Results of MAGIC on Galactic sources
Javier Rico (for the MAGIC Collaboration)
TL;DR
This paper reviews recent MAGIC telescope results on Galactic sources, highlighting its unique capability to observe high-energy gamma-rays below 100 GeV and its findings on pulsars, binaries, supernova remnants, and unidentified sources.
Contribution
It provides a comprehensive overview of MAGIC's latest experimental results on various Galactic gamma-ray sources, emphasizing its unique observational capabilities.
Findings
Detection of gamma-ray emissions from pulsars.
Observation of binary systems and supernova remnants.
Identification of previously unknown gamma-ray sources.
Abstract
MAGIC is a single-dish Cherenkov telescope located on La Palma (Spain), hence with an optimal view on the Northern sky. Sensitive in the 30 GeV-30 TeV energy band, it is nowadays the only ground-based instrument being able to measure high-energy gamma-rays below 100 GeV. We review the most recent experimental results on Galactic sources obtained using MAGIC. These include pulsars, binary systems, supernova remnants and unidentified sources.
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