Column | Description |
pgc | PGC number |
Name | Common name |
Wmx | HI linewidth |
eW | Uncertainty in HI linewidth |
lgWmxi | Log inclination corrected HI linewidth |
elgWi | Uncertainty in log inclination corrected HI linewidth |
m21 | HI 21cm magnitude; m21=-2.5log(F_HI_)+17.4 |
em21 | Uncertainty in HI 21cm magnitude |
u | SDSS u band total AB magnitude; uncertainty ~0.05 mag |
g | SDSS g band total AB magnitude; uncertainty <0.05 mag |
r | SDSS r band total AB magnitude; uncertainty <0.05 mag |
i | SDSS i band total AB magnitude; uncertainty <0.05 mag |
z | SDSS z band total AB magnitude; uncertainty <0.05 mag |
W1 | WISE W1 (3.4 micron) band total AB magnitude; uncertainty <0.05 mag |
W2 | WISE W2 (4.6 micron) band total AB magnitude; uncertainty <0.05 mag |
Inc | Inclination angle from face-on; blank if <45 degrees |
eI | Uncertainty in inclination |
aeW2 | Half light radius in W2 band |
C82 | Concentration index; C82=5log(a80/a20) where a80 and a20 are semi-major axis radii enclosing 80% and 20% of total light at W2 band |
b/a | Axial ratio of semi-major to semi-minor axes of elliptical aperture used for photometry in W1 band |
u_bka | SDSS u band total AB magnitude, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuratin) |
g_bka | SDSS g band total AB magnitude, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuratin) |
r_bka | SDSS r band total AB magnitude, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuratin) |
i_bka | SDSS i band total AB magnitude, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuratin) |
z_bka | SDSS z band total AB magnitude, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuratin) |
W1_bka | WISE W1 band total AB magnitude, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuratin) |
W2_bka | Wise W2 band total AB magnitude, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuratin) |