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<ri:Resource created="2025-02-19T16:25:17Z" 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>Study of massive SMBHs hosted by FSRQs</title><shortName>J/MNRAS/511/5436</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/511/5436</identifier><altIdentifier>doi:10.26093/cds/vizier.75115436</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Diana A.</name></creator><creator><name>Caccianiga A.</name></creator><creator><name>Ighina L.</name></creator><creator><name>Belladitta S.</name></creator><creator><name>Moretti A.,Della Ceca R.</name></creator><date role="Updated">2025-03-03T20:14:32Z</date><date role="Created">2025-02-19T16:25:17Z</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>active-galactic-nuclei</subject><subject>quasars</subject><subject>black-holes</subject><subject>radio-sources</subject><subject>radio-continuum-emission</subject><subject>spectroscopy</subject><subject>photometry</subject><subject>ultraviolet-astronomy</subject><subject>visible-astronomy</subject><subject>extinction</subject><subject>galaxy-kinematics</subject><description>We present the space density evolution, from z = 1.5 up to z = 5.5, of the most massive (M =&gt; 10^9^ M_{sun}_) black holes hosted in jetted active galactic nuclei (AGNs). The analysis is based on a sample of 380 luminosity- selected ({lambda}L_1350_ =&gt; 10^46^ erg/s and P_5GHz_ =&gt; 10^27^ W/Hz) flat spectrum radio quasars (FSRQs) obtained from the Cosmic Lens All Sky Survey (CLASS). These sources are known to be face-on jetted AGNs (i.e. blazars) and can be exploited to infer the abundance of all the (misaligned) jetted AGNs, using a geometrical argument. We then compare the space density of the most massive supermassive black holes hosted in jetted AGNs with those present in the total population (mostly composed by non-jetted AGNs). We find that the space density has a peak at z ~ 3, which is significantly larger than the value observed in the total AGN population with similar optical/UV luminosities (z ~ 2.2), but not as extreme as the value previously inferred from X-ray-selected blazars (z ~&gt; 4). The jetted fraction (jetted AGNs/total AGNs) is overall consistent with the estimates in the local Universe (10-20 per cent) and at high redshift, assuming Lorentz bulk factors {Gamma} ~= 5. Finally, we find a marginal decrease in the jetted fraction at high redshifts (by a factor of ~2). All these evidences point towards a different evolutionary path in the jetted AGNs compared to the total AGN population.</description><source format="bibcode">2022MNRAS.511.5436D</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/511/5436</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/ApJS/194/45">J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/699/603">J/ApJ/699/603 : Evolution of Swift/BAT blazars (Ajello+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/72">VIII/72 : CLASS survey of radio sources (Myers+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/58">IX/58 : 2SXPS Swift X-ray telescope point source catalogue</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/154">V/154 : Sloan Digital Sky Surveys (SDSS), Release 16 (DR16)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/40">VIII/40 : GB6 catalog of radio sources (Gregory+ 1996)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/VIII/65">VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/349">II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL 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