MAGIC (telescope)

Major Atmospheric Gamma Imaging Cherenkov Telescopes
The first MAGIC telescope
Alternative namesMAGIC Edit this at Wikidata
Part ofRoque de los Muchachos Observatory Edit this on Wikidata
Location(s)La Palma, Atlantic Ocean, international waters
Coordinates28°45′43″N 17°53′24″W / 28.761944444444°N 17.89°W / 28.761944444444; -17.89 Edit this at Wikidata
Altitude2,200 m (7,200 ft) Edit this at Wikidata
WavelengthGamma rays (indirectly)
Built2004
First light2004, 2009 Edit this on Wikidata
Telescope styleIACT
reflecting telescope
gamma-ray telescope Edit this on Wikidata
Diameter17 m (55 ft 9 in) Edit this at Wikidata
Collecting area236 m2 (2,540 sq ft) Edit this at Wikidata
Focal lengthf/D 1.03
Mountingmetal structure
ReplacedHEGRA Edit this on Wikidata
Websitemagic.mpp.mpg.de Edit this at Wikidata
MAGIC (telescope) is located in Canary Islands
MAGIC (telescope)
Location of MAGIC
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MAGIC (Major Atmospheric Gamma Imaging Cherenkov Telescopes, later renamed to MAGIC Florian Goebel Telescopes) is a system of two Imaging Atmospheric Cherenkov telescopes situated at the Roque de los Muchachos Observatory on La Palma, one of the Canary Islands, at about 2200 m above sea level. MAGIC detects particle showers released by gamma rays, using the Cherenkov radiation, i.e., faint light radiated by the charged particles in the showers. With a diameter of 17 meters for the reflecting surface, it was the largest in the world before the construction of H.E.S.S. II.

The first telescope was built in 2004 and operated for five years in standalone mode. A second MAGIC telescope (MAGIC-II), at a distance of 85 m from the first one, started taking data in July 2009. Together they integrate the MAGIC telescope stereoscopic system.[1]

MAGIC is sensitive to cosmic gamma rays with photon energies between 50 GeV (later lowered to 25 GeV) and 30 TeV due to its large mirror; other ground-based gamma-ray telescopes typically observe gamma energies above 200–300 GeV. Gamma-ray astronomy also utilizes satellite-based detectors, which can detect gamma-rays in the energy range from keV up to several GeV.

  1. ^ "Technical status of the MAGIC telescopes", MAGIC collaboration, Proc. International Cosmic Rays Conference 2009, arXiv:0907.1211

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