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MAGIC upper limits on the high energy emission from GRBs

2007/09/10 by D. Bastieri, Bastieri, D., N. Galante +11
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Particle Detector Development and Performance

paper · pdf · doi:10.48550/arxiv.0709.1386

openalex publication_date 2007/09/10 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

During its cycle-1 observation period, between April 2005 and March 2006, the MAGIC telescope was able to observe nine Gamma Ray Burst (GRB) events since their early beginning. Other observations were performed during the following months in the cycle-2 observation period. The observations, with an energy threshold spanning from 80 to 200 GeV, did not reveal any gamma 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 in the metagalactic radiation field.

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