Fig. E.1
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Isochrone fitting results using the example of NGC 1978. (a) Best-fit isochrone model in the mF438W vs mF438W − mF814W CMD. (b) Best-fit isochrone model in the mF814W vs mF438W − mF814W CMD. (c): Corner plot of the posterior probability distributions of pairwise model parameters for the mF438W vs mF438W − mF814W CMD. The best-fit parameters are quoted in the labels. (d): Same as (c) but for the mF814W vs mF438W − mF814W CMD.
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