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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.

(a)

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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