A method to correct HILLAS parameters of imaging Cherenkov telescope data taken at different background light levels

Details A method to correct HILLAS parameters of imaging Cherenkov telescope data taken at different background light levels A method to correct HILLAS parameters of imaging Cherenkov telescope data taken at different background light levels

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2965k&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

During observations of γ showers with Cherenkov telescopes the background light conditions can vary, resulting in shifts of the values of the HILLAS image parameters. These changes increase when working with low 'tail' cuts for image cleaning. Here we present a first approach for correcting some of the variations. First tests of the method are carried out with HEGRA CT1 data.

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