Table B.1
Overview of DGS sources used in the SFR calibrations presented in this paper.
| Source | D a | 12 +log (O/H)a | FUV | MIPS 24 μmb | SFR |
| [Mpc] | [mJy] | [mJy] | [M⊙ yr-1] | ||
|
|
|||||
| I Zw 18* | 18.2 | 7.14 | 1.482 ± 0.220 | 6.1 ± 0.3* | 0.057 ± 0.021 |
| SBS 0335-052* | 56.0 | 7.25 | 0.805 ± 0.119 | 76.8 ± 3.2* | 0.890 ± 0.313 |
| HS 0822+3542 | 11.0 | 7.32 | 0.166 ± 0.025 | 3.2 ± 0.3* | 0.0031 ± 0.0011 |
| UGC 4483 | 3.2 | 7.46 | 1.011 ± 0.150 | 10.1 ± 0.5* | 0.0014 ± 0.0005 |
| [1.762 ± 0.261] | |||||
| Tol 1214-277* | 120.5 | 7.52 | 0.188 ± 0.028 | 6.8 ± 0.3* | 0.543 ± 0.194 |
| SBS 1415+437* | 13.6 | 7.55 | 1.124 ± 0.167 | 16.8 ± 1.7 | 0.030 ± 0.011 |
| SBS 1211+540 | 19.3 | 7.58 | 0.198 ± 0.029 | 3.3 ± 0.3* | 0.011 ± 0.004 |
| HS 1442+4250 | 14.4 | 7.60 | 0.590 ± 0.087 | 6.6 ± 0.3* | 0.016 ± 0.006 |
| [1.145 ± 0.170] | |||||
| VII Zw 403* | 4.5 | 7.66 | 2.485 ± 0.368 | 24.9 ± 2.4 | 0.007 ± 0.002 |
| SBS 1249+493 | 110.8 | 7.68 | 0.088 ± 0.013 | 4.3 ± 0.3* | 0.251 ± 0.089 |
| NGC 2366* | 3.2 | 7.70 | 8.627 ± 1.278 | 483.7 ± 13.3 | 0.022 ± 0.008 |
| UM 461* | 13.2 | 7.73 | 0.483 ± 0.072 | 34.4 ± 3.2* | 0.024 ± 0.009 |
| Mrk 209* | 5.8 | 7.74 | 1.920 ± 0.284 | 40.1 ± 2.3 | 0.010 ± 0.004 |
| UM 133* | 22.7 | 7.82 | 0.560 ± 0.083 | 9.4 ± 0.5* | 0.043± 0.016 |
| [0.978 ± 0.145] | |||||
| NGC 4861* | 7.5 | 7.89 | 7.911 ± 1.172 | 262.7 ± 10.0 | 0.085 ± 0.030 |
| NGC 6822-Hubble V* | 0.5 | 7.96 | 7.619 ± 1.129 | 970.6 ± 18.1 | 0.0008 ± 0.0003 |
| NGC 1569* | 3.1 | 8.02 | 179.284 ± 26.562 | 6709.9 ± 154.4 | 0.348 ± 0.124 |
| Mrk 930* | 77.8 | 8.03 | 1.100 ± 0.163 | 152.4 ± 5.6 | 3.095 ± 1.085 |
| HS 0052+2536* | 191.0 | 8.04 | 0.262 ± 0.039 | 20.7 ± 1.2* | 2.963 ± 1.045 |
| Mrk 1089* | 56.6 | 8.10 | 3.509 ± 0.520 | 391.4 ± 7.6 | 4.436 ± 1.558 |
| NGC 4449* | 4.2 | 8.20 | 73.385 ± 8.379 | 1967.1 ± 19.7 | 0.226 ± 0.080 |
| NGC 625* | 3.9 | 8.22 | 6.253 ± 0.926 | 717.1 ± 16.6 | 0.038 ± 0.013 |
| II Zw 40* | 12.1 | 8.23 | 20.374 ± 3.018 | 1361.3 ± 54.4 | 0.831 ± 0.294 |
| Haro 2* | 21.7 | 8.23 | 2.888 ± 0.428 | 663.3 ± 12.8 | 0.954 ± 0.334 |
| NGC 4214* | 2.9 | 8.26 | 34.892 ± 5.169 | 1495.7 ± 29.1 | 0.063 ± 0.023 |
| NGC 1705* | 5.1 | 8.27 | 12.768 ± 1.892 | 43.9 ± 0.9 | 0.038 ± 0.014 |
| Haro 3* | 19.3 | 8.28 | 3.794 ± 0.562 | 714.7 ± 25.3 | 0.840 ± 0.294 |
| UM 448* | 87.8 | 8.32 | 1.890 ± 0.280 | 522.5 ± 18.2 | 11.994 ± 4.193 |
| UM 311* | 23.5 | 8.36 | 1.422 ± 0.211 | 145.2 ± 6.5 | 0.291 ± 0.102 |
| Haro 11* | 92.1 | 8.36 | 2.398 ± 0.355 | 1854.4 ± 96.3 | 43.010 ± 15.022 |
| NGC 1140* | 20.0 | 8.38 | 5.923 ± 0.877 | 271.0 ± 9.1 | 0.530 ± 0.189 |
| HS 2352+2733 | 116.7 | 8.40 | 0.044 ± 0.007 | 2.6 ± 0.3* | 0.155 ± 0.055 |
Notes. Different galaxies are ordered in increasing order of oxygen abundance. The first, second, and third columns specify the name of the source, distance, and oxygen abundance, respectively. Galaxies from the complete galaxy sample (i.e., with FIR line detections for [Cii], [Oi]63, and [Oiii]88) are indicated with an asterisk behind their name. GALEX FUV and MIPS 24 μm photometry results are presented in Cols. 4 and 5. The last column gives the SFR, as estimated from the GALEX FUV and MIPS 24 μm measurements and the calibrations presented in Hao et al. (2011) and Kennicutt et al. (2009).
Distances and oxygen abundances are adopted from Madden et al. (2013).
MIPS 24 μm flux densities with an asterisk correspond to total galaxy fluxes and were retrieved from Bendo et al. (2012b).
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