[ Previous | Next | ADS ]

Confirmation by AGILE of increased gamma-ray emission from the blazar 3C 279

ATel #5682; E. Striani, M. Tavani (INAF/IAPS and Univ. Tor Vergata), C. Pittori, F. Verrecchia, F. Lucarelli (ASDC and INAF/OAR), S. Colafrancesco (INAF/OAR and Wits University, Johannesburg), S. Vercellone (INAF/IASF-Pa), A. Bulgarelli, F. Gianotti, M. Trifoglio, V. Fioretti (INAF/IASF-Bo), M. Cardillo, G. Piano, I. Donnarumma, E. Del Monte, Y. Evangelista, M. Feroci, F. Lazzarotto, L. Pacciani, P. Soffitta, E. Costa, I. Lapshov, M. Rapisarda, A. Argan, G. Pucella, S. Sabatini, V. Vittorini (INAF/IAPS), A. Chen, A. Giuliani, S. Mereghetti, P. Caraveo, F. Perotti (INAF/IASF-Mi), F. Fuschino, M. Galli, C. Labanti, M. Marisaldi, G. Di Cocco (INAF/IASF-Bo), A. Pellizzoni, A. Trois (INAF/OA-Cagliari), M. Pilia (ASTRON, the Netherlands), G. Barbiellini, E. Vallazza (INFN Trieste), F. Longo (Univ. Trieste and INFN Trieste), A. Morselli, P. Picozza (INFN and Univ. Roma Tor Vergata), M. Prest (Univ. dell'Insubria), P. Lipari, D. Zanello (INFN and Univ. Roma Sapienza), P. W. Cattaneo, A. Rappoldi (INFN Pavia), A. Antonelli (INAF/OAR and ASDC), P. Giommi (ASDC), L. Salotti and G. Valentini (ASI).
on 22 Dec 2013; 14:10 UT
Credential Certification: Edoardo Striani (edoardo.striani@iasf-roma.inaf.it)

Subjects: Gamma Ray, >GeV, TeV, VHE, AGN, Blazar

AGILE confirms the detection of an enhanced gamma-ray emission from the FSRQ 3C 279 reported by the Fermi-LAT in ATel #5680.

A preliminary analysis of the gamma-ray emission detected from 2013-12-19 T06:00 to 2013-12-21 T06:00 (E > 100 MeV) yields a flux F = (600 +/- 170)x10^-8 ph cm^-2 s^-1, in agreement with the flux reported by Fermi-LAT.

AGILE analysis reveals that on December 22, 2013 the increased gamma-ray activity from 3C 279 is still ongoing.

This measurement was obtained with AGILE observing a large portion of the sky in spinning mode.

Multifrequency observations of the 3C 279 are strongly encouraged.