Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7298
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dc.contributor.authorAditi Agarwal-
dc.date.accessioned2018-06-15T05:11:32Z-
dc.date.available2018-06-15T05:11:32Z-
dc.date.issued2018-04-
dc.identifier.citationBulletin de la Societe Royale des Sciences de Liege, Vol. 87, pp. 321-324en_US
dc.identifier.issn0037-9565-
dc.identifier.urihttp://hdl.handle.net/2248/7298-
dc.descriptionOpen Accessen_US
dc.description.abstractTo search for optical variability on a wide range of timescales, we have carried out photometric monitoring of a dozen blazars. CCD magnitudes in B, V, R and I pass-bands were determined for > 10,000f new optical observations from 300 nights made during 2011 – 2016, with an average length of 4 h each, using seven optical telescopes: four in Bulgaria, one in Greece, and two in India. We measured multiband optical flux and colour variations on diverse timescales. Blazar variability studies helped us in understanding their nature and extreme conditions within the emission region. To explain possible physical causes of the observed spectral variability, we also investigated spectral energy distributions using B, V, R, I, J and K pass-band data.en_US
dc.language.isoenen_US
dc.publisherBulletin de la Societe Royale des Sciences de Liegeen_US
dc.relation.urihttps://popups.uliege.be/0037-9565/index.php?id=7758-
dc.rights© Bulletin de la Societe Royale des Sciences de Liege-
dc.subjectAstronomyen_US
dc.subjectAstrophysicsen_US
dc.subjectVariabilityen_US
dc.subjectPhotometryen_US
dc.subjectExtragalacticen_US
dc.subjectAGNen_US
dc.titleMulti-band optical variability studies of Blazarsen_US
dc.typeArticleen_US
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