Fig. 9.
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The LF of carbon stars in F160W (top) and [3.6] (bottom), normalized to 17 and 14 mag, respectively. The LF of the carbon stars sample as selected by Boyer et al. (2019) is shown in black; the LF of the carbon stars synthetic population produced in this work is reported in magenta, while the synthetic LF obatined by considering the cuts proposed by G22 (see Section 3) is displayed in blue.
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