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<ri:Resource created="2025-02-18T16:38:21Z" 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>UVW1 galaxy sources in CDFS deep field</title><shortName>J/MNRAS/511/4882</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/511/4882</identifier><altIdentifier>doi:10.26093/cds/vizier.75114882</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sharma M.</name></creator><creator><name>Page M.J.</name></creator><creator><name>Breeveld A.A.</name></creator><date role="Updated">2025-03-03T20:14:30Z</date><date role="Created">2025-02-18T16:38:21Z</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>catalogs</subject><subject>ultraviolet-photometry</subject><subject>redshifted</subject><subject>spectroscopy</subject><subject>surveys</subject><description>We present the rest-frame ultraviolet (UV) galaxy luminosity function (LF) and luminosity density (LD) measurements in the far-UV (1500 {AA}) wavelength, in the redshift range z = 0.6-1.2. The UV LF is derived using XMM-Newton Optical Monitor (XMM-OM), UV (1600-4000 {AA}) observations of the Chandra Deep Field South, over an area of 396 arcmin^2^. Using the deep UV imaging of the CDFS, we identified &gt; 2500 galaxies in our sample with UVW1AB &lt;= 24.5 mag. This sample, along with various other catalogues containing redshift information, is used to calculate the binned representation of the galaxy UV LF in the two redshift bins 0.6 &lt;= z &lt; 0.8 and 0.8 &lt;= z &lt; 1.2, having a wide range of 1500 {AA} rest-frame UV magnitudes ({Delta}M_1500_ ~= 3), reaching ~= 1-1.5 magnitudes fainter than previous studies at similar redshifts. The binned LF is described well by the Schechter function form. Using maximum-likelihood, the Schechter function is fitted to the unbinned data to obtain the best-fitting values of the the UV galaxy LF parameters. We find that characteristic magnitude M* brightens by 0.8 mag from z = 0.7 to z = 1, implying an increase in the star formation activity between these redshifts, as reported by past studies. Our estimate of the faint- end slope -1.10^{+0.19}^_{-0.18}_ is on the shallower side compared with previous studies at z = 0.7, whereas a value of -1.56^{+0.19}^_{-0.18}_ estimated for z = 1.0, agrees with previous results given the uncertainties.</description><source format="bibcode">2022MNRAS.511.4882S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/511/4882</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/MNRAS/506/473">J/MNRAS/506/473 : UV luminosity functions of SFR galaxies (Page+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/378">II/378 : XMM-OM Serendipitous Source Survey Catalogue (XMM-SUSS6.0)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/796/60">J/ApJ/796/60 : ECDFS galaxies photometric redshifts &amp; counterparts</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/801/97">J/ApJ/801/97 : GOODS-S &amp; UDS stellar mass catalogs from CANDELS</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/183/295">J/ApJS/183/295 : A K-selected catalog of the ECDFS from MUSYC (Taylor+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/189/270">J/ApJS/189/270 : MUSYC optical imaging in ECDF-S (Cardamone+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/742/3">J/ApJ/742/3 : Photometric catalogs for ECDF-S and CDF-N (Rafferty+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/191/124">J/ApJS/191/124 : Optical spectroscopy of ECDF-S X-ray sources</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/512/A12">J/A+A/512/A12 : VLT/VIMOS spectroscopy in GOODS-South field (Balestra+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/465/1099">J/A+A/465/1099 : Redshift catalog of 691 objects in CDFS (Ravikumar+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/253">II/253 : Chandra Deep Field South: multi-colour data (Wolf+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/421/41">J/A+A/421/41 : FORS Deep Field UV to blue photometry (Gabasch+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/261">II/261 : GOODS initial results (Giavalisco+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/803/34">J/ApJ/803/34 : z~4-10 galaxies from HST legacy fields (Bouwens+, 2015)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/511/4882</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/511/4882</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/511/4882</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/511/4882</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/511/4882</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/511/4882</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/MNRAS/511/4882/table3 (CDFS UVW1 source catalogue)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/511/4882/table3?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/511/4882/table3?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/511/4882/table3?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>53.21690389</ra><dec>-27.74170306</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/35935 35957</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/511/4882?format=ascii</footprint><waveband>UV</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/511/4882/table3</name><description>CDFS UVW1 source catalogue</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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