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<ri:Resource created="2024-03-01T09:58:30Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>BVRI photometry of S5 0716+714</title><shortName>J/ApJ/928/86</shortName><identifier>ivo://CDS.VizieR/J/ApJ/928/86</identifier><altIdentifier>doi:10.26093/cds/vizier.19280086</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gorbachev M.A.</name></creator><creator><name>Butuzova M.S.</name></creator><creator><name>Sergeev S.G.</name></creator><creator><name>Nazarov S.V.</name></creator><creator><name>Zhovtan A.V.</name></creator><date role="Updated">2024-11-06T20:24:35Z</date><date role="Created">2024-03-01T09:58:30Z</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>bl-lacertae-objects</subject><subject>photometry</subject><subject>visible-astronomy</subject><description>Multiband optical photometry data of blazar S5 0716+714 obtained from 2002 to 2019 reveal stable color index change with flux variability. We analyzed this trend under variability caused by the Doppler factor change in the presence of a curved photon energy spectrum. A break in the energy spectrum of emitting electrons, caused by radiative losses, or log-parabolic electron energy distribution, or the synchrotron self-absorption acting in a compact jet part forms such the photon spectrum. We explained the observed color index change with variability by geometric effects only under the assumption that the radiating region is the synchrotron self-absorbed core and the bright optically thin jet. In this framework, we estimated the magnetic field strength in the optically thick part of the radiating region. These values correspond to other independent estimates of the magnetic field near the black hole, further supporting our assumption.</description><source format="bibcode">2022ApJ...928...86G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/928/86</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/327/61">J/A+A/327/61 : BV(RI)c photometry of S5 0716+714 (Ghisellini+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/402/151">J/A+A/402/151 : S5 0716+714 UBVRI photometry (Raiteri+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/129/1818">J/AJ/129/1818 : Photometry of S5 0716+714 (Wu+, 2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/451/435">J/A+A/451/435 : BV(RI)c photometry of S5 0716+714 (Montagni+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AZh/83/310">J/AZh/83/310 : BV(RI)c photometry of S5 0716+714 (Amirkhanyan+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/133/1599">J/AJ/133/1599 : B'V'R' photometry of S5 0716+714 (Wu+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/136/1846">J/AJ/136/1846 : BVRI light curves of S5 0716+714 (Zhang+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/185/511">J/ApJS/185/511 : Optical microvariability of S5 0716+714 (Poon+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/108">J/AJ/143/108 : B'V'R' photometry of the BL Lac object S5 0716+714 (Wu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/558/A92">J/A+A/558/A92 : S5 0716+714 microvariability observation (Bhatta+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/783/83">J/ApJ/783/83 : BVRI photometry of S5 0716+714 (Liao+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/18">J/ApJS/218/18 : 2004-2012 BVRI observations of blazar S5 0716+714 (Dai+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/601/A12">J/A+A/601/A12 : S5 0716+714 VLBI K- and Q-band variability (Lee+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/154/42">J/AJ/154/42 : BVRI photometry of S5 0716+714 in 2012 (Hong+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PAZh/43/407">J/PAZh/43/407 : S5 0716+714 polarization + brightness 1991-2004</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/619/A45">J/A+A/619/A45 : S5 0716+714 multi-wavelength curves (MAGIC Coll.+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/155/31">J/AJ/155/31 : 2005-2012 BVRI observations of S5 0716+714 (Hong+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/880/155">J/ApJ/880/155 : RI photometry of blazars S5 0716+714 and 3C 273 (Liu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/884/92">J/ApJ/884/92 : 7yrs of VRI obs. of S5 0716+714 and its flares (Xu+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/888/30">J/ApJ/888/30 : BVRI &amp; spectroscopic light curves of S5 0716+714 (Feng+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/902/42">J/ApJ/902/42 : Spectroscopic monitoring of blazar S5 0716+714 (Feng+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/247/49">J/ApJS/247/49 : gri obs. of the blazar S5 0716+714 (2017-2019) (Xiong+, 2020)</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/928/86</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/928/86</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/928/86</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/928/86</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/928/86</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/928/86</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><coverage><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Optical</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/928/86/table1</name><description>Observational log and results in the B,V,R,I bands</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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