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<ri:Resource created="2026-04-28T11:15:08Z" status="active" updated="2026-06-15T00:00:00Z" 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>IceCube neutrinos-CAZ blazar light curves assoc.</title><shortName>J/A+A/708/A383</shortName><identifier>ivo://CDS.VizieR/J/A+A/708/A383</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Kouch P.M.</name></creator><creator><name>Hovatta T.</name></creator><creator><name>Lindfors E.</name></creator><creator><name>Liodakis I.</name></creator><creator><name>Koljonen K.I.I.</name></creator><creator><name>Paggi A.</name></creator><date role="Updated">2026-05-19T14:14:26Z</date><date role="Created">2026-04-28T11:15:08Z</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>neutrino-astronomy</subject><subject>radio-sources</subject><description>The IceCube Neutrino Observatory has detected several hundred high-energy neutrinos from cosmic sources. Despite numerous studies searching for their origin, it is still not known which sources emit them. A few likely individual associations exist with active galactic nuclei (AGN), mostly with blazars which are AGN with jets pointed toward Earth. Nonetheless, on a population level, blazar-neutrino correlation strengths are rather weak. This could mean that blazars as a population do not emit high-energy neutrinos, or that the detection power of the tests is insufficient due to the strong atmospheric neutrino background. By assuming an increase in high-energy neutrino emission during major blazar flares, in our previous studies we leveraged the arrival time of the neutrinos to boost the detection power. In this paper we utilize the same principle while substantially increasing the number of blazars. We search for the spatio-temporal correlation of 356 IceCube high-energy neutrinos with major optical flares of 3225 radio- and 3814 gamma-ray-selected blazars. We find that, despite the increase in data size, the number of likely spatio-temporal associations remains low and the overall correlation strengths weak. Two individual associations drive our strongest and the only &gt;2{sigma} post-trial spatio-temporal correlation, occurring with the BL Lac objects of the radio-selected blazar sample. We estimate that &lt;~8% of the detected cosmic neutrinos were emitted by blazars during major optical flares. As a complementary analysis, we compare the synchrotron peak frequency, redshift, Doppler factor, X-ray brightness, and optical variability of spatially neutrino-associated blazars to those of the general blazar population. We find that spatially neutrino-associated blazars of the tested samples have higher than average Doppler factor and X-ray brightness.</description><source format="bibcode">2026A&amp;A...708A.383K</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/708/A383</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/A+A/690/A111">J/A+A/690/A111 : IceCube neutrinos-blazars association (Kouch+, 2024)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/708/A382">J/A+A/708/A382 : 7918 blazar-selected AGN CAZ catalog and LC (Kouch+, 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