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<ri:Resource created="2022-07-07T13:24:57Z" 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>Multiwavelength cross-correlations in blazars</title><shortName>J/MNRAS/480/5517</shortName><identifier>ivo://CDS.VizieR/J/MNRAS/480/5517</identifier><altIdentifier>doi:10.26093/cds/vizier.74805517</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liodakis I.</name></creator><creator><name>Romani R.W.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Kiehlmann S.</name></creator><creator><name>Max-Moerbeck W.,Readhead A.C.S.</name></creator><creator><name>Zheng W.</name></creator><date role="Updated">2024-08-18T20:21:35Z</date><date role="Created">2022-07-07T13:24:57Z</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>gamma-ray-astronomy</subject><description>Blazars are known for their energetic multiwavelength flares from radio wavelengths to high-energy {gamma}-rays. In this work, we study radio, optical, and {gamma}-ray light curves of 145 bright blazars spanning up to 8 yr, to probe the flaring activity and interband correlations. Of these, 105 show &gt;1{sigma} correlations between one or more wavebands, 26 of which have a &gt;3{sigma} correlation in at least one wavelength pair, as measured by the discrete correlation function. The most common and strongest correlations are found between the optical and {gamma}-ray bands, with fluctuations simultaneous within our ~30d resolution. The radio response is usually substantially delayed with respect to the other wavelengths with median time lags of ~100-160d. A systematic flare identification via Bayesian block analysis provides us with a first uniform sample of flares in the three bands, allowing us to characterize the relative rates of multiband and 'orphan' flares. 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