'Angular resolution 0' presentation slideshows

Recent Results and Prospects of High- Energy Neutrino Astronomy APPIC Meeting May 8, 2014 Paris

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Non-imaging Air Cherenkov Technique for studies of Cosmic Ray Origin and Gamma-astronomy.

Non-imaging Air Cherenkov Technique for studies of Cosmic Ray Origin and Gamma-astronomy. L.A.Kuzmichev (SINP MSU) On behalf on the Tunka and SCORE Collaboration February, 2011. Abstract.

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Dave Kieda & Stephan LeBohec University of Utah Department of Physics and Astronomy John Davis

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Instrumentation for Astroparticle Physics

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Highlight results from the MAGIC telescopes

Highlight results from the MAGIC telescopes. Elisa Prandini * Padova University & INFN From neutrino to multimessenger astronomy : status and perspectives Marseilles 4 th April 2011. *Mail to: prandini@pd.infn.it. Outline. MAGIC: a low energy threshold IACT Recent results Galactic

492 views • 42 slides

Recent Results from the ANTARES Neutrino Experiment

http://antares.in2p3.fr. Recent Results from the ANTARES Neutrino Experiment. P.Vernin CEA Saclay, IRFU On behalf of the Antares collaboration. ANTARES shore station. 40 km submarine cable. 22 Institutes from 7 European countries. -2500m. ANTARES Collaboration & detector site. Bucarest.

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ARGO-YBJ experiment in Tibet

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Collaborators :

Magnetic Field measurements at milliarcsecond resolution around massive young stellar objects. Gabriele Surcis. Collaborators : W.H.T. Vlemmings ( Chalmers Uni, Sweden ), H.J. van Langevelde (JIVE , Leiden Uni, The Netherlands),

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Combining Gamma and Neutrino Observations

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Calorimetry Upgrades at Forward Rapidities for the PHENIX detector

Calorimetry Upgrades at Forward Rapidities for the PHENIX detector. Mickey Chiu University of Illinois at Urbana-Champaign. Approach: internal expertise + new expert groups. N C C. INFN Trieste, Italy UC Riverside, US Brookhaven Lab, US Iowa State, US Moscow State, Russia

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High Energy Neutrino Flux studied in the ANTARES Deep-Sea Telescope

High Energy Neutrino Flux studied in the ANTARES Deep-Sea Telescope. research goals: deep cosmos the detector setup: deep sea status and performance point-source  flux diffuse  flux future aims summary. Herbert Löhner, KVI, University Groningen, The Netherlands

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AGENDA (km3net2p3.fr)

AGENDA (http://km3net.in2p3.fr). Manage password: wp20710. Pending Issues. Physics Priority < 1 TeV: Dark matter 1-100 TeV: HESS sources, GRBs >1 PeV: Diffuse flux, GZK, AGN Evaluation of NEMO geometry Evaluate effect of energy measurement on sensitivity

223 views • 14 slides