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SUMMARY:The GAMMA-400 gamma-ray telescope for precision gamma-ray emission
  investigations
DTSTART;VALUE=DATE-TIME:20151009T050000Z
DTEND;VALUE=DATE-TIME:20151009T052500Z
DTSTAMP;VALUE=DATE-TIME:20260422T074605Z
UID:indico-contribution-455@cern.ch
DESCRIPTION:Speakers: Nikolay Topchiev (Lebedev Physical Institute)\nThe G
 AMMA-400 gamma-ray telescope with excellent angular and energy resolutions
  is designed to search for signatures of dark matter in the fluxes of gamm
 a-ray emission and electrons + positrons. Precision investigations of gamm
 a-ray emission from Galactic Center\, Crab\, Vela\, Cygnus\, Geminga\, and
  other regions will be performed\, as well as diffuse gamma-ray emission\,
  along with measurements of high-energy electron + positron and nuclei flu
 xes. Furthermore\, it will study gamma-ray bursts and gamma-ray emission f
 rom the Sun during periods of solar activity. The GAMMA-400 energy range i
 s expected to be from ~20 MeV up to TeV energies for gamma rays\, up to 10
  TeV for electrons + positrons\, and up to 10E15 eV for cosmic-ray nuclei.
  For 100-GeV gamma rays\, the GAMMA-400 angular resolution is ~0.01° and 
 energy resolution is ~1%\; the proton rejection factor is ~5x10E5. GAMMA-4
 00 will be installed onboard the Russian space observatory.\n\nhttps://ind
 ico.particle.mephi.ru/event/2/contributions/455/
LOCATION:Milan Hotel 4* Verdi&Bellini
URL:https://indico.particle.mephi.ru/event/2/contributions/455/
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