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SUMMARY:GAMMA-400 gamma-ray telescope construction features
DTSTART;VALUE=DATE-TIME:20181022T124000Z
DTEND;VALUE=DATE-TIME:20181022T151000Z
DTSTAMP;VALUE=DATE-TIME:20260422T082219Z
UID:indico-contribution-1370@cern.ch
DESCRIPTION:Speakers: S Suchkov (LPI)\nSpace-based GAMMA-400 gamma-ray tel
 escope will be installed on the Russian space observatory. GAMMA-400 is in
 tended for precision measurements of gamma-radiation in the energy range f
 rom 20 MeV to several TeV of discrete sources in the Galactic plane\, espe
 cially\, Galactic Center\, etc. measuring of the energy spectra of galacti
 c and extragalactic diffuse gamma-radiation\, which may be associated with
  the annihilation or decay of dark matter particles. Main parameters of th
 e gamma-ray telescope are: angular resolution ~0.01° at Eγ =100 GeV and 
 energy resolution ~1% at Eγ =100 GeV\, calorimeter thickness 22 r.l.\, pr
 oton rejection 105.\n\nhttps://indico.particle.mephi.ru/event/22/contribut
 ions/1370/
LOCATION:Hotel Intourist Kolomenskoye 4* Petrovskiy hall
URL:https://indico.particle.mephi.ru/event/22/contributions/1370/
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