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eXtreme19

22–25 Jan 2019
Padova
Europe/Rome timezone

Support: extreme19@dfa.unipd.it

Session

Connection to UHECR

24 Jan 2019, 14:40
Polo di Psicologia - room 3I (3rd floor, building 2) (Padova)

Polo di Psicologia - room 3I (3rd floor, building 2)

Padova

Via Venezia, 12-14 Padova

Conveners

Connection to UHECR

  • Jonathan Biteau (IPNO, Univ. Paris-Sud, Univ. Paris/Saclay, CNRS/IN2P3)

Presentation materials

There are no materials yet.

  1. 115. Cosmic Ray Production from (Extreme) Blazars
    Dr Andrew Taylor (DESY)
    24/01/2019, 14:40
    Main track
    Talk
    Extreme blazars prove themselves to be efficient particles accelerators, giving rise to some of the highest energy, and hardest spectral emission of all blazars. The nature of processes giving rise to this emission remains, with both leptonic and hadronic scenarios being put forward. I will try to balance up the arguments for and against these two scenarios, highlighting potential means by...
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  2. 87. Ultra-high energy cosmic ray anisotropies measured with the Pierre Auger Observatory
    Prof. Guenter Sigl (Universität Hamburg)
    24/01/2019, 15:20
    Main track
    Talk
    Recently the Pierre Auger Observatory has observed a dipolar anisotropy of amplitude ~ 6.5% above 8 x 10^{18} eV that is unrelated to the Galactic plane. While the significance is largest above 8 x 10^{18} eV, the cosmic-ray data indicate a growth of the dipolar amplitude from 4 to 32 EeV and beyond. Furthermore, above 4 x 10^{19} eV, indications have been found for intermediate-scale...
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  3. 61. The Telescope Array experiment
    Dr Armando di Matteo (ULB, Brussels, Belgium)
    24/01/2019, 15:40
    Main track
    Talk
    The Telescope Array (TA), located in Millard County, Utah, US (39.3° N, 112.9° W, 1400 m a.s.l.), is the largest cosmic ray detector in the Northern Hemisphere. Its main array for the study of cosmic rays with the highest energies (up to 100 EeV and beyond) consists of 507 surface detector (SD) stations on a 1.2 km-spacing square grid overlooked by 38 fluorescence detector (FD) telescopes at...
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