Table B.3
Overview of literature data for dwarf galaxies used for the SFR calibrations presented in this paper.
| Source | D L a | Ref | FUV | MIPS 24 μm/IRAS 25 μm | log SFR |
| [Mpc] | [mJy] | [mJy] | [log M⊙ yr-1] | ||
|
|
|||||
| NGC 4713 | 19.9 | 1 | 13.308 ± 1.972 | 186.5 ± 50.4 | –0.13 |
| NGC 4490 | 8.7 | 1 | 10.248 ±1.518 | 1394.8 ± 55.9 | −0.45 |
| NGC 1156 | 7.1 | 1 | 23.307 ± 3.453 | 447.1 ± 18.0 | –0.74 |
| NGC 4299 | 18.7 | 1 | 8.996 ± 1.333 | 210.4 ± 8.5 | –0.28 |
| NGC 693 | 23.4 | 1 | 0.973 ± 0.144 | 550.0 ± 50.0 | –0.08 |
| NGC 814 | 24.1 | 1 | 0.321 ± 0.048 | 897.2 ± 62.8 | 0.14 |
| NGC 4294 | 17 | 1 | 5.249 ± 0.778 | 192.5 ± 57.8 | –0.52 |
| VCC 1326 | 17 | 1 | 0.290 ± 0.043 | 418.4 ± 54.4 | –0.49 |
| NGC 4522 | 17 | 1 | 2.766 ± 0.410 | 211.2 ± 48.6 | –0.62 |
| NGC 6821 | 25.1 | 1 | 6.920 ± 1.025 | 307.4 ± 46.1 | –0.02 |
Notes. The dwarf galaxies from the Dwarf Galaxy Survey are also part of the literature sample but they are not repeated here as they correspond to the sources in Table B.1. The first, second, and third columns specify the name of the source, luminosity distance, and reference to the literature work, respectively. The subsequent columns provide the GALEX FUV and MIPS 24 μm or IRAS 25 μm flux densities and star formation rates which are estimated from the GALEX FUV and MIPS 24 μm/IRAS 25 μm measurements and the calibrations presented in Hao et al. (2011) and Kennicutt et al. (2009), respectively.
Distances for galaxies with redshifts z< 0.01 are obtained from the Nearby Galaxies Catalog (Tully 1988), if available, while for other galaxies distances are derived from the redshifts reported on NED. For Virgo cluster galaxies, we retrieve distances from the Goldmine database (Gavazzi et al. 2003), based on results reported in Gavazzi et al. (1999). For galaxies with redshifts z ≥ 0.01, the luminosity distances are calculated for a spatially flat cosmology with H0 = 67.3 km s-1 Mpc-1, Ωλ = 0.685 and Ωm = 0.315 (Planck Collaboration 2014).
Reference. (1) Brauher et al. (2008).
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