30 September 2014 to 3 October 2014
C.U.M.O. Noto (SR), Italy
Europe/Rome timezone
RICAP-14 The Roma International Conference on Astroparticle Physics in Noto, Sicily, Italy

Session

V Plenary Session

2 Oct 2014, 09:00
C.U.M.O. Noto (SR), Italy

C.U.M.O. Noto (SR), Italy

Conveners

V Plenary Session

  • Zhan-Arys Dzhilkibaev (Institute for Nuclear Research)

Presentation materials

There are no materials yet.

  1. Stefano Gabici (APC)
    02/10/2014, 09:00
    oral
    I will review some of the recent results of galactic gamma ray astronomy, both in the GeV and TeV domain. I will focus on those results which shed new light on some aspects of the process of acceleration of cosmic rays in the Galaxy.
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  2. Prof. Miguel Mostafa (Penn State Univ.)
    02/10/2014, 09:35
    oral
    The TeV energy band is a very exciting window into the origin of high energy cosmic radiation, particle acceleration, and the annihilation of dark matter particles. Above a few hundred GeV, ground-based experiments of very large effective areas open a new domain to study extragalactic sources at intermediate redshifts, galaxy clusters, gamma ray bursts, AGN and their flaring states, extended...
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  3. Rubén López-Coto (nstitut de Física d'Altes Energies - IFAE)
    02/10/2014, 10:10
    oral
    MAGIC is one of the main detectors for performing ground-based observations of VHE gamma-ray sources. It consists of two 17m diameter Imaging Atmospheric Cherenkov telescopes. The telescopes are located at 2200 m a.s.l. at the Roque de los Muchachos, on the Canary island of la Palma, Spain. They are designed to observe gamma rays with energies above ~50 GeV. The system recently underwent a...
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