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<ri:Resource created="2023-10-27T06:46:09Z" status="active" updated="2025-05-19T20:08:55Z" 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>COSMOS2020; 230 quiescent galaxies at 3&lt;z&lt;5</title><shortName>J/AJ/165/248</shortName><identifier>ivo://CDS.VizieR/J/AJ/165/248</identifier><altIdentifier>doi:10.26093/cds/vizier.51650248</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gould K.M.L.</name></creator><creator><name>Brammer G.</name></creator><creator><name>Valentino F.</name></creator><creator><name>Whitaker K.E.</name></creator><creator><name>Weaver J.R.,del Lagos C. P</name></creator><creator><name>Rizzo F.</name></creator><creator><name>Franco M.</name></creator><creator><name>Hsieh B.-C.</name></creator><creator><name>Ilbert O.</name></creator><creator><name>Jin S.,Magdis G.</name></creator><creator><name>McCracken H. J</name></creator><creator><name>Mobasher B.</name></creator><creator><name>Shuntov M.</name></creator><creator><name>Steinhardt C.L.,Strait V.</name></creator><creator><name>Toft S.</name></creator><date role="Updated">2025-05-19T20:08:55Z</date><date role="Created">2023-10-27T06:46:09Z</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>star-forming-regions</subject><subject>redshifted</subject><subject>infrared-astronomy</subject><description>We select and characterize a sample of massive (log(M*/M{sun})&gt;10.6) quiescent galaxies (QGs) at 3&lt;z&lt;5 in the latest Cosmological Evolution Survey catalog (COSMOS2020). QGs are selected using a new rest-frame color-selection method, based on their probability of belonging to the quiescent group defined by a Gaussian mixture model (GMM) trained on rest-frame colors (NUV-U, U-V, V J) of similarly massive galaxies at 2&lt;z&lt;3. We calculate the quiescent probability threshold above which a galaxy is classified as quiescent using simulated galaxies from the shark semi-analytical model. We find that, at z&gt;=3 in shark, the GMM/NUVU-VJ method outperforms classical rest-frame UVJ selection and is a viable alternative. We select galaxies as quiescent based on their probability in COSMOS2020 at 3&lt;z&lt;5, and compare the selected sample to both UVJ- and NUVrJ-selected samples. We find that, although the new selection matches UVJ and NUVrJ in number, the overlap between color selections is only ~50%-80%, implying that rest-frame color commonly used at lower-redshift selections cannot be equivalently used at z&gt;3. We compute median rest-frame spectral energy distributions for our sample and find the median QG at 3&lt;z&lt;5 has a strong Balmer/4000{AA} break, and residual NUV flux indicating recent quenching. We find the number densities of the entire quiescent population (including post-starbursts) more than doubles from 3.5{+/-}2.2x10^-6^Mpc^-3^ at 4&lt;z&lt;5 to 1.4{+/-}0.4x10^-5^Mpc^-3^ at 3&lt;z&lt;4, confirming that the onset of massive galaxy quenching occurs as early as 3&lt;z&lt;5.</description><source format="bibcode">2023AJ....165..248G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/165/248</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/VII/233">VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/1184">J/AJ/131/1184 : Recalibration of optical photometry (Maiz-Apellaniz+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/682/985">J/ApJ/682/985 : FIREWORKS photometry of GOODS CDF-S (Wuyts+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/735/86">J/ApJ/735/86 : NEWFIRM MBS; 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