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Fig. 3


Comparison of a) SFR-stellar mass and b) sSFR-stellar mass relations of our BAT6 sample to the samples of extreme starbursts (star symbols; Atek et al. 2014) and blue compact dwarf galaxies (empty diamonds; Rodríguez-Muñoz et al. 2015). The colour scale and the overplotted lines are the same as in Fig. 2. The host galaxies of GRB 060614A and 061021, while included in the plots, were excluded from the comparison of specific SFRs (see text) because their measured SFR is below the completeness limit of the two surveys (log  SFR [ M yr-1 ] ~ −1).

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