Fig. 7
I-band stellar luminosity function for dw1335-29 (top) and dw1340-30 (bottom). Each panel shows the observed (bold line) and completeness-corrected (thin line) luminosity functions to the point where the completeness drops bellow 30%. The corresponding signals from the Sobel edge detection are shown below the respective luminosity function. The maximum (dashed line) indicates the location of the TRGB.
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