Table 1
Near-infrared and optical luminosities and morphologies of CIG galaxies.
| CIG | fKs | log (LK) | Code | log (LB) | Morpho. |
| Jy | [LK, ⊙ ] | [L⊙] | RC3 | ||
|
|
|||||
| 1 | 0.0548 ± 0.0020 | 11.227 ± 0.016 | 1 | 10.57 | 5.0 ± 1.5 |
| 2 | 0.0087 ± 0.0010 | 10.407 ± 0.050 | 1 | 9.84 | 6.0 ± 1.5 |
| 3 | 0.00539 ± 0.00053 | − | −1 | − | 4.0 ± 1.5 |
| 4 | 0.2855 ± 0.0021 | 10.9777 ± 0.0032 | 1 | 10.28 | 3.0 ± 1.5 |
| 5 | 0.01320 ± 0.00043 | 10.686 ± 0.014 | 1 | 9.95 | 0.0 ± 1.5 |
| 6 | 0.0129 ± 0.0013 | 10.205 ± 0.042 | 1 | 9.80 | 7.0 ± 1.5 |
| 7 | 0.0197 ± 0.0012 | 11.270 ± 0.027 | 1 | 10.35 | 4.0 ± 1.5 |
| ... | ... | ... | ... | ... | ... |
Notes. AMIGA sample (n = 1050). Units: log (LK) given in units of Ks-band solar luminosity (LK, ⊙ = 5.0735 × 1025 W); log (LB) given in units of solar bolometric luminosity (L⊙ = 3.842 × 1026 W); 1 Jy = 10-26 W m-2 Hz-1. Code for the infrared luminosity: − 1 if the galaxy does not have distance data; 0 if the galaxy does not have NIR data; 1 if the galaxy has NIR data and distance; 2 if there are 2 NIR sources for the galaxy, the brightest one is selected (see text). log (LB) and morphology data from Fernández Lorenzo et al. (2012).
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