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dc.contributor.authorPolednikova, Jana
dc.contributor.authorEderoclite, Alessandro
dc.contributor.authorCepa, Jordi
dc.contributor.authorDiego Onsurbe, José Antonio de
dc.contributor.authorGonzález Serrano, José Ignacio 
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2023-01-10T15:52:12Z
dc.date.available2023-01-10T15:52:12Z
dc.date.issued2012
dc.identifier.issn1824-8039
dc.identifier.urihttps://hdl.handle.net/10902/27118
dc.description.abstractThe AGN unified scenario suggests that the type 2 quasars are the obscured counterparts of type 1 quasars where the difference is caused only by the orientation of the object. Optical microvari ability is supposed to arise from the regions which are closer to the supermassive black hole at the center of the AGN. The search for microvariability is an important test for the AGN unified scenario. We present first results from the microvariability campaign carried out at San Pedro Martit observatory. We have targeted three brightest (V mag < 17) type 2 quasars from SDSS. Using analysis of variance (ANOVA), we have detected significant microvariability events in two out of three type 2 quasars we have observedes_ES
dc.format.extent3 p.es_ES
dc.language.isoenges_ES
dc.publisherSissa Medialabes_ES
dc.rights© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.es_ES
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/4.0/*
dc.sourcePoS - Proceedings of science, 2012, 071es_ES
dc.titleOptical microvariability in type 2 quasarses_ES
dc.typeinfo:eu-repo/semantics/conferenceObjectes_ES
dc.rights.accessRightsopenAccesses_ES
dc.type.versionpublishedVersiones_ES


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