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

Authors :
F. Mauri
Marco Feroci
Luigi Pacciani
P. Lipari
M. Galli
Piergiorgio Picozza
Massimo Rapisarda
A. Argan
Andrea Bulgarelli
L. A. Antonelli
Claudio Labanti
Enrico Costa
F. Verrecchia
B. Preger
P. A. Caraveo
Neil Gehrels
V. Vittorini
E. Vallazza
M. Trifoglio
E. Del Monte
C. Pittori
A. Pellizzoni
P. Romano
S. Vercellone
F. Perotti
A. Giuliani
G. Di Cocco
L. Salotti
A. Zambra
J. P. Osborne
David N. Burrows
L. Foggetta
M. Prest
I. Lapshov
Alessio Trois
Paolo Soffitta
M. Basset
Sandro Mereghetti
Francesco Lazzarotto
Y. Evangelista
V. La Parola
Martino Marisaldi
P. T. O'Brien
G. Chincarini
Marco Tavani
I. Donnarumma
A. W. Chen
Fulvio Gianotti
F. Fuschino
A. Morselli
G. Barbiellini
Paolo Giommi
Francesco Longo
G. Pucella
DEL MONTE, E
Feroci, M
Pacciani, L
Evangelista, Y
Donnarumma, I
Soffitta, P
Costa, E
Lapshov, I
Lazzarotto, F
Rapisarda, M
Argan, A
BARBIELLINI AMIDEI, Guido
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, Francesco
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., N
Chincarini, G
Gehrels, N
LA PAROLA, V
O'BRIEN P., T
OSBORNE J., P
Preger, B
Pittori, C
ANTONELLI L., A
Verrecchia, F
Giommi, P
Salotti, L.
Source :
Astronomy & Astrophysics. 478:L5-L9
Publication Year :
2007
Publisher :
EDP Sciences, 2007.

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 $\sim 19$ hours 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 of the optical afterglow were performed by the Swift UVOT and the Palomar automated 60-inch telescopes without any significant detection. Similarly the Very Large Array did not detect a radio afterglow. This is the first GRB event with a firm upper limit in the 100 MeV -- 30 GeV energy range, associated with an X-ray afterglow.<br />Comment: 7 pages, 4 figures (of which 2 in color), contains online material. Accepted for publication by Astronomy & Astrophysics Letters

Details

ISSN :
14320746 and 00046361
Volume :
478
Database :
OpenAIRE
Journal :
Astronomy & Astrophysics
Accession number :
edsair.doi.dedup.....8db2c0f277bf48b8bb8582fcbc2c1ade
Full Text :
https://doi.org/10.1051/0004-6361:20078816