gptkbp:instanceOf
|
Imaging atmospheric Cherenkov telescope
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gptkbp:collaboratesWith
|
gptkb:MAGIC_Collaboration
over 165 scientists
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gptkbp:country
|
gptkb:Spain
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gptkbp:elevation
|
2200 meters above sea level
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gptkbp:fieldOfView
|
3.5 degrees
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gptkbp:firstLight
|
2004
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gptkbp:fundedBy
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gptkb:European_Union
gptkb:German_BMBF
Armenian SCS
Bulgarian NSF
Croatian MZOS
Italian INFN
Polish MNiSzW
Spanish MICINN
Swiss SNF
|
https://www.w3.org/2000/01/rdf-schema#label
|
MAGIC telescope
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gptkbp:locatedIn
|
gptkb:Roque_de_los_Muchachos_Observatory
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gptkbp:locatedOn
|
La Palma
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gptkbp:MAGIC-I
|
First telescope, operational since 2004
|
gptkbp:MAGIC-II
|
Second telescope, operational since 2009
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gptkbp:notableFinds
|
Detection of pulsed gamma rays from the Crab Pulsar above 25 GeV
Detection of very high energy gamma rays from distant active galactic nuclei
|
gptkbp:numberOfSatellites
|
2
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gptkbp:observationMethod
|
Imaging atmospheric Cherenkov technique
|
gptkbp:operatedBy
|
gptkb:Max_Planck_Institute_for_Physics
Institut de Fisica d'Altes Energies
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gptkbp:primaryMirrorDiameter
|
17 meters
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gptkbp:range
|
50 GeV to 50 TeV
|
gptkbp:relatedTo
|
gptkb:VERITAS
gptkb:Cherenkov_Telescope_Array
gptkb:H.E.S.S.
|
gptkbp:scientificGoals
|
Gamma-ray astronomy
|
gptkbp:telescopeType
|
Reflecting telescope
|
gptkbp:troopContributingCountries
|
gptkb:Armenia
gptkb:Brazil
gptkb:Bulgaria
gptkb:Croatia
gptkb:Finland
gptkb:France
gptkb:Germany
gptkb:India
gptkb:Italy
gptkb:Japan
gptkb:Poland
gptkb:Russia
gptkb:Spain
gptkb:Switzerland
gptkb:UK
gptkb:USA
|
gptkbp:wavelengthRange
|
Very high energy gamma rays
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gptkbp:website
|
https://magic.mpp.mpg.de/
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gptkbp:bfsParent
|
gptkb:PIC_(Spain)
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gptkbp:bfsLayer
|
7
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