Column information for the table: FP: SDSS Distances
Table Description: "The Sloan Digital Sky Survey Peculiar Velocity Catalogue", C. Howlett, K. Said, J.R. Lucey, M. Colless, F. Qin, Y, Lai, R.B. Tully, 2022, MNRAS, 515, 953
ColumnDescription
pgc PGC number
Dc75 Preferred galaxy luminosity distance assuming H0=75 km/s/Mpc from multiple FP fits as function of group richness
DMc75 Preferred luminosity distance modulus H0=75 km/s/Mpc from multiple FP fits as function of group richness
Dc100 Preferred galaxy luminosity distance assuming H0=100 km/s/Mpc from multiple FP fits as function of group richness
DMc100 Prefered luminosity distance modulus H0=100 km/s/Mpc from multiple FP fits as function of group richness
eDMc Uncertainty in preferred distance modulus from multiple FP fits as function of group richness
DM100 Luminosity distance modulus H0=100 km/s/Mpc from a single fit to full sample
eDM Uncertainty in distance modulus from a single fit to full sample
logDc Preferred: Mean log distance ratio from multiple FP fits as function of group richness
elogDc Standard deviation in log distance ratio, multiple FP fits
skewc Alpha parameter of skew-normal pdf, multiple FP fits
logD Mean log distance ratio from a single fit to full sample
elogD Standard deviation in log distance ratio, single fit
skew Alpha parameter of skew-normal pdf, single FP fit
czh Heliocentric velocity
eczh Error in heliocentric velocity
czcmb Velocity in CMB frame
gczcmb Velocity in CMB frame of Tempel+17 group
Nest Nest ID from 2MASS group catalog of Tully 2015
1PGC PGC ID of dominant galaxy in Nest
IDt17 Group ID in Tempel+17 SDSS DR10 group catalog
Ngt17 Number of galaxies in Tempel+17 group
J2000 RA & dec J2000 in hours, min, sec, °, min, sec
Ra Right ascension J2000 in degrees
Dec Declination J2000 in degrees
glon Galactic longitude
glat Galactic latitude
sgl Supergalactic longitude
sgb Supergalactic latitude
gmag SDSS g magnitude, de Vaucouleurs fit
egmag Error on SDSS g magnitude
rmag SDSS r magnitude, de Vaucouleurs fit
ermag Error on SDSS r magnitude
rad r-band angular radius, de vaucouleurs fit
erad Error on r-band angular radius, de vaucouleurs fit
boa r-band axial ratio, de Vaucouleurs fit
eboa Error in r-band axial ratio, de Vaucouleurs fit
Exg Milky Way extinction in g band from Schlafly & Finkbeiner (2011)
Exr Milky Way extinction in r band from Schlafly & Finkbeiner (2011)
kcg k-correction at g band from Chilingarian 2014 using g-r colors
kcr k-correction at r band from Chilingarian 2014 using g-r colors
Mr Absolute magnitude, accounting for k-correction, evolution, and Galactic extinction
sig Velocity dispersion from Portsmouth catalog (Thomas+13)
esig Error on velocity dispersion from Portsmouth catalog (Thomas+13)
M Galaxy morphology: 0=unclear; 1=spiral; 2=elliptical (Tempel+14)
In 1: in SDSS_NYU VAGC DR7 footprint; 0: outside footprint
Bar_N Number density at galay location per (Mpc/h)^3
r r=log R_e where R_e is the intrinsic effective radius in kpc/h derived from the angular effective radius: rad
er Uncertainty in r
i i=log I_e where I_e is the mean surface brightness within the angular effective radius (see Eq 8 & 9 in Said+20) in L_sun/pc^2
ei Uncertainty in s
s s=log sigma_0 where sigma_0 is the central velocity dispersion in km/s
es Uncertainty in i
Sn Weight given galaxy in fundamental plane fit
objid SDSS objid
specid SDSS specid
plate SDSS spectroscopic plate number