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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).

(a)

Distances and oxygen abundances are adopted from Madden et al. (2013).

(b)

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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