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<ri:Resource created="2016-06-06T07:42:16Z" 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>Optical flux behaviour of Fermi blazars</title><shortName>J/A+A/591/A21</shortName><identifier>ivo://CDS.VizieR/J/A+A/591/A21</identifier><altIdentifier>doi:10.26093/cds/vizier.35910021</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Marchesini E.J.</name></creator><creator><name>Andruchow I.</name></creator><creator><name>Cellone S.A.</name></creator><creator><name>Combi J.A.</name></creator><creator><name>Zibecchi L.,Marti J.</name></creator><creator><name>Romero G.E.</name></creator><creator><name>Munoz-Arjonilla A.J.</name></creator><creator><name>Luque-Escamilla P.,Sanchez-Sutil J.R.</name></creator><date role="Updated">2017-10-12T13:00:38Z</date><date role="Created">2016-06-06T07:42:16Z</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><description>We aim at investigating the time-behaviour of a sample of gamma-ray blazars. We present the results from a 13 month-long optical photometry monitoring campaign of the blazars PKS0048-097, PKS0754+100, [HB89] 0827+243, PKS0851+202, PKS1253-055, PKS1510-089, PKS1749+096, PKS2230+114 and PKS2251+158. We analyse the variability of each object, focusing on different time-scales (long term, short term, and microvariability), in an attempt to achieve a statistical comparison of the results. 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