RoboPol: connection between optical polarization plane rotations and gamma-ray flares in blazars
| dc.contributor.author | D. Blinov | |
| dc.contributor.author | V. Pavlidou | |
| dc.contributor.author | I. Papadakis | |
| dc.contributor.author | S. Kiehlmann | |
| dc.contributor.author | I. Liodakis | |
| dc.contributor.author | G. V. Panopoulou | |
| dc.contributor.author | E. Angelakis | |
| dc.contributor.author | M. Balokovi´c | |
| dc.contributor.author | T. Hovatta | |
| dc.contributor.author | O. G. King | |
| dc.contributor.author | A. Kus | |
| dc.contributor.author | N. Kylafis | |
| dc.contributor.author | A. Mahabal | |
| dc.contributor.author | S. Maharana | |
| dc.contributor.author | I. Myserlis | |
| dc.contributor.author | E. Paleologou | |
| dc.contributor.author | I. Papamastorakis | |
| dc.contributor.author | E. Pazderski | |
| dc.contributor.author | T. J. Pearson | |
| dc.contributor.author | A. Ramaprakash | |
| dc.contributor.author | A. C. S. Readhead | |
| dc.contributor.author | P. Reig | |
| dc.contributor.author | K. Tassis | |
| dc.contributor.author | J. A. Zensus | |
| dc.contributor.organization | fi=Tuorlan observatorio|en=Tuorla Observatory| | |
| dc.contributor.organization | fi=Turun luonnontieteiden ja lääketieteen tutkijakollegium (TCSM)|en=Turku Collegium for Science and Medicine (TCSM)| | |
| dc.contributor.organization-code | 1.2.246.10.2458963.20.90670098848 | |
| dc.converis.publication-id | 30133792 | |
| dc.converis.url | https://research.utu.fi/converis/portal/Publication/30133792 | |
| dc.date.accessioned | 2022-10-28T13:18:30Z | |
| dc.date.available | 2022-10-28T13:18:30Z | |
| dc.description.abstract | We 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.pagerange | 1296 | |
| dc.format.pagerange | 1306 | |
| dc.identifier.jour-issn | 0035-8711 | |
| dc.identifier.olddbid | 181194 | |
| dc.identifier.oldhandle | 10024/164288 | |
| dc.identifier.uri | https://www.utupub.fi/handle/11111/37536 | |
| dc.identifier.urn | URN:NBN:fi-fe2021042718865 | |
| dc.language.iso | en | |
| dc.okm.affiliatedauthor | Hovatta, Talvikki | |
| dc.okm.affiliatedauthor | Dataimport, LLK:n yhteiset | |
| dc.okm.discipline | 115 Astronomy and space science | en_GB |
| dc.okm.discipline | 115 Avaruustieteet ja tähtitiede | fi_FI |
| dc.okm.internationalcopublication | international co-publication | |
| dc.okm.internationality | International publication | |
| dc.okm.type | A1 ScientificArticle | |
| dc.publisher | OXFORD UNIV PRESS | |
| dc.publisher.country | United Kingdom | en_GB |
| dc.publisher.country | Britannia | fi_FI |
| dc.publisher.country-code | GB | |
| dc.relation.doi | 10.1093/mnras/stx2786 | |
| dc.relation.ispartofjournal | Monthly Notices of the Royal Astronomical Society | |
| dc.relation.issue | 1 | |
| dc.relation.volume | 474 | |
| dc.source.identifier | https://www.utupub.fi/handle/10024/164288 | |
| dc.title | RoboPol: connection between optical polarization plane rotations and gamma-ray flares in blazars | |
| dc.year.issued | 2018 |
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