VERITAS array

E701441

The VERITAS array is a ground-based gamma-ray observatory consisting of multiple imaging atmospheric Cherenkov telescopes used to study very high-energy astrophysical phenomena.

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VERITAS array canonical 1

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Statements (47)

Predicate Object
instanceOf gamma-ray observatory ⓘ
abbreviation VERITAS ⓘ
altitude about 1268 meters above sea level ⓘ
collaborationIncludes institutions from Canada ⓘ
institutions from Germany ⓘ
institutions from Ireland ⓘ
institutions from the United Kingdom ⓘ
institutions from the United States ⓘ
commissioned 2007 ⓘ
comparableTo H.E.S.S. ⓘ
MAGIC telescopes ⓘ
constructionCompleted 2007 ⓘ
country United States ⓘ
energyRange ~85 GeV to >30 TeV ⓘ
fieldOfView about 3.5 degrees ⓘ
firstLight 2007 ⓘ
fullName Very Energetic Radiation Imaging Telescope Array System ⓘ
hasCapability stereoscopic imaging of air showers ⓘ
time-resolved observations of variable sources ⓘ
locatedIn Arizona ⓘ
Fred Lawrence Whipple Observatory ⓘ
United States ⓘ
locatedNear Amado, Arizona ⓘ
mirrorDiameter 12 meters ⓘ
numberOfTelescopes 4 ⓘ
observes very-high-energy gamma rays ⓘ
operatedBy Smithsonian Astrophysical Observatory ⓘ
VERITAS Collaboration ⓘ
partOf ground-based very-high-energy gamma-ray observatory network ⓘ
precursor Whipple 10 m gamma-ray telescope ⓘ
primaryObjective study of very-high-energy gamma-ray sources ⓘ
scientificDiscipline astroparticle physics ⓘ
gamma-ray astronomy ⓘ
high-energy astrophysics ⓘ
studies Galactic Center region ⓘ
linked to: Milky Way center

active galactic nuclei ⓘ
cosmic-ray acceleration ⓘ
dark matter candidates ⓘ
extragalactic background light ⓘ
gamma-ray binaries ⓘ
gamma-ray bursts ⓘ
pulsar wind nebulae ⓘ
pulsars ⓘ
starburst galaxies ⓘ
supernova remnants ⓘ
telescopeType imaging atmospheric Cherenkov telescope ⓘ
usesTechnique imaging atmospheric Cherenkov technique ⓘ

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Full triples — surface form annotated when it differs from this entity's canonical label.