Methods to determine the angular resolution of the HEGRA extended air shower scintillator array

Details Methods to determine the angular resolution of the HEGRA extended air shower scintillator array Methods to determine the angular resolution of the HEGRA extended air shower scintillator array

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aph.....5..379m&link_type=abstract

ASTROPARTICLE PHYSICS, Volume 5, Issue ASTROPARTICLE PHYSICS, p. 379-392.

Physics

6

Scientific paper

A precise knowledge of the angular resolution of scintillator arrays used to observe extended air showers (EAS) is of key importance in the search for VHE/UHE gamma point sources. Four independent methods have been used to determine the mean resolution for which a value of of 0.8 deg(1.0 deg) at a proton threshold of 50 (40) TeV has been found for the HEGRA EAS-array.

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