{ "id": "1703.10616", "version": "v1", "published": "2017-03-30T18:01:37.000Z", "updated": "2017-03-30T18:01:37.000Z", "title": "The Carnegie-Chicago Hubble Program. III. The Distance to NGC 1365 via the Tip of the Red Giant Branch", "authors": [ "In Sung Jang", "Dylan Hatt", "Rachael L. Beaton", "Myung Gyoon Lee", "Wendy L. Freedman", "Barry F. Madore", "Taylor J. Hoyt", "Andrew J. Monson", "Jeffrey A. Rich", "Victoria Scowcroft", "Mark Seibert" ], "comment": "18 pages, 9 figures, 2 tables, submitted to ApJ", "categories": [ "astro-ph.GA" ], "abstract": "The Carnegie-Chicago Hubble Program seeks to anchor the distance scale of Type Ia supernovae via the Tip of the Red Giant Branch (TRGB). Based on deep $Hubble$ $Space$ $Telescope$ ACS/WFC imaging, we present an analysis of the TRGB for the metal-poor halo of NGC 1365, a giant spiral galaxy in the Fornax Cluster that is host to the supernova SN2012fr. We have measured its extinction-corrected TRGB magnitude to be F814W = 27.34 $\\pm 0.03_{stat} \\pm0.01_{sys}$ mag. In advance of future direct calibration by $Gaia$, we set a provisional TRGB luminosity via the Large Magellanic Cloud and find a true distance modulus $\\mu_0 = 31.29 \\pm 0.04_{stat}\\pm0.05_{sys}$ mag or $D = 18.4 \\pm 0.03_{stat} \\pm0.04_{sys}$ Mpc. This high-fidelity measurement shows excellent agreement with recent Cepheid-based distances to NGC 1365 and suggests no significant difference in the distances derived from stars of Population I and II. We revisit the error budget for the $CCHP$ path to the Hubble Constant based on this analysis of one of our most distant hosts, finding a 2.5\\% measurement is feasible with our current sample.", "revisions": [ { "version": "v1", "updated": "2017-03-30T18:01:37.000Z" } ], "analyses": { "keywords": [ "red giant branch", "type ia supernovae", "giant spiral galaxy", "carnegie-chicago hubble program seeks", "provisional trgb luminosity" ], "note": { "typesetting": "TeX", "pages": 18, "language": "en", "license": "arXiv", "status": "editable" } } }