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American Astronomical Society, Astrophysical Journal, 1(676), p. L13-L16, 2008

DOI: 10.1086/587170

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Agile Detection of a Strong Gamma-Ray Flare from the Blazar 3C 454.3

Journal article published in 2008 by S. Vercellone, A. W. Chen ORCID, A. Giuliani ORCID, A. Bulgarelli ORCID, I. Donnarumma ORCID, I. Lapshov, M. Tavani, V. Cocco, A. Argan ORCID, G. Barbiellini, E. D. Monte, P. Caraveo, G. D. Paris, E. Costa ORCID, F. D'Ammando and other authors.
This paper is made freely available by the publisher.
This paper is made freely available by the publisher.

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Abstract

We report the first blazar detection by the AGILE satellite. AGILE detected 3C 454.3 during a period of strongly enhanced optical emission in July 2007. AGILE observed the source with a dedicated repointing during the period 2007 July 24-30 with its two co-aligned imagers, the Gamma-Ray Imaging Detector and the hard X-ray imager Super-AGILE sensitive in the 30 MeV-50 GeV and 18-60 keV, respectively. Over the entire period, AGILE detected gamma-ray emission from 3C 454.3 at a significance level of 13.8-$σ$ with an average flux (E$>$100 MeV) of $(280 ± 40) \times 10^{-8}$ photons cm$^{-2}$ s$^{-1}$. The gamma-ray flux appears to be variable towards the end of the observation. No emission was detected by Super-AGILE in the energy range 20-60 keV, with a 3-$σ$ upper limit of $2.3 \times 10^{-3}$ photons cm$^{-2}$ s$^{-1}$. The gamma-ray flux level of 3C 454.3 detected by AGILE is the highest ever detected for this quasar and among the most intense gamma-ray fluxes ever detected from Flat Spectrum Radio Quasars. Comment: Accepted by Astrophysical Journal Letters; 14 pages, 3 EPS Figures, 1 Table