Open Access

Table A.2.

The extinction-related results obtained from SED modeling with CIGALE, including the AGN component.

GMC V_B90 B_B90 E_BV_factor E_BV_lines E_BVs
[mag] [mag] [mag] [mag] [mag]
1 2.87 ± 0.04 3.58 ± 0.05 0.10 ± 0.00 7.00 ± 0.09 0.70 ± 0.01
2 3.00 ± 0.17 3.70 ± 0.21 0.33 ± 0.33 5.00 ± 2.80 0.73 ± 0.05
3 6.14 ± 0.04 6.20 ± 0.02 0.40 ± 0.00 3.00 ± 0.00 1.20 ± 0.00
4 6.10 ± 0.01 7.60 ± 0.01 0.45 ± 0.09 3.50 ± 0.90 1.50 ± 0.00
5 6.10 ± 0.01 7.60 ± 0.01 0.45 ± 0.09 3.50 ± 0.90 1.50 ± 0.00
6 4.90 ± 0.01 6.10 ± 0.01 0.40 ± 0.00 3.00 ± 0.00 1.20 ± 0.00
7 3.20 ± 0.01 4.00 ± 0.01 0.80 ± 0.01 1.00 ± 0.05 0.80 ± 0.01
8 3.00 ± 0.17 3.70 ± 0.21 0.29 ± 0.31 5.40 ± 2.70 0.73 ± 0.04
9 2.80 ± 0.11 3.50 ± 0.14 0.10 ± 0.02 7.00 ± 0.34 0.70 ± 0.03
10 2.90 ± 0.03 3.60 ± 0.04 0.10 ± 0.05 7.00 ± 0.41 0.70 ± 0.01

Notes. The columns represent the GMC number, A V Balmer $ A_\mathrm{{V}}^\mathrm{{Balmer}} $ as presented in Table 8, the slope of the attenuation curve, the scaling factor between E(B-V) for lines and continuum, the color excess for nebular emission lines, and the color excess for the stellar continuum.

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