Fig. 3.

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Absolute G-band magnitudes for BSGs in the mass range 8.9–66.89 M⊙ obtained from Martins et al. (2005) and Brott et al. (2011) (see Table A.1). The solid red line shows the fit and the vertical grey lines indicate the different mass regimes. The masses are shown on a logarithmic scale. As a reference, the obtained magnitudes for MS dwarf stars from Paper I are also shown.
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