Fig. 7
V-band extinction in magnitudes, AV,g, as obtained from the Hα to Hβ Balmer decrement, versus the stellar continuum V-band extinction (AV,s), as derived from the spectral synthesis-fitting with STARLIGHT for all non-AGN galaxies. The straight solid and dashed lines show the relations between AV,g and AV,s found by Calzetti et al. (2000) and Kreckel et al. (2013), respectively.
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