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Fig. 1.

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Left panel: HRD of RGB of NGC 1261, with RGBb stars highlighted in orange and by a blue dashed line referring to the RGBb luminosity obtained from the fit. The errors on log LRGBb already include the systematics due to the number of RGB stars (see Appendix B) and the distance modulus (Baumgardt & Hilker 2018). Right panel: KDE (light blue zone) of luminosity distribution (lower labels) and relative fit (orange line). The blue line represents the histogram of the RGB luminosity with Poissonian errors (upper labels).

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