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VERSION:2.0
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BEGIN:VEVENT
SUMMARY:High Energy Gamma Ray Instruments for Dark Matter Searches
DTSTART;VALUE=DATE-TIME:20191113T010000Z
DTEND;VALUE=DATE-TIME:20191113T013000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182652Z
UID:indico-contribution-417-36@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Teshima\, Masahiro (ICRR\, the University of Tokyo)\
 nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1505/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1505/
END:VEVENT
BEGIN:VEVENT
SUMMARY:TeV dark matter search at the Galactic center with the CTA
DTSTART;VALUE=DATE-TIME:20191113T013000Z
DTEND;VALUE=DATE-TIME:20191113T020000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182652Z
UID:indico-contribution-417-69@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Zaharijas\, Gabrijela (University of Nova Gorica)\nH
 igh-energy gamma rays are among the most promising tools to constrain or r
 eveal the nature of dark matter (DM)\, in particular the Weakly Interactin
 g Massive Particles models.  The Cherenkov Telescope Array (CTA) is well i
 nto its pre-construction phase and will soon probe the high-energy gamma-r
 ay sky in the 20 GeV - 300 TeV energy range.  Thanks to its improved energ
 y and angular resolutions as well as significantly larger effective area\,
  the CTA will probe a parameter space of heavier dark matter (above 100 Ge
 V)\, with unprecedented sensitivity\, reaching the DM thermal annihilation
  rate at the TeV regime. \n\nThis talk will summarise the planned DM searc
 h strategies with CTA\, focusing on the signal of DM in the centre of our 
 Galaxy. As observed with the Fermi LAT at lower energies\, this region exh
 ibits complex large-scale gamma-ray emission and the CTA is expected to be
  the first ground based observatory able to detect it. In this talk we rep
 ort on the collaboration effort to study the impact of extended astrophysi
 cal backgrounds on DM search\, based on the astrophysical emission observe
 d with the Fermi LAT at lower energies and to suggest the promising data a
 nalysis and observational strategies for the upcoming CTA data.\n\nhttps:/
 /indico.icrr.u-tokyo.ac.jp/event/259/contributions/1562/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1562/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Current and Future WIMP Searches with Fermi-LAT\, HAWC\, and SWGO
DTSTART;VALUE=DATE-TIME:20191113T030000Z
DTEND;VALUE=DATE-TIME:20191113T033000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182652Z
UID:indico-contribution-419-27@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Albert\, Andrea (Los Alamos National Lab)\nEvidence 
 suggests ~85% of the mass in the Universe is dark matter (DM). Several pro
 mising DM theories predict that it is a fundamental particle. The most fam
 ous of which is the Weakly Interacting Massive Particle (WIMP). WIMPs that
  annihilate at a weak-scale cross section that were in thermal equilibrium
  in the Universe produce the observed DM abundance today. DM particles are
  theorized to interact and produce standard model particles\, like gamma r
 ays. So far\, no definitive gamma-ray signal has been detected\, but curre
 nt experiments have started excluding several thermal WIMP models. I will 
 discuss the current status of DM searches with gamma-ray observatories lik
 e the Fermi LAT and HAWC. I will also discuss how both future analysis wit
 h current observatories and future observatories like CTA and SWGO will pr
 obe thermal WIMP models for masses from 5 GeV to ~100 TeV.\n\nhttps://indi
 co.icrr.u-tokyo.ac.jp/event/259/contributions/1523/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1523/
END:VEVENT
BEGIN:VEVENT
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:20250110T182652Z
UID:indico-contribution-419-65@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Hütten\, Moritz (Max Planck Institute for Physics)\
 nThe Cherenkov Telescope Array (CTA) represents the next-generation ground
 -based gamma-ray observatory in the energy range between 30 GeV and 300 Te
 V. It will open the window to gamma-ray searches for annihilation or decay
  of heavy (TeV) Weakly Interacting Massive Particles (WIMPs) in astrophysi
 cal Dark Matter (DM) budgets with unprecedented sensitivity. In this talk\
 , I will review the current prospects for WIMP searches with CTA in dwarf 
 spheroidal galaxies orbiting our Milky Way\, enhanced annihilation in clos
 e-by dark halos\, and galaxy clusters of the local Universe. I will also o
 utline the current knowledge of the DM targets and foreseen observation st
 rategies\, on which the success of the searches crucially depends.\n\nhttp
 s://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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