Observations of VHE gamma-Ray Sources with the MAGIC Telescope

TL;DR

The paper discusses the MAGIC telescope's capabilities, observational strategies, and initial results in detecting very high energy gamma-ray sources, highlighting its contributions to gamma-ray astronomy since 2004.

Contribution

It presents the MAGIC telescope's design, operational procedures, and early observational results, including the detection of various gamma-ray sources, and outlines future developments.

Findings

Detection of gamma-ray sources like SNRs, pulsars, and AGNs.

Operational success of the MAGIC telescope since 2004.

Plans for constructing a second MAGIC telescope.

Abstract

The MAGIC telescope with its 17m diameter mirror is today the largest operating single-dish Imaging Air Cherenkov Telescope (IACT). It is located on the Canary Island La Palma, at an altitude of 2200m above sea level, as part of the Roque de los Muchachos European Northern Observatory. The MAGIC telescope detects celestial very high energy gamma-radiation in the energy band between about 50 GeV and 10 TeV. Since Autumn of 2004 MAGIC has been taking data routinely, observing various objects like supernova remnants (SNRs), gamma-ray binaries, Pulsars, Active Galactic Nuclei (AGN) and Gamma-ray Bursts (GRB). We briefly describe the observational strategy, the procedure implemented for the data analysis, and discuss the results for individual sources. An outlook to the construction of the second MAGIC telescope is given.