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In support of ongoing projects we have compiled a database of supernovae withhost metallicities determined from spectroscopy in the Sloan Digital Sky Survey(SDSS) which we are providing as a catalog for the general use of thecommunity. Here we provide metallicity values in the KK04 (Kobulnicky & Kewley2004), T04 (Tremonti et al. 2004), and D16 (Dopita et al. 2016) diagnostics aswell as a compilation of the relevant line fluxes to allow users to computetheir own metallicities. The sample presented here has approximately 1700objects with a metallicity in at least one diagnostic, with about 1200 objectsin KK04 of which over 300 are core-collapse SNe or about twice the number ofcore-collapse objects present in the compilation of Kelly & Kirshner (2012)reflecting the recent considerable improvement in SNe detection capabilities.We find some differences in the metallicity distributions between the subtypesof both Type II and Type Ia SNe and speculate that metallicity may play a rolein if Type II SNe events happen as IIb & IIn or as standard Type II.

Supernovae SDSS Host Metallicity Catalog and Resulting Metallicity Distributions by SNe Type