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    Author
    Gillanders, Gary (6)
    Lang, Mark (6)
    Subject
    Astrophysics - High Energy Astrophysical Phenomena (6)
    Astrophysics - Instrumentation and Methods for Astrophysics (1)... View MoreDate Issued
    2011 (6)
    TypeArticle (6)

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    Discovery of TeV Gamma Ray Emission from Tycho's Supernova Remnant 

    Lang, Mark; Gillanders, Gary (2011)
    We report the discovery of TeV gamma-ray emission from the Type Ia supernova remnant (SNR) G120.1+1.4, known as Tycho's supernova remnant. Observations performed in the period 2008-2010 with the VERITAS ground-based gamma-ray ...
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    VERITAS Observations of the TeV Binary LS I +61 303 During 2008-2010 

    Lang, Mark; Gillanders, Gary (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 ...
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    Multiwavelength Observations of the VHE Blazar 1ES 2344+514 

    Lang, Mark; Gillanders, Gary (2011)
    Multiwavelength observations of the high-frequency-peaked blazar 1ES2344+514 were performed from 2007 October to 2008 January. The campaign represents the first contemporaneous data on the object at very high energy (VHE, ...
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    TeV and Multi-wavelength Observations of Mrk 421 in 2006-2008 

    Lang, Mark; Gillanders, Gary (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 ...
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    Detection of Pulsed Gamma Rays Above 100 GeV from the Crab Pulsar 

    Lang, Mark; Gillanders, Gary (2011)
    We report the detection of pulsed gamma rays from the Crab pulsar at energies above 100 Gigaelectronvolts (GeV) with the VERITAS array of atmospheric Cherenkov telescopes. The detection cannot be explained on the basis of ...
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    VERITAS: Status and Highlights 

    Lang, Mark; Gillanders, Gary (2011)
    The VERITAS telescope array has been operating smoothly since 2007, and has detected gamma-ray emission above 100 GeV from 40 astrophysical sources. These include blazars, pulsar wind nebulae, supernova remnants, gamma-ray ...
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