%0 Journal Article
%A Manganaro, Marina
%A Pedaletti, Giovanna
%A Doert, Marlene
%A Bastieri, Denis
%A Ramazani, Vandad Fallah
%A Gasparrini, Dario
%A Lindfors, Elina
%A Lott, Benoit
%A Nievas, Mireia
%A Rani, Bindu
%A Thompson, David
%A Angelakis, Emmanouil
%A Borman, George
%A Gurwell, Mark
%A Hovatta, Talvikki
%A Itoh, Ryosuke
%A Jorstad, Svetlana
%A Kraus, Alex
%A Krichbaum, Thomas
%A Kuin, Paul
%A Lähteenmäki, Anne
%A Larionov, Valeri
%A Lien, Amy
%A Myserlis, Ioannis
%A Tornikoski, Merja
%A Troitsky, Ivan
%A Zensus, J.
%T Multiwavelength Picture of the Blazar S5 0716+714 during Its Brightest Outburst
%D 2016
%@ 2075-4434
%U https://hdl.handle.net/20.500.14352/19153
%X S5 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.
%~