Published May 16, 1998 | Version v1
Journal article

Search for GeV GRBs at Chacaltaya

  • 1. Istituto di Cosmogeofisica del C.N.R., Torino (Italy)
  • 2. Dipartimento di Fisica Generale dell'Universita' di Torino (Italy)
  • 3. Department of Physics, Ehime University, Ehime 790 (Japan)
  • 4. Department of Physics, Okayama University, Okayama 700 (Japan)
  • 5. Department of Physics, Tokyo Institute of Technology, Meguro, Tokyo 152 (Japan)
  • 6. Institute of Physical and Chemical Research, Wako, Saitama 351-01 (Japan)
  • 7. Instituto de Investigaciones Fisicas, Universidad Mayor de San Andres, La Paz (Bolivia, Plurinational State of)
  • 8. NASA Goddard Space Flight Center, Greenbelt, Maryland 20771 (United States)
  • 9. NASA Marshall Space Flight Center, Huntsville, Alabama 35812 (United States)

Description

In this paper we present the results of a search for GeV Gamma Ray Bursts made by the INCA experiment during the first 9 months of operation. INCA, an air shower array located at Mount Chacaltaya (Bolivia) at 5200 m a.s.l., has been searching for GRBs since December 1996. Up to August, 1997, 34 GRBs detected by BATSE occurred in the field of view of the experiment. For any burst, the counting rate of the array in the 2 hours interval around the burst trigger time has been studied. No significant excess has been observed. Assuming for the bursts a power low energy spectrum extending up to 1 TeV with a slope α=-2 and a duration of 10 s, the obtained 1 GeV-1 TeV energy fluence upper limits range from 7.9 10-5 erg cm-2 to 3.5 10-3 erg cm-2 depending on the event zenith angles

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
428
Journal Issue
1
Journal Page Range
p. 914-920
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.