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VERSION:2.0
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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:20250110T182623Z
UID:indico-contribution-336-1535@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Yoichi Asaoka (WISE\, Waseda University)\nThe CALori
 metric Electron Telescope (CALET)\, which is currently conducting direct c
 osmic-ray observations onboard the International Space Station (ISS)\, use
 s an all-calorimetric instrument with total vertical thickness of 30 radia
 tion lengths and fine imaging capability. The instrument is optimized for 
 cosmic-ray electron measurements by achieving large proton rejection and e
 xcellent energy resolution well into the TeV energy region. In addition\, 
 very wide dynamic range of energy measurements and absolute charge identif
 ication capability of the instrument enable us to measure proton and nucle
 i spectra as well as electron and gamma-ray spectra. The CALET mission goa
 ls include the investigation of acceleration and propagation of galactic c
 osmic rays\, of possible nearby sources\, and of potential signature of da
 rk matter. Since the start of observation in October 2015\, smooth and con
 tinuous operations have taken place. In this talk\, we will give a brief s
 ummary of the recent results obtained with CALET and discuss about the dar
 k matter search using the CALET all-electron spectrum.\n\nhttps://indico.i
 crr.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:20250110T182623Z
UID:indico-contribution-336-1661@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Rubén López-Coto (INFN Padova)\nThe origin and pro
 pagation of cosmic rays is one of the most important questions in astropar
 ticle physics nowadays. To perform Indirect searches of Dark Matter search
 ing for their products in the local cosmic ray spectra\, we first need to 
 comprehend what is the background coming from astrophysical sources. We ca
 n only model this background by achieving a deep understanding of cosmic r
 ay propagation. Although the transport of these cosmic rays through the ga
 laxy make them lose the information about their origin due to interstellar
  magnetic fields\, we can directly study the properties of their propagati
 on using gamma rays. In this talk\, I will give a review of current measur
 ements of magnetic fields and cosmic ray propagation parameters using gamm
 a rays.\n\nhttps://indico.icrr.u-tokyo.ac.jp/event/259/contributions/1661/
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:20250110T182623Z
UID:indico-contribution-336-1574@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Yutaka Ohira (The university of Tokyo)\nIn this talk
 \, I'll review recent theoretical studies and observational results about 
 propagation processes of cosmic rays in our galaxy.\n\nhttps://indico.icrr
 .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/
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