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SUMMARY:CTA Dark Matter searches in dwarf galaxies\, dark halos\, and gala
 xy clusters
DTSTART;VALUE=DATE-TIME:20191113T023000Z
DTEND;VALUE=DATE-TIME:20191113T030000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182823Z
UID:indico-contribution-1539@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Moritz Hütten (Max Planck Institute for Physics)\nT
 he Cherenkov Telescope Array (CTA) represents the next-generation ground-b
 ased gamma-ray observatory in the energy range between 30 GeV and 300 TeV.
  It will open the window to gamma-ray searches for annihilation or decay o
 f heavy (TeV) Weakly Interacting Massive Particles (WIMPs) in astrophysica
 l Dark Matter (DM) budgets with unprecedented sensitivity. In this talk\, 
 I will review the current prospects for WIMP searches with CTA in dwarf sp
 heroidal galaxies orbiting our Milky Way\, enhanced annihilation in close-
 by dark halos\, and galaxy clusters of the local Universe. I will also out
 line the current knowledge of the DM targets and foreseen observation stra
 tegies\, on which the success of the searches crucially depends.\n\nhttps:
 //indico.icrr.u-tokyo.ac.jp/event/259/contributions/1539/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1539/
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