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oai:docta.ucm.es:20.500.14352/438072024-09-06T16:24:12Zcom_20.500.14352_14col_20.500.14352_15

PG 1553+113: Five years of observations with MAGIC Antoranz Canales, Pedro Barrio Uña, Juan Abel Contreras González, José Luis Fonseca González, María Victoria Miranda Pantoja, José Miguel Scapin, Valeria 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 +/- 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/Large Area Telescope 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 VHEs with archival data available for other wavelengths. The mean spectral energy distribution can be modeled with a one-zone synchrotron self-Compton model, which gives the main physical parameters governing the VHE emission in the blazar jet. 2023-06-20T03:32:37Z 2023-06-20T03:32:37Z 2023-06-20T03:32:37Z 2012-03-20 journal article https://hdl.handle.net/20.500.14352/43807 0004-637X 10.1088/0004-637X/748/1/46 eng CSD2007-00042 CSD2009-00064 DO02-353 127740 SFB823/C4 SFB876/C3 745/N-HESS-MAGIC/2010/0 open access IOP Publishing