Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-11-24
Astrophys.J.694:294-301,2009
Astronomy and Astrophysics
Astrophysics
13 pages, 8 figures, accepted for publication in the Astrophysical Journal
Scientific paper
10.1088/0004-637X/694/1/294
We report the Suzaku observations of the high luminosity blazar SWIFT J0746.3+2548 (J0746) conducted in November 2005. This object, with z = 2.979, is the highest redshift source observed in the Suzaku Guaranteed Time Observer (GTO) period, is likely to show high gamma-ray flux peaking in the MeV range. As a result of the good photon statistics and high signal-to-noise ratio spectrum, the $Suzaku$ observation clearly confirms that J0746 has an extremely hard spectrum in the energy range of 0.3-24 keV, which is well represented by a single power-law with a photon index of 1.17 and Galactic absorption. The multiwavelength spectral energy distribution of J0746 shows two continuum components, and is well modeled assuming that the high-energy spectral component results from Comptonization of the broad-line region photons. In this paper we search for the bulk Compton spectral features predicted to be produced in the soft X-ray band by scattering external optical/UV photons by cold electrons in a relativistic jet. We discuss and provide constraints on the pair content resulting from the apparent absence of such features.
Edwards Philip G.
Kataoka Jun
Madejski Greg
Pursimo Tapio
Romani Roger
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