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<ri:Resource created="2019-03-06T14:03:20Z" 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>Stellar mass-metallicity relation. I.</title><shortName>J/ApJ/856/15</shortName><identifier>ivo://CDS.VizieR/J/ApJ/856/15</identifier><altIdentifier>doi:10.26093/cds/vizier.18560015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Leethochawalit N.</name></creator><creator><name>Kirby E.N.</name></creator><creator><name>Moran S.M.</name></creator><creator><name>Ellis R.S.</name></creator><creator><name>Treu T.</name></creator><date role="Updated">2019-03-07T14:49:29Z</date><date role="Created">2019-03-06T14:03:20Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>spectroscopy</subject><subject>metallicity</subject><subject>stellar-masses</subject><subject>surveys</subject><description>We present the stellar mass-stellar metallicity relationship (MZR) in the galaxy cluster Cl0024+1654 at z~0.4 using full-spectrum stellar population synthesis modeling of individual quiescent galaxies. The lower limit of our stellar mass range is M*=10^9.7^M_{sun}_, the lowest galaxy mass at which individual stellar metallicity has been measured beyond the local universe. We report a detection of an evolution of the stellar MZR with observed redshift at 0.037+/-0.007dex per Gyr, consistent with the predictions from hydrodynamical simulations. Additionally, we find that the evolution of the stellar MZR with observed redshift can be explained by an evolution of the stellar MZR with the formation time of galaxies, i.e., when the single stellar population (SSP)-equivalent ages of galaxies are taken into account. This behavior is consistent with stars forming out of gas that also has an MZR with a normalization that decreases with redshift. Lastly, we find that over the observed mass range, the MZR can be described by a linear function with a shallow slope ([Fe/H]{propto}(0.16+/-0.03)logM*). The slope suggests that galaxy feedback, in terms of mass-loading factor, might be mass-independent over the observed mass and redshift range.</description><source format="bibcode">2018ApJ...856...15L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/856/15</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/III/232">III/232 : STELIB: A library of stellar spectra at R~2000 (Le Borgne+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/372/391">J/A+A/372/391 : Spectroscopic Survey of Cl 0024+1654 (Czoske+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/591/53">J/ApJ/591/53 : I photometry of Cl 0024+16 (Treu+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/2644">J/AJ/126/2644 : CL 0024+1654 UBVI photometry (Alexov+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/127/2002">J/AJ/127/2002 : Star Formation Rate of NFGS galaxies (Kewley+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/634/977">J/ApJ/634/977 : Redshifts in Cl 0024+16 members (Moran+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/371/703">J/MNRAS/371/703 : MILES library of empirical spectra (Sanchez-Blazquez+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/665/1067">J/ApJ/665/1067 : Velocities in Cl 0024+16 and MS 0451-03 (Moran+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/1138">J/ApJ/659/1138 : Intermediate-redshift spiral galaxies Vmax (Moran+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/671/1503">J/ApJ/671/1503 : Cl 0024+16 and MS 0451-03 spectrophotometry (Moran+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/404/1639">J/MNRAS/404/1639 : MILES base models &amp; new line index system (Vazdekis+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/200/8">J/ApJS/200/8 : AGES: the AGN and Galaxy Evolution Survey (Kochanek+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/432/3141">J/MNRAS/432/3141 : Morphological classification of PM2GC gal. 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