{ "id": "2205.08548", "version": "v1", "published": "2022-05-17T18:00:01.000Z", "updated": "2022-05-17T18:00:01.000Z", "title": "Distances to Local Group Galaxies via Population II, Stellar Distance Indicators I: The Sculptor Dwarf Spheroidal", "authors": [ "Quang H. Tran", "Taylor J. Hoyt", "Wendy L. Freedman", "Barry F. Madore", "Elias K. Oakes", "William Cerny", "Dylan Hatt", "Rachael L. Beaton" ], "comment": "16 pages, 14 figures", "categories": [ "astro-ph.GA", "astro-ph.CO" ], "abstract": "We determine the distance to the Sculptor Dwarf Spheroidal via three Population II stellar distance indicators: (a) the Tip of the Red Giant Branch (TRGB), (b) RR Lyrae variables (RRLs), and (c) the ridgeline of the blue horizontal branch (HB). High signal-to-noise, wide-field $VI$ imaging that covers an area $48' \\times 48'$ and reaches a photometric depth approximately 2 mag fainter than the HB was acquired with the Magellan-Baade 6.5m telescope. The true modulus derived from Sculptor's TRGB is found to be $\\mu^\\mathrm{TRGB}_o = 19.59 \\pm 0.07_\\mathrm{stat} \\pm 0.05_\\mathrm{sys}$ mag. Along with periods adopted from the literature, newly acquired RRL phase points are fit with template light curves to determine $\\mu_{W_{I,V-I}}^\\mathrm{RRL} = 19.60 \\pm 0.01_\\mathrm{stat} \\pm 0.05_\\mathrm{sys}$ mag. Finally, the HB distance is found to be $\\mu^\\mathrm{HB}_o = 19.54 \\pm 0.03_\\mathrm{stat} \\pm 0.09_\\mathrm{sys}$ mag. Absolute calibrations of each method are anchored by independent geometric zero-points, utilizes a different class of stars, and are determined from the same photometric calibration.", "revisions": [ { "version": "v1", "updated": "2022-05-17T18:00:01.000Z" } ], "analyses": { "keywords": [ "sculptor dwarf spheroidal", "stellar distance indicators", "local group galaxies", "acquired rrl phase points", "population" ], "note": { "typesetting": "TeX", "pages": 16, "language": "en", "license": "arXiv", "status": "editable" } } }