M_d/M_∗ as a function of metallicity for a sample of nearby galaxies taken from the KINGFISH (black filled circles; Kennicutt et al. 2011), and the DGS (red filled squares; Madden et al. 2013) Herschel guaranteed time key projects, and a sample of high redshift (z> 1), star forming galaxies from Magnelli et al. (2012a) (green filled diamonds). Metallicities of the z> 1 star forming galaxies were estimated using the mass-metallicity relation and converted into the Denicoló et al. (2002) system. GRBH 031203 (Symeonidis et al. 2014, cyan pentagon), GRBH 980425 (Michałowski et al. 2014, grey pentagon), and the subset of GRBHs with known metallicity from HPM14 (pink pentagons; GRBHs 980703, 020819B, 050223, 051022) and from this paper (blue pentagons) are also plotted. Filled symbols correspond to Herschel detections, and upper limits are shown as downward arrows. A ring around the data point indicates galaxies that hosted a GRB with afterglow extinction A_V,GRB> 1 mag. The solid black line is the best-fit power law to the combined KINGFISH and DGS data taken from Rémy-Ruyer et al. (2013), and the dashed lines represent the 3σ dispersion.