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<ri:Resource created="2020-06-13T10:32:43Z" 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>AGN feedback</title><shortName>J/MNRAS/471/28</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/471/28</identifier><altIdentifier>doi:10.26093/cds/vizier.74710028</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kalfountzou E.</name></creator><creator><name>Stevens J.A.</name></creator><creator><name>Jarvis M.J.</name></creator><creator><name>Hardcastle M.J.</name></creator><creator><name>Wilner D.,Elvis M.</name></creator><creator><name>Page M.J.</name></creator><creator><name>Trichas M.</name></creator><creator><name>Smith D.J.B.</name></creator><date role="Updated">2024-08-17T20:20:23Z</date><date role="Created">2020-06-13T10:32:43Z</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>millimeter-astronomy</subject><subject>photometry</subject><subject>submillimeter-astronomy</subject><description>Several studies support the existence of a link between the active galactic nucleus (AGN) and star formation activity. Radio jets have been argued to be an ideal mechanism for direct interaction between the AGN and the host galaxy. A drawback of previous surveys of AGN is that they are fundamentally limited by the degeneracy between redshift and luminosity in flux-density limited samples. To overcome this limitation, we present far-infrared Herschel observations of 74 radio-loud quasars (RLQs), 72 radio-quiet quasars (RQQs) and 27 radio galaxies (RGs), selected at 0.9&lt;z&lt;1.1, which span over two decades in optical luminosity. By decoupling luminosity from evolutionary effects, we investigate how the star formation rate (SFR) depends on AGN luminosity, radio-loudness and orientation. We find that (1) the SFR shows a weak correlation with the bolometric luminosity for all AGN sub-samples, (2) the RLQs show an SFR excess of about a factor of 1.4 compared to the RQQs, matched in terms of black hole mass and bolometric luminosity, suggesting that either positive radio-jet feedback or radio AGN triggering is linked to star formation triggering, and (3) RGs have lower SFRs by a factor of 2.5 than the RLQ sub-sample with the same BH mass and bolometric luminosity. We suggest that there is some jet power threshold at which radio-jet feedback switches from enhancing star formation (by compressing gas) to suppressing it (by ejecting gas). This threshold depends on both galaxy mass and jet power.</description><source format="bibcode">2017MNRAS.471...28K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/471/28</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></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/471/28</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/471/28</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/471/28</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/471/28</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/471/28</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/471/28</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/471/28/tablea1 (Herschel photometry of the objects studied in this work)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/471/28/tablea1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/471/28/tablea1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/471/28/tablea1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>261.079</ra><dec>50.9612</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>5/1519 6/2300 2313 2839 2949 4150 4793 4825 4857 4860 4863 5034 5046 5355 5357 5371 5399 5692 5738 5778 5785 5798 5817 5844 5858 5881 5883 5936 5974 5988 6028 6033 6044 6048 6069 6071 6075 6110 6208 6220 6233 6389 6408 6420-6421 6429 6472 6503 6510-6511 6536 6576 6578 7169 7186 7223 7235 7240 7257 7260 7305 7360 7451 7511 7888 8197 8200 9303 9327 9343 9391 9394 9402 9415 9431 9435 9462-9463 9469 9482 9604 9635 9642 9820-9821 9824 9853 9863 9922 9927 9977 9992 10052 10153 10189 10191 10214 10567 10602-10603 10611 10618 10622 10663 10700 10774 10781 10877 10880 10888 10977 10996 11033 11073 11087 11094 11099 11116 11147 11159 11171 11237 11311-11312 11366 11400 11464 11476 11502 11504 11551 11597 11787 11809 11813 11815 12010 12560 17765 19414 19747 20435 20439 20441 21854 22505 26036 26323 27097 27114 27254 27310 27371 27425 27498 27520 27711 27742 27755 31399 32509</spatial><spectral>1.528037907652962e-22 3.243176138527326e-21</spectral><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/471/28?format=ascii</footprint><waveband>Millimeter</waveband></coverage><tableset><schema><name>default</name><table><name>J/MNRAS/471/28/tablea1</name><description>Herschel photometry of the objects studied in this work</description><column><name>SimbadName</name><description>Simbad column added by the CDS</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="24*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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