INTEGRAL results on GRB 030320: A long gamma-ray burst detected at the edge of the field of view
Open Access
- 17 November 2003
- journal article
- letter
- Published by EDP Sciences in Astronomy & Astrophysics
- Vol. 411 (1) , L321-L325
- https://doi.org/10.1051/0004-6361:20031232
Abstract
GRB 030320 is the 5th gamma-ray burst (GRB) detected by INTEGRAL in the field of view (FoV). It is so far the GRB with the largest off-axis angle with respect to the INTEGRAL pointing direction, near to the edge of the FoV of both main instruments, IBIS and SPI. Nevertheless, it was possible to determine its position and to extract spectra and fluxes. The GRB nature of the event was confirmed by an IPN triangulation. It is a ~60 s long GRB with two prominent peaks separated by ~35 s. The spectral shape of the GRB is best represented by a single power law with a photon index . The peak flux in the 20–200 keV band is determined to ~5.7 photons cm-2 s-1 and the GRB fluence to erg cm-2. Analysing the spectral evolution of the GRB, a “hard-to-soft” behaviour emerges. A search for an optical counterpart has been carried out, but none was found.Keywords
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This publication has 20 references indexed in Scilit:
- IBIS: The Imager on-board INTEGRALAstronomy & Astrophysics, 2003
- SPI: The spectrometer aboard INTEGRALAstronomy & Astrophysics, 2003
- The INTEGRAL missionAstronomy & Astrophysics, 2003
- The INTEGRAL Science Data Centre (ISDC)Astronomy & Astrophysics, 2003
- INTEGRAL Spectrometer SPI's GRB detection capabilitiesAstronomy & Astrophysics, 2003
- Monte Carlo simulations and generation of the SPI responseAstronomy & Astrophysics, 2003
- The Spiros imaging software for the Integral SPI spectrometerAstronomy & Astrophysics, 2003
- Polarization of the prompt γ-ray emission from the γ-ray burst of 6 December 2002Nature, 2003
- Gamma-Ray Burst AfterglowsAnnual Review of Astronomy and Astrophysics, 2000
- Gamma-ray bursts from stellar mass accretion disks around black holesThe Astrophysical Journal, 1993