Table A.1
Logarithmic of the fluxes from FUV to Spitzer 8.0 μm band 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(FUV) | F(NUV) | F(Hα) | F(3.4 μm) | F(3.6 μm) | F(4.5 μm) | F(4.6 μm) | F(5.8 μm) | F(8.0 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 Hz) | |
|
|
|||||||||
| 1 | 16.18 ± 0.00 | 16.15 ± 0.00 | 14.22 ± 0.07 | 14.77 ± 0.02 | 14.79 ± 0.03 | 14.54 ± 0.05 | 14.50 ± 0.02 | 15.01 ± 0.05 | 15.24 ± 0.07 |
| 2 | 15.66 ± 0.01 | 15.58 ± 0.01 | 13.67 ± 0.07 | 14.58 ± 0.02 | 14.62 ± 0.03 | 14.52 ± 0.05 | 14.39 ± 0.02 | 14.80 ± 0.05 | 14.92 ± 0.07 |
| 3 | 16.13 ± 0.00 | 16.01 ± 0.00 | 14.11 ± 0.07 | 14.66 ± 0.02 | 14.70 ± 0.03 | 14.47 ± 0.05 | 14.32 ± 0.02 | 14.68 ± 0.05 | 14.87 ± 0.07 |
| 4 | 15.92 ± 0.01 | 15.83 ± 0.01 | 14.11 ± 0.07 | 14.57 ± 0.02 | 14.48 ± 0.04 | 14.25 ± 0.06 | 14.23 ± 0.03 | 14.57 ± 0.06 | 14.73 ± 0.07 |
| 5 | 15.92 ± 0.00 | 15.82 ± 0.00 | 13.70 ± 0.07 | 14.35 ± 0.02 | 14.35 ± 0.03 | 14.15 ± 0.05 | 14.03 ± 0.02 | 14.73 ± 0.05 | 14.96 ± 0.07 |
| 6 | 16.22 ± 0.00 | 16.09 ± 0.00 | 14.23 ± 0.07 | 14.38 ± 0.05 | 14.46 ± 0.05 | 14.44 ± 0.05 | 14.23 ± 0.04 | 14.63 ± 0.07 | 15.10 ± 0.07 |
| 7 | 16.19 ± 0.00 | 16.14 ± 0.00 | 14.65 ± 0.07 | 14.44 ± 0.03 | 14.53 ± 0.03 | 14.48 ± 0.05 | 14.37 ± 0.02 | 14.82 ± 0.05 | 15.20 ± 0.07 |
| 8 | 15.04 ± 0.02 | 14.92 ± 0.02 | 13.47 ± 0.07 | 13.87 ± 0.05 | 14.01 ± 0.04 | 14.06 ± 0.05 | 13.91 ± 0.02 | 14.24 ± 0.05 | 14.45 ± 0.07 |
| 9 | 15.47 ± 0.02 | 15.45 ± 0.02 | 13.65 ± 0.07 | 14.30 ± 0.04 | 14.11 ± 0.08 | 13.68 ± 0.14 | 13.56 ± 0.15 | 14.38 ± 0.07 | 14.35 ± 0.09 |
| 10 | 16.06 ± 0.01 | 15.95 ± 0.01 | 13.77 ± 0.07 | 14.47 ± 0.03 | 14.54 ± 0.03 | 14.27 ± 0.05 | 14.15 ± 0.03 | 14.55 ± 0.05 | 14.65 ± 0.07 |
Notes. FUV, NUV and Hα fluxes have been corrected for Galactic extinction assuming a colour excess of E(B−V) = 0.07 mag (van den Bergh 2000) and Cardelli et al. (1989) extinction law with RV = 3.1. 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. The full table is available at the CDS.
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