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SUMMARY:Capabilities of gamma ray telescope GAMMA-400 for lateral aperture
DTSTART;VALUE=DATE-TIME:20201005T150000Z
DTEND;VALUE=DATE-TIME:20201005T170000Z
DTSTAMP;VALUE=DATE-TIME:20260518T054811Z
UID:indico-contribution-2439@cern.ch
DESCRIPTION:Speakers: Anna Mikhailova (NRNU MEPHI)\nThe future γ-ray tele
 scope GAMMA-400 will provide fundamentally new data on discrete sources an
 d spectra of γ-ray emissions and electrons + positrons due to it's unique
  angular and energy resolution in wide energy range from 20 MeV up to seve
 ral TeVs.The gamma-ray telescope consists of the anticoincidence system\, 
 the converter-tracker\, the time-of-flight system\, the position-sensitive
  and electromagnetic calorimeters (CC1 and CC2)\, the scintillation detect
 ors of the calorimeter (S3 and S4) and lateral anticoincidence detectors o
 f the calorimeter LD. To extend the capabilities of the instrument to meas
 ure Gamma-Ray bursts\, Monte-Carlo simulations were performed for lateral 
 aperture of the instrument. The second-level trigger based on signals from
  CC2\, LD\, S3\, and S4 allows registering of Gamma Ray Bursts in the ener
 gy range ~10 -300 MeV with high effective area about 1m^2\n\nhttps://indic
 o.particle.mephi.ru/event/35/contributions/2439/
LOCATION:Discord Poster Server
URL:https://indico.particle.mephi.ru/event/35/contributions/2439/
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