Deep-sea research infrastructure for high-energy neutrino astronomy-Reference-Cited by-同舟云学术

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Deep-sea research infrastructure for high-energy neutrino astronomy

Published:2010-05 Issue:1-3 Volume:617 Page:495-498
ISSN:0168-9002
Container-title:Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
language:en
Short-container-title:Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

Author:

Löhner H.

Publisher

Elsevier BV

Subject

Instrumentation,Nuclear and High Energy Physics

Reference19 articles.

1. First Observation of the Greisen-Zatsepin-Kuzmin Suppression

2. The Pierre Auger Collaboration, 〈http://www.auger.org〉.

3. The Pierre Auger Collaboration, Science 318 (5852), 938; Astropart. Phys. 29 (2008) 188.

4. Upper Limit on the Diffuse Flux of Ultrahigh Energy Tau Neutrinos from the Pierre Auger Observatory

5. The IceCube Collaboration, 〈http://www.icecube.wisc.edu〉.

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