| Column | Description |
|---|
| pgc | PGC number |
| Name | Common name |
| Inc | Measured inclination from face on |
| eI | Uncertainty in inclination |
| Vh | Heliocentric velocity from HI measurement |
| 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 |
| g | SDSS g band total AB magnitude |
| r | SDSS r band total AB magnitude |
| i | SDSS i band total AB magnitude |
| z | SDSS z band total AB magnitude |
| W1 | WISE W1 (3.4 micron) band total AB magnitude |
| W2 | WISE W2 (4.6 micron) band total AB magnitude |
| b/aS | Axial ratio of semi-major to semi-minor axes of elliptical aperture used for photometry with SDSS images |
| b/aW | Axial ratio of semi-major to semi-minor axes of elliptical aperture used for photometry with WISE images |
| aeu | Half light radius in u band |
| aeg | Half light radius in g band |
| aer | Half light radius in r band |
| aei | Half light radius in i band |
| aez | Half light radius in z band |
| aeW1 | Half light radius in W1 band |
| aeW2 | Half light radius in W2 band |
| u_bka | SDSS u band total AB magnitude, mc=mtotal-Ab-Ak-Aa, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuration) |
| g_bka | SDSS g band total AB magnitude, mc=mtotal-Ab-Ak-Aa, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuration) |
| r_bka | SDSS r band total AB magnitude, mc=mtotal-Ab-Ak-Aa, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuration) |
| i_bka | SDSS i band total AB magnitude, mc=mtotal-Ab-Ak-Aa, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuration) |
| z_bka | SDSS z band total AB magnitude, mc=mtotal-Ab-Ak-Aa, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuration) |
| W1_bka | WISE W1 band total AB magnitude, mc=mtotal-Ab-Ak-Aa, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuration) |
| W2_bka | Wise W2 band total AB magnitude, mc=mtotal-Ab-Ak-Aa, corrected for Milky Way obscuration, redshift k-correction, and aperture effect (not host obscuration) |
| Aiu | u band dust attenuation in host |
| eAu | Uncertainty in u band dust attenuation in host |
| Aig | g band dust attenuation in host |
| eAg | Uncertainty in g band dust attenuation in host |
| Air | r band dust attenuation in host |
| eAr | Uncertainty in r band dust attenuation in host |
| Aii | i band dust attenuation in host |
| eAi | Uncertainty in i band dust attenuation in host |
| Aiz | z band dust attenuation in host |
| eAz | Uncertainty in z band dust attenuation in host |
| AiW1 | W1 band dust attenuation in host |
| eAW1 | Uncertainty in W1 band dust attenuation in host |
| AiW2 | W2 band dust attenuation in host |
| eAW2 | Uncertainty in W2 band dust attenuation in host |
| u_bkai | SDSS u band total AB magnitude, mc=mtotal-Ab-Ak-Aa-Ai, corrected for Milky Way obscuration, redshift k-correction, aperture effect, and host obscuration |
| g_bkai | SDSS g band total AB magnitude, mc=mtotal-Ab-Ak-Aa-A-, corrected for Milky Way obscuration, redshift k-correction, aperture effect, and host obscuration |
| r_bkai | SDSS r band total AB magnitude, mc=mtotal-Ab-Ak-Aa-Ai, corrected for Milky Way obscuration, redshift k-correction, aperture effect, and host obscuration |
| i_bkai | SDSS i band total AB magnitude, mc=mtotal-Ab-Ak-Aa-Ai, corrected for Milky Way obscuration, redshift k-correction, aperture effect, and host obscuration |
| z_bkai | SDSS z band total AB magnitude, mc=mtotal-Ab-Ak-Aa-Ai, corrected for Milky Way obscuration, redshift k-correction, aperture effect, and host obscuration |
| W1_bkai | WISE W1 band total AB magnitude, mc=mtotal-Ab-Ak-Aa-Ai, corrected for Milky Way obscuration, redshift k-correction, aperture effect, and host obscuration |
| W2_bkai | Wise W2 band total AB magnitude, mc=mtotal-Ab-Ak-Aa-Ai, corrected for Milky Way obscuration, redshift k-correction, aperture effect, and host obscuration |
| pW2 | Predicted value for dust corrected W2-band magnitude |
| Gu | u band host dust attenuation factor |
| Gg | g band host dust attenuation factor |
| Gr | r band host dust attenuation factor |
| Gi | i band host dust attenuation factor |
| Gz | z band host dust attenuation factor |
| GW1 | W1 band host dust attenuation factor |
| GW2 | W2 band host dust attenuation factor |
| pGu | Predicted u band host dust attenuation factor |
| pGg | Predicted g band host dust attenuation factor |
| pGr | Predicted r band host dust attenuation factor |
| pGi | Predicted i band host dust attenuation factor |
| pGz | Predicted z band host dust attenuation factor |
| pGW1 | Predicted W1 band host dust attenuation factor |
| pGW2 | Predicted W2 band host dust attenuation factor |
| pAu | Predicted u band extinction of host |
| pAg | Predicted g band extinction of host |
| pAr | Predicted r band extinction of host |
| pAi | Predicted i band extinction of host |
| pAz | Predicted z band extinction of host |
| pAW1 | Predicted W1 band extinction of host |
| pAW2 | Predicted W2 band extinction of host |
| P1W2 | Principal component, calculated at W2 band, Equation 4 |
| eP1W2 | Uncertainty in Principal component, calculated at W2 band |
| P1pW2 | Principal component, predicted at W2 band |
| P1W1 | Principal component, calculated at W1 band |
| S | Quality flag, SDSS images; range best=5 to worst=0 |
| W | Quality flag, WISE images; range best=5 to worst=0 |
| So | Source of attenuation parameter: 0=predicted W2, 1=observed W1, 2=W2 through attenuation formulation of sect. 2.2.2 |