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<ri:Resource created="2024-02-09T13:29:55Z" 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 population properties from LEGA-C DR2</title><shortName>J/ApJ/927/164</shortName><identifier>ivo://CDS.VizieR/J/ApJ/927/164</identifier><altIdentifier>doi:10.26093/cds/vizier.19270164</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Borghi N.</name></creator><creator><name>Moresco M.</name></creator><creator><name>Cimatti A.</name></creator><creator><name>Huchet A.</name></creator><creator><name>Quai S.</name></creator><creator><name>Pozzetti L.</name></creator><date role="Updated">2024-11-06T20:23:48Z</date><date role="Created">2024-02-09T13:29:55Z</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>chemical-abundances</subject><subject>stellar-ages</subject><subject>visible-astronomy</subject><description>We take advantage of the publicly available LEGA-C spectroscopic survey to measure the stellar population properties of 140 individual massive and passive galaxies at z~0.7. We develop and publicly release PyLick, a flexible Python code to measure UV to near-IR spectral indices. With PyLick we study the H/K ratio as a new diagnostic based on the pseudo-Lick CaII H and K indices and find that a cut in H/K&lt;1.1 can be used jointly with other criteria to select (or verify the purity of) samples of passive galaxies. By combining photometric and spectroscopic criteria, we select a reliable sample of passively evolving galaxies. We constrain single-burst stellar ages, metallicities [Z/H], and [{alpha}/Fe] with an optimized set of Lick indices, exploring in detail the robustness of our measurement against different combinations. Even without imposing cosmological priors, the derived ages follow a clear trend compatible with the expected cosmological aging of the universe. We observe no significant redshift evolution for the metal abundance with respect to the values derived at z=0, with median [Z/H]=0.08+/-0.18 and [{alpha}/Fe]=0.13+/-0.11. Finally, we analyze the relations between log age, [Z/H], [{alpha}/Fe], and the stellar velocity dispersion, finding slopes of (0.5+/-0.1), (0.3+/-0.2), and (0.2+/-0.1), respectively; the small scatter of &lt;0.2dex points to rather homogeneous and short star formation histories. Overall, these results confirm and extend low- redshift findings of a mass-downsizing evolution. This work further strengthens the possibility of selecting pure samples of passive galaxies to be exploited reliably as cosmic chronometers to place independent cosmological constraints.</description><source format="bibcode">2022ApJ...927..164B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/927/164</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/ApJS/82/197">J/ApJS/82/197 : Mean UV Spectra of Stellar Groups (Fanelli+ 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/94/687">J/ApJS/94/687 : Old stellar populations. V. 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