The VERITAS Standard Data Analysis
Written by Michael Daniel for the VERITAS Collaboration   
Tuesday, 10 July 2007

Contribution to the 30th International Cosmic Ray Conference, Merida, Mexico, July 2007

abs/0709.4006

  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.

Last Updated ( Thursday, 29 November 2007 )