'Icecube' diaporamas de présentation

Next Generation Neutrino Telescopes NIAPP Topical Workshop Munich , July 2014

Next Generation Neutrino Telescopes NIAPP Topical Workshop Munich , July 2014. Christian Spiering , DESY Zeuthen. Existing detectors. Baikal NT200+. Antares. AMANDA. IceCube. 3600 m. Lake Baikal. 1366 m. NT200. NT200+. 3600 m. NT200. 1366 m. 2500m. 4 50 m. 70 m.

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AstroParticle Physics PRC, May 2009 Christian Spiering

AstroParticle Physics PRC, May 2009 Christian Spiering. Overview. ?. total expenditures DESY/Astroparticle. Baikal: 1988-2008 Amanda: 1995-2009 IceCube: since 2000 MAGIC (YIG): since 2006 CTA (prototype): since 2008

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KM3NeT

A next generation neutrino telescope. KM3NeT. Els de Wolf Nikhef /University of Amsterdam on behalf of the KM3NeT consortium TeVPA 2008, 27 September 2008. What is KM3NeT?. Acronym for KM3Ne utrino T elescope A research facility in the Mediterranean Sea

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AstroParticle Physics PRC, May 2009 Christian Spiering

AstroParticle Physics PRC, May 2009 Christian Spiering. Overview. ?. total expenditures DESY/Astroparticle. Baikal: 1988-2008 Amanda: 1995-2009 IceCube: since 2000 MAGIC (YIG): since 2006 CTA (prototype): since 2008

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IceCube

IceCube. IceCube predecessor: AMANDA ( A ntarctic M uon A nd N eutrino D etector A rray) Completed in year 2000 From 2005 on: Amanda will merge with its successor experiment IceCube (currently in construction). p. p. e ?. ? 0. ? +. n. ?. ?. cosmic rays + gamma-rays.

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Carlos de los Heros Uppsala University

dark matter searches with IceCube. Carlos de los Heros Uppsala University. IDM2010, Montpellier, July 20-25.2010. conclusions. IceCube is 92% complete (taking data with 79 strings from May) Plan to reach 86 strings after the 2010/11 deployment season

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IceCube Collaboration

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AMANDA and IceCube neutrino telescopes at the South Pole

AMANDA and IceCube neutrino telescopes at the South Pole. Per Olof Hulth Stockholm University. Members of the AMANDA SU group. Senior members Christian Bohm Per Olof Hulth Klas Hultqvist Christian Walck Forskarassistent Stephan Hundertmark Resarch students Thomas Burgess

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Vrije Universiteit Brussel, Belgium

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First All-Sky Measurement of Muon Flux with IceCube

First All-Sky Measurement of Muon Flux with IceCube. IceCube REU Summer 2008 Kristin Rosenau Advisor: Teresa Montaruli. IceCube Neutrino Telescope. Located at the geographic South Pole Buried beneath roughly 1.5 km of ice, extending down to 2.5 km.

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Imaging the Neutrino Universe with AMANDA and IceCube

Imaging the Neutrino Universe with AMANDA and IceCube. Motivations for neutrino astronomy Selected AMANDA results IceCube: Status and Plans. David Hardtke University of California, Berkeley. Lake Louise Winter Institute February 2005. Neutrino Astronomy. Neutrino Production and Detection.

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Imaging the Neutrino Universe with AMANDA and IceCube

Imaging the Neutrino Universe with AMANDA and IceCube. Motivations for neutrino astronomy Selected AMANDA results IceCube: Status and Plans. David Hardtke University of California, Berkeley. Lake Louise Winter Institute February 2005. Neutrino Astronomy. Neutrino Production and Detection.

282 views • 18 slides

Dark Matter Detection

Dark Matter Detection. John Kelley IceCube Journal Club 27 February 2008. Image: NASA, ESA, and M.J. Jee (Johns Hopkins University). image: PDG (Particle Adventure). What is dark matter?. Experimental evidence is pretty overwhelming galaxy rotation, lensing, structure formation, CMB, etc.

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Optical Follow-up for IceCube

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IceCube < - > AMANDA Clock Integration: Keeping Time

IceCube < - > AMANDA Clock Integration: Keeping Time. Lawrence Berkeley National Laboratory Gerald Przybylski March 21, 2005 IceCube Collaboration Meeting. The Goal. Synchronizing IceCube and AMANDA events to 10ns or better (do we all agree 10ns is a good goal)

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Final Sample

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