Now showing items 21-40 of 45

• #### Observation of Extended VHE Emission from the Supernova Remnant IC 443 with VERITAS ﻿

(2009)
We present evidence that the very-high-energy (VHE, E &gt; 100 GeV) gamma-ray emission coincident with the supernova remnant IC 443 is extended. IC 443 contains one of the best-studied sites of supernova remnant/molecular ...
• #### Observation of gamma-ray emission from the galaxy M87 above 250 GeV with VERITAS ﻿

(2008)
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 TeV gamma-rays. Here we report the detection ...
• #### Observations of the shell-type SNR Cassiopeia A at TeV energies with VERITAS ﻿

(2010)
We report on observations of very high-energy gamma rays from the shell-type supernova remnant Cassiopeia A with the VERITAS stereoscopic array of four imaging atmospheric Cherenkov telescopes in Arizona. The total exposure ...
• #### Observations of the Unidentified TeV Gamma-Ray Source TeV J2032+4130 with the Whipple Observatory 10 m Telescope ﻿

(2006)
We report on observations of the sky region around the unidentified TeV gamma-ray source TeV J2032+4130 carried out with the Whipple Observatory 10 m atmospheric Cherenkov telescope for a total of 65.5 hrs between 2003 and ...
• #### Recent Results from the VERITAS Collaboration ﻿

(2002)
A decade after the discovery of TeV gamma-rays from the blazar Mrk 421 (Punch et al. 1992), the list of TeV blazars has increased to five BL Lac objects: Mrk 421 (Punch et al. 1992; Petry et al. 1996; Piron et al. 2001), ...
• #### A Search for Pulsed TeV Gamma Ray Emission from the Crab Pulsar ﻿

(1999)
We present the results of a search for pulsed TeV emission from the Crab pulsar using the Whipple Observatory's 10m gamma-ray telescope. The direction of the Crab pulsar was observed for a total of 73.4 hours between 1994 ...
• #### A Search for Pulsed TeV Gamma Ray Emission from the Crab Pulsar ﻿

(1999)
We present the results of a search for pulsed TeV emission from the Crab pulsar using the Whipple Observatory's 10m gamma-ray telescope. The direction of the Crab pulsar was observed for a total of 73.4 hours between 1994 ...
• #### Search for Pulsed TeV Gamma-ray Emission from the Crab Pulsar ﻿

(1999)
We present the results of a search for pulsed TeV emission from the Crab pulsar using the Whipple Observatory's 10 m gamma-ray telescope. The direction of the Crab pulsar was observed for a total of 73.4 hours between 1994 ...
• #### Search for Pulsed TeV Gamma-ray Emission from the Crab Pulsar ﻿

(1999)
We present the results of a search for pulsed TeV emission from the Crab pulsar using the Whipple Observatory's 10 m gamma-ray telescope. The direction of the Crab pulsar was observed for a total of 73.4 hours between 1994 ...
• #### Status of the VERITAS Observatory ﻿

(2008)
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 array of four telescopes. A number of ...
• #### TeV and Multi-wavelength Observations of Mrk 421 in 2006-2008 ﻿

(2011)
We report on TeV gamma-ray observations of the blazar Mrk 421 (redshift of 0.031) with the VERITAS observatory and the Whipple 10m Cherenkov telescope. The excellent sensitivity of VERITAS allowed us to sample the TeV ...
• #### TeV Gamma-Ray Observations of the Perseus and Abell 2029 Galaxy Clusters ﻿

(2006)
Galaxy clusters might be sources of TeV gamma rays emitted by high-energy protons and electrons accelerated by large scale structure formation shocks, galactic winds, or active galactic nuclei. Furthermore, gamma rays may ...
• #### VERITAS 2008 - 2009 monitoring of the variable gamma-ray source M87 ﻿

(2010)
M87 is a nearby radio galaxy that is detected at energies ranging from radio to VHE gamma-rays. Its proximity and its jet, misaligned from our line-of-sight, enable detailed morphological studies and extensive modeling at ...
• #### VERITAS Discovery of &gt;200GeV Gamma-ray Emission from the Intermediate-frequency-peaked BL Lac Object W Comae ﻿

(2008)
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 between January and April 2008. A strong outburst ...
• #### VERITAS Observations of a Very High Energy Gamma-ray Flare from the Blazar 3C 66A ﻿

(2009)
The intermediate-frequency peaked BL Lacertae (IBL) object 3C 66A is detected during 2007 - 2008 in VHE (very high energy: E &gt; 100 GeV) gamma-rays with the VERITAS stereoscopic array of imaging atmospheric Cherenkov ...
• #### VERITAS observations of the BL Lac 1ES 1218+304 ﻿

(2009)
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=0.182. A gamma-ray signal was detected with ...
• #### VERITAS Observations of the gamma-Ray Binary LS I +61 303 ﻿

(2008)
LS I +61 303 is one of only a few high-mass X-ray binaries currently detected at high significance in very high energy gamma-rays. The system was observed over several orbital cycles (between September 2006 and February ...
• #### VERITAS Observations of the TeV Binary LS I +61 303 During 2008-2010 ﻿

(2011)
We present the results of observations of the TeV binary LS I +61 303 with the VERITAS telescope array between 2008 and 2010, at energies above 300 GeV. In the past, both ground-based gamma-ray telescopes VERITAS and MAGIC ...
• #### VERITAS Observations of the Unusual Extragalactic Transient Swift J164449.3+573451 ﻿

(2011)
We report on very-high-energy ($&gt;$100 GeV) gamma-ray observations of Swift J164449.3+573451, an unusual transient object first detected by the {\it Swift} Observatory and later detected by multiple radio, optical and ...
• #### VERITAS Upper Limit on the VHE Emission from the Radio Galaxy NGC 1275 ﻿

(2009)
The recent detection by the Fermi gamma-ray space telescope of high-energy gamma-rays from the radio galaxy NGC 1275 makes the observation of the very high energy (VHE: E &gt; 100 GeV) part of its broadband spectrum ...