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Table 8.

GMC attenuations.

GMC (FHα/FHβ)obs AVBalmer AVCIGALE A V S T A R L I G H T $ \tilde{A_\mathrm{{V}}}^{\small { {\text{STARLIGHT}}}} $
[mag] [mag] [mag]
1 3.81 ± 0.32 1.08 ± 0.11 3.57 ± 0.02 2.12
2 8.32 ± 1.70 2.89 ± 0.30 3.58 ± 0.02 2.42
3 29.79 ± 16.90 5.06 ± 0.56 6.04 ± 0.11 4.44
4 45.69 ± 37.94 5.87 ± 0.67 6.06 ± 0.00 5.67
5 43.43 ± 37.37 5.81 ± 0.65 6.24 ± 0.02 4.66
6 29.14 ± 16.45 5.04 ± 0.54 6.08 ± 0.01 4.10
7 21.21 ± 10.11 4.38 ± 0.47 5.07 ± 0.02 2.97
8 19.18 ± 10.04 4.18 ± 0.45 3.53 ± 0.01 2.28
9 17.01 ± 7.84 3.96 ± 0.42 3.54 ± 0.01 1.84
10 11.13 ± 5.05 3.36 ± 0.37 3.54 ± 0.12 2.11

Notes. Attenuation estimates for the studied GMCs derived from the Balmer decrement (AVBalmer), CIGALE (AVCIGALE), and effective AV ( A V S T A R L I G H T $ \tilde{A_\mathrm{{V}}}^{{\small { {\text{STARLIGHT}}}}} $) from STARLIGHT. The first two columns correspond to the GMC number and the Hα over Hβ observed flux ratio, from left to right, respectively.

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