G |
Name | Schema Table | Database | Description | Type | Length | Unit | Default Value | Unified Content Descriptor |
g_score |
twomass_xsc |
2MASS |
galaxy score: 1(extended) < g_score < 2(point-like). |
real |
4 |
|
|
CODE_MISC |
gain |
MultiframeDetector |
WSA |
Detector gain {image extension keyword: GAIN} |
real |
4 |
electrons/ADU |
-0.9999995e9 |
?? |
gal_contam |
twomass_psc |
2MASS |
Extended source "contamination" flag. |
smallint |
2 |
|
|
CODE_MISC |
galGrad |
Plate |
SSA |
Gradient of galaxy instrumental mag scale |
float |
8 |
mags per instrumental mag |
|
FIT_PARAM_VALUE |
galZp |
Plate |
SSA |
Zeropoint of galaxy instrumental scale |
float |
8 |
mag |
|
PHOT_ZPT |
gauSig |
calDetection, commDetection, dxsDetection, dxsListRemeasurement, gcsDetection, gcsListRemeasurement, gpsDetection, gpsListRemeasurement, lasDetection, lasListRemeasurement, udsDetection, udsListRemeasurement |
WSA |
RMS of axes of ellipse fit {catalogue TType keyword: Gaussian_sigma} |
real |
4 |
pixels |
|
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 = (σ_a²+σ_b²)^{1/2} |
gCorMagB |
Source |
SSA |
B band magnitude assuming object is galaxy |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_BJ |
gCorMagI |
Source |
SSA |
I band magnitude assuming object is galaxy |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_I |
gCorMagR1 |
Source |
SSA |
R1 band magnitude assuming object is galaxy |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_R |
gCorMagR2 |
Source |
SSA |
R2 band magnitude assuming object is galaxy |
real |
4 |
mag |
-99.999995 |
PHOT_PHG_R |
getCal1 |
Plate |
SSA |
1st profile calibration polynomial coefficient |
float |
8 |
|
|
FIT_PARAM_VALUE |
getCal2 |
Plate |
SSA |
2nd profile calibration polynomial coefficient |
float |
8 |
|
|
FIT_PARAM_VALUE |
getCal3 |
Plate |
SSA |
3rd profile calibration polynomial coefficient |
float |
8 |
|
|
FIT_PARAM_VALUE |
getCal4 |
Plate |
SSA |
4th profile calibration polynomial coefficient |
float |
8 |
|
|
FIT_PARAM_VALUE |
getCal5 |
Plate |
SSA |
5th profile calibration polynomial coefficient |
float |
8 |
|
|
FIT_PARAM_VALUE |
getCal6 |
Plate |
SSA |
6th profile calibration polynomial coefficient |
float |
8 |
|
|
FIT_PARAM_VALUE |
glat |
twomass_psc |
2MASS |
Galactic latitude rounded to 0.001 deg. |
real |
4 |
degrees |
|
POS_GAL_LAT |
glat |
twomass_scn |
2MASS |
Galactic latitude of scan center, as computed from ra and dec above. |
real |
4 |
degrees |
|
POS_GAL_LAT |
glat |
twomass_xsc |
2MASS |
Galactic latitude (decimal deg) based on peak pixel. |
real |
4 |
degrees |
|
POS_GAL_LAT |
glon |
twomass_psc |
2MASS |
Galactic longitude rounded to 0.001 deg. |
real |
4 |
degrees |
|
POS_GAL_LON |
glon |
twomass_scn |
2MASS |
Galactic longitude of scan center, as computed from ra and dec above. |
real |
4 |
degrees |
|
POS_GAL_LON |
glon |
twomass_xsc |
2MASS |
Galactic longitude (decimal deg) based on peak pixel. |
real |
4 |
degrees |
|
POS_GAL_LON |
gMag |
Detection |
SSA |
Magnitude calculated on assumption object is galaxy |
real |
4 |
mag |
|
MODEL_MAG_VALUE |
gradient |
Plate |
SSA |
Gradient of linear portion of profile cal. curve |
real |
4 |
|
|
FIT_PARAM_VALUE |
grpMem |
Multiframe |
WSA |
Group membership (0=F, 1=T) {image primary HDU keyword: GRPMEM} |
tinyint |
1 |
|
0 |
CODE_MEM |
grpNum |
Multiframe |
WSA |
Group number applied to all members {image primary HDU keyword: GRPNUM} |
int |
4 |
|
-99999999 |
NUMBER |
gsDec |
Multiframe |
WSA |
Declination of guide star {image primary HDU keyword: GSDEC} |
float |
8 |
degrees |
-0.9999995e9 |
POS_EQ_DEC_MAIN |
gsRa |
Multiframe |
WSA |
Right ascension of guide star {image primary HDU keyword: GSRA} |
float |
8 |
hours |
-0.9999995e9 |
POS_EQ_RA_MAIN |
guiding |
Multiframe |
WSA |
Guider status (OFF|ON|PAUSED) {image primary HDU keyword: GUIDING} |
varchar |
10 |
|
NONE |
|