activity
20032026
most citedDesign Concepts for the Cherenkov Telescope Array

902 citations · 8.4k across the 129 of their papers we have counts for

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astro-ph2008★ 112 cited

The June 2008 flare of Markarian 421 from optical to TeV energies

The Agile Collaboration, Webt Collaboration, Magic Collaboration +2

We present optical, X-ray, high energy ( GeV) and very high energy ( GeV; VHE) observations of the high-frequency peaked blazar Mrk 421 taken betwee…

astro-ph2008★ 60 cited

Discovery of Very High-Energy Gamma-Ray Radiation from the BL Lac 1ES 0806+524

VERITAS Collaboration, V. Acciari, E. Aliu +90

The high-frequency-peaked BL-Lacertae object \objectname{1ES 0806+524}, at redshift z=0.138, was observed in the very-high-energy (VHE) gamma-ray regime by VERITAS between November…

astro-ph2008★ 54 cited

Status of the VERITAS Observatory

J. Holder, V. A. Acciari, E. Aliu +79

VERITAS, an Imaging Atmospheric Cherenkov Telescope (IACT) system for gammma-ray astronomy in the GeV-TeV range, has recently completed its first season of observations with a full…

astro-ph2008★ 9 cited

VERITAS Observations of the BL Lac Object 1ES 1218+304

Pascal Fortin

The VERITAS collaboration reports the detection of very-high-energy (VHE) gamma-ray emission from the high-frequency-peaked BL Lac object 1ES 1218+304 located at a redshift of z=0.…

astro-ph2008★ 99 cited

VERITAS Discovery of >200GeV Gamma-ray Emission from the Intermediate-frequency-peaked BL Lac Object W Comae

VERITAS Collaboration, V. A. Acciari, E. Aliu +80

We report the detection of very high-energy gamma-ray emission from the intermediate-frequency-peaked BL Lacertae object W Comae (z=0.102) by VERITAS. The source was observed betwe…

astro-ph2008★ 103 cited

Observation of gamma-ray emission from the galaxy M87 above 250 GeV with VERITAS

V. A. Acciari, M. Beilicke, G. Blaylock +74

The multiwavelength observation of the nearby radio galaxy M87 provides a unique opportunity to study in detail processes occurring in Active Galactic Nuclei from radio waves to Te…