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<ri:Resource created="2024-04-11T11:39:05Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Distances to Local Group galaxies. II. Fornax dSph</title><shortName>J/ApJ/929/116</shortName><identifier>ivo://CDS.VizieR/J/ApJ/929/116</identifier><altIdentifier>doi:10.26093/cds/vizier.19290116</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Oakes E.K.</name></creator><creator><name>Hoyt T.J.</name></creator><creator><name>Freedman W.L.</name></creator><creator><name>Madore B.F.</name></creator><creator><name>Tran Q.H.</name></creator><creator><name>Cerny W.,Beaton R.L.</name></creator><creator><name>Seibert M.</name></creator><date role="Updated">2024-11-06T20:24:42Z</date><date role="Created">2024-04-11T11:39:05Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>dwarf-galaxies</subject><subject>population-ii-stars</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>photometry</subject><subject>local-group</subject><description>We determine three independent Population II distance moduli to the Fornax dwarf spheroidal (dSph) galaxy, using wide-field, ground-based VI imaging acquired with the Magellan-Baade telescope at Las Campanas Observatory. After subtracting foreground stars using Gaia EDR3 proper motions, we measure an I-band tip of the red giant branch (TRGB) magnitude of I_0_^TRGB^=16.753+/-0.03_stat_+/-0.037_sys_mag, with a calibration based in the LMC giving a distance modulus of {mu}_0_^TRGB^=20.80+/-0.037_stat_+/-0.057_sys_mag. We determine an RR Lyrae (RRL) distance from template mean magnitudes, with periods adopted from the literature. Adopting a Gaia DR2 calibration of first overtone RRL period-luminosity and period-Wesenheit relations, we find {mu}_0_^PLZ^=20.74+/-0.01_stat_+/-0.12_sys_mag and {mu}_0_^PWZ^=20.68+/-0.02_stat_+/-0.07_sys_mag. Finally, we determine a distance from Fornax's horizontal branch (HB) and two galactic globular cluster calibrators, giving {mu}_0_^HB^=20.83+/-0.03_stat_+/-0.09_sys_mag. These distances are each derived from homogeneous IMACS photometry, are anchored to independent geometric zero-points, and utilize different classes of stars. We therefore average over independent uncertainties and report the combined distance modulus &lt;{mu}_0_&gt;=20.770+/-0.042_stat_+/-0.024_sys_mag (corresponding to a distance of 143+/-3kpc).</description><source format="bibcode">2022ApJ...929..116O</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/929/116</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/195">VII/195 : Globular Clusters in the Milky Way (Harris, 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/202">VII/202 : Globular Clusters in the Milky Way (Harris, 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/355">I/355 : Gaia DR3 Part 1. 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