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Fig. C.3.

Fig. C.3. Refer to the following caption and surrounding text.

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Comparison of H0 between different ways of calibrating a given set of hosts and a gievn SN fitter. It is computed as the result with the hosts calibrated through any means minus the result with the hosts calibrated through a specific calibration type (such as only Cepheids, only TRGB, or only F25 TRGB). The results with the star mark the literature results for the given (reduced) set of calibrating a given set of hosts. The triangle shows a case where for the BayesSN fitter only 32 out of the 35 hosts were calibrated due to several missing supernovae.

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