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Systematic Physical Characterization of the γ-Ray Spectra of 2FHL Blazars



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van den Berg, Jacobus P. and Bottcher, Markus and Domínguez Díaz, Alberto and López Moya, Marcos (2019) Systematic Physical Characterization of the γ-Ray Spectra of 2FHL Blazars. Astrophysical journal, 874 (1). ISSN 0004-637X

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Official URL: http://dx.doi.org/10.3847/1538-4357/aafdfd


We test different physically motivated models for the spectral shape of the gamma-ray emission in a sample of 128 blazars with known redshifts detected by the Fermi Large Area Telescope (LAT) at energies above 50. GeV. The first nine years of LAT data in the energy range from 300. MeV to 2. TeV are analyzed in order to extend the spectral energy coverage of the 2FHL blazars in our sample. We compare these spectral data to four leptonic models for the production of gamma-rays through Compton scattering by a population of electrons with different spectral shapes. In the first three models we consider Compton scattering in the Thomson regime with different acceleration mechanisms for the electrons. In the fourth model we consider Compton scattering by a pure power-law distribution of electrons with spectral curvature due to scattering in the Klein-Nishina regime. The majority of blazar gamma-ray spectra are preferentially fit with either a power law with exponential cutoff in the Thomson regime or a power-law electron distribution with Compton scattering in the Klein-Nishina regime, while a log-parabola with a low-energy power-law and broken power-law spectral shape in the Thomson regime appears systematically disfavored, which is likely a consequence of the restriction to pure Thomson scattering that we imposed on those models. This finding may be an indication that the gamma-ray emission from flat-spectrum radio quasars (FSRQs) in the 2FHL catalog is dominated by Compton scattering of radiation from the dusty torus, while in the case of BL Lac objects, it is dominated by synchrotron self-Compton radiation.

Item Type:Article
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© 2019. The American Astronomical Society. All rights reserved. Additional support for science analysis during the operations phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d'Etudes Spatiales in France. This work performed in part under DOE Contract DE-AC02-76SF00515.; The authors thank Markos Georganopoulos and the anonymous reviewer for useful comments. J.P.v.d.B. acknowledges the support of the National Astrophysics and Space Science Program (NASSP) in South Africa. M.B. acknowledges support through the South African Research Chair Initiative (SARChI) of the Department of Science and Technology and the National Research Foundation<SUP>3</SUP> (NRF) of South Africa under NRF SARChI Chair grant no. 64789. A.D. thanks the support of the Juan de la Cierva program from the Spanish MEC.

Uncontrolled Keywords:Log-parabolic spectra; Particle-acceleration; Emission; Band
Subjects:Sciences > Physics > Nuclear physics
ID Code:55986
Deposited On:05 Jul 2019 10:10
Last Modified:05 Jul 2019 10:10

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