Published May 25, 2009 | Version v1
Journal article

Observation of GRBs with the MAGIC Telescope

  • 1. Max-Planck-Institut fuer Physik, Foehringer Ring 6, D-80805 Muenchen (Germany)
  • 2. INAF Roma, Viale del Parco Mellini 84, I-00136 Roma (Italy)
  • 3. Universita degli Studi di Padova, via Marzolo 8, I-35131 Padova (Italy)
  • 4. Instituto de Astrofisica de Canarias, via Lactea s/n, E-38205 La Laguna, Tenerife (Spain)
  • 5. INFN Trieste, via F Valerio 2, I-34127 Trieste (Italy)
  • 6. Universita degli Studi di Udine, via delle Scienze 208, I-33100 Udine (Italy)

Description

After three years since the beginning of operation, the MAGIC telescope could observe several GRB events in the prompt and early afterglow phase. Thanks to its innovative design, the telescope could promptly react to incoming GCN alerts and rapidly slew to the burst coordinates within a typical delay of 50 seconds, performing observations with an energy threshold spanning from 80 to 200 GeV. The observations did not reveal any γ-ray emission. The computed upper limits are compatible with a power law extrapolation, where intrinsic fluxes are evaluated taking into account the attenuation due to the scattering with the Extragalactic Background Light.

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
1133
Journal Issue
1
Journal Page Range
p. 334-337
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
6. Huntsville symposium on gamma-ray burst
Dates
20-23 Oct 2008
Place
Huntsville, AL (United States)

Optional Information

Notes
(c) 2009 American Institute of Physics