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<ri:Resource created="2014-03-28T12:11:59Z" 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>MgII absorption systems for Flat-Spectrum Radio QSOs</title><shortName>J/ApJ/754/38</shortName><identifier>ivo://CDS.VizieR/J/ApJ/754/38</identifier><altIdentifier>doi:10.26093/cds/vizier.17540038</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chand H.</name></creator><creator><name>Gopal-Krishna</name></creator><date role="Updated">2017-10-16T14:58:17Z</date><date role="Created">2014-03-28T12:11:59Z</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>line-intensities</subject><subject>redshifted</subject><subject>spectroscopy</subject><subject>radio-sources</subject><description>The conventional wisdom that the rate of incidence of MgII absorption systems, dN/dz (excluding "associated systems" having a velocity {beta}c relative to the active galactic nucleus (AGN) of less than ~5000km/s), is totally independent of the background AGNs has been challenged by a recent finding that dN/dz for strong MgII absorption systems toward distant blazars is 2.2+/-^0.8^_0.6_ times the value known for normal optically selected quasars (QSOs). This has led to the suggestion that a significant fraction of even the absorption systems with {beta} as high as ~0.1 may have been ejected by the relativistic jets in the blazars, which are expected to be pointed close to our direction. Here, we investigate this scenario using a large sample of 115 flat-spectrum radio-loud quasars (FSRQs) that also possess powerful jets, but are only weakly polarized. We show, for the first time, that dN/dz toward FSRQs is, on the whole, quite similar to that known for QSOs and that the comparative excess of strong MgII absorption systems seen toward blazars is mainly confined to {beta}&lt;0.15. The excess relative to FSRQs probably results from a likely closer alignment of blazar jets with our direction; hence, any gas clouds accelerated by them are more likely to be on the line of sight to the active quasar nucleus.</description><source format="bibcode">2012ApJ...754...38C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/754/38</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/VII/258">VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/546/A67">J/A+A/546/A67 : Catalog of strong MgII absorbers (Lawther+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/131">J/ApJ/748/131 : MgII absorbers in SDSS-DR7 quasar catalog (Shen+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/732/110">J/ApJ/732/110 : SDSS 2175{AA} extinction bump candidates (Jiang+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/714/1521">J/ApJ/714/1521 : Spectroscopy of galaxies around distant QSOs (Chen+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/698/819">J/ApJ/698/819 : MgII and LRGs cross-correlation analysis (Lundgren+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/679/239">J/ApJ/679/239 : Associated MgII absorbers (Vanden+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/171/61">J/ApJS/171/61 : All-Sky Survey of FSRQs - CRATES (Healey+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/660/1093">J/ApJ/660/1093 : Weak MgII absorbers at 0.4&lt;z&lt;2.4 (Narayanan+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/639/766">J/ApJ/639/766 : SDSS-DR3 strong MgII absorbers (Prochter+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/354/L25">J/MNRAS/354/L25 : MgII absorbers in SDSS QSOs (Bouche+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/106/848">J/AJ/106/848 : QSO MgII absorption line systems (Drinkwater+, 1993)</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/754/38</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/754/38</mirrorURL><mirrorURL title="VizieR at SAAO: 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