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Table 2

Sample of the far-IR and sub-mm photometry.

Galaxy PACS 70 μma PACS 110 μma PACS 160a SPIRE 250 μm SPIRE 350 μm SPIRE 500 μm
ID (Jy) (Jy) (Jy) (Jy) (Jy) (Jy)

HCG16a 0.413 ± 0.021 0.697 ± 0.035 1.026 ± 0.051 0.503 ± 0.109 0.350 ± 0.057 <0.040 ± 0.030
HCG16b 6.836 ± 0.342 10.95 ± 0.55 10.71 ± 0.54 4.271 ± 0.331 1.558 ± 0.130 0.485 ± 0.052
HCG16c 13.30 ± 0.66 15.99 ± 0.80 12.61 ± 0.63 3.984 ± 0.291 1.379 ± 0.106 0.385 ± .037
HCG16d 12.04 ± 0.60 12.21 ± 0.61 8.234 ± 0.411 2.222 ± 0.190 0.737 ± 0.075 0.210 ± .035
HCG40a <0.249 ± 0.012b 0.103 ± 0.005 0.195 ± 0.010 <0.040 ± 0.030 <0.026 ± 0.020 <0.045 ± 0.030
HCG40b 0.121 ± 0.006 0.306 ± 0.015 0.318 ± 0.016 <0.030 ± 0.020 <0.026 ± 0.012 <0.045 ± 0.009
HCG40c 0.991 ± 0.049 2.258 ± 0.113 3.002 ± 0.150 1.260 ± 0.096 0.580 ± 0.046 0.230 ± 0.021
HCG40d 1.103 ± 0.055 1.710 ± 0.086 1.625 ± 0.081 0.640 ± 0.051 0.280 ± 0.025 0.100 ± 0.013
HCG40e 0.072 ± 0.004 0.134 ± 0.007 0.368 ± 0.018 <0.030 ± 0.022 <0.026 ± 0.013 <0.045 ± 0.010

Notes. The full table is available at the CDS.

(a)

The PACS photometry presented here was performed on the maps reduced by the Scanamoprhos mapper.

(b)

With upper limits are marked objects whose emission was under the detection limit.

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