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<ri:Resource created="2025-02-25T16:40:20Z" 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>HST/ACS stellar photometry for Reticulum II</title><shortName>J/ApJ/944/43</shortName><identifier>ivo://CDS.VizieR/J/ApJ/944/43</identifier><altIdentifier>doi:10.26093/cds/vizier.19440043</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Simon J.D.</name></creator><creator><name>Brown T.M.</name></creator><creator><name>Mutlu-Pakdil B.</name></creator><creator><name>Ji A.P.</name></creator><creator><name>Drlica-Wagner A.,Avila R.J.</name></creator><creator><name>Martinez-Vazquez C.E.</name></creator><creator><name>Li T.S.</name></creator><creator><name>Balbinot E.</name></creator><creator><name>Bechtol K.,Frebel A.</name></creator><creator><name>Geha M.</name></creator><creator><name>Hansen T.T.</name></creator><creator><name>James D.J.</name></creator><creator><name>Pace A.B.</name></creator><creator><name>Aguena M.,Alves O.</name></creator><creator><name>Andrade-Oliveira F.</name></creator><creator><name>Annis J.</name></creator><creator><name>Bacon D.</name></creator><creator><name>Bertin E.</name></creator><creator><name>Brooks D.,Burke D.L.</name></creator><creator><name>Rosell A.C.</name></creator><creator><name>Kind M.C.</name></creator><creator><name>Carretero J.</name></creator><creator><name>Costanzi M.,da Costa L.N.</name></creator><creator><name>De Vicente J.</name></creator><creator><name>Desai S.</name></creator><creator><name>Doel P.</name></creator><creator><name>Everett S.</name></creator><creator><name>Ferrero I.,Frieman J.</name></creator><creator><name>Garcia-Bellido J.</name></creator><creator><name>Gatti M.</name></creator><creator><name>Gerdes D.W.</name></creator><creator><name>Gruen D.,Gruendl R.A.</name></creator><creator><name>Gschwend J.</name></creator><creator><name>Gutierrez G.</name></creator><creator><name>Hinton S.R.</name></creator><creator><name>Hollowood D.L.,Honscheid K.</name></creator><creator><name>Kuehn K.</name></creator><creator><name>Kuropatkin N.</name></creator><creator><name>Marshall J.L.</name></creator><creator><name>Mena-Fernandez J.,Miquel R.</name></creator><creator><name>Palmese A.</name></creator><creator><name>Paz-Chinchon F.</name></creator><creator><name>Pereira M.E.S.</name></creator><creator><name>Pieres A.,Malagon A.A.P.</name></creator><creator><name>Raveri M.</name></creator><creator><name>Rodriguez-Monroy M.</name></creator><creator><name>Sanchez E.</name></creator><creator><name>Santiago B.,Scarpine V.</name></creator><creator><name>Sevilla-Noarbe I.</name></creator><creator><name>Smith M.</name></creator><creator><name>Suchyta E.</name></creator><creator><name>Swanson M.E.C.,Tarle G.</name></creator><creator><name>To C.</name></creator><creator><name>Vincenzi M.</name></creator><creator><name>Weaverdyck N.</name></creator><creator><name>Wilkinson R.D.</name></creator><date role="Updated">2025-03-07T20:10:39Z</date><date role="Created">2025-02-25T16:40:20Z</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>local-group</subject><subject>hst-photometry</subject><subject>visible-astronomy</subject><description>The ultra-faint dwarf galaxy Reticulum II (Ret II) exhibits a unique chemical evolution history, with 72_-12_^+10^% of its stars strongly enhanced in r-process elements. We present deep Hubble Space Telescope photometry of Ret II and analyze its star formation history. As in other ultra-faint dwarfs, the color-magnitude diagram is best fit by a model consisting of two bursts of star formation. If we assume that the bursts were instantaneous, then the older burst occurred around the epoch of reionization, forming ~80% of the stars in the galaxy, while the remainder of the stars formed ~3Gyr later. When the bursts are allowed to have nonzero durations, we obtain slightly better fits. The best-fitting model in this case consists of two bursts beginning before reionization, with approximately half the stars formed in a short (100Myr) burst and the other half in a more extended period lasting 2.6Gyr. Considering the full set of viable star formation history models, we find that 28% of the stars formed within 500+/-200Myr of the onset of star formation. The combination of the star formation history and the prevalence of r-process-enhanced stars demonstrates that the r-process elements in Ret II must have been synthesized early in its initial star-forming phase. We therefore constrain the delay time between the formation of the first stars in Ret II and the r-process nucleosynthesis to be less than 500Myr. This measurement rules out an r-process source with a delay time of several Gyr or more, such as GW170817.</description><source format="bibcode">2023ApJ...944...43S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/944/43</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/J/AJ/129/2714">J/AJ/129/2714 : JHK photometry of M92 variable stars (Del Principe+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/708/560">J/ApJ/708/560 : Spectroscopy of UMa II and Coma Ber (Frebel+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/778/149">J/ApJ/778/149 : Abundances for 3 stars in Sgr dSph (McWilliam+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/786/74">J/ApJ/786/74 : EW measurements of 6 Segue 1 red giants (Frebel+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A146">J/A+A/562/A146 : Chemical abundances of 8 metal-poor stars (Ishigaki+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/808/95">J/ApJ/808/95 : Spectroscopy of Reticulum II (Simon+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/802/93">J/ApJ/802/93 : Abundance analysis of 5 stars in Sculptor (Simon+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/830/93">J/ApJ/830/93 : Abund. of the Ret II brightest red giant members (Ji+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/817/41">J/ApJ/817/41 : Abundances of 4 metal-poor red giants in BooII (Ji+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/151/82">J/AJ/151/82 : The 4 brightest red giants in Ret 2 (Roederer+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/838/44">J/ApJ/838/44 : Abund. of the brightest member of Tuc III (Hansen+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/850/137">J/ApJ/850/137 : ISLAndS project. 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