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<ri:Resource created="2011-06-20T08:54:17Z" 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>Lyman break galaxies at z~1.8-2.8</title><shortName>J/ApJ/697/1410</shortName><identifier>ivo://CDS.VizieR/J/ApJ/697/1410</identifier><altIdentifier>doi:10.26093/cds/vizier.16971410</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ly C.</name></creator><creator><name>Malkan M.A.</name></creator><creator><name>Treu T.</name></creator><creator><name>Woo J.-H.</name></creator><creator><name>Currie T.</name></creator><creator><name>Hayashi M.,Kashikawa N.</name></creator><creator><name>Motohara K.</name></creator><creator><name>Shimasaku K.</name></creator><creator><name>Yoshida M.</name></creator><date role="Updated">2018-01-04T08:22:37Z</date><date role="Created">2011-06-20T08:54:17Z</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>photometry</subject><subject>redshifted</subject><subject>spectroscopy</subject><description>A photometric sample of ~8000 V&lt;25.3 candidate Lyman break galaxies (LBGs) has been selected by combining Subaru/Suprime-Cam BVRCi'z' optical data with deep GALEX/NUV imaging of the Subaru Deep Field. Follow-up spectroscopy confirmed 24 LBGs at 1.5&lt;~z&lt;~2.7. Among the optical spectra, 12 have Ly{alpha} emission with rest-frame equivalent widths of ~5-60{AA}. The success rate for identifying LBGs as NUV-dropouts at 1.5&lt;z&lt;2.7 is 86%. The rest-frame UV (1700{AA}) luminosity function (LF) is constructed from the photometric sample with corrections for stellar contamination and z&lt;1.5 interlopers (lower limits). The LF is 1.7+/-0.1 (1.4+/-0.1 with a hard upper limit on stellar contamination) times higher than those of z~2 BXs and z~3 LBGs.</description><source format="bibcode">2009ApJ...697.1410L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/697/1410</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/B/subaru">B/subaru : Log of Subaru Prime Focus Camera Exposures (ADAC NAOJ, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/401/1521">J/MNRAS/401/1521 : Stellar masses of Lyman break galaxies at z~3 (Magdis+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/380/986">J/MNRAS/380/986 : Lyman-break galaxies from GALEX (Burgarella+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/657/738">J/ApJ/657/738 : SDF galaxies multi-photometry (Ly+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/58/313">J/PASJ/58/313 : Ly{alpha} emitters in the SUBARU Deep Field (Shimasaku+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASJ/57/165">J/PASJ/57/165 : Ly{alpha} emitters in the SUBARU Deep Field (Taniguchi+,</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/592/728">J/ApJ/592/728 : Lyman break galaxies at redshift z~3 (Steidel+, 2003)</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/ApJ/697/1410</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/697/1410</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/697/1410</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/697/1410</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/697/1410</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/697/1410</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/ApJ/697/1410/table1 (Properties of spectroscopically targeted NUV-dropouts and BzKs)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/697/1410/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/697/1410/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/697/1410/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>201.1325</ra><dec>27.703967</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/10297 10298 10299</spatial><spectral>2.680029793928555e-19 9.736485774071566e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/697/1410?format=ascii</footprint><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/697/1410/table1</name><description>Properties of spectroscopically targeted NUV-dropouts and BzKs</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Cross-correlated redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>f_z</name><description>[d] low S/N (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>R</name><description>? Cross-correlation signal to noise</description><ucd>stat.snr</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Temp</name><description>Template yielding the highest R value (4)</description><ucd>meta.id;stat.fit</ucd></column><column><name>F(Lya)</name><description>? 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