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

Abstract

We report the first blazar detection by AGILE. AGILE detected 3C 454.3 during a period of strongly enhanced optical emission in 2007 July. 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 SuperAGILE sensitive in the 30 MeV to 50 GeV and 18-60 keV ranges, respectively. Over the entire period, AGILE detected γ-ray emission from 3C 454.3 at a significance level of 13.8 σ with an average flux (E> 100 MeV) of (280 ± 40) x 10-8 photons cm -2 s-1. The γ-ray flux appears to be variable toward 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 x 10-3 photons cm-2 s-1. The γ-ray flux level of 3C 454.3 detected by AGILE is the highest ever detected for this quasar and among the most intense γ-ray fluxes ever detected from flat-spectrum radio quasars. © 2008. The American Astronomical Society. All rights reserved Subject heading: gamma rays: observations-quasars: individual (3C 454.3).