Metallicity-corrected Tip of the Red Giant Branch Distance to NGC 4258

TL;DR

This paper presents a highly precise distance measurement to NGC 4258 using a metallicity-corrected TRGB method with HST data, comparing it with other distance indicators like Cepheids and masers.

Contribution

It introduces a modified TRGB technique that fully accounts for metallicity effects, achieving one of the most precise TRGB distance measurements to NGC 4258.

Findings

Distance modulus u(TRGB) = 29.28 +/- 0.04 (random) +/- 0.12 (systematic) mag

Distance to NGC 4258 is 7.18 +/- 0.13 +/- 0.40 Mpc

Method compares favorably with Cepheid and maser distances

Abstract

We have determined the distance to NGC 4258 using observations made with the Hubble Space Telescope (HST) and the Wide Field, Advanced Camera for Surveys (ACS/WFC). We apply a modified technique that fully accounts for metallicity effects on the use of the luminosity of the tip of the red giant branch (TRGB) to determine one of the most precise TRGB distance moduli to date: u(TRGB) = 29.28 +/- 0.04 (random) +/- 0.12 (systematic) mag (7.18 +/- 0.13 +/- 0.40 Mpc). We discuss this distance modulus with respect to other recent applications of the TRGB method to NGC 4258, and with several other techniques (Cepheids and masers) that are equally competitive in their precision, but different in their systematics.