posted on 2012-10-24, 09:21authored byDel Monte E, M. Feroci, L. Pacciani, Y. Evangelista, I. Donnarumma, P. Soffitta, E. Costa, I. Lapshov, F. Lazzarotto, A. Argan, G. Pucella, M. Tavani, A. Trois, V. Vittorini, P. Lipari, M. Rapisarda, G. Barbiellini, M. Basset, L. Foggetta, F. Longo, E. Vallazza, A. Bulgarelli, Di Cocco G, F. Fuschino, F. Gianotti, C. Labanti, M. Marisaldi, M. Trifoglio, P. Caraveo, A. Chen, A. Giuliani, S. Mereghetti, A. Pellizzoni, F. Perotti, S. Vercellone, M. Galli, F. Mauri, A. Morselli, P. Picozza, M. Prest, A. Zambra, P. Romano, G. Chincarini, D. N. Burrows, N. Gehrels, La Parola V, P. T. O'Brien, J. P. Osborne, B. Preger, C. Pittori, L. A. Antonelli, F. Verrecchia, P. Giommi, L. Salotti
GRB 070724B is the first gamma ray burst localized by SuperAGILE, the hard X-ray monitor aboard the AGILE satellite. The coordinates of the event were published ~19 h after the trigger. The Swift X-Ray Telescope pointed at the SuperAGILE location and detected the X-ray afterglow inside the SuperAGILE error circle. The AGILE gamma-ray Tracker and Minicalorimeter did not detect any significant gamma ray emission associated with GRB 070724B in the MeV and GeV range, neither prompt nor delayed. Searches for the optical afterglow were performed by the Swift UVOT and the Palomar automated 60-inch telescopes, resulting in no significant detection. Similarly, the Very Large Array did not detect any radio afterglow. This is the first GRB event associated with an X-ray afterglow with a firm upper limit in the 100 MeV-30 GeV energy range.
History
Citation
Astronomy & Astrophysics, 2008, 478 (1)
Version
VoR (Version of Record)
Published in
Astronomy & Astrophysics
Publisher
EDP Sciences for European Southern Observatory (ESO)