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<ri:Resource created="2023-06-16T14:11:12Z" 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>Type I quasars luminosity distances</title><shortName>J/A+A/674/A163</shortName><identifier>ivo://CDS.VizieR/J/A+A/674/A163</identifier><altIdentifier>doi:10.26093/cds/vizier.36740163</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Huang L.</name></creator><creator><name>Wang H.</name></creator><creator><name>Gao Z.</name></creator><creator><name>Zeng X.</name></creator><creator><name>Chang Z.</name></creator><date role="Updated">2024-11-28T20:03:40Z</date><date role="Created">2023-06-16T14:11:12Z</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>quasars</subject><subject>radio-sources</subject><subject>stellar-distance</subject><description>We use the anticorrelation between the equivalent width (EW) of the CIV 1549{AA} emission line and the continuum luminosity in the quasars rest frame (Baldwin effect) to measure their luminosity distance as well as estimate cosmological parameters. We obtain a sample of 471 Type I quasars with the UV-optical spectra and EW (CIV) measurements in the redshift range of 2.3&lt;z&lt;7.1 including 25 objects at 5&lt;z&lt;7.1, which can be used to investigate the CIV Baldwin effect and determine cosmological luminosity distance. The relation EW(CIV)~({lambda}L{lambda}){gamma} can be applied to check the inverse correlation between the CIV EW and L{lambda} of quasars and give their distance, and the data suggest that the EW of CIV is inversely correlated with continuum monochromatic luminosities. On the other hand, we also consider dividing the Type I quasar sample into various redshift bins, which can be used to check if the CIV EW-luminosity relation depends on the redshift. Finally, we apply a combination of Type I quasars and Type Ia supernovae (SNIa) of the Pantheon sample to test the property of dark energy concerning whether or not its density deviates from the constant, and give the statistical results</description><source format="bibcode">2023A&amp;A...674A.163H</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/674/A163</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></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/A+A/674/A163</accessURL><mirrorURL 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arraysize="*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>SDSS name of Type I quasars (HHMMSS.ss+DDMMSS.s)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>z</name><description>Redshift</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>rmag</name><description>SDSS r magnitude</description><unit>mag</unit><ucd>phot.mag;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_rmag</name><description>Error on r magnitude</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>EW(CIV)</name><description>Equivalent width of the CIV 1549{AA} emission line</description><unit>0.1nm</unit><ucd>spect.line.eqWidth</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_EW(CIV)</name><description>Error on EW(C IV)</description><unit>0.1nm</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>F2500</name><description>Rest-frame flux at 2500{AA}</description><unit>1e-07W.Hz**-1.m**-2</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_F2500</name><description>Error on Rest-frame flux at 2500{AA}</description><unit>1e-07W.Hz**-1.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>GammaUV</name><description>UV-optical power-law index</description><ucd>spect.index</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>DM</name><description>Distance modulus</description><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_DM</name><description>Error on distance modulus</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>_RA</name><description>Right Ascension (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Declination (J2000) from SIMBAD (not part of the original data)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>