GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew

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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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Detalles Bibliográficos
Autor principal: Gotz, D.
Otros Autores: 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.
Formato: Capítulo de libro
Lenguaje:Inglés
Publicado: Elsevier B.V. 2004
Acceso en línea:Registro en Scopus
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Biblioteca Central Dr. Luis F. Leloir (FCEN) de Universidad de Buenos Aires
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100 1 |a Gotz, D. 
245 1 0 |a GRB 030131: A long Gamma-ray Burst detected with INTEGRAL during a satellite slew 
260 |b Elsevier B.V.  |c 2004 
270 1 0 |m Gotz, D.; Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF), CNR, Via Bassini 15, Milano I-20133, Italy 
506 |2 openaire  |e Política editorial 
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504 |a Winkler, C., (2003) A&A, , in press 
504 |a Mereghetti, S., (2003) A&A, , in press 
504 |a Courvoisier, T., (2003) A&A, , in press 
504 |a Mereghetti, S., 2003, these proceedings; Preece, R.D., (1998) ApJ, 496, p. 849 
504 |a Ubertini, P., (2003) A&A, , in press 
504 |a Vedrenne, G., (2003) A&A, , in press 
504 |a Borkowski, J., Götz, D., Mereghetti, S., (2003) GCN, p. 1836 
504 |a Mereghetti, S., (2003) GCN, p. 1847 
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504 |a Gorosabel, J., (2003) GCN, p. 1866 
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520 3 |a 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.  |l eng 
593 |a Istituto di Astrofisica Spaziale e Fisica Cosmica (IASF), CNR, Via Bassini 15, Milano I-20133, Italy 
593 |a UC Berkeley Space Sciences Laboratory, Berkeley CA 94720-7450, United States 
593 |a Integral Science Data Centre, Chemin d'Écogia 16, CH-1290 Versoix, Switzerland 
593 |a IASF - CNR, Sezione di Roma, via Fosso del Cavaliere 100, I-00133 Roma, Italy 
593 |a Dipartimento di Fisica, Università di Ferrara, Via Paradiso 12, I-44100 Ferrara, Italy 
593 |a Space Telescope Science Institute, 3700 San Martin Drive, Baltimore, MD 21218, United States 
593 |a Instituto de Astrofísica de Andalucía (IAA-CSIC), P.O. Box 03004, E-18080 Granada, Spain 
593 |a Department of Physics and Astronomy, Clemson University, Clemson, SC 29634-0978, United States 
593 |a Astronomical Observatory, University of Copenhagen, Juliane Maries Vej 30, 2100 Copenhagen, Denmark 
593 |a Astronomical Institute, Academy of Sciences of the Czech Republic, CZ-251 65 Ondrejov, Czech Republic 
593 |a Service d'Astrophysique, CEA/Saclay, Orme des Merisiers Bât. 709, F-91191 Gif-sur-Yvette, France 
593 |a Instituto de Astronomia y Fisica Del Espacio, CONICET, cc67, suc 28, 1428 Buenos Aires, Argentina 
593 |a Osservatorio Astronomico di Trieste, Via G.B. Tiepolo 11, I-34131 Trieste, Italy 
593 |a IASF - CNR, Sezione di Bologna, via Piero Gobetti 101, I-40129 Bologna, Italy 
593 |a ESA-ESTEC, RSSD, Keplerlaan 1, 2201 AZ Noordwijk, Netherlands 
700 1 |a Mereghetti, S. 
700 1 |a Hurley, K. 
700 1 |a Deluit, S. 
700 1 |a Feroci, M. 
700 1 |a Frontera, F. 
700 1 |a Fruchter, A. 
700 1 |a Gorosabel, J. 
700 1 |a Hartmann, D.H. 
700 1 |a Hjorth, J. 
700 1 |a Huded, R. 
700 1 |a Mirabel, I.F. 
700 1 |a Pian, E. 
700 1 |a Pizzichini, G. 
700 1 |a Ubertini, P. 
700 1 |a Winkler, C. 
773 0 |d Elsevier B.V., 2004  |g v. 132  |h pp. 316-319  |p Nucl. Phys. B Proc. Suppl.  |x 09205632  |w (AR-BaUEN)CENRE-1779  |t Nuclear Physics B - Proceedings Supplements 
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856 4 0 |u https://doi.org/10.1016/j.nuclphysbps.2004.04.056  |y DOI 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_09205632_v132_n_p316_Gotz  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_09205632_v132_n_p316_Gotz  |y Registro en la Biblioteca Digital 
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