activity
19952010
most citedVERITAS: the Very Energetic Radiation Imaging Telescope Array System

355 citations · 580 across the 8 of their papers we have counts for

collaborators

8 papers

cond-mat.other2010★ 1 cited

Driving LED in a Nanosecond Regime by a Fast Operational Amplifier

Joachim Rose, Stella Bradbury, Isabel Bond +4

It is widely believed that the generation of high speed optical signals is not the job for an LED. However this work is done to show that there are techniques which can be used to…

astro-ph.IM2010★ 23 cited

Stellar intensity interferometry: Experimental steps toward long-baseline observations

Stephan LeBohec, Ben Adams, Isobel Bond +12

Experiments are in progress to prepare for intensity interferometry with arrays of air Cherenkov telescopes. At the Bonneville Seabase site, near Salt Lake City, a testbed observat…

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-ph2001★ 355 cited

VERITAS: the Very Energetic Radiation Imaging Telescope Array System

T. C. Weekes

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 combi…

astro-ph1999★ 20 cited

Correlated variability of Mkn 421 at X-ray and TeV wavelengths on timescales of hours

L. Maraschi, G. Fossati, F. Tavecchio +26

Mkn 421 was observed for about two days with BeppoSAX, prior to and partly overlapping the start of a 1 week continuous exposure with ASCA in April 1998, as part of a world-wide mu…

astro-ph1997

A Multi-frequency campaign on the gamma-ray loud blazar W Comae

M. Maisack, K. Mannheim, R. D. Geckeler +10

We report preliminary results of a multi-frequency campaign on the TeV candidate blazar W Comae (z=0.102). Flux limits by Whipple and HEGRA show that the TeV flux must be considera…