Fig. 8
a) Cumulative distributions of the galaxies stellar mass; b) mass vs. gas-phase metallicity. The dotted line is the M−Z relation from Sánchez et al. (2013) converted from PP04 to the M13 version of the O3N2 calibrator. c) mass vs. mass-weighted stellar metallicity. The dotted line is the M − Z relation from Sánchez et al. (2013) and the solid line is the Panter et al. (2008) relation. The green dots show the elliptical SN Ia hosts.
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