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

Bibcode
2009RMxAC..35...62G
García López, R. J.
Referencia bibliográfica

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/)

Fecha de publicación:
5
2009
Número de autores
1
Número de autores del IAC
1
Número de citas
0
Número de citas referidas
0
Descripción
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.
Tipo
Sin árbitro
Rayos gamma
Restos de supernova

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