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VLVnT13 - Very Large Volume Neutrino Telescope Workshop 2013

5–7 Aug 2013
AlbaNova University Center
Europe/Stockholm timezone

Session

Physics, Reconstruction, and Software I.

PRS1
5 Aug 2013, 14:00
AlbaNova University Center

AlbaNova University Center

Presentation materials

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  1. 314. IceVeto: Extended PeV neutrino astronomy in the Southern Hemisphere with IceCube.
    Dr Jan Auffenberg (University of Wisconsin Madison)
    05/08/2013, 14:00
    Physics, Reconstruction, and Software
    IceCube, the world’s largest high-energy neutrino observatory, built at the South Pole, recently reported evidence of an astrophysical neutrino flux extending to PeV energies in the Southern Hemisphere. This observation raises the question of how the sensitivity in this energy range could be further increased. In the downgoing sector, in IceCube’s case the Southern Hemisphere,...
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  2. 322. Sensitivity of the KM3NeT detector to a neutrino flux from the Fermi Bubbles.
    Dr Paolo Piattelli (INFN - Laboratori Nazionali del Sud)
    05/08/2013, 14:20
    Physics, Reconstruction, and Software
    A recent analysis of the Fermi data provides evidence of the emission of high energy gamma rays (up to 100 GeV) with a high-intensity E-2 spectrum. This emission was detected as originating from two large areas around the Galactic center, spanning 50° above and below the Galactic center and 40° in longitude, with no evidence of spacial variation both in the spectrum shape and in the...
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  3. 323. Sensitivity of the KM3NeT detector to neutrino fluxes from Galactic point-like sources
    Prof. Paul KOOIJMAN (U. of Amsterdam/Utrecht U./Nikhef)
    05/08/2013, 14:40
    Physics, Reconstruction, and Software
    The KM3NeT collaboration has started the implementation of the first phase of a cubic-kilometre-scale neutrino telescope in the Northern hemisphere with an integrated platform for Earth and deep sea sciences. The location in the Mediterranean Sea will allow for surveying a large part of the sky, including most of the Galactic Plane and the Galactic Centre, thus complementing the sky...
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  4. 347. Detection of Extended Galactic Sources with an Underwater Neutrino Telescope
    Dr Antonios Tsirigotis (Hellenic Open University), Dr Dimitrios Lenis (INPP, NCSR Demokritos)
    05/08/2013, 15:00
    Physics, Reconstruction, and Software
    In this study we investigate the capability of a Very Large Volume Neutrino Telescope to discover extended Galactic sources. We focus to the brightest HESS gamma rays sources which are considered also as very high energy neutrino emitters. We use the un-binned method taking into account both the spatial and the energy distribution of high energy neutrinos and we investigate parts of...
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