GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew
A long Gamma-Ray Burst (GRB) was detected with the instruments on board the INTEGRAL satellite on January 31 2003. Although most of the GRB, which lasted ∼150 seconds, occurred during a satellite slew, the automatic software of the INTEGRAL Burst Alert System was able to detect it in near-real time....
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todo:paper_09205632_v132_n_p316_Gotz2023-10-03T15:44:53Z GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew Gotz, D. Mereghetti, S. Hurley, K. Deluit, S. Feroci, M. Frontera, F. Fruchter, A. Gorosabel, J. Hartmann, D.H. Hjorth, J. Huded, R. Mirabel, I.F. Pian, E. Pizzichini, G. Ubertini, P. Winkler, C. A long Gamma-Ray Burst (GRB) was detected with the instruments on board the INTEGRAL satellite on January 31 2003. Although most of the GRB, which lasted ∼150 seconds, occurred during a satellite slew, the automatic software of the INTEGRAL Burst Alert System was able to detect it in near-real time. Here we report the results obtained with the IBIS instrument, which detected GRB 030131 in the 15 keV - 200 keV energy range, The burst displays a complex time profile with numerous peaks. The peak spectrum can be described by a single power law with photon index γ ≃1.7 and has a flux of ∼2 photons cm -2 s-1 in the 20-200 keV energy band. The high sensitivity of IBIS has made it possible for the first time to perform detailed time-resolved spectroscopy of a GRB with a fluence of 7×10-6 erg cm-2 (20-200 keV). © 2004 Elsevier B .V. All rights reserved. CONF info:eu-repo/semantics/openAccess http://creativecommons.org/licenses/by/2.5/ar http://hdl.handle.net/20.500.12110/paper_09205632_v132_n_p316_Gotz |
institution |
Universidad de Buenos Aires |
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I-28 |
repository_str |
R-134 |
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Biblioteca Digital - Facultad de Ciencias Exactas y Naturales (UBA) |
description |
A long Gamma-Ray Burst (GRB) was detected with the instruments on board the INTEGRAL satellite on January 31 2003. Although most of the GRB, which lasted ∼150 seconds, occurred during a satellite slew, the automatic software of the INTEGRAL Burst Alert System was able to detect it in near-real time. Here we report the results obtained with the IBIS instrument, which detected GRB 030131 in the 15 keV - 200 keV energy range, The burst displays a complex time profile with numerous peaks. The peak spectrum can be described by a single power law with photon index γ ≃1.7 and has a flux of ∼2 photons cm -2 s-1 in the 20-200 keV energy band. The high sensitivity of IBIS has made it possible for the first time to perform detailed time-resolved spectroscopy of a GRB with a fluence of 7×10-6 erg cm-2 (20-200 keV). © 2004 Elsevier B .V. All rights reserved. |
format |
CONF |
author |
Gotz, D. Mereghetti, S. Hurley, K. Deluit, S. Feroci, M. Frontera, F. Fruchter, A. Gorosabel, J. Hartmann, D.H. Hjorth, J. Huded, R. Mirabel, I.F. Pian, E. Pizzichini, G. Ubertini, P. Winkler, C. |
spellingShingle |
Gotz, D. Mereghetti, S. Hurley, K. Deluit, S. Feroci, M. Frontera, F. Fruchter, A. Gorosabel, J. Hartmann, D.H. Hjorth, J. Huded, R. Mirabel, I.F. Pian, E. Pizzichini, G. Ubertini, P. Winkler, C. GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew |
author_facet |
Gotz, D. Mereghetti, S. Hurley, K. Deluit, S. Feroci, M. Frontera, F. Fruchter, A. Gorosabel, J. Hartmann, D.H. Hjorth, J. Huded, R. Mirabel, I.F. Pian, E. Pizzichini, G. Ubertini, P. Winkler, C. |
author_sort |
Gotz, D. |
title |
GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew |
title_short |
GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew |
title_full |
GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew |
title_fullStr |
GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew |
title_full_unstemmed |
GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew |
title_sort |
grb 030131: a long gamma-ray burst detected with integral during a satellite slew |
url |
http://hdl.handle.net/20.500.12110/paper_09205632_v132_n_p316_Gotz |
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