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<ri:Resource created="2021-12-17T15:47:23Z" 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>CLEAR. II. SFRs of quiescent galaxies</title><shortName>J/ApJ/898/171</shortName><identifier>ivo://CDS.VizieR/J/ApJ/898/171</identifier><altIdentifier>doi:10.26093/cds/vizier.18980171</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Estrada-Carpenter V.</name></creator><creator><name>Papovich C.</name></creator><creator><name>Momcheva I.</name></creator><creator><name>Brammer G.</name></creator><creator><name>Simons R.,Bridge J.</name></creator><creator><name>Cleri N.J.</name></creator><creator><name>Ferguson H.</name></creator><creator><name>Finkelstein S.L.</name></creator><creator><name>Giavalisco M.,Jung I.</name></creator><creator><name>Matharu J.</name></creator><creator><name>Trump J.R.</name></creator><creator><name>Weiner B.</name></creator><date role="Updated">2023-06-16T15:30:29Z</date><date role="Created">2021-12-17T15:47:23Z</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>hst-photometry</subject><subject>redshifted</subject><description>The origin of the correlations between mass, morphology, quenched fraction, and formation history in galaxies is difficult to define, primarily due to the uncertainties in galaxy star formation histories (SFHs). SFHs are better constrained for higher redshift galaxies, observed closer to their formation and quenching epochs. Here we use "nonparametric" SFHs and a nested sampling method to derive constraints on the formation and quenching timescales of quiescent galaxies at 0.7&lt;z&lt;2.5. We model deep HST grism spectroscopy and photometry from the CLEAR (CANDELS Ly{alpha} Emission at Reionization) survey. The galaxy formation redshifts, z50 (defined as the point where they had formed 50% of their stellar mass) range from z_50_~2 (shortly prior to the observed epoch) up to z_50_~5-8. We find that early formation redshifts are correlated with high stellar-mass surface densities, log{Sigma}_1_/(M_{sun}_kpc^-2^)&gt;10.25, where {Sigma}_1_ is the stellar mass within 1pkpc (proper kpc). Quiescent galaxies with the highest stellar-mass surface density, log{Sigma}_1_/(M_{sun}_kpc^-2^)&gt;10.25, show a minimum formation redshift: all such objects in our sample have z_50_&gt;2.9. Quiescent galaxies with lower surface density, log{Sigma}_1_/(M_{sun}_kpc^-2^)=9.5-10.25, show a range of formation epochs (z_50_~1.5-8), implying these galaxies experienced a range of formation and assembly histories. We argue that the surface density threshold log{Sigma}_1_/(M_{sun}_kpc^-2^)&gt;10.25 uniquely identifies galaxies that formed in the first few Gyr after the big bang, and we discuss the implications this has for galaxy formation models.</description><source format="bibcode">2020ApJ...898..171E</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/898/171</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/I/347">I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)</relatedResource><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/ApJS/172/615">J/ApJS/172/615 : GALFIT result for GEMS galaxies (Haussler+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/528/A35">J/A+A/528/A35 : Infrared luminosity in GOODS fields (Magnelli+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/735/86">J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/73">J/ApJ/763/73 : Surface density profiles of GOODS-South gal. 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