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GRB 070724B: the first gamma ray burst localized by SuperAGILE and its Swift X-ray afterglow

Authors :
Del Monte, E.
Feroci, M.
Pacciani, L.
Evangelista, Y.
Donnarumma, I.
Soffitta, P.
Costa, E.
Lapshov, I.
Lazzarotto, F.
Rapisarda, M.
Argan, A.
Barbiellini, G.
Basset, M.
Bulgarelli, A.
Caraveo, P.
Chen, A.
Di Cocco, G.
Foggetta, L.
Fuschino, F.
Galli, M.
Gianotti, F.
Giuliani, A.
Labanti, C.
Lipari, P.
Longo, F.
Marisaldi, M.
Mauri, F.
Mereghetti, S.
Morselli, A.
Pellizzoni, A.
Perotti, F.
Picozza, P.
Prest, M.
Pucella, G.
Tavani, M.
Trifoglio, M.
Trois, A.
Vallazza, E.
Vercellone, S.
Vittorini, V.
Zambra, A.
Romano, P.
Burrows, D.
Chincarini, G.
Gehrels, N.
La Parola, V.
O'Brien, P.
Osborne, J.
Preger, B.
Pittori, C.
Antonelli, L.
Verrecchia, F.
Giommi, P.
Salotti, L.
Source :
Astronomy and Astrophysics; January 2008, Vol. 478 Issue: 1 pL5-L9, 5p
Publication Year :
2008

Abstract

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.

Details

Language :
English
ISSN :
00046361 and 14320746
Volume :
478
Issue :
1
Database :
Supplemental Index
Journal :
Astronomy and Astrophysics
Publication Type :
Periodical
Accession number :
ejs13473541