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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

F
Name	Schema Table	Database	Description	Type	Length	Unit	Default Value	Unified Content Descriptor
F1	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	Flux in IRAC band 1	real	4	mJy	-999.9
f1	hipparcos_new_reduction	GAIADR1	Percentage rejected data	int	4			arith.ratio;stat.value
F1_err	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	1sigma flux error (IRAC band 1)	real	4	mJy	-999.9
F1_rms	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	RMS dev. of detection from F1	real	4	mJy	-999.9
F2	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	Flux in IRAC band 2	real	4	mJy	-999.9
f2	hipparcos_new_reduction	GAIADR1	Goodness of fit	float	8			stat.fit.goodness
F2_err	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	1sigma flux error (IRAC band 2)	real	4	mJy	-999.9
F2_rms	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	RMS dev. of detection from F2	real	4	mJy	-999.9
F3	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	Flux in IRAC band 3	real	4	mJy	-999.9
F3_6	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	3.6um IRAC (Band 1) flux	real	4	mJy	-999.9
F3_6_err	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	3.6um IRAC (Band 1) 1 sigma error	real	4	mJy	-999.9
F3_6_rms	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	RMS deviation of the individual detections from the final flux for 3.6um IRAC (Band 1)	real	4	mJy	-999.9
F3_err	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	1sigma flux error (IRAC band 3)	real	4	mJy	-999.9
F3_rms	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	RMS dev. of detection from F3	real	4	mJy	-999.9
F4	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	Flux in IRAC band 4	real	4	mJy	-999.9
F4_5	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	4.5um IRAC (Band 2) flux	real	4	mJy	-999.9
F4_5_err	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	4.5um IRAC (Band 2) 1 sigma error	real	4	mJy	-999.9
F4_5_rms	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	RMS deviation of the individual detections from the final flux for 4.5um IRAC (Band 2)	real	4	mJy	-999.9
F4_err	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	1sigma flux error (IRAC band 4)	real	4	mJy	-999.9
F4_rms	glimpse_hrc_inter, glimpse_mca_inter	GLIMPSE	RMS dev. of detection from F4	real	4	mJy	-999.9
F5_8	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	5.8um IRAC (Band 3) flux	real	4	mJy	-999.9
F5_8_err	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	5.8um IRAC (Band 3) 1 sigma error	real	4	mJy	-999.9
F5_8_rms	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	RMS deviation of the individual detections from the final flux for 5.8um IRAC (Band 3)	real	4	mJy	-999.9
F8_0	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	8.0um IRAC (Band 4) flux	real	4	mJy	-999.9
F8_0_err	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	8.0um IRAC (Band 4) 1 sigma error	real	4	mJy	-999.9
F8_0_rms	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	RMS deviation of the individual detections from the final flux for 8.0um IRAC (Band 4)	real	4	mJy	-999.9
f_resFlux	nvssSource	NVSS	[PS* ] Residual Code	varchar	2			meta.code
fCor_100	iras_psc	IRAS	Flux correction factor applied (times 1000, 100 micron)	smallint	2			instr.param
fCor_12	iras_psc	IRAS	Flux correction factor applied (times 1000, 12 micron)	smallint	2			instr.param
fCor_25	iras_psc	IRAS	Flux correction factor applied (times 1000, 25 micron)	smallint	2			instr.param
fCor_60	iras_psc	IRAS	Flux correction factor applied (times 1000, 60 micron)	smallint	2			instr.param
Fe	ravedr5Source	RAVE	[Fe/H] abundance of Fe	real	4	dex		phys.abund.Z
Fe_N	ravedr5Source	RAVE	Number of used spectral lines in calc. of [Fe/H]	smallint	2			meta.number
fg_flg	twomass_xsc	TWOMASS	flux-growth convergence flag.	varchar	6			meta.code
FH	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	2MASS All-Sky PSC H Band flux	real	4	mJy	-999.9
FH_err	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	2MASS All-Sky PSC H Band 1 sigma error	real	4	mJy	-999.9
FiberNumber	ravedr5Source	RAVE	Instrument fiber number (2df) [1..150]	tinyint	1			meta.id;instr.part
field	nvssSource	NVSS	Name of the original survey image field from which the component was derived.	varchar	8			obs.field
field1	iras_asc	IRAS	object field #1 (magnitude/other)	smallint	2			obs.field
field2	iras_asc	IRAS	object field #2 (magnitude/other)	smallint	2			obs.field
field3	iras_asc	IRAS	object field #3 (size/other)	smallint	2			obs.field
fieldID	ProgrammeFrame	ATLASDR4	UID of position on sky, set just after ProgrammeBuilder runs	int	4		-99999999	meta.bib
fieldID	ProgrammeFrame	ATLASDR5	UID of position on sky, set just after ProgrammeBuilder runs	int	4		-99999999	meta.bib
fieldID	ProgrammeFrame	ATLASv20180209	UID of position on sky, set just after ProgrammeBuilder runs	int	4		-99999999	meta.bib
fieldID	RequiredMergeLogMultiEpoch	ATLASDR3	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredMergeLogMultiEpoch	ATLASDR4	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredMergeLogMultiEpoch	ATLASDR5	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredMergeLogMultiEpoch	ATLASv20160425	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredMergeLogMultiEpoch	ATLASv20180209	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredMergeLogMultiEpoch	VPHASDR3	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredMergeLogMultiEpoch	VPHASv20160112	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredMergeLogMultiEpoch	VPHASv20170222	UID of position on sky. References Required{productType}.fieldID	int	4		-99999999	??
fieldID	RequiredStack	ATLASDR1	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	ATLASDR2	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	ATLASDR3	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	ATLASDR4	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	ATLASDR5	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	ATLASv20131127	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	ATLASv20160425	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	ATLASv20180209	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	VPHASDR3	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	VPHASv20160112	UID of position on sky.	int	4		-99999999	??
fieldID	RequiredStack	VPHASv20170222	UID of position on sky.	int	4		-99999999	??
fieldID	StdFieldInfo	ATLASDR1	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	ATLASDR2	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	ATLASDR3	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	ATLASDR4	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	ATLASDR5	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	ATLASv20131127	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	ATLASv20160425	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	ATLASv20180209	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	VPHASDR3	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	VPHASv20160112	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	StdFieldInfo	VPHASv20170222	The fieldID is a UID identifying each of the 43 standard fields that are observed as part of the calibration observations	int	4			obs.field
fieldID	rosat_bsc, rosat_fsc	ROSAT	identification number of SASS field	varchar	8			obs.field
FieldName	ravedr5Source	RAVE	Center of Observed Field (RA/Dec)	varchar	8			meta.id;meta.file
fieldName	StdFieldInfo	ATLASDR1	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	ATLASDR2	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	ATLASDR3	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	ATLASDR4	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	ATLASDR5	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	ATLASv20131127	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	ATLASv20160425	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	ATLASv20180209	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	VPHASDR3	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	VPHASv20160112	reference name of field	varchar	16		NONE	????
fieldName	StdFieldInfo	VPHASv20170222	reference name of field	varchar	16		NONE	????
fieldName	first08Jul16Source, firstSource, firstSource12Feb16	FIRST	Name of the coadded image containing the source (encodes the position of the field center).	varchar	12			obs.image
fileName	Multiframe	ATLASDR1	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	ATLASDR2	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	ATLASDR3	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	ATLASDR4	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	ATLASDR5	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	ATLASv20131127	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	ATLASv20160425	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	ATLASv20180209	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	VPHASDR3	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	VPHASv20160112	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileName	Multiframe	VPHASv20170222	the filename for the multiframe, eg. server:/path/filename.fit	varchar	256		'NONE'	meta.id;meta.file
fileNameRoot	ExternalProduct	ATLASDR2	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	ATLASDR3	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	ATLASDR4	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	ATLASDR5	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	ATLASv20131127	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	ATLASv20160425	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	ATLASv20180209	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	VPHASDR3	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	VPHASv20160112	File name root of the products	varchar	32
fileNameRoot	ExternalProduct	VPHASv20170222	File name root of the products	varchar	32
fileTimeStamp	Multiframe	ATLASDR1	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	ATLASDR2	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	ATLASDR3	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	ATLASDR4	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	ATLASDR5	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	ATLASv20131127	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	ATLASv20160425	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	ATLASv20180209	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	VPHASDR3	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	VPHASv20160112	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
fileTimeStamp	Multiframe	VPHASv20170222	Time stamp digits (from the original CASU directory name and file time stamp) for enforcing uniqueness	bigint	8		-99999999	??
filter1	RequiredDiffImage	ATLASDR1	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	ATLASDR2	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	ATLASDR3	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	ATLASDR4	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	ATLASDR5	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	ATLASv20131127	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	ATLASv20160425	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	ATLASv20180209	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	VPHASDR3	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	VPHASv20160112	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter1	RequiredDiffImage	VPHASv20170222	UID of OMEGACAM narrow band (primary) filter	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASDR1	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASDR2	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASDR3	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASDR4	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASDR5	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASv20131127	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASv20160425	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	ATLASv20180209	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	VPHASDR3	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	VPHASv20160112	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filter2	RequiredDiffImage	VPHASv20170222	UID of OMEGACAM broad band (reference) filter to be subtracted	tinyint	1			meta.code;instr.filter
filterID	Filter	ATLASDR2	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	ATLASDR4	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	ATLASDR5	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	ATLASv20131127	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	ATLASv20160425	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	ATLASv20180209	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	VPHASDR3	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	VPHASv20160112	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter	VPHASv20170222	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter, FilterSections, RequiredFilters, RequiredStack	ATLASDR1	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Filter, RequiredMergeLogMultiEpoch	ATLASDR3	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z,6=blank)	tinyint	1			meta.code;instr.filter
filterID	Multiframe	ATLASDR1	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	ATLASDR2	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	ATLASDR3	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	ATLASDR4	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	ATLASDR5	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	ATLASv20131127	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	ATLASv20160425	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	ATLASv20180209	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	VPHASDR3	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	VPHASv20160112	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	Multiframe	VPHASv20170222	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z)	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASDR1	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASDR2	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASDR3	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASDR4	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASDR5	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASv20131127	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASv20160425	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	ATLASv20180209	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	VPHASDR3	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	VPHASv20160112	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	MultiframeDetector	VPHASv20170222	UID of combined filter (assigned in OSA: 1=u,2=g,3=r,4=i,5=z) {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	tinyint	1		0	meta.code;instr.filter
filterID	atlasDetection	ATLASDR1	UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	atlasDetection	ATLASDR3	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	atlasDetection	ATLASDR4	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	atlasDetection	ATLASDR5	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	atlasDetection	ATLASv20131127	UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	atlasDetection	ATLASv20160425	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	atlasDetection	ATLASv20180209	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	atlasDetection, atlasDetectionUncorr	ATLASDR2	UID of combined filter (assigned in VSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	vphasDetection	VPHASv20160112	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	vphasDetection	VPHASv20170222	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterID	vphasDetection, vphasDetectionUncorr	VPHASDR3	UID of combined filter (assigned in OSA: 1=Z,2=Y,3=J,4=H,5=Ks,8=blank)	tinyint	1			meta.code;instr.filter
filterName	Multiframe	ATLASDR1	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	ATLASDR2	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	ATLASDR3	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	ATLASDR4	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	ATLASDR5	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	ATLASv20131127	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	ATLASv20160425	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	ATLASv20180209	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	VPHASDR3	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	VPHASv20160112	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterName	Multiframe	VPHASv20170222	VST combined filter name {image primary HDU keyword: HIERARCH ESO INS FILT1 NAME}	varchar	16		'NONE'	??
filterType	Filter	ATLASDR2	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	ATLASDR3	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	ATLASDR4	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	ATLASDR5	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	ATLASv20160425	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	ATLASv20180209	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	VPHASDR3	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	VPHASv20160112	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
filterType	Filter	VPHASv20170222	The type of filter BROAD, NARROW, BROADLIST	varchar	16		NONE
fInt	first08Jul16Source, firstSource, firstSource12Feb16	FIRST	integrated flux densities	real	4	mJy		phot.flux.density;em.radio.750-1500MHz
Fit_Flag_Binney	ravedr5Source	RAVE	See final paragraph 3 (Binney et al. 2014)	int	4			meta.code.qual
Fitmag_I	denisDR3Source	DENIS	Magnitude in I band from PSF fit	float	8	mag
Fitmag_J	denisDR3Source	DENIS	Magnitude in J band from PSF fit	float	8	mag
Fitmag_K	denisDR3Source	DENIS	Magnitude in K band from PSF fit	float	8	mag
FitQuality_Binney	ravedr5Source	RAVE	Given by symbol F in eq 15 of Binney et al. (2014)	real	4			meta.code.qual
FJ	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	2MASS All-Sky PSC J Band flux	real	4	mJy	-999.9
FJ_err	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	2MASS All-Sky PSC J Band 1 sigma error	real	4	mJy	-999.9
FKs	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	2MASS All-Sky PSC Ks Band flux	real	4	mJy	-999.9
FKs_err	glimpse1_hrc, glimpse1_mca, glimpse2_hrc, glimpse2_mca	GLIMPSE	2MASS All-Sky PSC Ks Band 1 sigma error	real	4	mJy	-999.9
Flag_I	denisDR3Source	DENIS	Image and source flag in I band This flag is the concatenation of image and source flags, in hexadecimal format. For the image flag, the first two digits contain: Bit 0 - clouds during observation; Bit 1 - electronic Read-Out problem; Bit 2 - internal temperature problem; Bit 3 - very bright star; Bit 4 - bright star; Bit 5 - stray light; Bit 6 - unknown problem. For the source flag, the last two digits contain: Bit 0 - source might be a dust on mirror; Bit 1 - source is a ghost detection of a bright star; Bit 2 - source is saturated; Bit 3 - source is multiple detect.	varchar	5
Flag_J	denisDR3Source	DENIS	Image and source flag in J band This flag is the concatenation of image and source flags, in hexadecimal format. For the image flag, the first two digits contain: Bit 0 - clouds during observation; Bit 1 - electronic Read-Out problem; Bit 2 - internal temperature problem; Bit 3 - very bright star; Bit 4 - bright star; Bit 5 - stray light; Bit 6 - unknown problem. For the source flag, the last two digits contain: Bit 0 - source might be a dust on mirror; Bit 1 - source is a ghost detection of a bright star; Bit 2 - source is saturated; Bit 3 - source is multiple detect.	varchar	5
Flag_K	denisDR3Source	DENIS	Image and source flag in K band This flag is the concatenation of image and source flags, in hexadecimal format. For the image flag, the first two digits contain: Bit 0 - clouds during observation; Bit 1 - electronic Read-Out problem; Bit 2 - internal temperature problem; Bit 3 - very bright star; Bit 4 - bright star; Bit 5 - stray light; Bit 6 - unknown problem. For the source flag, the last two digits contain: Bit 0 - source might be a dust on mirror; Bit 1 - source is a ghost detection of a bright star; Bit 2 - source is saturated; Bit 3 - source is multiple detect.	varchar	5
Flag_mult	denisDR3Source	DENIS	Multiplicity flag; if set to 1, this flag indicates that the source was detected in two consecutive images, and that the 2 measurements have been combined.	tinyint	1
FLAGS	mgcDetection	MGC	Extraction flags	int	4
flame_flags	gaia_source	GAIADR2	Flags from Apsis-FLAME analysis	bigint	8			meta.code
flatCor	MultiframeDetector	ATLASDR1	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	ATLASDR2	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	ATLASDR3	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	ATLASDR4	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	ATLASDR5	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	ATLASv20131127	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	ATLASv20160425	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	ATLASv20180209	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	VPHASDR3	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	VPHASv20160112	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatCor	MultiframeDetector	VPHASv20170222	Flat correction done {image extension keyword: FLATCOR}	tinyint	1		0
flatID	Multiframe	ATLASDR1	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	ATLASDR2	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	ATLASDR3	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	ATLASDR4	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	ATLASDR5	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	ATLASv20131127	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	ATLASv20160425	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	ATLASv20180209	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	VPHASDR3	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	VPHASv20160112	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flatID	Multiframe	VPHASv20170222	UID of library calibration flatfield frame {image extension keyword: FLATSRC}	bigint	8		-99999999	obs.field
flux_100	iras_psc	IRAS	Averaged non-color corrected 100 micron flux density	real	4	Jansky (1.0E-26 W/m**2/Hz)		phot.flux.density;em.IR.60-100um
flux_12	iras_psc	IRAS	Averaged non-color corrected 12 micron flux density	real	4	Jansky (1.0E-26 W/m**2/Hz)		phot.flux.density;em.IR.8-15um
flux_25	iras_psc	IRAS	Averaged non-color corrected 25 micron flux density	real	4	Jansky (1.0E-26 W/m**2/Hz)		phot.flux.density;em.IR.15-30um
flux_60	iras_psc	IRAS	Averaged non-color corrected 60 micron flux density	real	4	Jansky (1.0E-26 W/m**2/Hz)		phot.flux.density;em.IR.30-60um
fMaj	first08Jul16Source, firstSource, firstSource12Feb16	FIRST	major axes derived from the elliptical Gaussian model for the source before deconvolution.	real	4	arcsec		phys.angSize.smajAxis
fMin	first08Jul16Source, firstSource, firstSource12Feb16	FIRST	minor axes derived from the elliptical Gaussian model for the source before deconvolution.	real	4	arcsec		phys.angSize.sminAxis
focus	twomass_scn	TWOMASS	Focus setting of telescope at beginning of scan.	smallint	2			instr.tel.focalLength
focus	twomass_sixx2_scn	TWOMASS	telescope focus setting	smallint	2
FootPrint_Flag	ravedr5Source	RAVE	1 => in RAVE selection function footprint, 0 => outside footprint	tinyint	1			meta.code.qual
fPA	first08Jul16Source, firstSource, firstSource12Feb16	FIRST	position angle (east of north) derived from the elliptical Gaussian model for the source before deconvolution.	real	4	degrees		pos.posAng
fPeak	first08Jul16Source, firstSource, firstSource12Feb16	FIRST	peak flux densities	real	4	mJy		phot.flux.density;em.radio.750-1500MHz
fQual_100	iras_psc	IRAS	100 micron flux density quality.	smallint	2			meta.code.qual
fQual_12	iras_psc	IRAS	12 micron flux density quality.	smallint	2			meta.code.qual
fQual_25	iras_psc	IRAS	25 micron flux density quality.	smallint	2			meta.code.qual
fQual_60	iras_psc	IRAS	60 micron flux density quality.	smallint	2			meta.code.qual
frac_c	ravedr5Source	RAVE	Fraction of spectrum used [Chemical pipeline] (Note 2)	real	4			stat.value
frame_rotator_object_type	gaia_source	GAIADR2	The type of the source mainly used for frame rotation	int	4			meta.code
frameSetID	atlasMergeLog	ATLASDR1	frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure	bigint	8			obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasMergeLog	ATLASDR2	frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure	bigint	8			obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasMergeLog	ATLASDR3	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasMergeLog	ATLASDR4	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasMergeLog	ATLASDR5	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasMergeLog	ATLASv20131127	frame set ID, unique over the whole VSA via programme ID prefix, assigned by merging procedure	bigint	8			obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasMergeLog	ATLASv20160425	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasMergeLog	ATLASv20180209	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASDR1	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASDR2	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASDR3	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASDR4	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASDR5	UID of the set of frames that this merged source comes from	bigint	8			meta.id
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASv20131127	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASv20160425	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	atlasSource	ATLASv20180209	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	vphasMergeLog	VPHASDR3	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	vphasMergeLog	VPHASv20160112	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	vphasMergeLog	VPHASv20170222	frame set ID, unique over the whole OSA via programme ID prefix, assigned by merging procedure	bigint	8			meta.id;obs.field
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	vphasSource	VPHASDR3	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	vphasSource	VPHASv20160112	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetID	vphasSource	VPHASv20170222	UID of the set of frames that this merged source comes from	bigint	8			meta.bib
			Each merged source in the merged source tables come from a set of individual passband frames (with different filters and/or different epochs of observation). In the WSA, a frame is generally the image provided by one detector (dither-stacked and interlaced as appropriate); hence a frame set comprises a set of individual detector frames in different passbands and/or at different observation epochs. Each frame set is uniquely identified by the attribute frameSetID, and this references a row in the corresponding merge log for the source table (for example, vhsSource.frameSetID references whsMergeLog.frameSetID. The merge log in turn references the full set of image descriptive data held in the tables MultiframeDetector and ultimately Multiframe (these two tables map directly onto the multi-extension FITS file hierarchy of extension FITS headers beneath a single primary HDU FITS header - primary HDU FITS keys will be found in Multiframe, while the corresponding extension FITS keys for each primary set will be found in table MultiframeDetector). In this way, you can trace the provenance of a merged source record right back to the individual image frames from which it is derived.
frameSetTolerance	Programme	ATLASDR1	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	ATLASDR2	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	ATLASDR3	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	ATLASDR4	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	ATLASDR5	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	ATLASv20131127	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	ATLASv20160425	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	ATLASv20180209	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	VPHASDR3	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	VPHASv20160112	The match tolerance for different passband frames	real	4	Degrees		??
frameSetTolerance	Programme	VPHASv20170222	The match tolerance for different passband frames	real	4	Degrees		??
frameType	Multiframe	ATLASDR1	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	ATLASDR2	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	ATLASDR3	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	ATLASDR4	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	ATLASDR5	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	ATLASv20131127	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	ATLASv20160425	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	ATLASv20180209	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	VPHASDR3	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	VPHASv20160112	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
frameType	Multiframe	VPHASv20170222	The type of multiframe (eg. stack|tile|mosaic|difference|calibration|interleaved etc). A multiframe can have a combination of different types.	varchar	64		normal	meta.code.class
			The frame types and their abbreviations are: confidence = "conf" dark = "dark" deep = "deep" difference = "diff" filtered = "filt" flat = "flat" interleaved = "leav" mosaic = "mosaic" sky = "sky" stack = "stack" default value = "normal"
fringeID	Multiframe	ATLASDR1	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	ATLASDR2	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	ATLASDR3	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	ATLASDR4	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	ATLASDR5	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	ATLASv20131127	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	ATLASv20160425	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	ATLASv20180209	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	VPHASDR3	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	VPHASv20160112	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeID	Multiframe	VPHASv20170222	UID of library calibration fringe frame {image extension keyword: DEFRINGE}	bigint	8		-99999999	obs.field
fringeScale	Multiframe	ATLASDR1	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	ATLASDR2	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	ATLASDR3	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	ATLASDR4	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	ATLASDR5	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	ATLASv20131127	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	ATLASv20160425	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	ATLASv20180209	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	VPHASDR3	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	VPHASv20160112	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fringeScale	Multiframe	VPHASv20170222	Fringe frame scale factor {image extension keyword: DEFRINGE}	real	4		-0.9999995e9	??
fromAllSky	twompzPhotoz	TWOMPZ	Is the WISE designation from the wise_allskysc catalogue 0 NO/1 YES	tinyint	1		0
FWHM_IMAGE	mgcDetection	MGC	FWHM assuming a gaussian core	real	4	pixel