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Fig. 8

image

a) Cumulative distributions of the galaxies stellar mass; b) mass vs. gas-phase metallicity. The dotted line is the MZ 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 MZ 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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