Published May 16, 1998 | Version v1
Journal article

Performance and scientific results of the BeppoSAX Gamma-Ray Burst Monitor

  • 1. Istituto di Astrofisica Spaziale-CNR-Frascati (Italy)
  • 2. Dipartimento di Fisica-Universita di Ferrara-Ferrara (Italy)
  • 3. Istituto Tecnologie e Studio Radiazioni Extraterrestre-CNR-Bologna (Italy)
  • 4. Istituto Astronomico-Universita La Sapienza-Roma (Italy)
  • 5. BeppoSAX-SOC-Nuova Telespazio-Roma (Italy)

Description

The Italian-Dutch satellite for X-ray Astronomy BeppoSAX is successfully operating on a 600 km equatorial orbit since May 1996. We present here the in-flight performance of the Gamma Ray Burst Monitor (GRBM) experiment during its first year of operation. The GRBM is performing very well, providing an amount of data on GRBs, some of which confirmed by other experiments onboard satellites. It also joined the 3rd Interplanetary Network as a new near-earth node. Important results have been obtained for GRBs (e.g. GRB970228) simultaneously detected in the Wide Field Cameras onboard the same satellite

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
428
Journal Issue
1
Journal Page Range
p. 451-455
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
4. Huntsville gamma-ray burst symposium
Dates
15-20 Sep 1997
Place
Huntsville, AL (United States)

Optional Information

Notes
(c) 1998 American Institute of Physics.