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Table 2:

FIR and FUV data for the WR galaxy sample analyzed in this work.

Galaxy
$f_{\rm 12~\mu m}$ $f_{\rm 25~\mu m}$ $f_{\rm 60~\mu m}$ $f_{\rm 100~\mu m}$ $F_{\rm FIR}$ Reg. $m_{\rm FUV}$ $f_{\rm FUV}$
  [Jy] [Jy] [Jy] [Jy] a b [mag] c
HCG 31 0.110 $\pm$ 0.020 0.580 $\pm$ 0.040 3.92 $\pm$ 0.31 5.84 $\pm$ 0.47 2.01 $\pm$ 0.16 AC 14.97 $\pm$ 0.06 7.54 $\pm$ 0.44
            B 16.80 $\pm$ 0.09 3.32 $\pm$ 0.26
            E 18.01 $\pm$ 0.08 0.456 $\pm$ 0.035
            F 18.24 $\pm$ 0.11 0.460 $\pm$ 0.047
            G 15.93 $\pm$ 0.06 3.11 $\pm$ 0.18
            H 20.63 $\pm$ 0.40 0.0041 $\pm$ 0.0014
Mkn 1087 0.103 $\pm$ 0.029 0.414 $\pm$ 0.058 3.03 $\pm$ 0.33 4.44 $\pm$ 0.40 1.54 $\pm$ 0.16 ... ... ...
Haro 15 0.118 $\pm$ 0.034 0.297 $\pm$ 0.089 1.36 $\pm$ 0.12 1.97 $\pm$ 0.20 0.690 $\pm$ 0.064 ... 15.12 $\pm$ 0.07 9.41 $\pm$ 0.57
Mkn 1199 0.282 $\pm$ 0.031 1.28 $\pm$ 0.09 6.82 $\pm$ 0.34 8.85 $\pm$ 0.53 3.33 $\pm$ 0.18 ... ... ...
Mkn 5 <0.0503 <0.0533 0.21 $\pm$ 0.04 <0.8473 <1.75 ... 17.76 $\pm$ 0.07 1.59 $\pm$ 0.10
IRAS 08208+2816 0.126 $\pm$ 0.029 0.278 $\pm$ 0.067 1.15 $\pm$ 0.09 1.70 $\pm$ 0.17 0.588 $\pm$ 0.051 ... 16.59 $\pm$ 0.07 3.75 $\pm$ 0.23
IRAS 08339+6517 0.250 $\pm$ 0.025 1.13 $\pm$ 0.02 5.81 $\pm$ 0.04 6.48 $\pm$ 0.09 2.71 $\pm$ 0.02   15.37 $\pm$ 0.06 10.7 $\pm$ 0.6
            c 19.70 $\pm$ 0.10 0.160 $\pm$ 0.014
POX 4 <0.987 0.153 $\pm$ 0.040 0.629 $\pm$ 0.057 <0.5798 <0.278 POX 4 16.03 $\pm$ 0.06 2.82 $\pm$ 0.16
            Comp. 19.06 $\pm$ 0.12 0.269 $\pm$ 0.030
UM 420 ... <0.275 0.411: 0.613: 0.211: ... 18.22 $\pm$ 0.06 0.377 $\pm$ 0.021
SBS 0926+606 <0.07553 <0.08818 0.269 $\pm$ 0.046 <0.5296 <0.154 A 16.71 $\pm$ 0.06 1.75 $\pm$ 0.09
            B 17.84 $\pm$ 0.10 0.829 $\pm$ 0.073
SBS 0948+532 ... ... ... ... ... ... ... ...
SBS 1054+365 <0.055 <0.100 0.536 $\pm$ 0.048 0.97 $\pm$ 0.15 0.296 $\pm$ 0.035 ... 16.67 $\pm$ 0.07 1.18 $\pm$ 0.08
SBS 1211+540 ... ... ... ... ... ... 18.40 $\pm$ 0.07 0.370 $\pm$ 0.022
SBS 1319+579 ... ... 0.209: 0.685: 0.154: ... 17.00 $\pm$ 0.06 0.864 $\pm$ 0.048
            A 18.60 $\pm$ 0.06 0.199 $\pm$ 0.010
SBS 1415+437 ... ... ... ... ... ... 16.22 $\pm$ 0.06 3.95 $\pm$ 0.22
III Zw 107 <0.0968 0.336 $\pm$ 0.050 1.37 $\pm$ 0.20 1.72 $\pm$ 0.31 0.662 $\pm$ 0.104 ... ... ...
Tol 9 0.111 $\pm$ 0.030 0.465 $\pm$ 0.051 2.71 $\pm$ 0.22 <5.516 <1.58 ... 17.57 $\pm$ 0.07 4.22 $\pm$ 0.22
Tol 1457-262 <0.117 0.611 $\pm$ 0.067 3.09 $\pm$ 0.19 3.68 $\pm$ 0.40 1.47 $\pm$ 0.11 ... 15.84 $\pm$ 0.07 6.95 $\pm$ 0.47
            Obj 1 16.15 $\pm$ 0.06 5.26 $\pm$ 0.29
            Obj 2 17.41 $\pm$ 0.13 1.64 $\pm$ 0.18
            #15 19.71 $\pm$ 0.21 0.199 $\pm$ 0.037
Arp 252 0.188 $\pm$ 0.023 0.994 $\pm$ 0.050 3.91 $\pm$ 0.20 4.11 $\pm$ 0.25 1.79 $\pm$ 0.10 A 18.67 $\pm$ 0.08 1.91 $\pm$ 0.13
            B 18.84 $\pm$ 0.07 0.441 $\pm$ 0.027
NGC 5253 2.50 $\pm$ 0.02 12.07 $\pm$ 0.05 29.84 $\pm$ 0.07 30.08 $\pm$ 0.21 13.49 $\pm$ 0.05 ... 12.81 $\pm$ 0.06 123.0 $\pm$ 6.5

Notes. (a) In units of 10-10 erg s-1 cm-2.
(b) Region within each system (HCG 31, IRAS 08339+6517, POX 4, SBS 0926+606, SBS 1319+579, Tol 1457-262, and Arp 252; see Paper I).
(c) In units of 10-14 erg s-1 cm-2 Å-1.


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