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SUMMARY:Background rejection methods for tens of TeV gamma-ray astronomy a
 pplicable to wide angle timing arrays
DTSTART;VALUE=DATE-TIME:20161013T114500Z
DTEND;VALUE=DATE-TIME:20161013T120000Z
DTSTAMP;VALUE=DATE-TIME:20260713T101250Z
UID:indico-contribution-757@cern.ch
DESCRIPTION:Speakers: abeer El shoukrofy (SINP MSU- Damanhour university)\
 nA 'knee-like' approximation of Cherenkov light Lateral Distribution Funct
 ions\, which we developed earlier\, now is used for the actual tasks of ba
 ckground rejection methods for high energy (Tens and hundreds of TeV) gamm
 a-ray astronomy. We use our methods basically for HiSCORE wide angle timin
 g array consisting of Cherenkov light detectors with spacing 100 m covered
  0.2 km2 presently and up to 5 km2 in future. However\, it can be applied 
 for other similar arrays. It is shown that application of multivariable ap
 proach (where 4 parameters of knee-like approximation are used) allows to 
 reach a large factor of background rejection but it strongly depends on nu
 mber of hit detectors.\n\nhttps://indico.particle.mephi.ru/event/4/contrib
 utions/757/
LOCATION:Milan Hotel Rossini
URL:https://indico.particle.mephi.ru/event/4/contributions/757/
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