UGR NameName of the source in UGR catalog
BZK NameName of the source in local BZK catalog
DRG NameName of the source in local DRG catalog
SMG NameName of the source in local SMG catalog
RAJ2000 coordinates
DecJ2000 coordinates
Obj. TypeE.g. 'GAL', 'QSO', 'STAR', etc.
Ph. RedshiftPhotometric redshift. '-1'=not observed '-2'=observation inconclusive.
Em. RedshiftRedshift obtained from emission features. '-1'=not observed '-2'=observation inconclusive.
Abs. RedshiftRedshift obtained from absorption features '-1'=not observed '-2'=observation inconclusive.
Sys. RedshiftSystemic redshift estimated from emission and/or absorption features.
SMG RedshiftRedshift obtained by Chapman et al. (2005)
Redshift Uncert.Whether or not redshift is uncertain.
CscalePhysical transverse size (in kpc) of 1" at this redshift. Assumes standard cosmology (h=.7, OmM=0.3, OmL=0.7, OmK=0.)
UMagU-band magnitude (AB)
BMagB-band magnitude (Vega)
GMagG-band magnitude (AB)
RMagR-band magnitude (AB)
ZMagz-band magnitude (Vega)
JMagJ-band magnitude (Vega)
KMagK-band magnitude (Vega).
U-G colorUMag-GMag
G-R colorGMag-RMag
R-J colorRMag-JMag
R-K colorRMag-KMag
3.6 µIRAC 3.6 micron magnitude (AB).
4.5 µIRAC 4.5 micron magnitude (AB).
5.8 µIRAC 5.8 micron magnitude (AB).
8.0 µIRAC 8.0 micron magnitude (AB).
24 µMIPS 24 micron flux (micro-Jy).
L1600Luminosity at 1600 Angstroms (units of 10^11 Lsun).
L5to8micron5-8.5 micron luminosity (units of 10^11 Lsun).
log(LFIR/L1600)Log ratio of IR to UV luminosity.
LBolBolometric luminosity (units of Lsun).
Threshhold nNumber n of sigma above background used for pixel selection (varies with redshift).
SizeMorphological size parameter (kpc^2).
GiniMorphological gini parameter.
MultiplicityMorphological multiplicity parameter.
Color disp.Morphological color dispersion parameter.
SED fitType of Salpeter SED fit: CSF (constant SFR), or decaying (TAUXX, XX is timescale in Myr).
EBminVE(B-V) excess using Salpeter IMF and constant SF.
AgeAge (in Myr) using Salpeter IMF and constant SF.
SEDSFRStar-formation rate (Msun/yr) derived from SED fit using Salpeter IMF and constant SF.
Stellar MassStellar mass (Msun) using Salpeter IMF and constant SF.