earliest modified Julian Date (mJD) of the W2 single-exposures covering the source.	float	8
w2mLQ	catwise_2020, catwise_prelim	WISE	-log(Q), Q = 1-P(chi-square); band-2	real	4
w2mlq	allwise_sc	WISE	Probability measure that the source is variable in W2 flux. The value is -ln(Q), where Q = 1 - P(χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	float	8
			The Q value is the fraction of all cases to be at least as large as that observed if the null hypothesis is true. The null hypothesis is that the flux is emitted by a non-variable astrophysical object. It may be false because the object is a true variable. It may also be false because the flux measurement is corrupted by artifacts such as cosmic rays, scattered light, etc. The smaller the Q value, the more implausible the null hypothesis, i.e., the more likely it is that the flux is either variable or corrupted or both.
w2mlq	wise_allskysc	WISE	Probability measure that the source is variable in W2 flux. The value is -log10(Q), where Q = 1 - P(Χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	int	4		-99999999
w2mpro	allwise_sc	WISE	W2 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W2 flux measurement has SNR<2. This column is null if the source is nominally detected in W2, but no useful brightness estimate could be made.	float	8	mag
w2mpro	catwise_2020, catwise_prelim	WISE	WPRO flux in mag units, band-2	real	4	mag
w2mpro	wise_allskysc	WISE	W2 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W2 flux measurement has SNR<2. This column is default if the source is nominally detected in W2, but no useful brightness estimate could be made.	real	4	mag	-0.9999995e9
w2mpro	wise_prelimsc	WISE	W2 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W2 flux measurement has SNR<2 This column is default if the source is nominally detected in W2, but no useful brightness estimate could be made	real	4	mag	-0.9999995e9
w2mpro_pm	catwise_2020, catwise_prelim	WISE	WPRO flux in mag units, band-2	real	4	mag
w2Ndf	catwise_2020, catwise_prelim	WISE	No. degrees of freedom in var chi-square; band-2	int	4
w2ndf	allwise_sc	WISE	Number of degrees of freedom in the flux variability chi-square, W2.	int	4
w2ndf	wise_allskysc	WISE	Number of degrees of freedom in the flux variability chi-square, W2.	bigint	8		-99999999
w2NM	catwise_2020, catwise_prelim	WISE	WPRO, N (of M), band-2 M == number of flux measurements for a given source; N == number of M sources that have SNR >= 3	int	4
w2nm	allwise_sc	WISE	Integer frame detection count. This column gives the number of individual 7.7s exposures on which this source was detected with SNR>3 in the W2 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	int	4
w2nm	wise_allskysc	WISE	Integer frame detection count in W2. This column gives the number of individual 7.7s exposures on which this source was detected with SNR>3 in the W2 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	bigint	8		-99999999
w2nm	wise_prelimsc	WISE	Integer frame detection count in W2 This column gives the number of individual 7.7s exposures on which this source was detected with SNR>3 in the W2 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures	bigint	8		-99999999
w2pa	allwise_sc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W2.	float	8	deg
w2pa	wise_allskysc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W2.	real	4	degrees	-0.9999995e9
w2pa	wise_prelimsc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W2	real	4	degrees	-0.9999995e9
w2rchi2	allwise_sc	WISE	Reduced χ2 of the W2 profile-fit photometry measurement. This column is null if the W2 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4
w2rchi2	catwise_2020, catwise_prelim	WISE	WPRO reduced chi^2, band-2	real	4
w2rchi2	wise_allskysc	WISE	Reduced chi-squared of the W2 profile-fit photometry measurement. This column is default if the W2 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4		-0.9999995e9
w2rchi2	wise_prelimsc	WISE	Reduced chi-squared of the W2 profile-fit photometry measurement This column is default if the W2 magnitude is a 95% confidence upper limit (i.e. the source is not detected)	real	4		-0.9999995e9
w2rchi2_pm	allwise_sc	WISE	Reduced χ2 of the W2 profile-fit photometry measurement including motion estimation. This column is null if the source is not detected in W2 magnitude or if the motion fit failed to converge or was not attempted.	real	4
w2rchi2_pm	catwise_2020, catwise_prelim	WISE	WPRO reduced chi^2, band-2	real	4
w2rsemi	allwise_sc	WISE	Semi-major axis of the elliptical aperture used to measure source in W2.	float	8	arcsec
w2rsemi	wise_allskysc	WISE	Semi-major axis of the elliptical aperture used to measure source in W2.	real	4	arcsec	-0.9999995e9
w2rsemi	wise_prelimsc	WISE	Semi-major axis of the elliptical aperture used to measure source in W2	real	4	arcsec	-0.9999995e9
w2Sat	catwise_2020, catwise_prelim	WISE	fraction of pixels saturated, band-2	real	4
w2sat	allwise_sc	WISE	Saturated pixel fraction, W2. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W2]~7 mag. Saturation may occur in fainter sources because of charged particle strikes.	float	8
w2sat	wise_allskysc	WISE	Saturated pixel fraction, W2. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W2]∼7 mag. Saturation may occur in fainter sources because of a charged particle strike.	real	4		-0.9999995e9
w2sat	wise_prelimsc	WISE	Saturated pixel fraction, W2 The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation	real	4		-0.9999995e9
w2sigflux	allwise_sc	WISE	Uncertainty in the "raw" W2 source flux measurement in profile-fit photometry in units of digital numbers. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w2sigflux	catwise_2020, catwise_prelim	WISE	WPRO raw flux uncertainty, band-2	real	4	dn
w2sigflux	wise_allskysc	WISE	Uncertainty in the "raw" W2 source flux measurement in profile-fit photometry in units of digital numbers. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	ADU	-0.9999995e9
w2sigflux	wise_prelimsc	WISE	Uncertainty in the "raw" W2 source flux measurement in profile-fit photometry in units of digital numbers This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w2sigflux_pm	catwise_2020, catwise_prelim	WISE	fit WPRO raw flux uncertainty, band-2	real	4	dn
w2sigm	allwise_sc	WISE	Uncertainty in the W2 "standard" aperture magnitude. This column is null if the W2 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm	catwise_2020, catwise_prelim	WISE	standard aperture mag uncertainty, band-2	real	4	mag
w2sigm	wise_allskysc	WISE	Uncertainty in the W2 "standard" aperture magnitude. This column is default if the W2 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm	wise_prelimsc	WISE	Uncertainty in the W2 "standard" aperture magnitude This column is default if the W2 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_1	allwise_sc	WISE	Uncertainty in the W2 5.5" radius aperture magnitude. This column is null if the the 5.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_1	catwise_2020, catwise_prelim	WISE	Aper 1 (5.50 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_1	wise_allskysc	WISE	Uncertainty in the W2 5.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_1	wise_prelimsc	WISE	Uncertainty in the W2 5.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_2	allwise_sc	WISE	Uncertainty in the W2 8.25" radius aperture magnitude. This column is null if the the 8.25" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_2	catwise_2020, catwise_prelim	WISE	Aper 2 (8.25 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_2	wise_allskysc	WISE	Uncertainty in the W2 8.25" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_2	wise_prelimsc	WISE	Uncertainty in the W2 8.25" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_3	allwise_sc	WISE	Uncertainty in the W2 11.0" radius aperture magnitude. This column is null if the the 11.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_3	catwise_2020, catwise_prelim	WISE	Aper 3 (11.00 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_3	wise_allskysc	WISE	Uncertainty in the W2 11.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_3	wise_prelimsc	WISE	Uncertainty in the W2 11.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_4	allwise_sc	WISE	Uncertainty in the W2 13.75" radius aperture magnitude. This column is null if the the 13.75" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_4	catwise_2020, catwise_prelim	WISE	Aper 4 (13.75 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_4	wise_allskysc	WISE	Uncertainty in the W2 13.75" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_4	wise_prelimsc	WISE	Uncertainty in the W2 13.75" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_5	allwise_sc	WISE	Uncertainty in the W2 16.5" radius aperture magnitude. This column is null if the the 16.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_5	catwise_2020, catwise_prelim	WISE	Aper 5 (16.50 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_5	wise_allskysc	WISE	Uncertainty in the W2 16.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_5	wise_prelimsc	WISE	Uncertainty in the W2 16.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_6	allwise_sc	WISE	Uncertainty in the W2 19.25" radius aperture magnitude. This column is null if the the 19.25" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_6	catwise_2020, catwise_prelim	WISE	Aper 6 (19.25 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_6	wise_allskysc	WISE	Uncertainty in the W2 19.25" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_6	wise_prelimsc	WISE	Uncertainty in the W2 19.25" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_7	allwise_sc	WISE	Uncertainty in the W2 22.0" radius aperture magnitude. This column is null if the the 22.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_7	catwise_2020, catwise_prelim	WISE	Aper 7 (22.00 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_7	wise_allskysc	WISE	Uncertainty in the W2 22.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_7	wise_prelimsc	WISE	Uncertainty in the W2 22.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigm_8	allwise_sc	WISE	Uncertainty in the W2 24.75" radius aperture magnitude. This column is null if the the 24.75" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w2sigm_8	catwise_2020, catwise_prelim	WISE	Aper 8 (24.75 arcsec), aperture mag uncertainty, band-2	real	4	mag
w2sigm_8	wise_allskysc	WISE	Uncertainty in the W2 24.75" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w2sigm_8	wise_prelimsc	WISE	Uncertainty in the W2 24.75" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w2sigmpro	allwise_sc	WISE	W2 profile-fit photometric measurement uncertainty in mag units. This column is null if the W2 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	float	8	mag
w2sigmpro	catwise_2020, catwise_prelim	WISE	WPRO flux uncertainty in mag units, band-2	real	4	mag
w2sigmpro	wise_allskysc	WISE	W2 profile-fit photometric measurement uncertainty. This column is default if the W2 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	real	4	mag	-0.9999995e9
w2sigmpro	wise_prelimsc	WISE	W2 profile-fit photometric measurement uncertainty This column is default if the W2 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable	real	4	mag	-0.9999995e9
w2sigmpro_pm	catwise_2020, catwise_prelim	WISE	WPRO flux uncertainty in mag units, band-2	real	4	mag
w2sigP1	catwise_2020, catwise_prelim	WISE	WPRO mag population sigma; band-2	real	4	mag
w2sigp1	allwise_sc	WISE	Standard deviation of the population of W2 fluxes measured on the w2m individual frames covering this source, in magnitudes. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is "null" if w2m<2 or if no individual frame measurements are possible.	float	8	mag
w2sigp1	wise_allskysc	WISE	Standard deviation of the population of W2 fluxes measured on the w2m individual frames covering this source. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w2m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w2sigp1	wise_prelimsc	WISE	Standard deviation of the population of W2 fluxes measured on the w2m individual frames covering this source This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w2m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w2sigP2	catwise_2020, catwise_prelim	WISE	WPRO mag uncertainty of the mean; band-2	real	4	mag
w2sigp2	allwise_sc	WISE	Standard deviation of the mean of the distribution of W2 fluxes (w2magp) computed from profile-fit measurements on the w2m individual frames covering this source, in magnitudes. This is equivalent to w2sigp1/sqrt(w2m). This column is "null" if w2m<2 or if no individual frame measurements are possible.	float	8	mag
w2sigp2	wise_allskysc	WISE	Standard deviation of the mean of the distribution of W2 fluxes (w2magp) computed from profile-fit measurements on the w2m individual frames covering this source. This column is default if w2m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w2sigp2	wise_prelimsc	WISE	Standard deviation of the mean of the distribution of W2 fluxes (w2magp) computed from profile-fit measurements on the w2m individual frames covering this source This column is default if w2m<2 or if no individual frame measurements are possible	real	4	mag	-0.9999995e9
w2sigsk	allwise_sc	WISE	The uncertainty in the W2 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70".	float	8	dn
w2sigsk	catwise_2020, catwise_prelim	WISE	frame sky background value uncertainty, band-2	real	4	dn
w2sigsk	wise_allskysc	WISE	The uncertainty in the W2 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70".	real	4	ADU	-0.9999995e9
w2sigsk	wise_prelimsc	WISE	The uncertainty in the W2 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70"	real	4	ADU	-0.9999995e9
w2sky	allwise_sc	WISE	The trimmed average of the W2 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	dn
			For profile-fit photometry, the sky background is measured on the individual single-exposure images that are used for source characterization. For aperture photometry, the sky background is measured on the Atlas Image.
w2sky	catwise_2020, catwise_prelim	WISE	frame sky background value, band-2	real	4	dn
w2sky	wise_allskysc	WISE	The trimmed average of the W2 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	ADU	-0.9999995e9
w2sky	wise_prelimsc	WISE	The trimmed average of the W2 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70" Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value	float	8	ADU	-0.9999995e9
w2snr	allwise_sc	WISE	W2 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w2flux) to flux uncertainty (w2sigflux)in the W2 profile-fit photometry measurement. This column is null if w2flux is negative, or if w2flux or w2sigflux are null.	float	8
w2snr	catwise_2020, catwise_prelim	WISE	S/N ratio, band-2	real	4
w2snr	wise_allskysc	WISE	W2 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w2flux) to flux uncertainty (w2sigflux) in the W2 profile-fit photometry measurement. This column is default if w2flux is negative, or if w2flux or w2sigflux are default.	real	4		-0.9999995e9
w2snr	wise_prelimsc	WISE	W2 profile-fit measurement signal-to-noise ratio This value is the ratio of the flux (w2flux) to flux uncertainty (w2sigflux)in the W2 profile-fit photometry measurement. This column is default if w2flux is negative, or if w2flux or w2sigflux are default.	real	4		-0.9999995e9
w2snr_pm	catwise_2020, catwise_prelim	WISE	flux S/N ratio, band-2	real	4
w3ba	allwise_sc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W3.	float	8	arcsec
w3ba	wise_allskysc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W3.	real	4	arcsec	-0.9999995e9
w3ba	wise_prelimsc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W3	real	4	arcsec	-0.9999995e9
w3cc_map	allwise_sc	WISE	Contamination and confusion map for this source in W3. This column contains the integer equivalent of the 9-bit binary number that specifies if the W3 measurement is believed to be contaminated by or a spurious detection of an image artifact.	int	4
			The elements of the binary array are: S 0 0 0 O H 0 P D. The leftmost bit, S, differentiates whether the band-detection is believed to be a real detection contaminated by an artifact ("0") or a spurious detection of an artifact ("1"). The remaining bits are set to "1" to denote contamination by different types of artifacts according to the letters: D - Diffraction spike. Source may be a spurious detection of or contaminated by a diffraction spike of a nearby bright star on the same image. P - Persistence. Source may be a spurious detection of or contaminated by a short-term latent (persistence) image left by a bright source. H - Halo. Source may be a spurious detection of or contaminated by the scattered light halo associated with a bright star. O (letter "o") - Optical ghost. Source may be a spurious detection of or contaminated by an optical ghost image caused by a nearby bright source on the same image. For example, a measurement that is believed to be a spurious detection of a diffraction spike and scattered light halo has a binary bit map value of "100001001" and w?cc_map=265.
w3cc_map	wise_allskysc	WISE	Contamination and confusion map for this source in W3. This column contains the integer equivalent of the 9-bit binary number that specifies if the W3 measurement is believed to be contaminated by or a spurious detection of an image artifact.	smallint	2
w3cc_map	wise_prelimsc	WISE	Contamination and confusion map for this source in W3 This column contains the integer equivalent of the 9-bit binary number that specifies if the W3 measurement is believed to be contaminated by or a spurious detection of an image artifact	smallint	2
w3cc_map_str	allwise_sc	WISE	Contamination and confusion string. This column is a character string that denotes all artifacts that may contaminate the W3 measurement of this source, in the priority order D,P,H,O,d,p,h,o. Lower-case letters denote cases where the source detection in this band is believed to be real but the measurement may be contaminated by the artifact. Upper-case letters denote cases where the source detection in this band may be a spurious detection of an artifact. This string is "null" if there are no artifacts that affect the measurement in this band. The value that appears in third element of the cc_flags string is the left-most character in w3cc_map_str. If w3cc_map_str is "null", then the corresponding cc_flags entry is "0".	varchar	9
			For example, a real detection that is contaminated by a diffraction spike and a latent (persistent) image has a w?cc_map_str="dp". A spurious detection of a diffraction spike that is also contaminated by a latent image has w?cc_map_str="Dp".
w3cc_map_str	wise_allskysc	WISE	Contamination and confusion string in W3. This column is a character string that denotes all artifacts that may contaminate the W3 measurement of this source, in the priority order D,P,H,O,d,p,h,o.	char	9
w3cc_map_str	wise_prelimsc	WISE	Contamination and confusion string in W3 This column is a character string that denotes all artifacts that may contaminate the W3 measurement of this source, in the priority order D,P,H,O	char	9
w3conf	allwise_sc	WISE	Estimated confusion noise in the W3 sky background annulus, in digital numbers. This number is the difference between the measured noise in the sky background w3sigsk and the noise measured in the same region on the Atlas Uncertainty Maps.	float	8	dn
w3conf	wise_allskysc	WISE	Estimated confusion noise in the W3 sky background annulus, in digital numbers. This number is the difference between the measured noise in the sky background w3sigsk and the noise measured in the same region on the Atlas Uncertainty Maps.	float	8	ADU	-0.9999995e9
w3conf	wise_prelimsc	WISE	Estimated confusion noise in the W3 sky background annulus, in digital numbers This number is the difference between the measured noise in the sky background w3sigsk and the noise measured in the same region on the Atlas Uncertainty Maps	float	8	ADU	-0.9999995e9
w3cov	allwise_sc	WISE	Mean pixel coverage in W3. This column gives the mean pixel value from the W3 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source.	float	8
			W3cov may differ from the integer frame coverage value given in w3m for two reasons. First, individual pixels in the measurement area may be masked or otherwise unusable, reducing the effective pixel count and thus the mean coverage value. Second, the effective sky area sampled by a pixels in single-exposure image varies across the focal plane because of field distortion. Distortion is corrected when coadding to generate the Atlas Images. Therefore, the effective number of pixels contributing to a pixel in the Atlas Coverage Map may be slightly smaller or larger than expected if there was no distortion.
w3cov	wise_allskysc	WISE	Mean pixel coverage in W3. This column gives the mean pixel value from the W3 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source.	real	4		-0.9999995e9
w3cov	wise_prelimsc	WISE	Mean pixel coverage in W3 This column gives the mean pixel value from the W3 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 8.25" centered on the position of this source	real	4		-0.9999995e9
w3dmag	wise_allskysc	WISE	Difference between maximum and minimum magnitude of the source from all usable single-exposure frames, W3. Single-exposure measurements with w3rchi2 values greater than 3.0 times the median are rejected from this computation.	real	4	mag	-0.9999995e9
w3flg	allwise_sc	WISE	W3 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg	wise_allskysc	WISE	W3 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	smallint	2		-9999
w3flg	wise_prelimsc	WISE	W3 "standard" aperture measurement quality flag This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit	smallint	2		-9999
w3flg_1	allwise_sc	WISE	W3 5.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_1	wise_allskysc	WISE	W3 5.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_1	wise_prelimsc	WISE	W3 5.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flg_2	allwise_sc	WISE	W3 8.25" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_2	wise_allskysc	WISE	W3 8.25" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_2	wise_prelimsc	WISE	W3 8.25" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flg_3	allwise_sc	WISE	W3 11.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_3	wise_allskysc	WISE	W3 11.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_3	wise_prelimsc	WISE	W3 11.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flg_4	allwise_sc	WISE	W3 13.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_4	wise_allskysc	WISE	W3 13.75" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_4	wise_prelimsc	WISE	W3 13.75" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flg_5	allwise_sc	WISE	W3 16.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_5	wise_allskysc	WISE	W3 16.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_5	wise_prelimsc	WISE	W3 16.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flg_6	allwise_sc	WISE	W3 19.25" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_6	wise_allskysc	WISE	W3 19.25" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_6	wise_prelimsc	WISE	W3 19.25" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flg_7	allwise_sc	WISE	W3 22.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_7	wise_allskysc	WISE	W3 22.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_7	wise_prelimsc	WISE	W3 22.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flg_8	allwise_sc	WISE	W3 24.75" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3flg_8	wise_allskysc	WISE	W3 24.75" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w3flg_8	wise_prelimsc	WISE	W3 24.75" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w3flux	allwise_sc	WISE	The "raw" W3 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w3flux	wise_allskysc	WISE	The "raw" W3 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	ADU	-0.9999995e9
w3flux	wise_prelimsc	WISE	The "raw" W3 source flux measured in profile-fit photometry in units of digital numbers This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w3frl	wise_prelimsc	WISE	Fraction of W3 pixels affected by latents This column gives the fraction of all W3 pixels in the stack of individual W3 exposures used to characterize this source that may be affected by the presence of a latent image produced by a bright source	real	4		-0.9999995e9
w3frtr	wise_allskysc	WISE	Fraction of W3 pixels affected by transients. This column gives the fraction of all W3 pixels in the stack of individual W3 exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 7.25", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.	real	4		-0.9999995e9
w3gerr	allwise_sc	WISE	Uncertainty in the W3 magnitude of source measured in elliptical aperture. CAUTION: A w3gerr value of 9.999 indicates that the measurement uncertainty is very large, or the uncertainty could not be computed. In either case, the w3gmag measurement should be considered highly suspect.	float	8	mag
w3gerr	wise_allskysc	WISE	Uncertainty in the W3 magnitude of source measured in elliptical aperture.	real	4	mag	-0.9999995e9
w3gerr	wise_prelimsc	WISE	Uncertainty in the W3 magnitude of source measured in elliptical aperture	real	4	mag	-0.9999995e9
w3gflg	allwise_sc	WISE	W3 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w3gflg	wise_allskysc	WISE	W3 elliptical aperture measurement quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag, w3mflg.	smallint	2		-9999
w3gflg	wise_prelimsc	WISE	W3 elliptical aperture measurement quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag	smallint	2		-9999
w3gmag	allwise_sc	WISE	W3 magnitude of source measured in the elliptical aperture described by w3rsemi, w3ba, and w3pa.	float	8	mag
w3gmag	wise_allskysc	WISE	W3 magnitude of source measured in the elliptical aperture described by w3rsemi, w3ba, and w3pa.	real	4	mag	-0.9999995e9
w3gmag	wise_prelimsc	WISE	W3 magnitude of source measured in the elliptical aperture described by w3rsemi, w3ba, and w3pa	real	4	mag	-0.9999995e9
w3k	allwise_sc	WISE	Stetson K variability index (Stetson, P. 1996, PASP, 108, 851) computed using the W3 profile-fit fluxes measured on the individual single-exposure images. This column is null if there are <3 single-exposure measurements available in W3.	float	8
w3m	allwise_sc	WISE	Integer frame coverage. This column gives the number of individual 8.8s W3 exposures on which a profile-fit measurement of this source was possible. This number can differ between the four bands because band-dependent criteria are used to select individual frames for inclusion in the coadded Atlas Images. This column is null if there is no frame coverage in this band at the position of this source.	int	4
w3m	wise_allskysc	WISE	Integer frame coverage in W3. This column gives the number of individual 8.8s W3 exposures on which a profile-fit measurement of this source was possible.	bigint	8		-99999999
w3m	wise_prelimsc	WISE	Integer frame coverage in W3 This column gives the number of individual 8.8s W3 exposures on which a profile-fit measurement of this source was possible.	bigint	8		-99999999
w3mag	allwise_sc	WISE	W3 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w3mcor. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag	wise_allskysc	WISE	W3 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness.	real	4	mag	-0.9999995e9
w3mag	wise_prelimsc	WISE	W3 "standard" aperture magnitude This is the curve-of-growth corrected source brightness measured in an 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness	real	4	mag	-0.9999995e9
w3mag_1	allwise_sc	WISE	W3 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_1	wise_allskysc	WISE	W3 5.5" radius aperture magnitude. This is the calibrated source brightness measured in a 5.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3.	real	4	mag	-0.9999995e9
w3mag_1	wise_prelimsc	WISE	W3 5.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_2	allwise_sc	WISE	W3 8.25" radius aperture magnitude. This is the calibrated source brightness measured in a 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_2	wise_allskysc	WISE	W3 8.25" radius aperture magnitude. This is the calibrated source brightness measured in a 8.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3.	real	4	mag	-0.9999995e9
w3mag_2	wise_prelimsc	WISE	W3 8.25" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_3	allwise_sc	WISE	W3 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_3	wise_allskysc	WISE	W3 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3.	real	4	mag	-0.9999995e9
w3mag_3	wise_prelimsc	WISE	W3 11.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_4	allwise_sc	WISE	W3 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_4	wise_allskysc	WISE	W3 13.75" radius aperture magnitude. This is the calibrated source brightness measured in a 13.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3.	real	4	mag.	-0.9999995e9
w3mag_4	wise_prelimsc	WISE	W3 13.75" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_5	allwise_sc	WISE	W3 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_5	wise_allskysc	WISE	W3 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3.	real	4	mag	-0.9999995e9
w3mag_5	wise_prelimsc	WISE	W3 16.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_6	allwise_sc	WISE	W3 19.25" radius aperture magnitude. This is the calibrated source brightness measured in a 19.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_6	wise_allskysc	WISE	W3 19.25" radius aperture magnitude. This is the calibrated source brightness measured in a 19.25" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3.	real	4	mag	-0.9999995e9
w3mag_6	wise_prelimsc	WISE	W3 19.25" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_7	allwise_sc	WISE	W3 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_7	wise_allskysc	WISE	W3 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_7	wise_prelimsc	WISE	W3 22.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
w3mag_8	allwise_sc	WISE	W3 24.75" radius aperture magnitude. This is the calibrated source brightness measured in a 24.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W3.	float	8	mag
w3mag_8	wise_allskysc	WISE	W3 24.75" radius aperture magnitude. This is the calibrated source brightness measured in a 24.75" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W3.	real	4	mag	-0.9999995e9
w3mag_8	wise_prelimsc	WISE	W3 24.75" radius aperture magnitude This column is default if this aperture measurement was not possible in W3	real	4	mag	-0.9999995e9
W3mag_ALLWISE	ravedr5Source	RAVE	W3 magnitude from ALLWISE	real	4	mag		phot.mag;em.opt
w3magp	allwise_sc	WISE	Magnitude computed from the inverse-variance-weighted mean of the profile-fit flux measurements on the w3m individual W3 frames covering this source. This differs from w3mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w3mpro is computed by fitting all W3 frames simultaneously and incorporating a robust error model. This column is "null" if w3m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w3mpro for the optimal flux measurement for point sources.	float	8	mag
w3magp	wise_allskysc	WISE	Inverse-variance-weighted mean W3 magnitude computed from profile-fit measurements on the w3m individual frames covering this source. This differs from w3mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w3mpro is computed by fitting all W3 frames simultaneously and incorporating a robust error model. This column is default if w3m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w3mpro for the optimal flux measurement for point sources.	real	4	mag	-0.9999995e9
w3magp	wise_prelimsc	WISE	Inverse-variance-weighted mean W3 magnitude computed from profile-fit measurements on the w3m individual frames covering this source This differs from w3mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w3mpro is computed by fitting all W3 frames simultaneously and incorporating a robust error model. This column is default if w3m=0, the mean flux is negative or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w3mcor	allwise_sc	WISE	W3 aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness, w3mag_2, to give the "standard-aperture" magnitude.	float	8	mag
w3mcor	wise_allskysc	WISE	W3 aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 8.25" aperture photometry brightness, w3mag_2, to give the "standard-aperture" magnitude.	real	4	mag	-0.9999995e9
w3mcor	wise_prelimsc	WISE	W3 aperture curve-of-growth correction, in magnitudes This correction is subtracted from the nominal 8.25" aperture photometry brightness, w3mag_2, to give the "standard-aperture" magnitude	real	4	mag	-0.9999995e9
w3mjdmax	allwise_sc, wise_allskysc	WISE	The latest modified Julian Date (mJD) of the W3 single-exposures covering the source.	float	8
w3mjdmean	allwise_sc, wise_allskysc	WISE	The average modified Julian Date (mJD) of the W3 single-exposures covering the source.	float	8
w3mjdmin	allwise_sc, wise_allskysc	WISE	The earliest modified Julian Date (mJD) of the W3 single-exposures covering the source.	float	8
w3mlq	allwise_sc	WISE	Probability measure that the source is variable in W3 flux. The value is -ln(Q), where Q = 1 - P(χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	float	8
			The Q value is the fraction of all cases to be at least as large as that observed if the null hypothesis is true. The null hypothesis is that the flux is emitted by a non-variable astrophysical object. It may be false because the object is a true variable. It may also be false because the flux measurement is corrupted by artifacts such as cosmic rays, scattered light, etc. The smaller the Q value, the more implausible the null hypothesis, i.e., the more likely it is that the flux is either variable or corrupted or both.
w3mlq	wise_allskysc	WISE	Probability measure that the source is variable in W3 flux. The value is -log10(Q), where Q = 1 - P(Χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	int	4		-99999999
w3mpro	allwise_sc	WISE	W3 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W3 flux measurement has SNR<2. This column is null if the source is nominally detected in W3, but no useful brightness estimate could be made.	float	8	mag
w3mpro	wise_allskysc	WISE	W3 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W3 flux measurement has SNR<2. This column is default if the source is nominally detected in W3, but no useful brightness estimate could be made.	real	4	mag	-0.9999995e9
w3mpro	wise_prelimsc	WISE	W3 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W3 flux measurement has SNR<2 This column is default if the source is nominally detected in W3, but no useful brightness estimate could be made	real	4	mag	-0.9999995e9
w3ndf	allwise_sc	WISE	Number of degrees of freedom in the flux variability chi-square, W3.	int	4
w3ndf	wise_allskysc	WISE	Number of degrees of freedom in the flux variability chi-square, W3.	bigint	8		-99999999
w3nm	allwise_sc	WISE	Integer frame detection count. This column gives the number of individual 8.8s exposures on which this source was detected with SNR>3 in the W3 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	int	4
w3nm	wise_allskysc	WISE	Integer frame detection count in W3. This column gives the number of individual 8.8s exposures on which this source was detected with SNR>3 in the W3 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	bigint	8		-99999999
w3nm	wise_prelimsc	WISE	Integer frame detection count in W3 This column gives the number of individual 8.8s exposures on which this source was detected with SNR>3 in the W3 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures	bigint	8		-99999999
w3pa	allwise_sc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W3.	float	8	deg
w3pa	wise_allskysc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W3.	real	4	degrees	-0.9999995e9
w3pa	wise_prelimsc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W3	real	4	degrees	-0.9999995e9
w3rchi2	allwise_sc	WISE	Reduced χ2 of the W3 profile-fit photometry measurement. This column is null if the W3 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4
w3rchi2	wise_allskysc	WISE	Reduced chi-squared of the W3 profile-fit photometry measurement. This column is default if the W3 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4		-0.9999995e9
w3rchi2	wise_prelimsc	WISE	Reduced chi-squared of the W3 profile-fit photometry measurement This column is default if the W3 magnitude is a 95% confidence upper limit (i.e. the source is not detected)	real	4		-0.9999995e9
w3rchi2_pm	allwise_sc	WISE	Reduced χ2 of the W3 profile-fit photometry measurement including motion estimation. This column is null if the source is not detected in W3 or if the motion fit failed to converge or was not attempted.	real	4
w3rsemi	allwise_sc	WISE	Semi-major axis of the elliptical aperture used to measure source in W3.	float	8	arcsec
w3rsemi	wise_allskysc	WISE	Semi-major axis of the elliptical aperture used to measure source in W3.	real	4	arcsec	-0.9999995e9
w3rsemi	wise_prelimsc	WISE	Semi-major axis of the elliptical aperture used to measure source in W3	real	4	arcsec	-0.9999995e9
w3sat	allwise_sc	WISE	Saturated pixel fraction, W3. The fraction of all pixels within the profile-fitting area source in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W3]~4 mag. Saturation may occur in fainter sources because of charged particle strikes.	float	8
w3sat	wise_allskysc	WISE	Saturated pixel fraction, W3. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W3]~4 mag. Saturation may occur in fainter sources because of a charged particle strike.	real	4		-0.9999995e9
w3sat	wise_prelimsc	WISE	Saturated pixel fraction, W3 The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation	real	4		-0.9999995e9
w3sigflux	allwise_sc	WISE	Uncertainty in the "raw" W3 source flux measurement in profile-fit photometry in units of digital numbers. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w3sigflux	wise_allskysc	WISE	Uncertainty in the "raw" W3 source flux measurement in profile-fit photometry in units of digital numbers. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	ADU	-0.9999995e9
w3sigflux	wise_prelimsc	WISE	Uncertainty in the "raw" W3 source flux measurement in profile-fit photometry in units of digital numbers This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w3sigm	allwise_sc	WISE	Uncertainty in the W3 "standard" aperture magnitude. This column is null if the W3 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm	wise_allskysc	WISE	Uncertainty in the W3 "standard" aperture magnitude. This column is default if the W3 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm	wise_prelimsc	WISE	Uncertainty in the W3 "standard" aperture magnitude This column is default if the W3 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_1	allwise_sc	WISE	Uncertainty in the W3 5.5" radius aperture magnitude. This column is null if the the 5.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_1	wise_allskysc	WISE	Uncertainty in the W3 5.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_1	wise_prelimsc	WISE	Uncertainty in the W3 5.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_2	allwise_sc	WISE	Uncertainty in the W3 8.25" radius aperture magnitude. This column is null if the the 8.25" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_2	wise_allskysc	WISE	Uncertainty in the W3 8.25" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_2	wise_prelimsc	WISE	Uncertainty in the W3 8.25" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_3	allwise_sc	WISE	Uncertainty in the W3 11.0" radius aperture magnitude. This column is null if the the 11.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_3	wise_allskysc	WISE	Uncertainty in the W3 11.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_3	wise_prelimsc	WISE	Uncertainty in the W3 11.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_4	allwise_sc	WISE	Uncertainty in the W3 13.75" radius aperture magnitude. This column is null if the the 13.75" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_4	wise_allskysc	WISE	Uncertainty in the W3 13.75" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_4	wise_prelimsc	WISE	Uncertainty in the W3 13.75" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_5	allwise_sc	WISE	Uncertainty in the W3 16.5" radius aperture magnitude. This column is null if the the 16.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_5	wise_allskysc	WISE	Uncertainty in the W3 16.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_5	wise_prelimsc	WISE	Uncertainty in the W3 16.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_6	allwise_sc	WISE	Uncertainty in the W3 19.25" radius aperture magnitude. This column is null if the the 19.25" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_6	wise_allskysc	WISE	Uncertainty in the W3 19.25" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_6	wise_prelimsc	WISE	Uncertainty in the W3 19.25" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_7	allwise_sc	WISE	Uncertainty in the W3 22.0" radius aperture magnitude. This column is null if the the 22.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_7	wise_allskysc	WISE	Uncertainty in the W3 22.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_7	wise_prelimsc	WISE	Uncertainty in the W3 22.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigm_8	allwise_sc	WISE	Uncertainty in the W3 24.75" radius aperture magnitude. This column is null if the the 24.75" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w3sigm_8	wise_allskysc	WISE	Uncertainty in the W3 24.75" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w3sigm_8	wise_prelimsc	WISE	Uncertainty in the W3 24.75" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w3sigmpro	allwise_sc	WISE	W3 profile-fit photometric measurement uncertainty in mag units. This column is null if the W3 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	float	8	mag
w3sigmpro	wise_allskysc	WISE	W3 profile-fit photometric measurement uncertainty. This column is default if the W3 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	real	4	mag	-0.9999995e9
w3sigmpro	wise_prelimsc	WISE	W3 profile-fit photometric measurement uncertainty This column is default if the W3 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable	real	4	mag	-0.9999995e9
w3sigp1	allwise_sc	WISE	Standard deviation of the population of W3 fluxes measured on the w3m individual frames covering this source, in magnitudes. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is "null" if w3m<2 or if no individual frame measurements are possible.	float	8	mag
w3sigp1	wise_allskysc	WISE	Standard deviation of the population of W3 fluxes measured on the w3m individual frames covering this source. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w3m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w3sigp1	wise_prelimsc	WISE	Standard deviation of the population of W3 fluxes measured on the w3m individual frames covering this source This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w3m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w3sigp2	allwise_sc	WISE	Standard deviation of the mean of the distribution of W3 fluxes (w3magp) computed from profile-fit measurements on the w3m individual frames covering this source, in magnitudes. This is equivalent to w3sigp1/sqrt(w3m). This column is "null" if w3m<2 or if no individual frame measurements are possible.	float	8	mag
w3sigp2	wise_allskysc	WISE	Standard deviation of the mean of the distribution of W3 fluxes (w3magp) computed from profile-fit measurements on the w3m individual frames covering this source. This column is default if w3m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w3sigp2	wise_prelimsc	WISE	Standard deviation of the mean of the distribution of W3 fluxes (w3magp) computed from profile-fit measurements on the w3m individual frames covering this source This column is default if w3m<2 or if no individual frame measurements are possible	real	4	mag	-0.9999995e9
w3sigsk	allwise_sc	WISE	The uncertainty in the W3 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70".	float	8	dn
w3sigsk	wise_allskysc	WISE	The uncertainty in the W3 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70".	real	4	ADU	-0.9999995e9
w3sigsk	wise_prelimsc	WISE	The uncertainty in the W3 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70"	real	4	ADU	-0.9999995e9
w3sky	allwise_sc	WISE	The trimmed average of the W3 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	dn
			For profile-fit photometry, the sky background is measured on the individual single-exposure images that are used for source characterization. For aperture photometry, the sky background is measured on the Atlas Image.
w3sky	wise_allskysc	WISE	The trimmed average of the W3 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	ADU	-0.9999995e9
w3sky	wise_prelimsc	WISE	The trimmed average of the W3 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70" Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value	float	8	ADU	-0.9999995e9
w3snr	allwise_sc	WISE	W3 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w3flux) to flux uncertainty (w3sigflux)in the W3 profile-fit photometry measurement. This column is null if w3flux is negative, or if w3flux or w3sigflux are null.	float	8
w3snr	wise_allskysc	WISE	W3 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w3flux) to flux uncertainty (w3sigflux) in the W3 profile-fit photometry measurement. This column is default if w3flux is negative, or if w3flux or w3sigflux are default.	real	4		-0.9999995e9
w3snr	wise_prelimsc	WISE	W3 profile-fit measurement signal-to-noise ratio This value is the ratio of the flux (w3flux) to flux uncertainty (w3sigflux)in the W3 profile-fit photometry measurement. This column is default if w3flux is negative, or if w3flux or w3sigflux are default.	real	4		-0.9999995e9
w4ba	allwise_sc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W4.	float	8	arcsec
w4ba	wise_allskysc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W4.	real	4	arcsec	-0.9999995e9
w4ba	wise_prelimsc	WISE	Axis ratio (b/a) of the elliptical aperture used to measure source in W4	real	4	arcsec	-0.9999995e9
w4cc_map	allwise_sc	WISE	Contamination and confusion map for this source in W4. This column contains the integer equivalent of the 9-bit binary number that specifies if the W4 measurement is believed to be contaminated by or a spurious detection of an image artifact.	int	4
			The elements of the binary array are: S 0 0 0 O H 0 P D. The leftmost bit, S, differentiates whether the band-detection is believed to be a real detection contaminated by an artifact ("0") or a spurious detection of an artifact ("1"). The remaining bits are set to "1" to denote contamination by different types of artifacts according to the letters: D - Diffraction spike. Source may be a spurious detection of or contaminated by a diffraction spike of a nearby bright star on the same image. P - Persistence. Source may be a spurious detection of or contaminated by a short-term latent (persistence) image left by a bright source. H - Halo. Source may be a spurious detection of or contaminated by the scattered light halo associated with a bright star. O (letter "o") - Optical ghost. Source may be a spurious detection of or contaminated by an optical ghost image caused by a nearby bright source on the same image. For example, a measurement that is believed to be a spurious detection of a diffraction spike and scattered light halo has a binary bit map value of "100001001" and w?cc_map=265.
w4cc_map	wise_allskysc	WISE	Contamination and confusion map for this source in W4. This column contains the integer equivalent of the 9-bit binary number that specifies if the W4 measurement is believed to be contaminated by or a spurious detection of an image artifact.	smallint	2
w4cc_map	wise_prelimsc	WISE	Contamination and confusion map for this source in W4 This column contains the integer equivalent of the 9-bit binary number that specifies if the W4 measurement is believed to be contaminated by or a spurious detection of an image artifact	smallint	2
w4cc_map_str	allwise_sc	WISE	Contamination and confusion string. This column is a character string that denotes all artifacts that may contaminate the W4 measurement of this source, in the priority order D,P,H,O,d,p,h,o. Lower-case letters denote cases where the source detection in this band is believed to be real but the measurement may be contaminated by the artifact. Upper-case letters denote cases where the source detection in this band may be a spurious detection of an artifact. This string is "null" if there are no artifacts that affect the measurement in this band. The value that appears in fourth element of the cc_flags string is the left-most character in w4cc_map_str. If w4cc_map_str is "null", then the corresponding cc_flags entry is "0".	varchar	9
			For example, a real detection that is contaminated by a diffraction spike and a latent (persistent) image has a w?cc_map_str="dp". A spurious detection of a diffraction spike that is also contaminated by a latent image has w?cc_map_str="Dp".
w4cc_map_str	wise_allskysc	WISE	Contamination and confusion string in W4. This column is a character string that denotes all artifacts that may contaminate the W4 measurement of this source, in the priority order D,P,H,O	char	9
w4cc_map_str	wise_prelimsc	WISE	Contamination and confusion string in W4 This column is a character string that denotes all artifacts that may contaminate the W4 measurement of this source, in the priority order D,P,H,O	char	9
w4conf	allwise_sc	WISE	Estimated confusion noise in the W4 sky background annulus, in digital numbers. This number is the difference between the measured noise in the sky background w4sigsk and the noise measured in the same region on the Atlas Uncertainty Maps.	float	8	dn
w4conf	wise_allskysc, wise_prelimsc	WISE	Estimated confusion noise in the W4 sky background annulus, in digital numbers This number is the difference between the measured noise in the sky background w4sigsk and the noise measured in the same region on the Atlas Uncertainty Maps	float	8	ADU	-0.9999995e9
w4cov	allwise_sc	WISE	Mean pixel coverage in W4. This column gives the mean pixel value from the W4 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 16.5" centered on the position of this source.	float	8
			W4cov may differ from the integer frame coverage value given in w4m for two reasons. First, individual pixels in the measurement area may be masked or otherwise unusable, reducing the effective pixel count and thus the mean coverage value. Second, the effective sky area sampled by a pixels in single-exposure image varies across the focal plane because of field distortion. Distortion is corrected when coadding to generate the Atlas Images. Therefore, the effective number of pixels contributing to a pixel in the Atlas Coverage Map may be slightly smaller or larger than expected if there was no distortion.
w4cov	wise_allskysc	WISE	Mean pixel coverage in W4. This column gives the mean pixel value from the W4 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 16.5" centered on the position of this source.	real	4		-0.9999995e9
w4cov	wise_prelimsc	WISE	Mean pixel coverage in W4 This column gives the mean pixel value from the W4 Atlas Tile Coverage Map within the "standard" aperture, a circular area with a radius of 17.0" centered on the position of this source	real	4		-0.9999995e9
w4dmag	wise_allskysc	WISE	Difference between maximum and minimum magnitude of the source from all usable single-exposure frames, W4. Single-exposure measurements with w4rchi2 values greater than 3.0 times the median are rejected from this computation.	real	4	mag	-0.9999995e9
w4flg	allwise_sc	WISE	W4 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg	wise_allskysc	WISE	W4 "standard" aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	smallint	2		-9999
w4flg	wise_prelimsc	WISE	W4 "standard" aperture measurement quality flag This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit	smallint	2		-9999
w4flg_1	allwise_sc	WISE	W4 11.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_1	wise_allskysc	WISE	W4 11.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_1	wise_prelimsc	WISE	W4 11.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flg_2	allwise_sc	WISE	W4 16.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_2	wise_allskysc	WISE	W4 16.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_2	wise_prelimsc	WISE	W4 16.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flg_3	allwise_sc	WISE	W4 22.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_3	wise_allskysc	WISE	W4 22.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_3	wise_prelimsc	WISE	W4 22.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flg_4	allwise_sc	WISE	W4 27.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_4	wise_allskysc	WISE	W4 27.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_4	wise_prelimsc	WISE	W4 27.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flg_5	allwise_sc	WISE	W4 33.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_5	wise_allskysc	WISE	W4 33.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_5	wise_prelimsc	WISE	W4 33.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flg_6	allwise_sc	WISE	W4 38.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_6	wise_allskysc	WISE	W4 38.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_6	wise_prelimsc	WISE	W4 38.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flg_7	allwise_sc	WISE	W4 44.0" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_7	wise_allskysc	WISE	W4 44.0" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_7	wise_prelimsc	WISE	W4 44.0" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flg_8	allwise_sc	WISE	W4 49.5" radius aperture magnitude quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4flg_8	wise_allskysc	WISE	W4 49.5" radius aperture magnitude quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag.	smallint	2		-9999
w4flg_8	wise_prelimsc	WISE	W4 49.5" radius aperture magnitude quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the standard aperture photometry quality flag	smallint	2		-9999
w4flux	allwise_sc	WISE	The "raw" W4 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w4flux	wise_allskysc	WISE	The "raw" W4 source flux measured in profile-fit photometry in units of digital numbers. This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	ADU	-0.9999995e9
w4flux	wise_prelimsc	WISE	The "raw" W4 source flux measured in profile-fit photometry in units of digital numbers This value may be negative. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w4frl	wise_prelimsc	WISE	Fraction of W4 pixels affected by latents This column gives the fraction of all W4 pixels in the stack of individual W4 exposures used to characterize this source that may be affected by the presence of a latent image produced by a bright source	real	4		-0.9999995e9
w4frtr	wise_allskysc	WISE	Fraction of W4 pixels affected by transients. This column gives the fraction of all W4 pixels in the stack of individual W4 exposures used to characterize this source that may be affected by transient events. This number is computed by counting the number of pixels in the single exposure Bit Mask images with value "21" that are present within the profile-fitting area, a circular region with radius of 15.0", centered on the position of this source, and dividing by the total number of pixels in the same area that are available for measurement.	real	4		-0.9999995e9
w4gerr	allwise_sc	WISE	Uncertainty in the W4 magnitude of source measured in elliptical aperture. CAUTION: A w4gerr value of 9.999 indicates that the measurement uncertainty is very large, or the uncertainty could not be computed. In either case, the w4gmag measurement should be considered highly suspect.	float	8	mag
w4gerr	wise_allskysc	WISE	Uncertainty in the W4 magnitude of source measured in elliptical aperture.	real	4	mag	-0.9999995e9
w4gerr	wise_prelimsc	WISE	Uncertainty in the W4 magnitude of source measured in elliptical aperture	real	4	mag	-0.9999995e9
w4gflg	allwise_sc	WISE	W4 elliptical aperture measurement quality flag. This flag indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit.	int	4
			The flag value is an integer that is the combination of one or more of the following values that signify different conditions: 0 - No contamination 1 - Source confusion - another source falls within the measurement aperture 2 - Presence of bad pixels in the measurement aperture 4 - Non-zero bit flag tripped (other than 2 or 18) 8 - All pixels are flagged as unusable, or the aperture flux is negative. In the former case, the aperture magnitude is "null". In the latter case, the aperture magnitude is a 95% confidence upper limit. 16 - Saturation - there are one or more saturated pixels in the measurement aperture 32 - The magnitude is a 95% confidence upper limit
w4gflg	wise_allskysc	WISE	W4 elliptical aperture measurement quality flag. Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag, w4mflg.	smallint	2		-9999
w4gflg	wise_prelimsc	WISE	W4 elliptical aperture measurement quality flag Indicates if one or more image pixels in the measurement aperture for this band is confused with nearby objects, is contaminated by saturated or otherwise unusable pixels, or is an upper limit. The flag values are as described for the "standard" aperture photometry quality flag	smallint	2		-9999
w4gmag	allwise_sc	WISE	W4 magnitude of source measured in the elliptical aperture described by w4rsemi, w4ba, and w4pa.	float	8	mag
w4gmag	wise_allskysc	WISE	W4 magnitude of source measured in the elliptical aperture described by w4rsemi, w4ba, and w4pa.	real	4	mag	-0.9999995e9
w4gmag	wise_prelimsc	WISE	W4 magnitude of source measured in the elliptical aperture described by w4rsemi, w4ba, and w4pa	real	4	mag	-0.9999995e9
w4k	allwise_sc	WISE	Stetson K variability index (Stetson, P. 1996, PASP, 108, 851) computed using the W4 profile-fit fluxes measured on the individual single-exposure images. This column is null if there are <3 single-exposure measurements available in W4.	float	8
w4m	allwise_sc	WISE	Integer frame coverage. This column gives the number of individual 8.8s W4 exposures on which a profile-fit measurement of this source was possible. This number can differ between the four bands because band-dependent criteria are used to select individual frames for inclusion in the coadded Atlas Images. This column is null if there is no frame coverage in this band at the position of this source.	int	4
w4m	wise_allskysc	WISE	Integer frame coverage in W4. This column gives the number of individual 8.8s W4 exposures on which a profile-fit measurement of this source was possible.	bigint	8		-99999999
w4m	wise_prelimsc	WISE	Integer frame coverage in W4 This column gives the number of individual 8.8s W4 exposures on which a profile-fit measurement of this source was possible	bigint	8		-99999999
w4mag	allwise_sc	WISE	W4 "standard" aperture magnitude. This is the curve-of-growth corrected source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". The curve-of-growth correction is given in w4mcor. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag	wise_allskysc, wise_prelimsc	WISE	W4 "standard" aperture magnitude This is the curve-of-growth corrected source brightness measured in an 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness	real	4	mag	-0.9999995e9
w4mag_1	allwise_sc	WISE	W4 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_1	wise_allskysc	WISE	W4 11.0" radius aperture magnitude. This is the calibrated source brightness measured in a 11.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_1	wise_prelimsc	WISE	W4 11.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
w4mag_2	allwise_sc	WISE	W4 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_2	wise_allskysc	WISE	W4 16.5" radius aperture magnitude. This is the calibrated source brightness measured in a 16.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_2	wise_prelimsc	WISE	W4 16.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
w4mag_3	allwise_sc	WISE	W4 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_3	wise_allskysc	WISE	W4 22.0" radius aperture magnitude. This is the calibrated source brightness measured in a 22.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_3	wise_prelimsc	WISE	W4 22.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
w4mag_4	allwise_sc	WISE	W4 27.5" radius aperture magnitude. This is the calibrated source brightness measured in a 27.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied.This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_4	wise_allskysc	WISE	W4 27.5" radius aperture magnitude. This is the calibrated source brightness measured in a 27.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_4	wise_prelimsc	WISE	W4 27.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
w4mag_5	allwise_sc	WISE	W4 33.0" radius aperture magnitude. This is the calibrated source brightness measured in a 33.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_5	wise_allskysc	WISE	W4 33.0" radius aperture magnitude. This is the calibrated source brightness measured in a 33.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_5	wise_prelimsc	WISE	W4 33.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
w4mag_6	allwise_sc	WISE	W4 38.5" radius aperture magnitude. This is the calibrated source brightness measured in a 38.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_6	wise_allskysc	WISE	W4 38.5" radius aperture magnitude. This is the calibrated source brightness measured in a 38.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_6	wise_prelimsc	WISE	W4 38.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
w4mag_7	allwise_sc	WISE	W4 44.0" radius aperture magnitude. This is the calibrated source brightness measured in a 44.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_7	wise_allskysc	WISE	W4 44.0" radius aperture magnitude. This is the calibrated source brightness measured in a 44.0" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_7	wise_prelimsc	WISE	W4 44.0" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
w4mag_8	allwise_sc	WISE	W4 49.5" radius aperture magnitude. This is the calibrated source brightness measured in a 49.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is null if an aperture measurement was not possible in W4.	float	8	mag
w4mag_8	wise_allskysc	WISE	W4 49.5" radius aperture magnitude. This is the calibrated source brightness measured in a 49.5" radius circular aperture centered on the source position on the Atlas Image. If the source is not detected in the aperture measurement, this is the 95% confidence upper limit to the brightness. The background sky reference level is measured in an annular region with inner radius of 50" and outer radius of 70". No curve-of-growth correction has been applied. This column is default if this aperture measurement was not possible in W4.	real	4	mag	-0.9999995e9
w4mag_8	wise_prelimsc	WISE	W4 49.5" radius aperture magnitude This column is default if this aperture measurement was not possible in W4	real	4	mag	-0.9999995e9
W4mag_ALLWISE	ravedr5Source	RAVE	W4 magnitude from ALLWISE	real	4	mag		phot.mag;em.opt
w4magp	allwise_sc	WISE	Magnitude computed from the inverse-variance-weighted mean of the profile-fit flux measurements on the w4m individual W4 frames covering this source. This differs from w4mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w4mpro is computed by fitting all W4 frames simultaneously and incorporating a robust error model. This column is "null" if w4m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w4mpro for the optimal flux measurement for point sources.	float	8	mag
w4magp	wise_allskysc	WISE	Inverse-variance-weighted mean W4 magnitude computed from profile-fit measurements on the w4m individual frames covering this source. This differs from w4mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w4mpro is computed by fitting all W4 frames simultaneously and incorporating a robust error model. This column is default if w4m=0, the mean flux is negative or if no individual frame measurements are possible. CAUTION: This is not a robust measurement of source brightness. It is provided as an internal repeatability diagnostic only. Users should always defer to w4mpro for the optimal flux measurement for point sources.	real	4	mag	-0.9999995e9
w4magp	wise_prelimsc	WISE	Inverse-variance-weighted mean W4 magnitude computed from profile-fit measurements on the w4m individual frames covering this source This differs from w4mpro in that it is computed by combining the profile-fit measurements from individual frames, whereas w4mpro is computed by fitting all W4 frames simultaneously and incorporating a robust error model. This column is default if w4m=0, the mean flux is negative or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w4mcor	allwise_sc	WISE	W4 aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 16.5" aperture photometry brightness, w4mag_2, to give the "standard-aperture" magnitude.	float	8	mag
w4mcor	wise_allskysc	WISE	W4 aperture curve-of-growth correction, in magnitudes. This correction is subtracted from the nominal 16.5" aperture photometry brightness, w4mag_2, to give the "standard-aperture" magnitude.	real	4	mag	-0.9999995e9
w4mcor	wise_prelimsc	WISE	W4 aperture curve-of-growth correction, in magnitudes This correction is subtracted from the nominal 16.5" aperture photometry brightness, w4mag_2, to give the "standard-aperture" magnitude	real	4	mag	-0.9999995e9
w4mjdmax	allwise_sc, wise_allskysc	WISE	The latest modified Julian Date (mJD) of the W4 single-exposures covering the source.	float	8
w4mjdmean	allwise_sc, wise_allskysc	WISE	The average modified Julian Date (mJD) of the W4 single-exposures covering the source.	float	8
w4mjdmin	allwise_sc, wise_allskysc	WISE	The earliest modified Julian Date (mJD) of the W4 single-exposures covering the source.	float	8
w4mlq	allwise_sc	WISE	Probability measure that the source is variable in W4 flux. The value is -ln(Q), where Q = 1 - P(χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	float	8
			The Q value is the fraction of all cases to be at least as large as that observed if the null hypothesis is true. The null hypothesis is that the flux is emitted by a non-variable astrophysical object. It may be false because the object is a true variable. It may also be false because the flux measurement is corrupted by artifacts such as cosmic rays, scattered light, etc. The smaller the Q value, the more implausible the null hypothesis, i.e., the more likely it is that the flux is either variable or corrupted or both.
w4mlq	wise_allskysc	WISE	Probability measure that the source is variable in W4 flux. The value is -log10(Q), where Q = 1 - P(Χ2). P is the cumulative chi-square distribution probability for the flux sample measured on the individual single-exposure images. The value is clipped at 9.	int	4		-99999999
w4mpro	allwise_sc	WISE	W4 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W4 flux measurement has SNR<2. This column is null if the source is nominally detected in W4, but no useful brightness estimate could be made.	float	8	mag
w4mpro	wise_allskysc	WISE	W4 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W4 flux measurement has SNR<2. This column is default if the source is nominally detected in W4, but no useful brightness estimate could be made.	real	4	mag	-0.9999995e9
w4mpro	wise_prelimsc	WISE	W4 magnitude measured with profile-fitting photometry, or the magnitude of the 95% confidence brightness upper limit if the W4 flux measurement has SNR<2 This column is default if the source is nominally detected in W4, but no useful brightness estimate could be made	real	4	mag	-0.9999995e9
w4ndf	allwise_sc	WISE	Number of degrees of freedom in the flux variability chi-square, W4.	int	4
w4ndf	wise_allskysc	WISE	Number of degrees of freedom in the flux variability chi-square, W4.	bigint	8		-99999999
w4nm	allwise_sc	WISE	Integer frame detection count. This column gives the number of individual 8.8s exposures on which this source was detected with SNR>3 in the W4 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	int	4
w4nm	wise_allskysc	WISE	Integer frame detection count in W4. This column gives the number of individual 8.8s exposures on which this source was detected with SNR>3 in the W4 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures.	bigint	8		-99999999
w4nm	wise_prelimsc	WISE	Integer frame detection count in W4 This column gives the number of individual 8.8s exposures on which this source was detected with SNR>3 in the W4 profile-fit measurement. This number can be zero for sources that are well-detected on the coadded Atlas Image, but too faint for detection on the single exposures	bigint	8		-99999999
w4pa	allwise_sc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W4.	float	8	deg
w4pa	wise_allskysc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W4.	real	4	degrees	-0.9999995e9
w4pa	wise_prelimsc	WISE	Position angle (degrees E of N) of the elliptical aperture major axis used to measure source in W4	real	4	degrees	-0.9999995e9
w4rchi2	allwise_sc	WISE	Reduced χ2 of the W4 profile-fit photometry measurement. This column is null if the W4 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4
w4rchi2	wise_allskysc	WISE	Reduced chi-squared of the W4 profile-fit photometry measurement. This column is default if the W4 magnitude is a 95% confidence upper limit (i.e. the source is not detected).	real	4		-0.9999995e9
w4rchi2	wise_prelimsc	WISE	Reduced chi-squared of the W4 profile-fit photometry measurement This column is default if the W4 magnitude is a 95% confidence upper limit (i.e. the source is not detected)	real	4		-0.9999995e9
w4rchi2_pm	allwise_sc	WISE	Reduced χ2 of the W4 profile-fit photometry measurement including motion estimation. This column is null if the source is not detected in W4 or if the motion fit failed to converge or was not attempted.	real	4
w4rsemi	allwise_sc	WISE	Semi-major axis of the elliptical aperture used to measure source in W4.	float	8	arcsec
w4rsemi	wise_allskysc	WISE	Semi-major axis of the elliptical aperture used to measure source in W4.	real	4	arcsec	-0.9999995e9
w4rsemi	wise_prelimsc	WISE	Semi-major axis of the elliptical aperture used to measure source in W4	real	4	arcsec	-0.9999995e9
w4sat	allwise_sc	WISE	Saturated pixel fraction, W4. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W4]~0 mag. Saturation may occur in fainter sources because of charged particle strikes.	float	8
w4sat	wise_allskysc	WISE	Saturated pixel fraction, W4. The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation. Saturation begins to occur for point sources brighter than [W4]~0 mag. Saturation may occur in fainter sources because of a charged particle strike.	real	4		-0.9999995e9
w4sat	wise_prelimsc	WISE	Saturated pixel fraction, W4 The fraction of all pixels within the profile-fitting area in the stack of single-exposure images used to characterize this source that are flagged as saturated. A value larger than 0.0 indicates one or more pixels of saturation	real	4		-0.9999995e9
w4sigflux	allwise_sc	WISE	Uncertainty in the "raw" W4 source flux measurement in profile-fit photometry in units of digital numbers. This column is null if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	dn
w4sigflux	wise_allskysc	WISE	Uncertainty in the "raw" W4 source flux measurement in profile-fit photometry in units of digital numbers. This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels.	real	4	ADU	-0.9999995e9
w4sigflux	wise_prelimsc	WISE	Uncertainty in the "raw" W4 source flux measurement in profile-fit photometry in units of digital numbers This column is default if no useful profile-fit measurement of the source is possible because of masked or otherwise unusable pixels	real	4	ADU	-0.9999995e9
w4sigm	allwise_sc	WISE	Uncertainty in the W4 "standard" aperture magnitude. This column is null if the W4 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm	wise_allskysc, wise_prelimsc	WISE	Uncertainty in the W4 "standard" aperture magnitude This column is default if the W4 "standard" aperture magnitude is an upper limit, or if an aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_1	allwise_sc	WISE	Uncertainty in the W4 11.0" radius aperture magnitude. This column is null if the the 11.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_1	wise_allskysc	WISE	Uncertainty in the W4 11.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_1	wise_prelimsc	WISE	Uncertainty in the W4 11.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_2	allwise_sc	WISE	Uncertainty in the W4 16.5" radius aperture magnitude. This column is null if the the 16.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_2	wise_allskysc	WISE	Uncertainty in the W4 16.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_2	wise_prelimsc	WISE	Uncertainty in the W4 16.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_3	allwise_sc	WISE	Uncertainty in the W4 22.0" radius aperture magnitude. This column is null if the the 22.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_3	wise_allskysc	WISE	Uncertainty in the W4 22.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_3	wise_prelimsc	WISE	Uncertainty in the W4 22.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_4	allwise_sc	WISE	Uncertainty in the W4 27.5" radius aperture magnitude. This column is null if the the 27.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_4	wise_allskysc	WISE	Uncertainty in the W4 27.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_4	wise_prelimsc	WISE	Uncertainty in the W4 27.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_5	allwise_sc	WISE	Uncertainty in the W4 33.0" radius aperture magnitude. This column is null if the the 33.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_5	wise_allskysc	WISE	Uncertainty in the W4 33.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_5	wise_prelimsc	WISE	Uncertainty in the W4 33.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_6	allwise_sc	WISE	Uncertainty in the W4 38.5" radius aperture magnitude. This column is null if the the 38.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_6	wise_allskysc	WISE	Uncertainty in the W4 38.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_6	wise_prelimsc	WISE	Uncertainty in the W4 38.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_7	allwise_sc	WISE	Uncertainty in the W4 44.0" radius aperture magnitude. This column is null if the the 44.0" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_7	wise_allskysc	WISE	Uncertainty in the W4 44.0" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_7	wise_prelimsc	WISE	Uncertainty in the W4 44.0" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigm_8	allwise_sc	WISE	Uncertainty in the W4 49.5" radius aperture magnitude. This column is null if the the 49.5" radius aperture magnitude is an upper limit, or if an aperture measurement was not possible.	float	8	mag
w4sigm_8	wise_allskysc	WISE	Uncertainty in the W4 49.5" radius aperture magnitude. This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible.	real	4	mag	-0.9999995e9
w4sigm_8	wise_prelimsc	WISE	Uncertainty in the W4 49.5" radius aperture magnitude This column is default if the corresponding aperture magnitude is an upper limit, or if that aperture measurement was not possible	real	4	mag	-0.9999995e9
w4sigmpro	allwise_sc	WISE	W4 profile-fit photometric measurement uncertainty in mag units. This column is null if the W4 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	float	8	mag
w4sigmpro	wise_allskysc	WISE	W4 profile-fit photometric measurement uncertainty. This column is default if the W4 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable.	real	4	mag	-0.9999995e9
w4sigmpro	wise_prelimsc	WISE	W4 profile-fit photometric measurement uncertainty This column is default if the W4 profile-fit magnitude is a 95% confidence upper limit or if the source is not measurable	real	4	mag	-0.9999995e9
w4sigp1	allwise_sc	WISE	Standard deviation of the population of W4 fluxes measured on the w4m individual frames covering this source, in magnitudes. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is "null" if w4m<2 or if no individual frame measurements are possible.	float	8	mag
w4sigp1	wise_allskysc	WISE	Standard deviation of the population of W4 fluxes measured on the w4m individual frames covering this source. This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w4m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w4sigp1	wise_prelimsc	WISE	Standard deviation of the population of W4 fluxes measured on the w4m individual frames covering this source This provides a measure of the characteristic uncertainty of the measurement of this source on individual frames. This column is default if w4m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w4sigp2	allwise_sc	WISE	Standard deviation of the mean of the distribution of W4 fluxes (w4magp) computed from profile-fit measurements on the w4m individual frames covering this source, in magnitudes. This is equivalent to w4sigp1/sqrt(w4m). This column is "null" if w4m<2 or if no individual frame measurements are possible.	float	8	mag
w4sigp2	wise_allskysc	WISE	Standard deviation of the mean of the distribution of W4 fluxes (w4magp) computed from profile-fit measurements on the w4m individual frames covering this source. This column is default if w4m<2 or if no individual frame measurements are possible.	real	4	mag	-0.9999995e9
w4sigp2	wise_prelimsc	WISE	Standard deviation of the mean of the distribution of W4 fluxes (w4magp) computed from profile-fit measurements on the w4m individual frames covering this source This column is default if w4m<2 or if no individual frame measurements are possible	real	4	mag	-0.9999995e9
w4sigsk	allwise_sc	WISE	The uncertainty in the W4 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70".	float	8	dn
w4sigsk	wise_allskysc	WISE	The uncertainty in the W4 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70"	real	4	ADU	-0.9999995e9.
w4sigsk	wise_prelimsc	WISE	The uncertainty in the W4 sky background value in units of digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70"	real	4	ADU	-0.9999995e9
w4sky	allwise_sc	WISE	The trimmed average of the W4 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	dn
			For profile-fit photometry, the sky background is measured on the individual single-exposure images that are used for source characterization. For aperture photometry, the sky background is measured on the Atlas Image.
w4sky	wise_allskysc	WISE	The trimmed average of the W4 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70". Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value.	float	8	ADU	-0.9999995e9
w4sky	wise_prelimsc	WISE	The trimmed average of the W4 sky background value in digital numbers measured in an annulus with an inner radius of 50" and outer radius of 70" Both profile-fit and aperture photometry source brightness measurements are made relative to this sky background value	float	8	ADU	-0.9999995e9
w4snr	allwise_sc	WISE	W4 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w4flux) to flux uncertainty (w4sigflux)in the W4 photometry measurement. This column is null if w4flux is negative, or if w4flux or w4sigflux are null.	float	8
w4snr	wise_allskysc	WISE	W4 profile-fit measurement signal-to-noise ratio. This value is the ratio of the flux (w4flux) to flux uncertainty (w4sigflux)in the W4 profile-fit photometry measurement. This column is default if w4flux is negative, or if w4flux or w4sigflux are default.	real	4		-0.9999995e9
w4snr	wise_prelimsc	WISE	W4 profile-fit measurement signal-to-noise ratio This value is the ratio of the flux (w4flux) to flux uncertainty (w4sigflux)in the W4 profile-fit photometry measurement. This column is default if w4flux is negative, or if w4flux or w4sigflux are default.	real	4		-0.9999995e9
warnFlag	firstSource	FIRST	Warning flag indicating that the source may be a sidelobe of a nearby bright source.	varchar	1			meta.code
wcs	RequiredDiffImage	ATLASDR1	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	ATLASDR2	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	ATLASDR3	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	ATLASDR4	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	ATLASDR5	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	ATLASv20131127	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	ATLASv20160425	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	ATLASv20180209	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	VPHASDR3	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	VPHASv20160112	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcs	RequiredDiffImage	VPHASv20170222	CASU difference image tool option to specify use of implicit WCS in the input files (y/n; recommended value=y)	varchar	1			??
wcsPass	CurrentAstrometry	ATLASDR1	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs.cdmatrix
wcsPass	CurrentAstrometry	ATLASDR2	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs.cdmatrix
wcsPass	CurrentAstrometry	ATLASDR3	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wcsPass	CurrentAstrometry	ATLASDR4	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wcsPass	CurrentAstrometry	ATLASDR5	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wcsPass	CurrentAstrometry	ATLASv20131127	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs.cdmatrix
wcsPass	CurrentAstrometry	ATLASv20160425	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wcsPass	CurrentAstrometry	ATLASv20180209	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wcsPass	CurrentAstrometry	VPHASDR3	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wcsPass	CurrentAstrometry	VPHASv20160112	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wcsPass	CurrentAstrometry	VPHASv20170222	Pass level of WCS {image extension keyword: WCSPASS}	tinyint	1		0	pos.wcs
wfrtype	Multiframe	ATLASDR1	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	ATLASDR2	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	ATLASDR3	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	ATLASDR4	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	ATLASDR5	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	ATLASv20131127	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	ATLASv20160425	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	ATLASv20180209	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	VPHASDR3	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	VPHASv20160112	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wfrtype	Multiframe	VPHASv20170222	WFR type {image primary HDU keyword: WFRTYPE}	varchar	4		NONE
wiseID	twompzPhotoz	TWOMPZ	WISE ID for wise_allskysc (cntr)	bigint	8		-99999999	meta.id
wiseX	twompzPhotoz	TWOMPZ	WISE source designation in allskysc {image primary HDU keyword: WISE_designation}	varchar	22		NONE	meta.id
wx	allwise_sc	WISE	The x-pixel coordinate of this source on the Atlas Image.	float	8	pix
wx	catwise_2020, catwise_prelim	WISE	x-pixel coordinate	real	4	pix
wx	wise_allskysc	WISE	The x-pixel coordinate of this source on the Atlas Image.	real	4	pixels
wx	wise_prelimsc	WISE	The x-pixel coordinate of this source on the Atlas Image	real	4	pixels
wy	allwise_sc	WISE	The y-pixel coordinate of this source on the Atlas Image.	float	8	pix
wy	catwise_2020, catwise_prelim	WISE	y-pixel coordinate	real	4	pix
wy	wise_allskysc	WISE	The y-pixel coordinate of this source on the Atlas Image.	real	4	pixels
wy	wise_prelimsc	WISE	The y-pixel coordinate of this source on the Atlas Image	real	4	pixels