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<ri:Resource created="2020-06-18T15:39:48Z" status="active" updated="2025-05-19T09:50:00Z" 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>Narrowband Ca photometry for dwarf spheroidal galaxies</title><shortName>J/ApJS/247/7</shortName><identifier>ivo://CDS.VizieR/J/ApJS/247/7</identifier><altIdentifier>doi:10.26093/cds/vizier.22470007</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Han S.-I.</name></creator><creator><name>Kim H.-S.</name></creator><creator><name>Yoon S.-J.</name></creator><creator><name>Lee Y.-W.</name></creator><creator><name>Arimoto N.</name></creator><creator><name>Okamoto S.,Ree C.H.</name></creator><date role="Updated">2021-09-06T19:12:15Z</date><date role="Created">2020-06-18T15:39:48Z</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>galaxies</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>A few dozen dwarf satellite galaxies of the Milky Way have been discovered, which are often viewed as the remaining building blocks of our Galaxy. The follow-up spectroscopy showed that dwarf galaxies have a sizeable spread in their metallicities. Several scenarios were suggested to explain the metallicity spread, which can be tested by the structural patterns of stellar subpopulations with distinct metallicities. However, such chemical plus structural examination, which we refer to as "chemostructural study", is hindered by the lack of stars with spectroscopic metallicity. Here we propose the Ca-by photometry as an alternative way to secure metallicities for a 2-3 orders of magnitude larger stellar sample than the spectroscopic sample and thus enable us to perform a chemostructural study on dwarf galaxies. In particular, we use the hk index [=(Ca-b)-(b-y)], whose validity as a photometric metallicity indicator (and crass insensitivity to age) for red-giant-branch stars was upheld via Galactic globular clusters, and observe three dwarf spheroidal galaxies-Draco, Sextans, and Canes Venatici I (CVnI)-with Subaru/Suprime-Cam. We find that in all the galaxies the metal-rich stellar populations are more centrally concentrated than the metal-poor counterparts, suggesting that the central regions of the galaxies underwent extended star formation. Such a negative radial metallicity gradient for Sextans and CVnI opposes the traditional spectroscopic results. We also find that their metallicity distribution functions (MDFs) can be characterized by a unimodal, skewed Gaussian shape with a metal-rich peak and a metal-poor tail.</description><source format="bibcode">2020ApJS..247....7H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/247/7</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/I/284">I/284 : The USNO-B1.0 Catalog (Monet+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/107/32">J/PASP/107/32 : uvby-hk photometry in M22 (Anthony-Twarog+ 1995)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/116/1922">J/AJ/116/1922 : CaII H and K filter photometry III. (Anthony-Twarog+, 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/119/1824">J/AJ/119/1824 : Caby photometry of {Omega} Centauri (Rey+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/125/1383">J/AJ/125/1383 : Stromgren photometry of NGC 6253 (Anthony-Twarog+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/1000">J/AJ/127/1000 : Stromgren &amp; Ca photom. of NGC 3680 (Anthony-Twarog+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/459/423">J/A+A/459/423 : VI and [Fe/H] of Fornax dSph RGB stars (Battaglia+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/454/333">J/A+A/454/333 : Computed Hbeta indices from ATLAS9 model (Castelli+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/895">J/AJ/131/895 : Stars in the Carina dwarf spheroidal galaxy (Koch+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/191/352">J/ApJS/191/352 : Abundances in stars of MW dwarf satellites (Kirby+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/411/1013">J/MNRAS/411/1013 : CaII triplet in Sextans dSph galaxy (Battaglia+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/142/127">J/AJ/142/127 : NGC 5822 UBVI and uvbyCaH{beta} photometry (Carraro+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/4">J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/778/L13">J/ApJ/778/L13 : Subaru new Ca filter transmission function (Lee+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/789/147">J/ApJ/789/147 : Star formation histories of LG dwarf galaxies (Weisz+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/216/19">J/ApJS/216/19 : Spectroscopic HK' index for 3 globular clusters (Lim+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/456/3757">J/MNRAS/456/3757 : Open-cluster density profiles (Seleznev, 2016)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/247/7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/247/7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/247/7</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/247/7</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/247/7</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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