Search for Gamma-Ray Emission from the Supernova Remnant IC 443 with the MAGIC Telescope

Bibcode
2009RMxAC..35...62G
García López, R. J.
Bibliographical reference

XII Latin American IAU Regional Meeting (Eds. G. Magris, G. Bruzual, & L. Carigi) Revista Mexicana de Astronomía y Astrofísica (Serie de Conferencias) Vol. 35, pp. 62-63 (2009) (http://www.astroscu.unam.mx/~rmaa/)

Advertised on:
5
2009
Number of authors
1
IAC number of authors
1
Citations
0
Refereed citations
0
Description
TeV observations of Supernova remnants (SNRs) and, in particular, of SNRs which appear to be physically related to EGRET sources are a prime target for the MAGIC telescope. MAGIC's spatial resolution and sensitivity can probe the main mechanism responsible for producing high energy photons in the SNR neighbourhood. Based on a recent systematical analysis of the molecular environment of the vicinity of all SNR-EGRET source pairs, the IC 443 remnant was chosen for observations with MAGIC. We briefly describe the observational strategy which provided the detection of a new very-high energy gamma-ray source: MAGIC J0616+225.
Type
Non-refereed
Gamma rays
Supernova remnants

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