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<ri:Resource created="2025-04-16T10:46:30Z" status="active" updated="2026-07-02T11:58:28Z" 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>SFHs of GOODS z=0-3.5 gal. with X-ray em.</title><shortName>J/ApJ/926/28</shortName><identifier>ivo://CDS.VizieR/J/ApJ/926/28</identifier><altIdentifier>doi:10.26093/cds/vizier/ba-wy-w</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gilbertson W.</name></creator><creator><name>Lehmer B.D.</name></creator><creator><name>Doore K.</name></creator><creator><name>Eufrasio R.T.</name></creator><creator><name>Basu-Zych A.,Brandt W.N.</name></creator><creator><name>Fragos T.</name></creator><creator><name>Garofali K.</name></creator><creator><name>Kovlakas K.</name></creator><creator><name>Luo B.</name></creator><creator><name>Tozzi P.,Vito F.</name></creator><creator><name>Williams B.F.</name></creator><creator><name>Xue Y.</name></creator><date role="Updated">2026-07-02T11:58:28Z</date><date role="Created">2025-04-16T10:46:30Z</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>spectral-energy-distribution</subject><subject>x-ray-binary-stars</subject><subject>redshifted</subject><subject>stellar-ages</subject><subject>stellar-masses</subject><description>The Chandra Deep Field-South and North surveys (CDFs) provide unique windows into the cosmic history of X-ray emission from normal (nonactive) galaxies. Scaling relations of normal-galaxy X-ray luminosity (L_X_) with star formation rate (SFR) and stellar mass (M_*_) have been used to show that the formation rates of low-mass and high-mass X-ray binaries (LMXBs and HMXBs, respectively) evolve with redshift across z~0-2 following L_HMXB_/SFR{propto}(1+z) and L_LMXB_/M*{propto}(1+z)^2-3^. However, these measurements alone do not directly reveal the physical mechanisms behind the redshift evolution of X-ray binaries (XRBs). We derive star formation histories for a sample of 344 normal galaxies in the CDFs, using spectral energy distribution (SED) fitting of FUV-to-FIR photometric data, and construct a self-consistent, age-dependent model of the X-ray emission from the galaxies. Our model quantifies how X-ray emission from hot gas and XRB populations vary as functions of host stellar-population age. We find that (1) the ratio L_X_/M_*_ declines by a factor of ~1000 from 0 to 10Gyr and (2) the X-ray SED becomes harder with increasing age, consistent with a scenario in which the hot gas contribution to the X-ray SED declines quickly for ages above 10Myr. When dividing our sample into subsets based on metallicity, we find some indication that L_X_/M_*_ is elevated for low-metallicity galaxies, consistent with recent studies of X-ray scaling relations. However, additional statistical constraints are required to quantify both the age and metallicity dependence of X-ray emission from star-forming galaxies.</description><source format="bibcode">2022ApJ...926...28G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/926/28</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/VIII/10">VIII/10 : Bell Laboratories H I Profiles (Stark+ 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/28">VIII/28 : Bell Laboratories H I Survey (Stark+ 1992)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/261">II/261 : GOODS initial results (Giavalisco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/79/77">J/ApJS/79/77 : Bell Lab. 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