{ "id": "2008.06089", "version": "v1", "published": "2020-08-13T19:49:01.000Z", "updated": "2020-08-13T19:49:01.000Z", "title": "Faint Stars in a Faint Galaxy: I. Ultra Deep Photometry of the Boötes I Ultra Faint Dwarf Galaxy", "authors": [ "Carrie Filion", "Vera Kozhurina-Platais", "Roberto Avila", "Imants Platais", "Rosemary F. G. Wyse" ], "comment": "21 pages, 15 figures, 2 tables; accepted for publication in ApJ", "categories": [ "astro-ph.GA", "astro-ph.IM" ], "abstract": "We present an analysis of new extremely deep images of the resolved stellar population of the Bo\\\"otes I ultra faint dwarf spheroidal galaxy. These new data were taken with the Hubble Space Telescope, using the Advanced Camera for Surveys (Wide Field Camera) and Wide Field Camera 3 (UVIS), with filters F606W and F814W (essentially V and I), as part of a program to derive the low-mass stellar initial mass function in this galaxy. We compare and contrast two approaches to obtaining the stellar photometry, namely ePSF and DAOPHOT. We identify likely members of Bo\\\"otes I based on the location of each star on the color-magnitude diagram, obtained with the DAOPHOT photometry from the ACS/WFC data. The probable members lie close to stellar isochrones that were chosen to encompass the known metallicity distribution derived from spectroscopic data of brighter radial-velocity member stars and are consistent with the main-sequence turnoff. The resulting luminosity function of the Bo\\\"otes I galaxy has a 50% completeness limit of 27.4 in F814W and 28.2 in F606W (Vega magnitude system), which corresponds to a limiting stellar mass of $\\le 0.3 M_\\odot$.", "revisions": [ { "version": "v1", "updated": "2020-08-13T19:49:01.000Z" } ], "analyses": { "keywords": [ "ultra faint dwarf galaxy", "ultra deep photometry", "faint dwarf spheroidal galaxy", "faint galaxy", "faint stars" ], "note": { "typesetting": "TeX", "pages": 21, "language": "en", "license": "arXiv", "status": "editable" } } }