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Fig. 1

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The redshift accuracy for simulated supernovae with (upper panel) and without (lower panel) a host galaxy photometric redshift. The ~2000 SNe of all different subtypes used to make this figure are a sub-sample of the full sample of simulated light curves. The redshift on the x axis (zsim) is the initial adopted redshift of the supernovae. The dotted lines indicate the |zfit − zsim|/(1 + zsim) > 0.15 limits.

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