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The VERITAS standard data analysis

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arxiv 0709.4006 v1 pith:ULCLGM3P submitted 2007-09-25 astro-ph

M.K. Daniel (for the VERITAS collaboration) This is my paper · ORCID
classification astro-ph
keywords analysisdataenergygammaraysveritasarrayastrophysical
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VERITAS is an array of Imaging Atmospheric Cherenkov Telescopes designed for very high energy gamma ray (E>100,GeV) observations of astrophysical sources. The experiment began its scientific observation program in the 2006/2007 observing season. We describe here the analysis chain for reducing the data, reconstructing the direction and energy of incident gamma rays and the rejection of background cosmic rays.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Combined VERITAS and NuSTAR observations of the gamma-ray binary HESS J0632+057

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    New NuSTAR and VERITAS spectra of HESS J0632+057 are well fitted by a pulsar-wind shock model, yielding a degenerate constraint with wind magnetization around 0.003 to 0.03 at the shock.

  2. Multi-wavelength observation of MAXI J1820+070 with MAGIC, VERITAS and H.E.S.S

    astro-ph.HE 2019-08 conditional novelty 4.0 of 10

    MAXI J1820+070 shows no significant very high energy gamma-ray emission above 182 GeV despite a bright X-ray outburst, and optical transient activity drops sharply during state transitions.

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