Fig. 8
Left panel: completeness-corrected LFs in the MKs for the C stars (upper) and M-giant stars (lower) in IC 1613. The smaller box in the lower panel shows the logarithmic LF of the M-giant stars. Right panel: completeness-corrected bolometric LFs for the C stars (upper panel) and M-giant stars (lower panel). The luminosities of the AGB tip with ages of 3,5,8, and 10 Gyr obtained from the Mbol-age relation of Rejkuba et al. (2006) are indicated as thick lines.
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