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Fermi LAT View of a Sample of Flaring gamma-Ray AGNs
Fermi LAT View of a Sample of Flaring gamma-Ray AGNs
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Fermi LAT View of a Sample of Flaring gamma-Ray AGNs
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Fermi LAT View of a Sample of Flaring gamma-Ray AGNs
Fermi LAT View of a Sample of Flaring gamma-Ray AGNs
Journal Article

Fermi LAT View of a Sample of Flaring gamma-Ray AGNs

2014
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Overview
Issue Title: Special Issue: Proceedings of the International Conference on Variability of Blazars: From Jansky to Fermi (VBJF) In the first 3.5 years of operations, Fermi detected several sources whose flaring activity brought them to exceed daily fluxes brighter than F(E > 100MeV) > 10^sup -6^ ph cm^sup -2^ s^sup -1^. These episodes were promptly reported to the scientific community by the Fermi collaboration by means of astronomer telegrams (ATels). We focus our attention on the sample composed by these flaring sources, most of which are blazars, known to be extremely variable over the whole electromagnetic spectrum, from radio to γ-ray energies. We study properties of the selected sample and compare them to general characteristics of the Fermi source catalogue.
Publisher
Springer Nature B.V