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VERSION:2.0
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BEGIN:VEVENT
SUMMARY:Recent Results and Dark Matter Search with CALET on the ISS
DTSTART;VALUE=DATE-TIME:20191113T043000Z
DTEND;VALUE=DATE-TIME:20191113T050000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182621Z
UID:indico-contribution-410-55@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Asaoka\, Yoichi (WISE\, Waseda University)\nThe CALo
 rimetric Electron Telescope (CALET)\, which is currently conducting direct
  cosmic-ray observations onboard the International Space Station (ISS)\, u
 ses an all-calorimetric instrument with total vertical thickness of 30 rad
 iation lengths and fine imaging capability. The instrument is optimized fo
 r cosmic-ray electron measurements by achieving large proton rejection and
  excellent energy resolution well into the TeV energy region. In addition\
 , very wide dynamic range of energy measurements and absolute charge ident
 ification capability of the instrument enable us to measure proton and nuc
 lei spectra as well as electron and gamma-ray spectra. The CALET mission g
 oals include the investigation of acceleration and propagation of galactic
  cosmic rays\, of possible nearby sources\, and of potential signature of 
 dark matter. Since the start of observation in October 2015\, smooth and c
 ontinuous operations have taken place. In this talk\, we will give a brief
  summary of the recent results obtained with CALET and discuss about the d
 ark matter search using the CALET all-electron spectrum.\n\nhttps://indico
 .icrr.u-tokyo.ac.jp/event/259/contributions/1535/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1535/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Constraints on cosmic ray propagation and magnetic fields using ga
 mma-ray observations
DTSTART;VALUE=DATE-TIME:20191113T053000Z
DTEND;VALUE=DATE-TIME:20191113T060000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182621Z
UID:indico-contribution-410-80@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: López-Coto\, Rubén (INFN Padova)\nThe origin and p
 ropagation of cosmic rays is one of the most important questions in astrop
 article physics nowadays. To perform Indirect searches of Dark Matter sear
 ching for their products in the local cosmic ray spectra\, we first need t
 o comprehend what is the background coming from astrophysical sources. We 
 can only model this background by achieving a deep understanding of cosmic
  ray propagation. Although the transport of these cosmic rays through the 
 galaxy make them lose the information about their origin due to interstell
 ar magnetic fields\, we can directly study the properties of their propaga
 tion using gamma rays. In this talk\, I will give a review of current meas
 urements of magnetic fields and cosmic ray propagation parameters using ga
 mma rays.\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/166
 1/
LOCATION:Remote talk
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1661/
END:VEVENT
BEGIN:VEVENT
SUMMARY:Propagation processes  of cosmic rays
DTSTART;VALUE=DATE-TIME:20191113T050000Z
DTEND;VALUE=DATE-TIME:20191113T053000Z
DTSTAMP;VALUE=DATE-TIME:20250110T182621Z
UID:indico-contribution-410-78@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Ohira\, Yutaka (The university of Tokyo)\nIn this ta
 lk\, I'll review recent theoretical studies and observational results abou
 t propagation processes of cosmic rays in our galaxy.\n\nhttps://indico.ic
 rr.u-tokyo.ac.jp/event/259/contributions/1574/
LOCATION:The University of Tokyo\, Kashiwa Campus
URL:https://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1574/
END:VEVENT
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