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<ri:Resource created="2021-09-28T06:31:25Z" 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>Evolu. star mass-metallicity relation. II.</title><shortName>J/ApJ/885/100</shortName><identifier>ivo://CDS.VizieR/J/ApJ/885/100</identifier><altIdentifier>doi:10.26093/cds/vizier.18850100</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Leethochawalit N.</name></creator><creator><name>Kirby E.N.</name></creator><creator><name>Ellis R.S.</name></creator><creator><name>Moran S.M.</name></creator><creator><name>Treu T.</name></creator><date role="Updated">2022-07-25T09:23:11Z</date><date role="Created">2021-09-28T06:31:25Z</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>chemical-abundances</subject><subject>metallicity</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><subject>visible-astronomy</subject><subject>spectroscopy</subject><subject>ultraviolet-photometry</subject><subject>infrared-photometry</subject><description>We present the stellar mass-[Fe/H] and mass-[Mg/H] relation of quiescent galaxies in two galaxy clusters at z~0.39 and z~0.54. We derive the age, [Fe/H], and [Mg/Fe] for each individual galaxy using a full-spectrum fitting technique. By comparing with the relations for z~0 Sloan Digital Sky Survey galaxies, we confirm our previous finding that the mass-[Fe/H] relation evolves with redshift. The mass-[Fe/H] relation at higher redshift has lower normalization and possibly steeper slope. However, based on our sample, the mass-[Mg/H] relation does not evolve over the observed redshift range. We use a simple analytic chemical evolution model to constrain the average outflow that these galaxies experience over their lifetime, via the calculation of mass-loading factor. We find that the average mass-loading factor {eta} is a power-law function of galaxy stellar mass, {eta}{prop}M*^-0.21{+/-}0.09^. The measured mass-loading factors are consistent with the results of other observational methods for outflow measurements and with the predictions where outflow is caused by star formation feedback in turbulent disks.</description><source format="bibcode">2019ApJ...885..100L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/885/100</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/ApJ/621/673">J/ApJ/621/673 : Line indices for 124 early-type galaxies (Thomas+, 2005)</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/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/ApJS/200/8">J/ApJS/200/8 : AGES: the AGN and Galaxy Evolution Survey (Kochanek+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/779/102">J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A21">J/A+A/562/A21 : AGN feedback from CO observations (Cicone+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/788/72">J/ApJ/788/72 : Observed sample of z~0.7 massive galaxies (Gallazzi+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/466/2570">J/MNRAS/466/2570 : Low ioniza. emission-line regions galaxies (Belfiore+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/856/15">J/ApJ/856/15 : Stellar mass-metallicity relation. 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