Subaru Hyper-Supreme Cam observations of IC 1396 - Source catalogue, member population, and sub-clusters of the complex

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Fig. 13

r₂ vs r₂–Y CMD of the 2425 candidate members of IC 1396 detected in this work. Isochrones and the black arrow have the same meaning as in Fig. 6. On the CMD, we show evolutionary tracks of mass 0.02, 0.04, 0.1, 0.2, 0.5, and 1.4 M_⊙ (Baraffe et al. 2015).

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