'Energy threshold' diaporamas de présentation

Yue Zhao TDLI & SJTU

Boosted Dark Matter Signatures at Neutrino Experiments. Yue Zhao TDLI & SJTU MCTP, University of Michigan NuFact2017, WG5. Outline:. DM review Unconventional DM Models Overview on detecting boosted DM and DM IND

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Cosmic-Ray Detection at the ARGO-YBJ observatory

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SPACE DETECTORS TUS and KLYPVE for STUDY of ULTRA HIGH ENERGY COSMIC RAYS

SPACE DETECTORS TUS and KLYPVE for STUDY of ULTRA HIGH ENERGY COSMIC RAYS. TALK AT THE INTERNATIONAL SEMINAR ON ULTRA HIGH ENERGY COSMIC RAYS 14 APRIL 2005 B. A. KHRENOV D.V. Skobeltsyn Institute of Nuclear Physics

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VHE GRBs with Milagro

VHE GRBs with Milagro. The Milagro Detector Why look for VHE GRBs Milagrito Result GRB 970417a Milagro Results GRB010921 Detection Probabilities Future Directions. Jordan Goodman University of Maryland. Techniques in TeV Astrophysics. High energy threshold

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A silicon microdosimeter for radiation quality assessment

A silicon microdosimeter for radiation quality assessment. S. AGOSTEO (1,2) , C.A. CASSELL (2,3) , A. FAZZI (1,2) , ) M.V. INTROINI (1,2) , M. LORENZOLI (1,2) , A. POLA (1,2) , E. SAGIA (2,3) , V. VAROLI (1,2). (1) INFN, Sezione di Milano, via Celoria 16, 20133 Milano, Italy.

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A silicon microdosimeter for radiation quality assessment

A silicon microdosimeter for radiation quality assessment. S. AGOSTEO (1,2) , C.A. CASSELL (2,3) , A. FAZZI (1,2) , ) M.V. INTROINI (1,2) , M. LORENZOLI (1,2) , A. POLA (1,2) , E. SAGIA (2,3) , V. VAROLI (1,2). (1) INFN, Sezione di Milano, via Celoria 16, 20133 Milano, Italy.

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Double beta decay study at LNGS (the experiments CUORE and CUORE-0)

Lucifer. made in the frame of LUCIFER experiment FP7/2007-2013 ERC grant agreement n. 247115. XXIV SEMINARIO NAZIONALE di FISICA NUCLEARE E SUBNUCLEARE OTRANTO, Serra degli Alimini, 21-27 Settembre 2012 Argomento : Studio del decadimento doppio beta ai LNGS

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Concept(s) for very low energy observations (=<10 GeV)

Concept(s) for very low energy observations (=<10 GeV). John Finley, Alexander Konopelko Department of Physics, Purdue University, 525 Northwestern Avenue, West Lafayette, IN 47907. Rationale.

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Radiation Physics

Radiation Physics. Ya-yun Hsiao. Outline. Radiodecay Interactions of radiations with matter. Example.

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KM3NeT, a deep sea neutrino telescope in the Mediterranean Sea

KM3NeT, a deep sea neutrino telescope in the Mediterranean Sea. Anastasios Belias for the KM3NeT Consortium. KM3NeT objectives The KM3NeT Design Study Outlook. We need Northern n -telescope to cover the Galactic Plane. Complementarity with Ice Cube coverage .

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Search of High Energy Cosmic Sources with the Plataforma Solar de Almeria: The GRAAL Experiment

Search of High Energy Cosmic Sources with the Plataforma Solar de Almeria: The GRAAL Experiment. Fernando Arqueros Universidad Complutense de Madrid. F. Arqueros. Multifrecuency Behaviour of High Energy Cosmic Sources . Frascati Workshop 2001.

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The islands method in the image analysis of atmospheric Cherenkov Telescopes data

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Performance of 10-100GeV gamma ray camera for SUBARU optical-infrared telescope

Performance of 10-100GeV gamma ray camera for SUBARU optical-infrared telescope. A.Asahara*, K.Komiyama#, G.Kosugi#, H.Kubo*, S.Miyazaki#, M.Mori c , M.Nakagiri#, D.Nishida*, R.Ogasawara#, R.Orito*, K.Sakurazawa?, T.Takata#, T .Tanimori* and T.Usuda#.

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Event Rate:

Study of the Performance of a Single Stand-Alone H.E.S.S. Telescope: Monte Carlo Simulations & Data.

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MAGIC observation of GRB 090102

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The MAGIC telescopes

MAGIC-II. MAGIC-I. Very-high energy observation of the peculiar transient event Swift J1644+57 with the MAGIC telescopes.

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IAC Technique and DM search

Indirect Dark Matter Search with the MAGIC Telescope: first results for the Draco dSph observation.

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Davies-Cotton f/1.0 Optics. Total mirror area = 106 m 2

Very Energetic Radiation Imaging Telescope Array System. NSB. Level 1: Programmable CFD for each pixel Level 2: Pattern selection trigger requires any 3 adjacent pixels to fire within 10 ns Trigger rate ~ 150 Hz With light cones ~ 225 Hz. T4. T3. T1.

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