Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm

Details Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm Tip of the Red Giant Branch Distances. I. Optimization of a Maximum Likelihood Algorithm

2006-03-03

arxiv.org/abs/astro-ph/0603073v1

Astron.J.132:2729-2742,2006

Astronomy and Astrophysics

Astrophysics

submitted to AJ

Scientific paper

10.1086/508925

Accurate distances to galaxies can be determined from the luminosities of stars at the Tip of the Red Giant Branch (TRGB). We use a Maximum Likelihood algorithm to locate the TRGB in galaxy color-magnitude diagrams. The algorithm is optimized by introducing reliable photometric errors and a completeness characterization determined with artificial star experiments. The program is extensively tested using Monte-Carlo simulations, artificial galaxies, and a sample of nearby dwarf galaxies observed with HST/WFPC2 and ACS. Our procedure is shown to be reliable, to have good accuracy, and to not introduce any systematic errors. The methodology is especially useful in cases where the TRGB approaches the photometric limit and/or the RGB is poorly populated.

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