Multiwavelength picture of the blazar S5 0716+714 during its brightest outburst

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dc.contributor.authorManganaro, Marina
dc.contributor.authorPedaletti, Giovanna
dc.contributor.authorDoert, Marlene
dc.contributor.authorBastieri, Denis
dc.contributor.authorRamazani, Vandad Fallah
dc.contributor.authorGasparrini, Dario
dc.contributor.authorLindfors, Elina
dc.contributor.authorLott, Benoit
dc.contributor.authorNievas, Mireia
dc.contributor.authorRani, Bindu
dc.contributor.authorThompson, David J.
dc.contributor.authorAngelakis, Emmanouil
dc.contributor.authorBorman, George
dc.contributor.authorGurwell, Mark
dc.contributor.authorHovatta, Talvikki
dc.contributor.authorItoh, Ryosuke
dc.contributor.authorJorstad, Svetlana
dc.contributor.authorKraus, Alex
dc.contributor.authorKrichbaum, Thomas P.
dc.contributor.authorKuin, Paul
dc.contributor.authorLähteenmäki, Anne
dc.contributor.authorLarionov, Valeri
dc.contributor.authorLien, Amy Yarleen
dc.contributor.authorMyserlis, Ioannis
dc.contributor.authorTornikoski, Merja
dc.contributor.authorTroitsky, Ivan
dc.contributor.authorZensus, J. Anton
dc.date.accessioned2019-11-20T11:00:41Z
dc.date.available2019-11-20T11:00:41Z
dc.date.issued2016-11-24
dc.description.abstractS5 0716+714 is a well known BL Lac object, and one of the brightest and most active blazars. The discovery in the Very High Energy band (VHE, E > 100 GeV) by MAGIC happened in 2008. In January 2015, the source went through the brightest optical state ever observed, triggering MAGIC follow-up and a VHE detection with ∼ 13σ significance (ATel ♯6999 ). Rich multiwavelength coverage of the flare allowed us to construct the broad-band spectral energy distribution of S5 0716+714 during its brightest outburst. In this work, we will present the preliminary analysis of MAGIC and Fermi-LAT data of the flaring activity in January and February 2015 for the HE (0.1 < HE < 300 GeV) and VHE band, together with radio (Metsähovi, OVRO, VLBA, Effelsberg), sub-millimeter (SMA), optical (Tuorla, Perkins, Steward, AZT-8+ST7, LX-200, Kanata), X-ray and UV (Swift-XRT and UVOT), in the same time-window and discuss the time variability of the multiwavelength light curves during this impressive outburst.en
dc.identifier.urihttp://hdl.handle.net/2003/38388
dc.identifier.urihttp://dx.doi.org/10.17877/DE290R-20321
dc.language.isoende
dc.relation.ispartofseriesGalaxies;4(4)
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/
dc.subjectBL Lacertae objects: individual: S5 0716+714en
dc.subjectGalaxies: activeen
dc.subjectGamma-rays: galaxiesen
dc.subject.ddc530
dc.titleMultiwavelength picture of the blazar S5 0716+714 during its brightest outbursten
dc.typeTextde
dc.type.publicationtypearticlede
dcterms.accessRightsopen access
eldorado.secondarypublicationtruede
eldorado.secondarypublication.primarycitationManganaro, M.; Pedaletti, G.; Doert, M.; Bastieri, D.; Fallah Ramazani, V.; Gasparrini, D.; Lindfors, E.; Lott, B.; Nievas, M.; Rani, B.; Thompson, D.J.; Angelakis, E.; Borman, G.; Gurwell, M.; Hovatta, T.; Itoh, R.; Jorstad, S.; Kraus, A.; Krichbaum, T.P.; Kuin, P.; Lähteenmäki, A.; Larionov, V.; Lien, A.Y.; Myserlis, I.; Tornikoski, M.; Troitsky, I.; Zensus, J.A.; The MAGIC and -LAT Collaborations. Multiwavelength Picture of the Blazar S5 0716+714 during Its Brightest Outburst. Galaxies 2016, 4, 69.de
eldorado.secondarypublication.primaryidentifierhttps://doi.org/10.3390/galaxies4040069de

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