A Search for QPOs in the Blazar OJ287: Preliminary Results from the 2015/2016 Observing Campaign

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dc.bibliographicCitation.firstPage41eng
dc.bibliographicCitation.issue4eng
dc.bibliographicCitation.volume4eng
dc.contributor.authorZola, S.
dc.contributor.authorValtonen, M.
dc.contributor.authorBhatta, G.
dc.contributor.authorGoyal, A.
dc.contributor.authorDebski, B.
dc.contributor.authorBaran, A.
dc.contributor.authorKrzesinski, J.
dc.contributor.authorSiwak, M.
dc.contributor.authorCiprini, S.
dc.contributor.authorGopakumar, A.
dc.contributor.authorJermak, H.
dc.contributor.authorNilsson, K.
dc.contributor.authorReichart, D.
dc.contributor.authorMatsumoto, K.
dc.contributor.authorSadakane, K.
dc.contributor.authorGazeas, K.
dc.contributor.authorKidger, M.
dc.contributor.authorPiirola, V.
dc.contributor.authorAlicavus, F.
dc.contributor.authorBaliyan, K.
dc.contributor.authorBerdyugin, A.
dc.contributor.authorBoyd, D.
dc.contributor.authorCampas Torrent, M.
dc.contributor.authorCampos, F.
dc.contributor.authorCarrillo Gómez, J.
dc.contributor.authorCaton, D.
dc.contributor.authorChavushyan, V.
dc.contributor.authorDalessio, J.
dc.contributor.authorDimitrov, D.
dc.contributor.authorDrozdz, M.
dc.contributor.authorEr, H.
dc.contributor.authorErdem, A.
dc.contributor.authorEscartin Pérez, A.
dc.contributor.authorFallah Ramazani, V.
dc.contributor.authorFilippenko, A.
dc.contributor.authorGarcia, F.
dc.contributor.authorGómez Pinilla, F.
dc.contributor.authorGopinathan, M.
dc.contributor.authorHaislip, J.
dc.contributor.authorHarmanen, J.
dc.contributor.authorHudec, R.
dc.contributor.authorHurst, G.
dc.contributor.authorIvarsen, K.
dc.contributor.authorJelinek, M.
dc.contributor.authorJoshi, A.
dc.contributor.authorKagitani, M.
dc.contributor.authorKaur, N.
dc.contributor.authorKeel, W.
dc.contributor.authorLaCluyze, A.
dc.contributor.authorLee, B.
dc.contributor.authorLindfors, E.
dc.contributor.authorLozano de Haro, J.
dc.contributor.authorMoore, J.
dc.contributor.authorMugrauer, M.
dc.contributor.authorNaves Nogues, R.
dc.contributor.authorNeely, A.
dc.contributor.authorNelson, R.
dc.contributor.authorOgloza, W.
dc.contributor.authorOkano, S.
dc.contributor.authorPandey, J.
dc.contributor.authorPerri, M.
dc.contributor.authorPihajoki, P.
dc.contributor.authorPoyner, G.
dc.contributor.authorProvencal, J.
dc.contributor.authorPursimo, T.
dc.contributor.authorRaj, A.
dc.contributor.authorReinthal, R.
dc.contributor.authorSadegi, S.
dc.contributor.authorSakanoi, T.
dc.contributor.authorSameer, null
dc.contributor.authorSalto González, J.-L.
dc.contributor.authorSchweyer, T.
dc.contributor.authorSoldán Alfaro, F.
dc.contributor.authorKaraman, N.
dc.contributor.authorSonbas, E.
dc.contributor.authorSteele, I.
dc.contributor.authorStocke, J.
dc.contributor.authorStrobl, J.
dc.contributor.authorTakalo, L.
dc.contributor.authorTomov, T.
dc.contributor.authorTremosa Espasa, L.
dc.contributor.authorValdes, J.
dc.contributor.authorValero Pérez, J.
dc.contributor.authorVerrecchia, F.
dc.contributor.authorWebb, J.
dc.contributor.authorYoneda, M.
dc.contributor.authorZejmo, M.
dc.contributor.authorZheng, W.
dc.contributor.authorTelting, J.
dc.contributor.authorSaario, J.
dc.contributor.authorReynolds, T.
dc.contributor.authorKvammen, A.
dc.contributor.authorGafton, E.
dc.contributor.authorKarjalainen, R.
dc.contributor.authorBlay, P.
dc.date.accessioned2022-07-07T08:56:58Z
dc.date.available2022-07-07T08:56:58Z
dc.date.issued2016
dc.description.abstractWe analyse the light curve in the R band of the blazar OJ287, gathered during the 2015/2016 observing season. We did a search for quasi-periodic oscillations (QPOs) using several methods over a wide range of timescales. No statistically significant periods were found in the high-frequency domain both in the ground-based data and in Kepler observations. In the longer-period domain, the Lomb–Scargle periodogram revealed several peaks above the 99% significance level. The longest one—about 95 days—corresponds to the innermost stable circular orbit (ISCO) period of the more massive black hole. The 43-day period could be an alias, or it can be attributed to accretion in the form of a two-armed spiral wave.eng
dc.description.versionpublishedVersioneng
dc.identifier.urihttps://oa.tib.eu/renate/handle/123456789/9644
dc.identifier.urihttps://doi.org/10.34657/8682
dc.language.isoengeng
dc.publisherBasel : MDPIeng
dc.relation.doihttps://doi.org/10.3390/galaxies4040041
dc.relation.essn2075-4434
dc.relation.ispartofseriesGalaxies : open access journal 4 (2016), Nr. 4eng
dc.rights.licenseCC BY 4.0 Unportedeng
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/eng
dc.subjectBL Lacertae objects: individual (OJ287)eng
dc.subjectGalaxies: activeeng
dc.subjectSupermassive black holeseng
dc.subject.ddc520eng
dc.titleA Search for QPOs in the Blazar OJ287: Preliminary Results from the 2015/2016 Observing Campaigneng
dc.typearticleeng
dc.typeTexteng
dcterms.bibliographicCitation.journalTitleGalaxies : open access journaleng
tib.accessRightsopenAccesseng
wgl.contributorKISeng
wgl.subjectPhysikeng
wgl.typeZeitschriftenartikeleng
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