Table 1
Sample overview.
| Galaxy | D | Incl | log10 ( ) |
log10 ( ) |
R 1/2 | Comment | Reference |
| (Mpc) | (°) | (L⊙) | (L⊙) | (kpc) | |||
|
|
|||||||
| UGC 8508 | 2.6 | 68 | 6.954 | 0.623 | 1, 2 | ||
| CVnIdwA | 3.6 | 49 | 7.199 | 1.784 | 1, 2 | ||
| NGC 3741 | 3.23 | 70 | 7.453 | 0.341 | 3 | ||
| WLM | 1.0 | 74 | 7.522 | 1.334 | 1, 2 | ||
| DDO 154 | 3.7 | 68 | 7.628 | 3.511 | 1, 2 | ||
| DDO 126 | 4.9 | 62 | 7.880 | 1.771 | 1, 2 | ||
| DDO 87 | 7.4 | 43 | 8.121 | 3.363 | 1, 2 | ||
| UGCA 442 | 4.37 | 64 | 8.150 | 1.906 | 3 | ||
| DDO 168 | 4.3 | 47 | 8.168 | 1.562 | 1, 2 | ||
| DDO 52 | 10.3 | 55 | 8.300 | 2.278 | 1, 2 | ||
| NGC 3109 | 1.37 | 70 | 8.314 | 2.700 | 3 | ||
| NGC 2366 | 3.4 | 65 | 8.548 | 2.899 | 1, 2 | ||
| UGC 7603 | 6.85 | 78 | 8.902 | 1.239 | 3 | ||
|
|
|||||||
| DC14 only | |||||||
|
|
|||||||
| IC 2574 | 3.89 | 51 | 9.352 | 4.352 | 4 | ||
| NGC 2976 | 3.63 | 54 | 9.516 | 1.505 | 4 | ||
| M33 | 0.84 | 55 | 9.690∗ | 3.325 | 5 | ||
| NGC 2403 | 3.18 | 55 | 10.074 | 8.846 | 2.215 | 4 | |
| NGC 3621 | 6.73 | 62 | 10.536 | 4.471 | 4 | ||
| NGC 3198 | 13.37 | 72 | 10.520 | 9.569 | 5.209 | 4 | |
| NGC 5055 | 9.04 | 51 | 11.096 | 10.182 | 4.100 | 4 | |
|
|
|||||||
| Problematic galaxies | |||||||
|
|
|||||||
| UGC 8490 | 4.76 | 50 | 9.028 | 1.167 | a | 3 | |
| NGC 7793 | 3.58 | 43 | 9.874 | 1.836 | b | 4 | |
| NGC 925 | 8.91 | 50 | 10.168 | 11.407 | c | 4 | |
| NGC 3521 | 14.2 | 69 | 11.472 | 4.514 | d | 4 | |
Notes. Columns 1–3 represent the galaxy name and distance and an indicative inclination. Columns 4–5 give the integrated 3.6 μm luminosity of the disk and bulge (if present). Column 6 gives the stellar half-light radius. Comments on the quality and data references are given in Cols. 7, 8.
Reference. (1) Little THINGS (Iorio et al. 2017); (2) Little THINGS (Oh et al. 2015); (3) SPARC (Lelli et al. 2016); (4) THINGS (de Blok et al. 2008); (5) Corbelli et al. (2014). Comments: (a) potential starburst; (b) uncertain inclination for outer disk; (c) extended bar; and (d) poorly constrained distance. * For M33 Col. 4 gives the stellar mass from Corbelli et al. (2014) (in M⊙) instead of the 3.6 μm luminosity.
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