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glossary for RESOLVE DR2 searchable online database

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 without foreground extinction corrections)
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
hitelescope Telescope used for observation (GBT = Green Bank 100m; AO = Arecibo 300m; ALFALFA = Arecibo Legacy Fast ALFA Survey (Arecibo 300m); S05-AO = Springob et al. (2005) catalog (Arecibo 300m); S05-GB300 = Springob et al. (2005) catalog (Green Bank 300ft) )
F21 Jy.km/s Total 21cm flux (use MHI = 2.36x10^5 (D/[Mpc])^2 *(F/[Jy.km/s]) to obtain masses in logMsun)
e_F21 Jy.km/s Uncertainty on total 21cm flux
rms_hi mJy rms noise of spectrum assuming 10 km/s channels
limflagmhi Flag indicating upper limit on F21 (0 = detection; 1=upper limit)
confused Flag indicating 21cm emission likely confused (0 = not confused; 1 = confused)
F21corr Jy.km/s Total 21cm flux after correction for confusion (use MHI = 2.36x10^5 (D/[Mpc])^2 *(F/[Jy.km/s]) to obtain masses in Msun)
e_F21corr_rand Jy.km/s Statistical uncertainty on total 21cm flux after correction for confusion
e_F21corr_sys Jy.km/s Additional systematic uncertainty on total 21cm flux after correction for confusion
deconf_mode Method used to correct 21cm flux for confusion and determine the additional systematic uncertainty (see Section 2.3.2 of Stark et al. (2016))
groupid_s Group dark matter halo mass, stellar-mass limited sample (By definition, all members of a group have the same values for each of the environment metrics.)
groupmass_s [solMass] Group dark matter halo mass, stellar-mass limited sample
groupid_b Group dark matter halo ID, baryonic mass-limited sample (By definition, all members of a group have the same values for each of the environment metrics.)
groupmass_b [solMass] Group dark matter halo mass, baryonic mass-limited sample
dens_s [solMass]/Mpc^2 Large-scale structure density, stellar mass-limited sample groups, uncorrected for edge-effects
dens_corr_s [solMass]/Mpc^2 Large-scale structure density, stellar mass-limited sample groups, corrected for edge-effects
dens_b [solMass]/Mpc^2 Large-scale structure density, baryonic mass-limited sample groups, uncorrected for edge-effects
dens_b_corr [solMass]/Mpc^2 Large-scale structure density, baryonic mass-limited sample groups, uncorrected for edge-effects
dist_s Projected distance to nearest M_h>10^12 halo, stellar mass-limited sample groups (Distances to nearest halo with mass > 10^12 Msun and heliocentric velocity separation <500 km/s are given relative to the virial radius of the nearest Mh>10^12 group, e.g., if a Mh=10^11 Msun halo lies at the virial radius of a Mh=10^12.5 Msun halo, dist_s = 1; Values only calculated for Mh<10^12 Msun groups)
f_dist_s Reliability Flag for dist_s (Flag=1 indicates that the corresponding distance may be unreliable due to proximity to survey boundary.)
dist_b Projected distance to nearest M_h>10^12 halo, baryonic mass-limited sample groups (Distances to nearest halo with mass > 10^12 Msun and heliocentric velocity separation <500 km/s are given relative to the virial radius of the nearest Mh>10^12 group, e.g., if a Mh=10^11 Msun halo lies at the virial radius of a Mh=10^12.5 Msun halo, dist_s = 1; Values only calculated for Mh<10^12 Msun groups)
f_dist_b Reliability Flag for dist_b (Flag=1 indicates that the corresponding distance may be unreliable due to proximity to survey boundary.)
f_s16sample_s Flag to select stellar mass-limited sample from Stark et al. (2016) (1 = in S16 stellar mass-limited sample)
f_s16sample_b Flag to select baryonic mass-limited sample from Stark et al. (2016) (1 = in S16 baryonic mass-limited sample)