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Table 1

Our new UVOT, WISE, Herschel/PACS and SPIRE, APEX/ LABOCA, ALMA and ATCA photometry results, the contribution of the WR region and the beam sizes. The limit is 2σ.

λobs Entire host WR region % FWHM Inst.
(μm) (mJy) (mJy) (′′)

0.2033 1.70 ± 0.05 0.15 ± 0.01 9 2.92 UVOT
0.2229 1.70 ± 0.05 0.15 ± 0.01 9 2.45 UVOT
0.2591 1.79 ± 0.06 0.14 ± 0.01 8 2.37 UVOT
3.4 4.3 ± 0.3 0.54 ± 0.04 1.3 6.1 WISE
4.6 2.3 ± 0.3 0.32 ± 0.03 14 6.4 WISE
12 11.9 ± 0.8 2.1 ± 0.1 18 6.5 WISE
22 28.7 ± 0.9 16 ± 1 56 12 WISE
100 327 ± 12 72 ± 5 19 6.7 × 6.9 PACS
160 323 ± 19 74 ± 9 13 10.7 × 12.1 PACS
250 231 ± 16 ···  ···  18.2 SPIRE
350 106 ± 8 ···  ···  24.9 SPIRE
500 43 ± 4 ···  ···  36.3 SPIRE
870 12.7 ± 1.8 ···  ···  19.5 APEX
2790.5 <0.43 0.123 ± 0.025 >29 1.9 × 1.8 ALMA
2790.5 ···  0.069a ± 0.028 ···  1.9 × 1.8 ALMA
1.05e5 0.40 ± 0.20 0.28 ± 0.03 70 10.3 × 7.0 ATCA
1.28e5 0.71 ± 0.19 0.29 ± 0.03 41 12.0 × 7.5 ATCA
1.63e5 1.11 ± 0.21 0.42 ± 0.04 38 13.5 × 8.3 ATCA
2.26e5 0.84 ± 0.16 0.60 ± 0.06 71 23 × 14 ATCA

Notes.

(a)

With free-free emission subtracted as described in Sect. 3.

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