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<ri:Resource created="2026-07-28T11:09:20Z" status="active" updated="2026-07-28T10:15:24Z" 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>Gas-phase mass-metallicity relation for LEGA-C gal.</title><shortName>J/ApJ/964/59</shortName><identifier>ivo://CDS.VizieR/J/ApJ/964/59</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lewis Z.J.</name></creator><creator><name>Andrews B.H.</name></creator><creator><name>Bezanson R.</name></creator><creator><name>Maseda M.</name></creator><creator><name>Bell E.F.</name></creator><creator><name>Dave R.,D'Eugenio F.</name></creator><creator><name>Franx M.</name></creator><creator><name>Gallazzi A.</name></creator><creator><name>de Graaff A.</name></creator><creator><name>Kaushal Y.,Nersesian A.</name></creator><creator><name>Newman J.A.</name></creator><creator><name>van der Wel A.</name></creator><creator><name>Wu P.-F.</name></creator><date role="Updated">2026-07-28T10:15:24Z</date><date role="Created">2026-07-28T11:09:20Z</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>spectroscopy</subject><subject>visible-astronomy</subject><subject>redshifted</subject><subject>extinction</subject><subject>chemical-abundances</subject><description>The massive end of the gas-phase mass-metallicity relation (MZR) is a sensitive probe of active galactic nuclei (AGN) feedback that is a crucial but highly uncertain component of galaxy evolution models. In this paper, we extend the z~0.7 MZR by ~0.5dex up to log(M*/M_{sun}_)~11.1. We use extremely deep VLT VIMOS spectra from the Large Early Galaxy Astrophysics Census (LEGA-C) survey to measure metallicities for 145 galaxies. The LEGA-C MZR matches the normalization of the z~0.8 DEEP2 MZR where they overlap, so we combine the two to create an MZR spanning from 9.3 to 11.1 log(M*/M_{sun}_). The LEGA-C+DEEP2 MZR at z~0.7 is offset to slightly lower metallicities (0.05-0.13 dex) than the z~0 MZR, but it otherwise mirrors the established power-law rise at low/intermediate stellar masses and asymptotic flattening at high stellar masses. We compare the LEGA-C+DEEP2 MZR to the MZR from two cosmological simulations (IllustrisTNG and SIMBA), which predict qualitatively different metallicity trends for high-mass galaxies. This comparison highlights that our extended MZR provides a crucial observational constraint for galaxy evolution models in a mass regime where the MZR is very sensitive to choices about the implementation of AGN feedback.</description><source format="bibcode">2024ApJ...964...59L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/964/59</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/II/373">II/373 : The fourth UltraVISTA data release (DR4) (Moneti+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/617/240">J/ApJ/617/240 : Oxygen abundances in the GOODS-North field (Kobulnicky+, 2004)</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/A+A/544/A156">J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/765/140">J/ApJ/765/140 : Stacked spectra of SDSS star forming galaxies (Andrews+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/777/18">J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/206/8">J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/469/2121">J/MNRAS/469/2121 : Mass-metallicity relations with CALIFA (Sanchez+ 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/239/27">J/ApJS/239/27 : LEGA-C DR2: galaxies in the COSMOS field (Straatman+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/484/3042">J/MNRAS/484/3042 : The gas-phase mass-metallicity relation (Sanchez+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/913/103">J/ApJ/913/103 : SED modelling of LEGA-C &amp; HST massive gal. 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