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<ri:Resource created="2020-04-21T14:53:37Z" status="active" updated="2025-06-13T15:25:00Z" 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>Quasars narrow absorption lines from SDSS</title><shortName>J/MNRAS/468/L6</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/468/L6</identifier><altIdentifier>doi:10.26093/cds/vizier.74689006</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Lu W.-J.</name></creator><creator><name>Lin Y.-R.</name></creator><creator><name>Qin Y.-P.</name></creator><creator><name>Huang W.-R.</name></creator><creator><name>Pan C.-J.</name></creator><creator><name>Huang H.-Y.,Yao M.</name></creator><creator><name>Nong W.-J.</name></creator><creator><name>Yao Z.-K.</name></creator><creator><name>Lu M.-M.</name></creator><creator><name>Pan D.-S.</name></creator><creator><name>Huang H.-Q.</name></creator><creator><name>Han Q.-L.</name></creator><date role="Updated">2024-08-17T20:19:00Z</date><date role="Created">2020-04-21T14:53:37Z</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>redshifted</subject><subject>line-intensities</subject><description>In this Letter, we report the discovery of a strong correlation between the variability of narrow absorption lines (NALs) and the ionizing continuum from a two-epoch spectral sample of 40 quasars containing 52 variable CIV {lambda}{lambda}1548, 1551 absorption doublets. According to the concordance index, this sample is classified into two subsamples. Subsample I shows an anti-correlation between the variations of absorption lines and the continuum, while Subsample II exhibits a positive correlation. These results imply that these variable CIV {lambda}{lambda}1548, 1551 absorption doublets are intrinsic to the corresponding quasars and that their variations are caused primarily by the fluctuations of the ionizing continuum. Based on our analysis, we propose that there might be two kinds of absorption gas: one that is very sensitive to the continuum variations, and another that is not. In addition, we suggest that in many cases the emergence or disappearance of NALs is caused by fluctuations of the ionizing continuum.</description><source format="bibcode">2017MNRAS.468L...6L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/468/L6</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/405/2302">J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/450/3904">J/MNRAS/450/3904 : Quasars narrow absorption lines from SDSS (Chen+, 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/468/L6</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/468/L6</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/468/L6</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/468/L6</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/468/L6</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/468/L6</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/468/L6/table1 (CIV absorption systems and the continuum data)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/468/L6/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/468/L6/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/468/L6/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>12.988545</ra><dec>0.0652181</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/4625 4646 4667 4813 5337 5363 5434 5504 6198 6213 6599 6916 8192 9374 9394 9406 9410-9411 10765 17754 17821 17840 18025 18834 19025 19094 19099 26023 26093 26199 26257 26331 27045 27058 27260 27303 27333 27658 27666 31531</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/468/L6?format=ascii</footprint></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/468/L6/table1</name><description>CIV absorption systems and the continuum data</description><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>SDSS</name><description>SDSS identifier, HHMMSS.ss+DDMMSS.s</description><ucd>meta.id.part</ucd><dataType xsi:type="vs:VOTableType" arraysize="18*">char</dataType></column><column><name>zem</name><description>Redshift derived from emission lines (1)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>zabs</name><description>Redshift derived from absorption lines (2)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fcont1</name><description>Flux of the pseudo-continuum for the earlier epoch (3)</description><unit>1e-19W.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Fcont1</name><description>Error of Fcont1</description><unit>1e-19W.m**-2.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fcont2</name><description>Flux of the pseudo-continuum for the later epoch (3)</description><unit>1e-19W.m**-2.nm**-1</unit><ucd>phot.flux</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Fcont2</name><description>Error of Fcont2</description><unit>1e-19W.m**-2.nm**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DFcont</name><description>Flux variability amplitude</description><ucd>src.var.amplitude</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_DFcont</name><description>Error of flux variability amplitude</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DEW48</name><description>Equivalent widths variability amplitude of C IV {lambda}1548</description><ucd>src.var.amplitude</ucd></column><column><name>e_DEW48</name><description>Error of equivalent widths variability amplitude</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DEW51</name><description>Equivalent widths variability amplitude of C IV {lambda}1551</description><ucd>src.var.amplitude</ucd></column><column><name>e_DEW51</name><description>Error of equivalent widths variability amplitude</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Index</name><description>[-1/1]? 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