VERITAS: the Very Energetic Radiation Imaging Telescope Array System
arXiv:astro-ph/0108478 · doi:10.1016/S0927-6505(01)00152-9
Abstract
The Very Energetic Radiation Imaging Telescope Array System (VERITAS) represents an important step forward in the study of extreme astrophysical processes in the universe. It combines the power of the atmospheric Cherenkov imaging technique using a large optical reflector with the power of stereoscopic observatories using arrays of separated telescopes looking at the same shower. The seven identical telescopes in VERITAS, each of aperture 10 m, will be deployed in a filled hexagonal pattern of side 80 m; each telescope will have a camera consisting of 499 pixels with a field of view of 3.5 deg VERITAS will substantially increase the catalog of very high energy (E > 100GeV) gamma-ray sources and greatly improve measurements of established sources.
44 pages, 16 figures
References in corpus (8)
- Very High Energy Gamma-Ray Astronomy
- Can cosmic strangelets reach the earth?
- Extragalactic background light absorption signal in the TeV gamma-ray spectra of blazars
- Gamma-ray Observations of the Galactic Plane at Energies E > 500 GeV
- A High Resolution Method for Measuring Cosmic Ray Composition beyond 10 TeV
- Flux Sensitivity of VERITAS
- Status of VHE Astronomy c.2000
- Detection Techniques of Microsecond Gamma-Ray Bursts using Ground-Based Telescopes
Cited by in corpus (193)
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- Astrophysical Origins of Ultrahigh Energy Cosmic Rays
- TeV gamma-rays and the largest masses and annihilation cross sections of neutralino dark matter
- An ISOCAM survey through gravitationally lensing galaxy clusters
- The Trigger System of the H.E.S.S. Telescope Array
- Dark matter searches with Cherenkov telescopes: nearby dwarf galaxies or local galaxy clusters?
- Constraints on Cosmic Rays, Magnetic Fields, and Dark Matter from Gamma-Ray Observations of the Coma Cluster of Galaxies with VERITAS and Fermi
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- Stochastic conversions of TeV photons into axion-like particles in extragalactic magnetic fields
- Systematic search for gamma-ray periodicity in active galactic nuclei detected by the Fermi Large Area Telescope
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- A new measurement of the Hubble constant and matter content of the Universe using extragalactic background light -ray attenuation
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- The Discovery of gamma-Ray Emission From The Blazar RGB J0710+591
- VERITAS Search for VHE Gamma-ray Emission from Dwarf Spheroidal Galaxies
- The observability of gamma-rays from neutralino annihilations in Milky Way substructure
- Coordinated Multiwavelength Observations of BL Lacertae in 2000
- Discovery of very high energy gamma rays from PKS 1424+240 and multiwavelength constraints on its redshift
- The Gamma-Ray Window to Intergalactic Magnetism
- Detection of Leptonic Dark Matter
- Gamma-ray observations of Tycho's SNR with VERITAS and Fermi
- Self-annihilation of the neutralino dark matter into two photons or a Z and a photon in the MSSM
- The Hunt for Pevatrons: The Case of Supernova Remnants
- Detection of Extended VHE Gamma Ray Emission from G106.3+2.7 with VERITAS
- Unidentified sources in the Fermi-LAT second source catalog: the case for DM subhalos
- Direct detection of primordial black hole relics as dark matter
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- Particle Dark Matter Constraints from the Draco Dwarf Galaxy
- Improved /hadron separation for the detection of faint gamma-ray sources using boosted decision trees
- Discovery of Very High-Energy Gamma-Ray Radiation from the BL Lac 1ES 0806+524
- MAGIC observations of the February 2014 flare of 1ES 1011+496 and ensuing constraint of the EBL density
- Evidence for proton acceleration up to TeV energies based on VERITAS and Fermi-LAT observations of the Cas A SNR
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- Multiwavelength Observations of 3C 66A during the WEBT campaign of 2003 - 2004
- Resummed Photon Spectra for WIMP Annihilation
- The TACTIC atmospheric Cherenkov Imaging telescope
- Electromagnetic transients as triggers in searches for gravitational waves from compact binary mergers
- Precision Photon Spectra for Wino Annihilation
- The Astrophysical Multimessenger Observatory Network (AMON): Performance and Science Program
- Novae as Tevatrons: Prospects for CTA and IceCube
- Observations of the BL Lac Object 3C 66A with STACEE
- Robust Gamma Ray Signature of WIMP Dark Matter
- Dark matter subhaloes as gamma-ray sources and candidates in the first Fermi-LAT catalogue
- Dissecting the Cygnus Region with TeV Gamma Rays and Neutrinos
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- The Impact of Plasma Instabilities on the Spectra of TeV Blazars
- Constraints on axion-like particle properties with very high energy gamma-ray observations of Galactic sources
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- Suzaku Wide Band Analysis of the X-ray Variability of TeV Blazar Mrk 421 in 2006
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