|
parameter
|
unit
|
description
|
|
name
|
|
RESOLVE galaxy identifier
|
|
RAdeg
|
deg
|
Right Ascension of photometric center in decimal degrees
|
|
DEdeg
|
deg
|
Declination of photometric center in decimal degrees
|
|
cz
|
km/s
|
Local group corrected velocity of galaxy
|
|
Grpcz
|
km/s
|
Velocity of group center, adopted galaxy velocity for survey membership
|
|
absrMag
|
mag
|
Absolute SDSS r-band magnitude (foreground extinction included)
|
|
umag
|
mag
|
Apparent SDSS u-band magnitude (provided without foreground extinction corrections)
|
|
e_umag
|
mag
|
Error in umag
|
|
gmag
|
mag
|
Apparent SDSS g-band magnitude (provided without foreground extinction corrections)
|
|
e_gmag
|
mag
|
Error in gmag
|
|
rmag
|
mag
|
Apparent SDSS r-band magnitude (provided without foreground extinction corrections)
|
|
e_rmag
|
mag
|
Error in rmag
|
|
imag
|
mag
|
Apparent SDSS i-band magnitude (provided without foreground extinction corrections)
|
|
e_imag
|
mag
|
Error in imag
|
|
zmag
|
mag
|
Apparent SDSS z-band magnitude (provided without foreground extinction corrections)
|
|
e_zmag
|
mag
|
Error in zmag
|
|
NUVmag
|
mag
|
Apparent GALEX NUV-band magnitude (*provided with foreground extinction corrections, unlike published table -- this will be corrected in DR2*; to get nuvmag without foreground extinction, compute NUVmag+extnuv)
|
|
e_NUVmag
|
mag
|
Error in NUVmag
|
|
uvm2mag
|
mag
|
Apparent Swift uvm2-band magnitude (provided without foreground extinction corrections)
|
|
e_uvm2mag
|
mag
|
Error in uvm2mag
|
|
2Jmag
|
mag
|
Apparent 2MASS J-band magnitude (provided without foreground extinction corrections)
|
|
e_2Jmag
|
mag
|
Error in 2Jmag
|
|
2Hmag
|
mag
|
Apparent 2MASS H-band magnitude (provided without foreground extinction corrections)
|
|
e_2Hmag
|
mag
|
Error in 2Hmag
|
|
2Kmag
|
mag
|
Apparent 2MASS K-band magnitude (provided without foreground extinction corrections)
|
|
e_2Kmag
|
mag
|
Error in 2Kmag
|
|
UYmag
|
mag
|
Apparent UKIDSS Y-band magnitude (provided without foreground extinction corrections)
|
|
e_UYmag
|
mag
|
Error in UYmag
|
|
UHmag
|
mag
|
Apparent UKIDSS H-band magnitude (provided without foreground extinction corrections)
|
|
e_UHmag
|
mag
|
Error in UHmag
|
|
UKmag
|
mag
|
Apparent UKIDSS K-band magnitude (provided without foreground extinction corrections)
|
|
e_UKmag
|
mag
|
Error in UKmag
|
|
b_a
|
|
axial ratio b/a
|
|
R50
|
arcsec
|
The half-light radius in r band
|
|
R90
|
arcsec
|
The 90%-light radius in r band
|
|
dgr
|
mag
|
The (g-r) color gradient
|
|
modelu_r
|
mag
|
SED modeled (u-r) color (foreground corrections and k-corrections implicity included)
|
|
modelu_i
|
mag
|
SED modeled (u-i) color (foreground corrections and k-corrections implicity included)
|
|
modelu_j
|
mag
|
SED modeled (u-J) color (foreground corrections and k-corrections implicity included)
|
|
modelu_k
|
mag
|
SED modeled (u-K) color (foreground corrections and k-corrections implicity included)
|
|
modelg_r
|
mag
|
SED modeled (g-r) color (foreground corrections and k-corrections implicity included)
|
|
modelg_i
|
mag
|
SED modeled (g-i) color (foreground corrections and k-corrections implicity included)
|
|
modelg_J
|
mag
|
SED modeled (g-J) color (foreground corrections and k-corrections implicity included)
|
|
modelg_K
|
mag
|
SED modeled (g-K) color (foreground corrections and k-corrections implicity included)
|
|
logMstar
|
log(Msun)
|
Log stellar mass
|
|
extu
|
mag
|
Foreground extinction in u band
|
|
extg
|
mag
|
Foreground extinction in r band
|
|
extr
|
mag
|
Foreground extinction in r band
|
|
exti
|
mag
|
Foreground extinction in i band
|
|
extz
|
mag
|
Foreground extinction in z band
|
|
extnuv
|
mag
|
Foreground extinction in NUV band
|
|
extuvm2
|
mag
|
Foreground extinction in uvm2 band
|
|
exty
|
mag
|
Foreground extinction in Y band
|
|
extj
|
mag
|
Foreground extinction in J band
|
|
exth
|
mag
|
Foreground extinction in H band
|
|
extk
|
mag
|
Foreground extinction in K band
|
|
FL_insample
|
|
Flag for galaxies brighter than -17.33 (A-semester) or -17.0 (B-semester) within Grpcz boundaries as used in Eckert et al. 2015
|