11–14 Oct 2016
Kyoto Research Park
Japan timezone

Session

Oct.11AM1

Oct.11AM1
11 Oct 2016, 09:10
Kyoto Research Park

Kyoto Research Park

Chudouji Awatacho 93, Shimogyo-ku Kyoto , Japan, 600-8815

Conveners

Oct.11AM1

  • Masaki Fukushima (Univ. Tokyo)

Presentation materials

There are no materials yet.

  1. Dmitri Ivanov (University of Utah)
    11/10/2016, 09:10

    This work summarizes the cosmic ray energy spectrum measurement by the Telescope Array Experiment (TA) in the energy range from 4 PeV to over 100 EeV. The TA is a hybrid detector that uses 3 air fluorescence detectors (FDs) overlooking a ground array of scintillation counters of 1200 m spacing. In May 2016, TA has collected 8 years of data. The TA low energy extension (TALE) extends the energy...

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  2. Markus Roth (KIT)
    11/10/2016, 09:30

    The flux of cosmic rays has been measured with unprecedented precision at the Pierre Auger Observatory. We report on the recent update of the all-sky flux of cosmic rays above $3{\times}10^{17}$eV obtained by combining four independent high-quality data sets collected for more than 10 years, with a total exposure exceeding 50,000 km$^2$sr yr. These measurements are based on data from the...

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  3. Dr Valerio Verzi (INFN Roma Tor Vergata)
    11/10/2016, 09:55

    The energy spectrum joint working group was re-established with membership from the Pierre Auger Observatory (Auger) and the Telescope Array experiment (TA). In-depth discussions on the energy determination and systematic uncertainties in the two experiments were made, resulting in a detailed comparison of the UHECR energy spectra observed in the southern and the northern hemispheres. The flux...

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