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Fig. B.1

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Comparing host galaxy mass estimates from optical and K-band photometry (phot) to mass estimates from Prospector (pro). SNe are colored by Hubble residual from NIR bands and fixing both x1 and c to zero. The tan regions indicate SNe which, depending on which mass estimate is used, cross the high mass/low mass threshold given a mass step location at 1010 M.

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