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<ri:Resource created="2017-09-27T08:58:59Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>QSO eHAQ0111+0641 spectra</title><shortName>J/A+A/606/A13</shortName><identifier>ivo://CDS.VizieR/J/A+A/606/A13</identifier><altIdentifier>doi:10.26093/cds/vizier.36060013</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Fynbo J.P.U.</name></creator><creator><name>Krogager J.-K.</name></creator><creator><name>Heintz K.E.</name></creator><creator><name>Geier S.</name></creator><creator><name>Moller P.,Noterdaeme P.</name></creator><creator><name>Christensen L.</name></creator><creator><name>Ledoux C.</name></creator><creator><name>Jakobsson P.</name></creator><date role="Updated">2017-10-26T11:52:35Z</date><date role="Created">2017-09-27T08:58:59Z</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>infrared-astronomy</subject><subject>spectroscopy</subject><description>It is important to understand the selection effects behind the quasar samples to fully exploit the potential of quasars as probes of cosmic chemical evolution and the internal gas dynamics of galaxies; in particular, it is vital to understand whether the selection criteria exclude foreground galaxies with certain properties, most importantly a high dust content. Here we present spectroscopic follow-up from the 10.4m GTC telescope of a dust-reddened quasar, eHAQ0111+0641, from the extended High AV Quasar (HAQ) survey. We find that the z=3.21 quasar has a foreground damped Lyman-{alpha} absorber (DLA) at z=2.027 along the line of sight. The DLA has very strong metal lines due to a moderately high metallicity with an inferred lower limit of 25% of the solar metallicity, but a very large gas column density along the line of sight in its host galaxy. This discovery is further evidence that there is a dust bias affecting the census of metals, caused by the combined effect of dust obscuration and reddening, in existing samples of z&gt;2 DLAs. The case of eHAQ0111+0641 illustrates that dust bias is not only caused by dust obscuration, but also dust reddening.</description><source format="bibcode">2017A&amp;A...606A..13F</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/606/A13</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic 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/606/A13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/606/A13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/606/A13</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/606/A13</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/606/A13</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/606/A13</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/A+A/606/A13/list</name><description>List of spectra</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>Nx</name><description>Number of pixels along X-axis</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ny</name><description>Number of spectra</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Obs.Date</name><description>Observation date (YYYY-MM-DDThh:mm:ss.sss)</description><ucd>time.epoch;obs</ucd><dataType xsi:type="vs:VOTableType" arraysize="23*">char</dataType></column><column><name>blambda</name><description>Lower valuer of spectral interval</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Blambda</name><description>Upper valuer of spectral interval</description><unit>0.1nm</unit><ucd>em.wl</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>dlambda</name><description>Spectral resolution</description><unit>0.1nm</unit><ucd>spect.resolution</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>size</name><description>Size of FITS file</description><unit>Kibyte</unit><ucd>phys.size;meta.fits</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>sp</name><description>Show the spectrum</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>FileName</name><description>Name of FITS file, in subdirectory sp</description><ucd>meta.id;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="28*">char</dataType></column><column><name>Title</name><description>Title of the FITS file</description><ucd>meta.title;meta.fits</ucd><dataType xsi:type="vs:VOTableType" arraysize="50*">char</dataType></column></table></schema></tableset></ri:Resource>