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Table 5:

S FR values (in units of $M_{\odot }$ yr-1) derived for each galaxy using different luminosities and calibrations.

Galaxy 		FUV U B H$\alpha $ FIR 15 $\mu $m 60 $\mu $m 1.4 GHz Assumed
  S07 Eq. (15) G84 Eq. (14) K98 K98 R01 C92 C02 S FR
HCG 31 4.0 $\pm$ 0.3 2.8 0.59 2.5 4.1 $\pm$ 0.4 3.3 $\pm$ 0.3 1.2 $\pm$ 0.2 2.8 $\pm$ 0.2 2.5 $\pm$ 0.2 3.1
'' AC (NGC 1741) 2.02 $\pm$ 0.12 1.5 0.27 1.2 2.88 $\pm$ 0.18 ... ... ... 1.98 $\pm$ 0.03 2.0
'' B 0.89 $\pm$ 0.07 0.68 0.14 0.67 0.24 $\pm$ 0.02 ... ... ... 0.19 $\pm$ 0.03 0.62
'' E 0.122 $\pm$ 0.009 0.073 0.009 0.057 0.118 $\pm$ 0.013 ... ... ... ... 0.10
'' F 0.123 $\pm$ 0.013 0.12 0.012 0.071 0.40 $\pm$ 0.03 ... ... ... ... 0.20
'' G (Mkn 1090) 0.83 $\pm$ 0.05 0.81 0.16 0.77 0.51 $\pm$ 0.03 ... ... ... 0.30 $\pm$ 0.04 0.49
'' H 0.011 $\pm$ 0.004 ... ... ... 0.004 $\pm$ 0.001 ... ... ... ... 0.008
Mkn 1087 ... 12.1 3.27 11.8 5.6 $\pm$ 0.4 10.3 $\pm$ 1.1 4.6 $\pm$ 1.3 8.8 $\pm$ 1.0 4.5 $\pm$ 0.2 6.3
'' N ... ... 0.076 0.39 0.180 $\pm$ 0.015 ... ... ... ... 0.12
Haro 15 6.8 $\pm$ 0.4 4.6 1.00 4.1 3.3 $\pm$ 0.4 2.8 $\pm$ 0.3 3.2 $\pm$ 0.9 2.4 $\pm$ 0.2 4.0 $\pm$ 0.2 3.6
Mkn 1199 ... 3.7 0.84 3.5 3.9 $\pm$ 0.6 5.2 $\pm$ 0.3 3.0 $\pm$ 0.3 4.7 $\pm$ 0.2 3.16 $\pm$ 0.10 3.7
'' NE ... 0.22 0.048 0.26 0.07 $\pm$ 0.02 ... ... ... ... 0.05
Mkn 5 0.0222 $\pm$ 0.0014 0.050 0.008 0.049 0.046 $\pm$ 0.011 <0.014 <0.03 0.067 $\pm$ 0.008 <0.10 0.040
IRAS 08208+2816 13.1 $\pm$ 0.8 6.4 1.48 5.8 11.3 $\pm$ 0.9 11.4 $\pm$ 1.0 <1.68 9.7 $\pm$ 0.8 16.4 $\pm$ 0.7 11.6
IRAS 08339+6517 6.4 $\pm$ 0.4 8.2 1.92 7.3 9.5 $\pm$ 0.5 8.93 $\pm$ 0.08 5.6 $\pm$ 0.6 8.36 $\pm$ 0.06 6.2 $\pm$ 0.9 7.0
'' Comp 0.095 $\pm$ 0.008 0.37 0.087 0.44 0.17 $\pm$ 0.02 ... ... ... ... 0.10
POX 4 0.57 $\pm$ 0.03 0.93 0.15 0.72 1.85 $\pm$ 0.06 0.31 $\pm$ 0.02 <7.48 0.31 $\pm$ 0.03 0.26 $\pm$ 0.03 0.54
'' Comp 0.054 $\pm$ 0.006 0.030 0.0063 0.041 0.012 $\pm$ 0.004 ... ... ... ... 0.031
UM 420 2.01 $\pm$ 0.11 1.9 0.30 1.4 3.7 $\pm$ 0.2 6.4 ... 5.4 1.9 $\pm$ 0.8 2.1
SBS 0926+606 3.4 $\pm$ 0.3 0.50 0.08 0.40 0.94 $\pm$ 0.06 0.26 $\pm$ 0.03 <0.86 0.20 $\pm$ 0.03 0.25 $\pm$ 0.06 0.95
'' A 0.53 $\pm$ 0.03 0.28 0.04 0.20 0.75 $\pm$ 0.04 ... ... ... ... 0.52
'' B 2.82 $\pm$ 0.25 0.25 0.04 0.22 0.19 $\pm$ 0.02 ... ... ... ... 1.4?

SBS 0948+532

 ... 1.1 0.11 0.53 6.2 $\pm$ 0.2 ... ... ... <0.95 4.2
SBS 1054+365 0.0073 $\pm$ 0.0005 0.013 0.0014 0.019 0.036 $\pm$ 0.001 0.016 <0.01 0.015 0.025 $\pm$ 0.004 0.018
SBS 1211+540 0.0062 $\pm$ 0.0004 0.009 0.0007 0.009 0.011 $\pm$ 0.001 ... ... ... <0.01 0.007
SBS 1319+579 0.069 $\pm$ 0.004 0.59 0.12 0.58 0.189 $\pm$ 0.012 0.24 ... 0.17 <0.07 0.15
SBS 1415+437 0.0331 $\pm$ 0.0018 0.022 0.0029 0.020 0.039 $\pm$ 0.002 ... ... ... <0.01 0.030
III Zw 107 ... 2.3 0.51 2.2 3.19 $\pm$ 0.15 2.3 $\pm$ 0.4 <2.24 2.0 $\pm$ 0.3 1.52 $\pm$ 0.09 2.0
Tol 9 0.77 $\pm$ 0.06 1.0 0.23 1.1 1.82 $\pm$ 0.13 1.59 $\pm$ 0.07 0.8 $\pm$ 0.2 1.19 $\pm$ 0.08 2.18 $\pm$ 0.04 1.3
Tol 1457-262 3.2 $\pm$ 0.2 2.6 0.53 2.3 5.0 $\pm$ 0.3 3.7 $\pm$ 0.3 <1.99 3.4 $\pm$ 0.2 5.4 $\pm$ 0.3 3.8
'' Obj 1 2.37 $\pm$ 0.13 1.8 0.35 1.6 3.7 $\pm$ 0.2 ... ... ... ... 2.4
'' Obj 2 0.74 $\pm$ 0.09 0.87 0.17 0.83 1.37 $\pm$ 0.06 ... ... ... ... 0.83
'' #15 0.089 $\pm$ 0.017 0.09 0.018 0.10 0.038 $\pm$ 0.003 ... ... ... ... 0.06
Arp 252 3.84 $\pm$ 0.26 5.3 1.26 5.0 7.2 $\pm$ 0.5 16.2 $\pm$ 0.9 11.6 $\pm$ 1.4 15.4 $\pm$ 0.8 49.2 $\pm$ 1.5 10
'' ESO 566-8 3.12 $\pm$ 0.22 4.5 1.01 4.1 6.7 $\pm$ 0.5 ... ... ... ... 3.8
'' ESO 566-7 0.72 $\pm$ 0.04 1.0 0.25 1.1 0.50 $\pm$ 0.04 ... ... ... ... 0.53
NGC 5253 0.190 $\pm$ 0.010 0.36 0.07 0.35 0.348 $\pm$ 0.017 0.12 0.15 0.11 0.037 $\pm$ 0.002 0.14

References. S07 = Salim et al. (2007); G84 = Gallagher et al. (1984); K98 = Kennicutt (1998); R01 = Roussel et al. (2001); C92 = Condon (1992); C02 = Condon et al. (2002) using the expression for M>5 $M_{\odot }$.


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