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arXiv · 1101.2764

PG 1553+113: five years of observations with MAGIC

MAGIC Collaboration·J. Aleksić·E. A. Alvarez·L. A. Antonelli·P. Antoranz·M. Asensio·M. Backes·J. A. Barrio·D. Bastieri·J. Becerra González·W. Bednarek·A. Berdyugin·K. Berger·E. Bernardini·A. Biland·O. Blanch·R. K. Bock·A. Boller·G. Bonnoli·D. Borla Tridon·I. Braun·T. Bretz·A. Cañellas·E. Carmona·A. Carosi·P. Colin·E. Colombo·J. L. Contreras·J. Cortina·L. Cossio·S. Covino·F. Dazzi·A. De Angelis·G. De Caneva·E. De Cea del Pozo·B. De Lotto·C. Delgado Mendez·A. Diago Ortega·M. Doert·A. Domínguez·D. Dominis Prester·D. Dorner·M. Doro·D. Elsaesser·D. Ferenc·M. V. Fonseca·L. Font·C. Fruck·R. J. García López·M. Garczarczyk·D. Garrido·G. Giavitto·N. Godinović·D. Hadasch·D. Häfner·A. Herrero·D. Hildebrand·D. Höhne-Mönch·J. Hose·D. Hrupec·B. Huber·T. Jogler·H. Kellermann·S. Klepser·T. Krähenbühl·J. Krause·A. La Barbera·D. Lelas·E. Leonardo·E. Lindfors·S. Lombardi·M. López·A. López-Oramas·E. Lorenz·M. Makariev·G. Maneva·N. Mankuzhiyil·K. Mannheim·L. Maraschi·M. Mariotti·M. Martínez·D. Mazin·M. Meucci·J. M. Miranda·R. Mirzoyan·H. Miyamoto·J. Moldón·A. Moralejo·P. Munar-Adrover·D. Nieto·K. Nilsson·R. Orito·I. Oya·D. Paneque·R. Paoletti·S. Pardo·J. M. Paredes·S. Partini·M. Pasanen·F. Pauss
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Abstract

We present the results of five years (2005-2009) of MAGIC observations of the BL Lac object PG 1553+113 at very high energies (VHEs, E > 100 GeV). Power law fits of the individual years are compatible with a steady mean photon index \Gamma = 4.27 $\pm$ 0.14. In the last three years of data, the flux level above 150 GeV shows a clear variability (probability of constant flux < 0.001%). The flux variations are modest, lying in the range from 4% to 11% of the Crab Nebula flux. Simultaneous optical data also show only modest variability that seems to be correlated with VHE gamma ray variability. We also performed a temporal analysis of (all available) simultaneous Fermi/LAT data of PG 1553+113 above 1 GeV, which reveals hints of variability in the 2008-2009 sample. Finally, we present a combination of the mean spectrum measured at very high energies with archival data available for other wavelengths. The mean spectral energy distribution can be modeled with a one-zone Synchrotron Self Compton (SSC) model, which gives the main physical parameters governing the VHE emission in the blazar jet.

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MAGIC Collaboration, J. Aleksić, E. A. Alvarez, L. A. Antonelli, P. Antoranz, M. Asensio, M. Backes, J. A. Barrio, D. Bastieri, J. Becerra González, W. Bednarek, A. Berdyugin, K. Berger, E. Bernardini, A. Biland, O. Blanch, R. K. Bock, A. Boller, G. Bonnoli, D. Borla Tridon, I. Braun, T. Bretz, A. Cañellas, E. Carmona, A. Carosi, P. Colin, E. Colombo, J. L. Contreras, J. Cortina, L. Cossio, S. Covino, F. Dazzi, A. De Angelis, G. De Caneva, E. De Cea del Pozo, B. De Lotto, C. Delgado Mendez, A. Diago Ortega, M. Doert, A. Domínguez, D. Dominis Prester, D. Dorner, M. Doro, D. Elsaesser, D. Ferenc, M. V. Fonseca, L. Font, C. Fruck, R. J. García López, M. Garczarczyk, D. Garrido, G. Giavitto, N. Godinović, D. Hadasch, D. Häfner, A. Herrero, D. Hildebrand, D. Höhne-Mönch, J. Hose, D. Hrupec, B. Huber, T. Jogler, H. Kellermann, S. Klepser, T. Krähenbühl, J. Krause, A. La Barbera, D. Lelas, E. Leonardo, E. Lindfors, S. Lombardi, M. López, A. López-Oramas, E. Lorenz, M. Makariev, G. Maneva, N. Mankuzhiyil, K. Mannheim, L. Maraschi, M. Mariotti, M. Martínez, D. Mazin, M. Meucci, J. M. Miranda, R. Mirzoyan, H. Miyamoto, J. Moldón, A. Moralejo, P. Munar-Adrover, D. Nieto, K. Nilsson, R. Orito, I. Oya, D. Paneque, R. Paoletti, S. Pardo, J. M. Paredes, S. Partini, M. Pasanen, F. Pauss. 2011-01-14. PG 1553+113: five years of observations with MAGIC. https://doi.org/10.1088/0004-637x/748/1/46

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