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Fig. 2

image

(JKs,Ks) and (HKs,Ks) CMDs for the resolved stars detected in near-infrared observation (upper) and for the commonly detected stars in the near-infrared and optical data of Battinelli et al. (2007a) (lower). The magnitude and color range of TRGB (Valenti et al. 2004) for the given metallicity of [Fe/H] = −1.75 ~ − 1.3 is indicated by the solid line. The estimated magnitude in Ks of TRGB in this study is indicated by an arrow at Ks = 18.2. The open circles are 82 C stars cross-identified in both the giJHKs photometry (this study) and CNTiO photometry of Albert et al. (2000).

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