G |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
g_flags |
masterDR2 |
SKYMAPPER |
Bitwise OR of Source Extractor flags from g-band measurements in photometry table |
smallint |
2 |
|
|
meta.code |
g_flux |
phot_variable_time_series_g_fov |
GAIADR1 |
G-band flux for each FoV observation |
float |
8 |
electrons/second |
|
phot.flux;em.opt |
g_flux_error |
phot_variable_time_series_g_fov |
GAIADR1 |
Estimated uncertainty on G-band flux for each FoV observation |
float |
8 |
electrons/second |
|
stat.error;phot.flux;em.opt |
g_mag_zero_oint_error |
ext_phot_zero_point |
GAIADR1 |
Uncertainty on G magnitude zero point |
float |
8 |
mag |
|
stat.error;phot.mag;arith.zp;em.opt |
g_mag_zero_point |
ext_phot_zero_point |
GAIADR1 |
G magnitude zero point |
float |
8 |
mag |
|
phot.mag;arith.zp;em.opt |
g_magnitude |
phot_variable_time_series_g_fov |
GAIADR1 |
G-band magnitude for each FoV observation |
float |
8 |
mag |
|
phot.mag;em.opt |
g_nch |
masterDR2 |
SKYMAPPER |
Number of g-band child sources combined into this object_id |
smallint |
2 |
|
|
meta.number |
g_nclip |
masterDR2 |
SKYMAPPER |
Number of g-band observations with magnitudes clipped from the final PSF magnitude estimate |
smallint |
2 |
|
|
meta.number |
g_ngood |
masterDR2 |
SKYMAPPER |
Number of g-band observations used |
smallint |
2 |
|
|
meta.number |
g_nimaflags |
masterDR2 |
SKYMAPPER |
Number of flagged pixels from bad, saturated, and crosstalk pixel masks from g-band measurements in photometry table |
int |
4 |
|
|
meta.code |
g_petro |
masterDR2 |
SKYMAPPER |
Mean g-band Petrosian magnitude |
real |
4 |
mag |
|
phot.mag;stat.mean |
g_psf |
masterDR2 |
SKYMAPPER |
Mean g-band PSF magnitude |
real |
4 |
mag |
|
phot.mag;stat.mean |
g_rchi2var |
masterDR2 |
SKYMAPPER |
Reduced chi-squared for a constant-magnitude model of the g-band PSF magnitude, including clipped sources |
real |
4 |
|
|
stat.fit.chi2 |
g_rp |
gaia_source |
GAIADR2 |
G-RP colour |
real |
4 |
mag |
|
phot.colour |
g_rp |
gaia_source |
GAIAEDR3 |
G-RP colour |
real |
4 |
mag |
|
phot.colour |
g_score |
twomass_xsc |
TWOMASS |
galaxy score: 1(extended) < g_score < 2(point-like). |
real |
4 |
|
|
meta.code |
gaia_avg_cont |
gaiaxwise_matches |
GAIAXWISE |
Mean contaminating relative flux within PSFs when constructing h_offsets for Gaia sources at the local density, magnitude and intrinsic positional uncertainty of the primary source. |
float |
8 |
dimensionless |
|
|
gaia_bp |
gaia_nonmatches, gaiaxwise_matches |
GAIAXWISE |
BP mean magnitude |
float |
8 |
mag |
|
phot.mag;em.op |
gaia_cont_p1 |
gaiaxwise_matches |
GAIAXWISE |
Probability of Gaia source having contaminant of at least 1% relative flux given its separation from its corresponding WISE detection, as given by equation 12 of Wilson & Naylor (2018b, MNRAS, 481, 2148). |
float |
8 |
dimensionless |
|
|
gaia_cont_p10 |
gaiaxwise_matches |
GAIAXWISE |
Probability of Gaia source having contaminant of at least 10% relative flux given its separation from its corresponding WISE detection. |
float |
8 |
dimensionless |
|
|
gaia_dec |
gaia_nonmatches, gaiaxwise_matches |
GAIAXWISE |
Celestial Declination |
float |
8 |
degrees |
|
pos.eq.dec;meta.main |
gaia_designation |
gaia_nonmatches, gaiaxwise_matches |
GAIAXWISE |
Unique source designation |
varchar |
32 |
dimensionless |
|
meta.id;meta.main |
gaia_dr2_dist1 |
masterDR2 |
SKYMAPPER |
Distance on sky to closest Gaia DR2 source |
real |
4 |
arcsec |
|
pos.angDistance |
gaia_dr2_dist2 |
masterDR2 |
SKYMAPPER |
Distance on sky to second-closest Gaia DR2 source |
real |
4 |
arcsec |
|
pos.angDistance |
gaia_dr2_id1 |
masterDR2 |
SKYMAPPER |
Unique identifier (source_id) of closest Gaia DR2 source |
bigint |
8 |
|
|
meta.id.cross |
gaia_dr2_id2 |
masterDR2 |
SKYMAPPER |
Unique identifier (source_id) of second-closest Gaia DR2 source |
bigint |
8 |
|
|
meta.id.cross |
gaia_g |
gaia_nonmatches, gaiaxwise_matches |
GAIAXWISE |
G-band mean magnitude |
float |
8 |
mag |
|
phot.mag;em.op |
gaia_p |
gaia_nonmatches |
GAIAXWISE |
match probability |
float |
8 |
dimensionless |
|
|
gaia_ra |
gaia_nonmatches, gaiaxwise_matches |
GAIAXWISE |
Celestial Right Ascension |
float |
8 |
degrees |
|
pos.eq.ra;meta.main |
gaia_rp |
gaia_nonmatches, gaiaxwise_matches |
GAIAXWISE |
RP mean magnitude |
float |
8 |
mag |
|
phot.mag;em.op |
gaia_source_ID |
gaia_nonmatches, gaiaxwise_matches |
GAIAXWISE |
Gaia integer unique source designation |
bigint |
8 |
dimensionless |
|
|
GAIN_R |
spectra |
SIXDF |
R gain |
real |
4 |
|
|
|
GAIN_V |
spectra |
SIXDF |
V gain |
real |
4 |
|
|
|
gainCor |
MultiframeDetector |
SHARKSv20210222 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
SHARKSv20210421 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
ULTRAVISTADR4 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSDR1 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSDR2 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSDR3 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSDR4 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSDR5 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSDR6 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20120926 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20130417 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20140409 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20150108 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20160114 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20160507 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20170630 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20180419 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20201209 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20231101 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VHSv20240731 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIDEODR2 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIDEODR3 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIDEODR4 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIDEODR5 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIDEOv20100513 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIDEOv20111208 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGDR2 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGDR3 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGDR4 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20110714 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20111019 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20130417 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20140402 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20150421 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20151230 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20160406 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20161202 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VIKINGv20170715 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCDEEPv20230713 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCDEEPv20240506 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCDR1 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCDR2 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCDR3 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCDR4 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCDR5 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20110816 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20110909 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20120126 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20121128 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20130304 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20130805 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20140428 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20140903 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20150309 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20151218 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20160311 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20160822 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20170109 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20170411 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20171101 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20180702 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20181120 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20191212 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20210708 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20230816 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VMCv20240226 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VVVDR1 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VVVDR2 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VVVDR5 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VVVXDR1 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VVVv20100531 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
MultiframeDetector |
VVVv20110718 |
Gain correction factor {image extension keyword: GAINCOR} |
real |
4 |
|
-0.9999995e9 |
|
gainCor |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Gain correction factor |
real |
4 |
|
-0.9999995e9 |
|
gal_contam |
twomass_psc |
TWOMASS |
Extended source "contamination" flag. |
smallint |
2 |
|
|
meta.code |
gal_contam |
twomass_sixx2_psc |
TWOMASS |
src contaminated by galaxy (check blanked/subtracted tbl) |
smallint |
2 |
|
|
|
galactic_lat |
igsl_source |
GAIADR1 |
Galactic latitude |
real |
4 |
degrees |
|
pos.galatic.lat |
galactic_lon |
igsl_source |
GAIADR1 |
Galactic longitude |
real |
4 |
degrees |
|
pos.galatic.lon |
galex_guv_dist |
masterDR2 |
SKYMAPPER |
Distance on sky to closest GALEX GUVcat AIS source |
real |
4 |
arcsec |
|
pos.angDistance |
galex_guv_id |
masterDR2 |
SKYMAPPER |
Unique identifier (objid) of closest GALEX GUVcat AIS source (Bianchi et al. 2017) |
bigint |
8 |
|
|
meta.id.cross |
gApFillFac |
StackObjectAttributes |
PS1DR2 |
Aperture fill factor from g filter stack detection. |
real |
4 |
|
-999 |
|
gApFlux |
StackObjectAttributes |
PS1DR2 |
Aperture flux from g filter stack detection. |
real |
4 |
Janskys |
-999 |
|
gApFluxErr |
StackObjectAttributes |
PS1DR2 |
Error in aperture flux from g filter stack detection. |
real |
4 |
Janskys |
-999 |
|
gApMag |
StackObjectThin |
PS1DR2 |
Aperture magnitude from g filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
gApMagErr |
StackObjectThin |
PS1DR2 |
Error in aperture magnitude from g filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
gApRadius |
StackObjectAttributes |
PS1DR2 |
Aperture radius for g filter stack detection. |
real |
4 |
arcsec |
-999 |
|
gauSig |
sharksDetection |
SHARKSv20210222 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
sharksDetection |
SHARKSv20210421 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
ultravistaDetection, ultravistaMapRemeasurement |
ULTRAVISTADR4 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
ultravistaMapRemeasAver |
ULTRAVISTADR4 |
Averaged RMS of axes of ellipse fit |
real |
4 |
pixels |
|
src.morph.param |
gauSig |
vhsDetection |
VHSDR2 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSDR3 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSDR4 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSDR5 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSDR6 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20120926 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20130417 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20140409 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20150108 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20160114 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20160507 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20170630 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20180419 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20201209 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20231101 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection |
VHSv20240731 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vhsDetection, vhsListRemeasurement |
VHSDR1 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
videoDetection |
VIDEODR2 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
videoDetection |
VIDEODR3 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
videoDetection |
VIDEODR4 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
videoDetection |
VIDEODR5 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
videoDetection |
VIDEOv20100513 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
videoDetection |
VIDEOv20111208 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
videoListRemeasurement |
VIDEOv20100513 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGDR2 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGDR3 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGDR4 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20111019 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20130417 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20140402 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20150421 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20151230 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20160406 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20161202 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection |
VIKINGv20170715 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingDetection, vikingListRemeasurement |
VIKINGv20110714 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vikingMapRemeasAver |
VIKINGZYSELJv20160909 |
Averaged RMS of axes of ellipse fit |
real |
4 |
pixels |
|
src.morph.param |
gauSig |
vikingMapRemeasAver |
VIKINGZYSELJv20170124 |
Averaged RMS of axes of ellipse fit |
real |
4 |
pixels |
|
src.morph.param |
gauSig |
vikingMapRemeasurement |
VIKINGZYSELJv20160909 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
vikingMapRemeasurement |
VIKINGZYSELJv20170124 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
Derived from the maximum and minimum spatial RMS of the object profile along any direction, ie. 0.5*(A_IMAGE² + B_IMAGE²)½ |
gauSig |
vmcDetection |
VMCDR1 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCDR2 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCDR3 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCDR4 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCDR5 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20110909 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20120126 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20121128 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20130304 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20130805 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20140428 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20140903 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20150309 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20151218 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20160311 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20160822 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20170109 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20170411 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20171101 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20180702 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20181120 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20191212 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20210708 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20230816 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection |
VMCv20240226 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcDetection, vmcListRemeasurement |
VMCv20110816 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcdeepDetection |
VMCDEEPv20230713 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vmcdeepDetection |
VMCDEEPv20240506 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vvvDetection |
VVVDR1 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vvvDetection |
VVVDR2 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vvvDetection, vvvDetectionPawPrints, vvvDetectionTiles |
VVVDR5 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
gauSig |
vvvDetection, vvvListRemeasurement |
VVVv20100531 |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
src.morph.param |
These are derived from the three general intensity-weighted second moments. The equivalence between them and a generalised elliptical Gaussian Distribution is used to derive Gaussian sigma = (σa²+σb²)½ |
Gauss_frac_1 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_frac_2 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_frac_3 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_mean_1 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_mean_2 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_mean_3 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_sigma_1 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_sigma_2 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
Gauss_sigma_3 |
ravedr5Source |
RAVE |
Property of multi-Gaussian distance modulus fit, see Section 9, eq. 5 |
real |
4 |
|
|
stat.fit.param |
GB |
target |
SIXDF |
galactic latitude |
float |
8 |
degrees |
|
|
gbJ2000 |
vvvVivaCatalogue |
VVVDR5 |
Galactic latitude {catalogue TType keyword: gbJ2000} |
float |
8 |
Degrees |
-999999500.0 |
pos.galactic.lat |
gcnf |
twomass_sixx2_psc, twomass_sixx2_xsc |
TWOMASS |
Group confusion flag 0=not confused or single apparation, 1=confused |
smallint |
2 |
|
|
|
gcntr |
twomass_sixx2_psc, twomass_sixx2_xsc |
TWOMASS |
A unique identifier for the merged group of apparitions of this source |
int |
4 |
|
|
|
gcvsID |
ogle3LpvLmcSource, ogle3LpvSmcSource |
OGLE |
GCVS ID |
varchar |
5 |
|
|
meta.id |
gdec |
StackObjectThin |
PS1DR2 |
Declination from g filter stack detection. |
float |
8 |
degrees |
-999 |
|
gdecErr |
StackObjectThin |
PS1DR2 |
Declination error from g filter stack detection. |
real |
4 |
arcsec |
-999 |
|
gEpoch |
StackObjectThin |
PS1DR2 |
Modified Julian Date of the mean epoch of images contributing to the the g-band stack (equinox J2000). |
float |
8 |
days |
-999 |
|
gerr |
decapsSource |
DECAPS |
Uncertainty in mean g-band flux (statistical only) {catalogue TType keyword: err[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.error;phot.flux;em.opt.B |
gerr |
smashdr2_deep, smashdr2_object |
SMASH |
Unceratinty in calibrated g-band magnitude |
real |
4 |
|
|
|
gerr_lbs |
decapsSource |
DECAPS |
Uncertainty in mean local background subtracted g-band flux (statistical only) {catalogue TType keyword: err_lbs[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.error;phot.flux;em.opt.B |
gexpTime |
StackObjectAttributes |
PS1DR2 |
Exposure time of the g filter stack. Necessary for converting listed fluxes and magnitudes back to measured ADU counts. |
real |
4 |
seconds |
-999 |
|
gExtNSigma |
StackObjectAttributes |
PS1DR2 |
An extendedness measure for the g filter stack detection based on the deviation between PSF and Kron (1980) magnitudes, normalized by the PSF magnitude uncertainty. |
real |
4 |
|
-999 |
|
gFlags |
MeanObject |
PS1DR2 |
Information flag bitmask for mean object from g filter detections. Values listed in ObjectFilterFlags. |
int |
4 |
|
0 |
|
gfracflux |
decapsSource |
DECAPS |
PSF-weighted fraction of g-band flux coming from this object (i.e., one minus the the fraction of flux in this object's PSF that comes from neighbouring objects?) {catalogue TType keyword: fracflux[1]} |
real |
4 |
|
-9.999995e8 |
stat.value;em.opt.B |
ginfoFlag |
StackObjectThin |
PS1DR2 |
Information flag bitmask indicating details of the g filter stack photometry. Values listed in DetectionFlags. |
bigint |
8 |
|
0 |
|
ginfoFlag2 |
StackObjectThin |
PS1DR2 |
Information flag bitmask indicating details of the g filter stack photometry. Values listed in DetectionFlags2. |
int |
4 |
|
0 |
|
ginfoFlag3 |
StackObjectThin |
PS1DR2 |
Information flag bitmask indicating details of the g filter stack photometry. Values listed in DetectionFlags3. |
int |
4 |
|
0 |
|
gippDetectID |
StackObjectAttributes, StackObjectThin |
PS1DR2 |
IPP internal detection identifier. |
bigint |
8 |
|
|
|
gKronFlux |
StackObjectAttributes |
PS1DR2 |
Kron (1980) flux from g filter stack detection. |
real |
4 |
Janskys |
-999 |
|
gKronFluxErr |
StackObjectAttributes |
PS1DR2 |
Error in Kron (1980) flux from g filter stack detection. |
real |
4 |
Janskys |
-999 |
|
gKronMag |
StackObjectThin |
PS1DR2 |
Kron (1980) magnitude from g filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
gKronMagErr |
StackObjectThin |
PS1DR2 |
Error in Kron (1980) magnitude from g filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
gKronRad |
StackObjectAttributes |
PS1DR2 |
Kron (1980) radius from g filter stack detection. |
real |
4 |
arcsec |
-999 |
|
GL |
target |
SIXDF |
galactic longitude |
float |
8 |
degrees |
|
|
Glat |
ravedr5Source |
RAVE |
Latitude (J2000 GCS) |
float |
8 |
deg |
|
pos.galactic.lat |
glat |
allwise_sc |
WISE |
Galactic latitude computed from the non-moving source fit equatorial position. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
deg |
|
|
glat |
catwise_2020, catwise_prelim |
WISE |
galactic latitude |
float |
8 |
deg |
|
|
glat |
masterDR2 |
SKYMAPPER |
Galactic latitude derived from ICRS coordinates. Not to be used as primary astrometric reference. |
real |
4 |
deg |
|
pos.galactic.lat |
glat |
smashdr2_deep, smashdr2_object |
SMASH |
Galactic latitude of field, in degrees |
float |
8 |
|
|
|
glat |
smashdr2_source |
SMASH |
Galactic latitude of field |
float |
8 |
degrees |
|
|
glat |
twomass_psc |
TWOMASS |
Galactic latitude rounded to 0.001 deg. |
real |
4 |
degrees |
|
pos.galactic.lat |
glat |
twomass_scn |
TWOMASS |
Galactic latitude of scan center, as computed from ra and dec above. |
real |
4 |
degrees |
|
pos.galactic.lat |
glat |
twomass_sixx2_scn |
TWOMASS |
galactic latitude (decimal deg) of scan center |
float |
8 |
deg |
|
|
glat |
twomass_xsc |
TWOMASS |
Galactic latitude (decimal deg) based on peak pixel. |
real |
4 |
degrees |
|
pos.galactic.lat |
glat |
wise_allskysc |
WISE |
Galactic latitude. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
degrees |
|
|
glat |
wise_prelimsc |
WISE |
Galactic latitude. CAUTION: This coordinate should not be used as an astrometric reference |
float |
8 |
degrees |
|
|
glJ2000 |
vvvVivaCatalogue |
VVVDR5 |
Galactic longitude {catalogue TType keyword: glJ2000} |
float |
8 |
Degrees |
-999999500.0 |
pos.galactic.lon |
globalSourceID |
sage_lmcIracSource, sage_lmcMips160Source, sage_lmcMips24Source, sage_lmcMips70Source |
SPITZER |
Unique identifier |
int |
4 |
|
|
|
globalSourceID |
sage_smcIRACv1_5Source |
SPITZER |
Unique identification number of each source in the catalog |
int |
4 |
|
|
|
Glon |
ravedr5Source |
RAVE |
Longitude (J2000 GCS) |
float |
8 |
deg |
|
pos.galactic.lon |
glon |
allwise_sc |
WISE |
Galactic longitude, computed from the non-moving source fit equatorial position. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
deg |
|
|
glon |
catwise_2020, catwise_prelim |
WISE |
galactic longitude |
float |
8 |
deg |
|
|
glon |
masterDR2 |
SKYMAPPER |
Galactic longitude derived from ICRS coordinates. Not to be used as primary astrometric reference. |
real |
4 |
deg |
|
pos.galactic.lon |
glon |
smashdr2_deep, smashdr2_object |
SMASH |
Galactic longitude of field, in degrees |
float |
8 |
|
|
|
glon |
smashdr2_source |
SMASH |
Galactic longitude of field |
float |
8 |
degrees |
|
|
glon |
twomass_psc |
TWOMASS |
Galactic longitude rounded to 0.001 deg. |
real |
4 |
degrees |
|
pos.galactic.lon |
glon |
twomass_scn |
TWOMASS |
Galactic longitude of scan center, as computed from ra and dec above. |
real |
4 |
degrees |
|
pos.galactic.lon |
glon |
twomass_sixx2_scn |
TWOMASS |
galactic longitude (decimal deg) of scan center |
float |
8 |
deg |
|
|
glon |
twomass_xsc |
TWOMASS |
Galactic longitude (decimal deg) based on peak pixel. |
real |
4 |
degrees |
|
pos.galactic.lon |
glon |
wise_allskysc |
WISE |
Galactic longitude. CAUTION: This coordinate should not be used as an astrometric reference. |
float |
8 |
degrees |
|
|
glon |
wise_prelimsc |
WISE |
Galactic longitude. CAUTION: This coordinate should not be used as an astrometric reference |
float |
8 |
degrees |
|
|
gmag |
smashdr2_deep, smashdr2_object |
SMASH |
Weighted-average, calibrated g-band magnitude, 99.99 if no detection |
real |
4 |
|
|
|
gmaglimit |
decapsSource |
DECAPS |
5 sigma g-band magnitude limit for deepest detection of this object (AB mag) {catalogue TType keyword: maglimit[1]} |
real |
4 |
mag |
-9.999995e8 |
phot.mag;em.opt.B |
gmean |
decapsSource |
DECAPS |
g-band mean flux, good detections only (3631 Jy) {catalogue TType keyword: mean[1]} |
real |
4 |
3631Jy |
|
phot.flux;em.opt.B |
gmean_lbs |
decapsSource |
DECAPS |
Mean g-band flux, using a local background subtraction (3631 Jy) {catalogue TType keyword: mean_lbs[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.mean;phot.flux;em.opt.B |
gMeanApMag |
MeanObject |
PS1DR2 |
Mean aperture magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanApMagErr |
MeanObject |
PS1DR2 |
Error in mean aperture magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanApMagNpt |
MeanObject |
PS1DR2 |
Number of measurements included in mean aperture magnitude from g filter detections. |
smallint |
2 |
|
-999 |
|
gMeanApMagStd |
MeanObject |
PS1DR2 |
Standard deviation of aperture magnitudes from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanKronMag |
MeanObject |
PS1DR2 |
Mean Kron (1980) magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanKronMagErr |
MeanObject |
PS1DR2 |
Error in mean Kron (1980) magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanKronMagNpt |
MeanObject |
PS1DR2 |
Number of measurements included in mean Kron (1980) magnitude from g filter detections. |
smallint |
2 |
|
-999 |
|
gMeanKronMagStd |
MeanObject |
PS1DR2 |
Standard deviation of Kron (1980) magnitudes from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanPSFMag |
MeanObject |
PS1DR2 |
Mean PSF magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanPSFMagErr |
MeanObject |
PS1DR2 |
Error in mean PSF magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanPSFMagMax |
MeanObject |
PS1DR2 |
Maximum PSF magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanPSFMagMin |
MeanObject |
PS1DR2 |
Minimum PSF magnitude from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gMeanPSFMagNpt |
MeanObject |
PS1DR2 |
Number of measurements included in mean PSF magnitude from g filter detections. |
smallint |
2 |
|
-999 |
|
gMeanPSFMagStd |
MeanObject |
PS1DR2 |
Standard deviation of PSF magnitudes from g filter detections. |
real |
4 |
AB magnitudes |
-999 |
|
gmedian |
decapsSource |
DECAPS |
Median g-band flux (3631 Jy) {catalogue TType keyword: median[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.median;phot.flux;em.opt.B |
gmedian_lbs |
decapsSource |
DECAPS |
Median local background subtracted g-band flux (3631 Jy) {catalogue TType keyword: median_lbs[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.median;phot.flux;em.opt.B |
gmomentR1 |
StackObjectAttributes |
PS1DR2 |
First radial moment for g filter stack detection. |
real |
4 |
arcsec |
-999 |
|
gmomentRH |
StackObjectAttributes |
PS1DR2 |
Half radial moment (r^0.5 weighting) for g filter stack detection. |
real |
4 |
arcsec^0.5 |
-999 |
|
gmomentXX |
StackObjectAttributes |
PS1DR2 |
Second moment M_xx for g filter stack detection. |
real |
4 |
arcsec^2 |
-999 |
|
gmomentXY |
StackObjectAttributes |
PS1DR2 |
Second moment M_xy for g filter stack detection. |
real |
4 |
arcsec^2 |
-999 |
|
gmomentYY |
StackObjectAttributes |
PS1DR2 |
Second moment M_yy for g filter stack detection. |
real |
4 |
arcsec^2 |
-999 |
|
gnFrames |
StackObjectThin |
PS1DR2 |
Number of input frames/exposures contributing to the g filter stack detection. |
int |
4 |
|
-999 |
|
gnmag |
decapsSource |
DECAPS |
Number of detections in g band {catalogue TType keyword: nmag[1]} |
smallint |
2 |
|
|
meta.number;em.opt.B |
gnmag_lbs |
decapsSource |
DECAPS |
Number of detections in g band {catalogue TType keyword: nmag_lbs[1]} |
smallint |
2 |
|
-9999 |
meta.number;em.opt.B |
gnmag_lbs_ok |
decapsSource |
DECAPS |
Number of good detections in g band {catalogue TType keyword: nmag_lbs_ok[1]} |
smallint |
2 |
|
-9999 |
meta.number;em.opt.B |
gnmag_ok |
decapsSource |
DECAPS |
Number of good detections in g band {catalogue TType keyword: nmag_ok[1]} |
smallint |
2 |
|
|
meta.number;em.opt.B |
gPlateScale |
StackObjectAttributes |
PS1DR2 |
Local plate scale for the g filter stack. |
real |
4 |
arcsec/pixel |
0 |
|
gpmag_APASSDR9 |
ravedr5Source |
RAVE |
g' magnitude from APASSDR9 |
real |
4 |
mag |
|
phot.mag;em.opt |
gpsfChiSq |
StackObjectAttributes |
PS1DR2 |
Reduced chi squared value of the PSF model fit for g filter stack detection. |
real |
4 |
|
-999 |
|
gpsfCore |
StackObjectAttributes |
PS1DR2 |
PSF core parameter k from g filter stack detection, where F = F0 / (1 + k r^2 + r^3.33). |
real |
4 |
|
-999 |
|
gPSFFlux |
StackObjectAttributes |
PS1DR2 |
PSF flux from g filter stack detection. |
real |
4 |
Janskys |
-999 |
|
gPSFFluxErr |
StackObjectAttributes |
PS1DR2 |
Error in PSF flux from g filter stack detection. |
real |
4 |
Janskys |
-999 |
|
gpsfLikelihood |
StackObjectAttributes |
PS1DR2 |
Likelihood that this g filter stack detection is best fit by a PSF. |
real |
4 |
|
-999 |
|
gPSFMag |
StackObjectThin |
PS1DR2 |
PSF magnitude from g filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
gPSFMagErr |
StackObjectThin |
PS1DR2 |
Error in PSF magnitude from g filter stack detection. |
real |
4 |
AB magnitudes |
-999 |
|
gpsfMajorFWHM |
StackObjectAttributes |
PS1DR2 |
PSF major axis FWHM from g filter stack detection. |
real |
4 |
arcsec |
-999 |
|
gpsfMinorFWHM |
StackObjectAttributes |
PS1DR2 |
PSF minor axis FWHM from g filter stack detection. |
real |
4 |
arcsec |
-999 |
|
gpsfQf |
StackObjectAttributes |
PS1DR2 |
PSF coverage factor for g filter stack detection. |
real |
4 |
|
-999 |
|
gpsfQfPerfect |
StackObjectAttributes |
PS1DR2 |
PSF-weighted fraction of pixels totally unmasked for g filter stack detection. |
real |
4 |
|
-999 |
|
gpsfTheta |
StackObjectAttributes |
PS1DR2 |
PSF major axis orientation from g filter stack detection. |
real |
4 |
degrees |
-999 |
|
gq25 |
decapsSource |
DECAPS |
25th percentile g-band flux (3631 Jy) {catalogue TType keyword: q25[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.value;phot.flux;em.opt.B |
gq25_lbs |
decapsSource |
DECAPS |
25th percentile local background subtracted g-band flux (3631 Jy) {catalogue TType keyword: q25_lbs[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.value;phot.flux;em.opt.B |
gq75 |
decapsSource |
DECAPS |
75th percentile g-band flux (3631 Jy) {catalogue TType keyword: q75[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.value;phot.flux;em.opt.B |
gq75_lbs |
decapsSource |
DECAPS |
75th percentile local background subtracted g-band flux (3631 Jy) {catalogue TType keyword: q75_lbs[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.value;phot.flux;em.opt.B |
gQfPerfect |
MeanObject |
PS1DR2 |
Maximum PSF weighted fraction of pixels totally unmasked from g filter detections. |
real |
4 |
|
-999 |
|
gra |
StackObjectThin |
PS1DR2 |
Right ascension from g filter stack detection. |
float |
8 |
degrees |
-999 |
|
graErr |
StackObjectThin |
PS1DR2 |
Right ascension error from g filter stack detection. |
real |
4 |
arcsec |
-999 |
|
GRATBLAZ_R |
spectra |
SIXDF |
R blaze direction |
varchar |
10 |
|
|
|
GRATBLAZ_V |
spectra |
SIXDF |
V blaze direction |
varchar |
10 |
|
|
|
GRATID_R |
spectra |
SIXDF |
grating ID in R frame |
varchar |
14 |
|
|
|
GRATID_V |
spectra |
SIXDF |
grating ID in V frame |
varchar |
14 |
|
|
|
GRATSET_R |
spectra |
SIXDF |
R grating micrometer setting |
real |
4 |
|
|
|
GRATSET_V |
spectra |
SIXDF |
V grating micrometer setting |
real |
4 |
|
|
|
GRATSLOT_R |
spectra |
SIXDF |
R grating slot ID |
char |
1 |
|
|
|
GRATSLOT_V |
spectra |
SIXDF |
V grating slot ID |
char |
1 |
|
|
|
groutedFlag |
MultiframeDetector |
SHARKSv20210222 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
SHARKSv20210421 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
ULTRAVISTADR4 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSDR1 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSDR2 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSDR3 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSDR4 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSDR5 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSDR6 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20120926 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20130417 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20140409 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20150108 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20160114 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20160507 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20170630 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20180419 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20201209 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20231101 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VHSv20240731 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIDEODR2 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIDEODR3 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIDEODR4 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIDEODR5 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIDEOv20111208 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGDR2 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGDR3 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGDR4 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20110714 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20111019 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20130417 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20140402 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20150421 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20151230 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20160406 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20161202 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VIKINGv20170715 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCDEEPv20230713 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCDEEPv20240506 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCDR1 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCDR2 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCDR3 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCDR4 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCDR5 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20110816 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20110909 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20120126 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20121128 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20130304 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20130805 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20140428 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20140903 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20150309 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20151218 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20160311 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20160822 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20170109 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20170411 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20171101 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20180702 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20181120 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20191212 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20210708 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20230816 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VMCv20240226 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VVVDR1 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VVVDR2 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VVVDR5 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VVVXDR1 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
MultiframeDetector |
VVVv20110718 |
Table has been grouted {catalogue extension keyword: GROUTED} |
tinyint |
1 |
|
0 |
|
groutedFlag |
sharksMultiframeDetector, ultravistaMultiframeDetector, vhsMultiframeDetector, videoMultiframeDetector, vikingMultiframeDetector, vmcMultiframeDetector, vvvMultiframeDetector |
VSAQC |
Table has been grouted |
tinyint |
1 |
|
0 |
|
grpNum |
Multiframe |
SHARKSv20210222 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
SHARKSv20210421 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
ULTRAVISTADR4 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSDR1 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSDR2 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSDR3 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSDR4 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSDR5 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSDR6 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20120926 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20130417 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20140409 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20150108 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20160114 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20160507 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20170630 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20180419 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20201209 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20231101 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VHSv20240731 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIDEODR2 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIDEODR3 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIDEODR4 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIDEODR5 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIDEOv20100513 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIDEOv20111208 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGDR2 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGDR3 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGDR4 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20110714 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20111019 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20130417 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20140402 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20150421 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20151230 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20160406 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20161202 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VIKINGv20170715 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCDEEPv20230713 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCDEEPv20240506 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCDR1 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCDR2 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCDR3 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCDR4 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCDR5 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20110816 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20110909 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20120126 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20121128 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20130304 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20130805 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20140428 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20140903 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20150309 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20151218 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20160311 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20160822 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20170109 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20170411 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20171101 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20180702 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20181120 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20191212 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20210708 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20230816 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VMCv20240226 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VVVDR1 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VVVDR2 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VVVDR5 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VVVXDR1 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VVVv20100531 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
Multiframe |
VVVv20110718 |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) {image primary HDU keyword: JITTRNUM} |
int |
4 |
|
-99999999 |
|
grpNum |
sharksMultiframe, ultravistaMultiframe, vhsMultiframe, videoMultiframe, vikingMultiframe, vmcMultiframe, vvvMultiframe |
VSAQC |
Value of 1st OBSNUM in jitter sequence (i.e. group number applied to all members) |
int |
4 |
|
-99999999 |
|
gsc2Class |
first08Jul16Source |
FIRST |
morphological classification in GSC-2 version 2.3.2 (s=stellar, g=nonstellar/galaxy) |
varchar |
1 |
|
|
|
gsc2Mag |
first08Jul16Source |
FIRST |
GSC2 F magnitude |
real |
4 |
mag |
|
|
gsc2Matches |
first08Jul16Source |
FIRST |
number of matches within a fiducial radius (10 arcsec) with GSC-2 version 2.3.2 |
int |
4 |
|
|
|
gsc2Sep |
first08Jul16Source |
FIRST |
separation of the nearest match in GSC-2 version 2.3.2 from the FIRST position |
real |
4 |
arcsec |
|
|
gscatter |
smashdr2_deep, smashdr2_object |
SMASH |
RMS scatter in g from multiple measurements of this object |
real |
4 |
|
|
|
gsky |
StackObjectAttributes |
PS1DR2 |
Residual background sky level at the g filter stack detection. |
real |
4 |
Janskys/arcsec^2 |
-999 |
|
gskyErr |
StackObjectAttributes |
PS1DR2 |
Error in residual background sky level at the g filter stack detection. |
real |
4 |
Janskys/arcsec^2 |
-999 |
|
gsMag |
combo17CDFSSource |
COMBO17 |
Absolute restframe magnitude in SDSS g (calculated from redshifted best_fit template, depending on redshift and filter extrapolation outside the COMBO-17 filter set can be necessary, only calculated for objects classified as galaxies) |
real |
4 |
mag |
|
|
gstackDetectID |
StackObjectAttributes, StackObjectThin |
PS1DR2 |
Unique stack detection identifier. |
bigint |
8 |
|
|
|
gstackImageID |
StackObjectAttributes, StackObjectThin |
PS1DR2 |
Unique stack identifier for g filter detection. |
bigint |
8 |
|
|
|
gstdev |
decapsSource |
DECAPS |
Standard deviation in g-band flux; may be default in rare cases of objects with 1 measurement {catalogue TType keyword: stdev[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.stdev;phot.flux;em.opt.B |
gstdev_lbs |
decapsSource |
DECAPS |
Standard deviation in local background subtracted g-band fluxes; may be default in rare cases of objects with 1 measurement {catalogue TType keyword: stdev_lbs[1]} |
real |
4 |
3631Jy |
-9.999995e8 |
stat.stdev;phot.flux;em.opt.B |
gxPos |
StackObjectAttributes |
PS1DR2 |
PSF x center location from g filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
gxPosErr |
StackObjectAttributes |
PS1DR2 |
Error in PSF x center location from g filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
gyPos |
StackObjectAttributes |
PS1DR2 |
PSF y center location from g filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
gyPosErr |
StackObjectAttributes |
PS1DR2 |
Error in PSF y center location from g filter stack detection. |
real |
4 |
sky pixels |
-999 |
|
gzp |
StackObjectAttributes |
PS1DR2 |
Photometric zeropoint for the g filter stack. Necessary for converting listed fluxes and magnitudes back to measured ADU counts. |
real |
4 |
magnitudes |
0 |
|