Fig. 4.
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Average attenuation curves of our sample using three different attenuation laws/recipes (Calzetti et al. 2000; Charlot & Fall 2000; Lo Faro et al. 2017) shown on the left. In the case of CF00 and LF17 curves, we show the combined curve of the ISM and the BC. Stellar masses of our sample are shown on the right, which were derived using the three attenuation curves as in the left panel. The arrows show the mean of the specific distribution.
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