51. MAGIC Observations and multiwavelength properties of the quasar 3C 279 in 2007 and 2009
- Author
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Silvia Pardo, Nikola Godinovic, M. Shayduk, P. Majumdar, Diego F. Torres, M. Pasanen, L. Font, Roberta Zanin, M. Doert, Stefano Covino, Nijil Mankuzhiyil, Daniela Dorner, Michael Backes, K. Berger, M. V. Fonseca, Julian Sitarek, J. Hose, A. Diago Ortega, Robert Wagner, A. De Angelis, P. Antoranz, Daniela Hadasch, R. Reinthal, Wlodek Bednarek, Alessandro Carosi, Daniel Ferenc, Tomislav Terzić, C. Fruck, Marc Ribó, Hiroko Miyamoto, Jelena Aleksić, Ignasi Reichardt, H. Vankov, Riccardo Paoletti, Aaron Dominguez, D. Tescaro, D. Garrido, V. Scalzotto, Dominik Elsaesser, Denis Bastieri, Q. Weitzel, Tihomir Surić, M. I. Martínez, P. G. Prada Moroni, S. Spiro, E. Lorenz, E. Colombo, A. Cañellas, A.Sillapää, Jose Miguel Miranda, Felicitas Pauss, B. Steinke, Ilana M. Braun, G. Maneva, Damir Lelas, K. Saito, Elisa Bernardini, A. Saggion, Adrian Biland, O. Tibolla, J. M. Paredes, Antonio Stamerra, M. Pilia, Giacomo Bonnoli, Victor Zabalza, Felix Spanier, L. Maraschi, Elina Lindfors, S. Rügamer, Juan Abel Barrio, C. Delgado Mendez, Ralph Bock, Karl Mannheim, Daniel Mazin, L. O. Takalo, Konstancja Satalecka, Michele Doro, S. Partini, Jose Luis Contreras, D. Borla Tridon, Francesco Dazzi, D. Dominis Prester, Takashi Saito, J. Storz, Dorota Sobczyńska, Masahiro Teshima, Juan Cortina, E. Leonardo, Francisco Prada, Reiko Orito, J. Becerra González, V. Scapin, Mosè Mariotti, P. Temnikov, Gianluca Giavitto, Fabio Zandanel, Martin Makariev, Oscar Blanch, Daniel Nieto, T. Schweizer, Dario Hrupec, Mario Meucci, E. Prandini, J. Rico, Kari Nilsson, M. A. Lopez, Aldo Treves, B. Huber, R. J. García López, A. La Barbera, Ivica Puljak, Pierre Colin, Saverio Lombardi, D. Hildebrand, L. Peruzzo, Andrei Berdyugin, A. Boller, L. Cossio, J. Moldón, Artemio Herrero, J. Pochon, Massimo Persic, M.Rüger, C. Schultz, D. Häfner, T. Krähenbühl, T. Jogler, N. Strah, Thomas Bretz, S. N. Shore, Wolfgang Rhode, E. De Cea del Pozo, M. Salvati, M. Thom, M. A. Perez-Torres, R. Mirzoyan, E. Carmona, Markus Garczarczyk, J. Krause, B. De Lotto, S. Klepser, Abelardo Moralejo, Patrick Vogler, L. A. Antonelli, Igor Oya, and Fabrizio Tavecchio
- Subjects
galaxies [Gamma rays] ,Astrophysics ,7. Clean energy ,01 natural sciences ,gamma rays: galaxies ,quasars: individual: 3C 279 ,law.invention ,Raigs gamma ,Spitzer Space Telescope ,law ,MAGIC (telescope) ,010303 astronomy & astrophysics ,SPITZER-SPACE-TELESCOPE ,Quasars: individual: 3C 279 ,Physics ,Astrophysics::Instrumentation and Methods for Astrophysics ,VARIABILITY ,Gamma rays: galaxies ,OPTICAL CONTINUUM ,astro-ph.CO ,Spectral energy distribution ,Electrónica ,Física nuclear ,OBJECTS ,Electricidad ,Astrophysics - Cosmology and Nongalactic Astrophysics ,Flare ,GAMMA-RAY FLARE ,Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Context (language use) ,individual: 3C 279 [Quasars] ,0103 physical sciences ,Quasars ,Quàsars ,ATMOSPHERIC CHERENKOV TELESCOPE ,010308 nuclear & particles physics ,Gamma rays ,Quasar ,Astronomy and Astrophysics ,Light curve ,Galaxies ,BLAZARS ,Physics::History of Physics ,Galàxies ,13. Climate action ,Space and Planetary Science ,JET ,ddc:520 ,RADIATION ,EMISSION ,Fermi Gamma-ray Space Telescope - Abstract
11 páginas, 11 figuras, 4 tablas.-- El Pdf del artículo es la versión pre-print: arXiv:1101.2522v2.-- MAGIC Collaboration: et al., [Context]: 3C 279, the first quasar discovered to emit VHE γ-rays by the MAGIC telescope in 2006, was reobserved by MAGIC in January 2007 during a major optical flare and from December 2008 to April 2009 following an alert from the Fermi space telescope on an exceptionally high γ-ray state. [Aims]: The January 2007 observations resulted in a detection on January 16 with significance 5.4σ, corresponding to a F (>150 GeV) (3.8 ± 0.8) × 10-11 ph cm-2 s-1 while the overall data sample does not show significant signal. The December 2008–April 2009 observations did not detect the source. We study the multiwavelength behaviour of the source at the epochs of MAGIC observations, collecting quasi-simultaneous data at optical and X-ray frequencies and for 2009 also γ-ray data from Fermi. [Methods]: We study the light curves and spectral energy distribution of the source. The spectral energy distributions of three observing epochs (including the February 2006, which has been previously published) are modelled with one-zone inverse Compton models and the emission on January 16, 2007 also with two zone model and with a lepto-hadronic model. [Results]: We find that the VHE γ-ray emission detected in 2006 and 2007 challenges standard one-zone model, based on relativistic electrons in a jet scattering broad line region photons, while the other studied models fit the observed spectral energy distribution more satisfactorily., The support of the German BMBF and MPG, the Italian INFN, the Swiss National Fund SNF, and the Spanish MICINN is gratefully acknowledged. This work was also supported by the Marie Curie program, by the CPAN CSD2007-00042 and MultiDark CSD2009-00064 projects of the Spanish Consolider-Ingenio 2010 programme, by grant DO02-353 of the Bulgarian NSF, by grant 127740 of the Academy of Finland, by the YIP of the Helmholtz Gemeinschaft, by the DFG Cluster of Excellence “Origin and Structure of the Universe”, and by the Polish MNiSzW Grant N N203 390834.
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- 2011
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