Latest results on galactic sources obtained with the MAGIC telescope

Abstract

The MAGIC telescope is the largest single-dish Imaging Atmospheric Cherenkov Telescope (IACT) with the lowest energy threshold among the current generation of IACTs as low as 25 GeV. Therefore, the MAGIC telescope is a perfect instrument to study the galactic sources especially in the context of observations with the satellite observatories Fermi and AGILE. This paper will give an overview of the MAGIC results on the galactic sources including detailed observations of binary systems, supernova remnants and the first detection of the Crab pulsar above 25 GeV .

2009 Fermi Symposium, eConf Proceedings C091122

References in corpus (9)

• VHE Gamma-Ray Observation of the Crab Nebula and its Pulsar with the MAGIC telescope
• Fermi Large Area Telescope Observations of the Crab Pulsar and Nebula
• Observation of Pulsed Gamma-rays Above 25 GeV from the Crab Pulsar with MAGIC
• Fermi LAT Observations of LS 5039
• Periodic very high energy gamma-ray emission from LS I +61 303 observed with the MAGIC telescope
• Search for VHE $\gamma$-ray emission from the globular cluster M13 with the MAGIC telescope
• Microquasar observations with the MAGIC telescope
• Observation of selected SNRs with the MAGIC Cherenkov Telescope
• Results from the observation of extragalactic objects with the MAGIC telescope