RoboPol: connection between optical polarization plane rotations and gamma-ray flares in blazars

dc.contributor.authorD. Blinov
dc.contributor.authorV. Pavlidou
dc.contributor.authorI. Papadakis
dc.contributor.authorS. Kiehlmann
dc.contributor.authorI. Liodakis
dc.contributor.authorG. V. Panopoulou
dc.contributor.authorE. Angelakis
dc.contributor.authorM. Balokovi´c
dc.contributor.authorT. Hovatta
dc.contributor.authorO. G. King
dc.contributor.authorA. Kus
dc.contributor.authorN. Kylafis
dc.contributor.authorA. Mahabal
dc.contributor.authorS. Maharana
dc.contributor.authorI. Myserlis
dc.contributor.authorE. Paleologou
dc.contributor.authorI. Papamastorakis
dc.contributor.authorE. Pazderski
dc.contributor.authorT. J. Pearson
dc.contributor.authorA. Ramaprakash
dc.contributor.authorA. C. S. Readhead
dc.contributor.authorP. Reig
dc.contributor.authorK. Tassis
dc.contributor.authorJ. A. Zensus
dc.contributor.organizationfi=Tuorlan observatorio|en=Tuorla Observatory|
dc.contributor.organizationfi=Turun luonnontieteiden ja lääketieteen tutkijakollegium (TCSM)|en=Turku Collegium for Science and Medicine (TCSM)|
dc.contributor.organization-code1.2.246.10.2458963.20.90670098848
dc.converis.publication-id30133792
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/30133792
dc.date.accessioned2022-10-28T13:18:30Z
dc.date.available2022-10-28T13:18:30Z
dc.description.abstractWe use results of our 3 yr polarimetric monitoring programme to investigate the previously suggested connection between rotations of the polarization plane in the optical emission of blazars and their gamma-ray flares in the GeV band. The homogeneous set of 40 rotation events in 24 sources detected by RoboPol is analysed together with the gamma-ray data provided by Fermi-LAT. We confirm that polarization plane rotations are indeed related to the closest gamma-ray flares in blazars and the time lags between these events are consistent with zero. Amplitudes of the rotations are anticorrelated with amplitudes of the gamma-ray flares. This is presumably caused by higher relativistic boosting (higher Doppler factors) in blazars that exhibit smaller amplitude polarization plane rotations. Moreover, the time-scales of rotations and flares are marginally correlated.
dc.format.pagerange1296
dc.format.pagerange1306
dc.identifier.jour-issn0035-8711
dc.identifier.olddbid181194
dc.identifier.oldhandle10024/164288
dc.identifier.urihttps://www.utupub.fi/handle/11111/37536
dc.identifier.urnURN:NBN:fi-fe2021042718865
dc.language.isoen
dc.okm.affiliatedauthorHovatta, Talvikki
dc.okm.affiliatedauthorDataimport, LLK:n yhteiset
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA1 ScientificArticle
dc.publisherOXFORD UNIV PRESS
dc.publisher.countryUnited Kingdomen_GB
dc.publisher.countryBritanniafi_FI
dc.publisher.country-codeGB
dc.relation.doi10.1093/mnras/stx2786
dc.relation.ispartofjournalMonthly Notices of the Royal Astronomical Society
dc.relation.issue1
dc.relation.volume474
dc.source.identifierhttps://www.utupub.fi/handle/10024/164288
dc.titleRoboPol: connection between optical polarization plane rotations and gamma-ray flares in blazars
dc.year.issued2018

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