Multiwavelength picture of the blazar S5 0716+714 during its brightest outburst
| Autor: | Manganaro, Marina, Pedaletti, Giovanna, Doert, Marlene, Bastieri, Denis, Ramazani, Vandad Fallah, Gasparrini, Dario, Lindfors, Elina, Lott, Benoit, Nievas, Mireia, Rani, Bindu, Thompson, David J., Angelakis, Emmanouil, Borman, George, Gurwell, Mark, Hovatta, Talvikki, Itoh, Ryosuke, Jorstad, Svetlana, Kraus, Alex, Krichbaum, Thomas P., Kuin, Paul, Lähteenmäki, Anne, Larionov, Valeri, Lien, Amy Yarleen, Myserlis, Ioannis, Tornikoski, Merja, Troitsky, Ivan, Zensus, J. Anton |
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| Rok vydání: | 2017 |
| Předmět: | |
| Zdroj: | Galaxies, vol. 4, issue 4, p. 69 (2016) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.3390/galaxies4040069 |
| Popis: | S5 0716+714 is a well known BL Lac object, 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 13{\sigma} 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 (Mets\"ahovi, 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. Comment: 7 pages, 3 figures, proceeding of the JETS 2016 conference |
| Databáze: | arXiv |
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