Table A.2
Logarithmic of the fluxes from W4 12 μm to LABOCA 870 μm bands of our set of H ii regions in mJy Hz obtained with centres and apertures given in Table B.1 in Paper I.
| ID | F(12 μm) | F(22 μm) | F(24 μm) | F(70 μm) | F(70 μm (pacs)) | F(100 μm) | F(160 μm) | F(250 μm) | F(870 μm) |
| log (mJy Hz) | log (mJy Hz) | log (mJy Hz) | log (mJy Hz) | log (mJy Hz) | log (mJy Hz) | log (mJy Hz) | log (mJy Hz) | log (mJy) | |
|
|
|||||||||
| 1 | 14.77 ± 0.02 | 14.83 ± 0.03 | 14.88 ± 0.02 | 15.67 ± 0.02 | 15.74 ± 0.02 | 15.88 ± 0.02 | 15.74 ± 0.02 | 15.35 ± 0.07 | **** ± **** |
| 2 | 14.64 ± 0.02 | 14.40 ± 0.03 | 14.45 ± 0.03 | 15.11 ± 0.02 | 14.83 ± 0.04 | 15.18 ± 0.04 | 15.27 ± 0.03 | 15.01 ± 0.07 | 13.25 ± 0.09 |
| 3 | 14.47 ± 0.03 | 14.56 ± 0.03 | 14.55 ± 0.03 | 15.26 ± 0.02 | 15.32 ± 0.02 | 15.64 ± 0.02 | 15.41 ± 0.02 | 15.04 ± 0.07 | 13.14 ± 0.11 |
| 4 | 14.38 ± 0.03 | 14.03 ± 0.05 | 13.80 ± 0.15 | 15.04 ± 0.03 | 15.29 ± 0.03 | 15.33 ± 0.05 | 15.30 ± 0.03 | 14.89 ± 0.07 | **** ± **** |
| 5 | 14.56 ± 0.02 | 14.54 ± 0.03 | 14.57 ± 0.02 | 15.18 ± 0.03 | 15.31 ± 0.02 | 15.42 ± 0.03 | 15.36 ± 0.03 | 15.01 ± 0.07 | 12.91 ± 0.12 |
| 6 | 14.73 ± 0.03 | 14.49 ± 0.03 | 14.41 ± 0.05 | 15.34 ± 0.03 | 15.42 ± 0.03 | 15.46 ± 0.04 | 15.37 ± 0.03 | 15.16 ± 0.07 | 13.26 ± 0.11 |
| 7 | 14.87 ± 0.02 | 15.07 ± 0.02 | 15.08 ± 0.02 | 15.77 ± 0.02 | 15.89 ± 0.02 | 15.87 ± 0.02 | 15.68 ± 0.02 | 15.27 ± 0.07 | 13.62 ± 0.08 |
| 8 | 14.04 ± 0.03 | 13.74 ± 0.05 | 13.99 ± 0.04 | 14.61 ± 0.03 | 14.47 ± 0.08 | 14.31 ± 0.17 | 14.89 ± 0.03 | 14.58 ± 0.07 | 12.72 ± 0.18 |
| 9 | 14.01 ± 0.07 | 13.92 ± 0.05 | 13.94 ± 0.09 | 14.54 ± 0.07 | **** ± **** | 14.66 ± 0.13 | 15.01 ± 0.04 | 14.71 ± 0.07 | 12.92 ± 0.15 |
| 10 | 14.29 ± 0.04 | 14.08 ± 0.04 | 14.26 ± 0.03 | 15.02 ± 0.03 | 14.96 ± 0.04 | 15.38 ± 0.03 | 15.03 ± 0.04 | 14.64 ± 0.07 | 12.82 ± 0.14 |
Notes. All the fluxes have been background subtracted. The errors include the uncertainties in the calibration and background subtraction. We did not take into account negative fluxes higher than the corresponding errors, in these cases the fluxes are represented by ****. The full table is available at the CDS.
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