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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Label Occurrences
VERITAS array canonical 1

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. NERFINISHED
MAGIC telescopes NERFINISHED
constructionCompleted 2007
country United States of America
surface form: United States
energyRange ~85 GeV to >30 TeV
fieldOfView about 3.5 degrees
firstLight 2007
fullName Very Energetic Radiation Imaging Telescope Array System NERFINISHED
hasCapability stereoscopic imaging of air showers
time-resolved observations of variable sources
locatedIn Arizona NERFINISHED
Fred Lawrence Whipple Observatory NERFINISHED
United States of America
surface form: United States
locatedNear Amado, Arizona NERFINISHED
mirrorDiameter 12 meters
numberOfTelescopes 4
observes very-high-energy gamma rays
operatedBy Smithsonian Astrophysical Observatory NERFINISHED
VERITAS Collaboration NERFINISHED
partOf ground-based very-high-energy gamma-ray observatory network
precursor Whipple 10 m gamma-ray telescope NERFINISHED
primaryObjective study of very-high-energy gamma-ray sources
scientificDiscipline astroparticle physics
gamma-ray astronomy
high-energy astrophysics
studies Galactic Center region NERFINISHED
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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