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<ri:Resource created="2017-02-22T10:08:30Z" 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>NIR spectroscopy of 1.5&lt;z&lt;3.5 broad-band QSOs</title><shortName>J/ApJ/817/55</shortName><identifier>ivo://CDS.VizieR/J/ApJ/817/55</identifier><altIdentifier>doi:10.26093/cds/vizier.18170055</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Shen Y.</name></creator><date role="Updated">2017-06-27T06:39:02Z</date><date role="Created">2017-02-22T10:08:30Z</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><subject>redshifted</subject><subject>line-intensities</subject><description>We study the rest-frame optical properties of 74 luminous (L_bol_=10^46.2-48.2^erg/s), 1.5&lt;z&lt;3.5 broad-line quasars with near-IR (JHK) slit spectroscopy. Systemic redshifts based on the peak of the [OIII]{lambda}5007 line reveal that redshift estimates from the rest-frame UV broad emission lines (mostly MgII) are intrinsically uncertain by ~200km/s (measurement errors accounted for). The overall full-width-at-half-maximum of the narrow [OIII] line is ~1000km/s on average. A significant fraction of the total [OIII] flux (~40%) is in a blueshifted wing component with a median velocity offset of ~700km/s, indicative of ionized outflows within a few kpc from the nucleus; we do not find evidence of significant [OIII] flux beyond ~10kpc in our slit spectroscopy. The [OIII] line is noticeably more asymmetric and weaker than that in typical less luminous low-z quasars. However, when matched in quasar continuum luminosity, low-z quasars have similar [OIII] profiles and strengths as these high-z systems. Therefore the exceptionally large width and blueshifted wing, and the relatively weak strength of [OIII] in high-z luminous quasars are mostly a luminosity effect rather than redshift evolution. The H{beta}-[OIII] region of these high-z quasars displays a similar spectral diversity and Eigenvector 1 correlations with anti-correlated [OIII] and optical FeII strengths, as seen in low-z quasars; but the average broad H{beta} width is larger by 25% than typical low-z quasars, indicating more massive black holes in these high-z systems. These results highlight the importance of understanding [OIII] in the general context of quasar parameter space in order to understand quasar feedback in the form of [OIII] outflows. The calibrated one-dimensional near-IR spectra are made publicly available, along with a composite spectrum.</description><source format="bibcode">2016ApJ...817...55S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/817/55</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/II/319">II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VII/260">VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/294">II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/452/2553">J/MNRAS/452/2553 : Sample of foreground-background QSO pairs (Johnson+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/804/L15">J/ApJ/804/L15 : SDSS-DR7 broad-line QSOs (Sun+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/426/2703">J/MNRAS/426/2703 : Type 1 AGN at low z. 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(Stern+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/753/125">J/ApJ/753/125 : NIR spectroscopy follow-up of 60 SDSS-DR7 QSOs (Shen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/423/600">J/MNRAS/423/600 : Type-1 low-z AGN emission properties (Stern+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/737/71">J/ApJ/737/71 : The [OIII] emission line in SDSS AGNs (Zhang+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/736/86">J/ApJ/736/86 : FeII emission in SDSS type 1 AGNs (Dong+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><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/ApJ/680/169">J/ApJ/680/169 : SDSS DR5 virial black hole masses (Shen+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/666/757">J/ApJ/666/757 : CIV 1549{AA} emission line in AGNs (Sulentic+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/459/55">J/A+A/459/55 : Narrow-band imaging of 5 Seyfert-1 galaxies (Bennert+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/456/953">J/A+A/456/953 : Narrow-band imaging of 6 Seyfert-2 galaxies (Bennert+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/130/381">J/AJ/130/381 : Blueshifted [O III] emission (Boroson+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/309/81">J/A+A/309/81 : X-ray properties of AGN (Wang+, 1996)</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/817/55</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/817/55</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/817/55</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/817/55</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/817/55</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/817/55</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/817/55/table2 (Spectral measurements)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/817/55/table2?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/817/55/table2?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/817/55/table2?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>26.772615</ra><dec>13.53611611</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/4112 4117 4139 4231 4387 4407 4656 4850 4993 5010 5520 5735 6049 6240 7353 8450 8553 8903 9918 10214 10313 10330 10963 11453 11845 17237 17241 17749 17816 18293 18388 18389 18523 18537 19094 19405 21847 22014 22357 22711 23057 23064 23210 25976 26071 26097 26277 26336 26348 26359 26369 26985 27007 27254 27346 27365 27416 27424 27480 27512 27561 27575 27605 28376 28570 30034 30039 31318 31333 31463 36767 49078</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/817/55?format=ascii</footprint><waveband>Infrared</waveband><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/817/55/table3</name><description>Composite spectrum</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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