Skip to main navigation Skip to search Skip to main content

Status of the IceCube neutrino observatory

  • J. Ahrens
  • , J. N. Bahcall
  • , X. Bai
  • , R. C. Bay
  • , T. Becka
  • , K. H. Becker
  • , D. Berley
  • , E. Bernardini
  • , D. Bertrand
  • , D. Z. Besson
  • , E. Blaufuss
  • , D. J. Boersma
  • , S. Böser
  • , C. Bohm
  • , O. Botner
  • , A. Bouchta
  • , O. Bouhali
  • , T. Burgess
  • , W. Carithers
  • , T. Castermans
  • J. Cavin, W. Chinowsky, D. Chirkin, B. Collin, J. Conrad, J. Cooley, D. F. Cowen, A. Davour, C. de Clercq, T. DeYoung, P. Desiati, R. Ehrlich, R. W. Ellsworth, P. A. Evenson, A. R. Fazely, T. Feser, T. K. Gaisser, J. Gallagher, R. Ganugapati, H. Geenen, A. Goldschmidt, J. A. Goodman, R. M. Gunasingha, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Hauschildt, D. Hays, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, G. S. Japaridze, A. Jones, A. Karle, H. Kawai, M. Kestel, N. Kitamura, R. Koch, L. Köpke, M. Kowalski, J. I. Lamoureux, H. Leich, I. Liubarsky, J. Madsen, H. S. Matis, C. P. McParland, T. Messarius, P. Mészáros, Y. Minaeva, R. H. Minor, P. Miočinović, H. Miyamoto, R. Morse, R. Nahnhauer, T. Neunhöffer, P. Niessen, D. R. Nygren, H. Ögelman, P. Olbrechts, S. Patton, R. Paulos, C. Pérez de los Heros, A. C. Pohl, J. Pretz, P. B. Price, G. T. Przybylski, K. Rawlins, S. Razzaque, E. Resconi, W. Rhode, M. Ribordy, S. Richter, H. G. Sander, K. Schinarakis, S. Schlenstedt, D. Schneider, R. Schwarz, D. Seckel, A. J. Smith, M. Solarz, G. M. Spiczak, C. Spiering, M. Stamatikos, T. Stanev, D. Steele, P. Steffen, T. Stezelberger, R. G. Stokstad, K. H. Sulanke, G. W. Sullivan, T. J. Sumner, I. Taboada, S. Tilav, N. van Eijndhoven, W. Wagner, C. Walck, R. R. Wang, C. H. Wiebusch, C. Wiedemann, R. Wischnewski, H. Wissing, K. Woschnagg, S. Yoshida
  • Johannes Gutenberg University Mainz
  • Institute for Advanced Studies
  • University of Delaware
  • University of California at Berkeley
  • University of Wuppertal
  • University of Maryland
  • German Electron Synchrotron
  • Université libre de Bruxelles
  • University of Kansas
  • Stockholm University
  • Uppsala University
  • Lawrence Berkeley National Laboratory
  • Universite de Mons
  • University of Wisconsin-Madison
  • Pennsylvania State University
  • Vrije Universiteit Brussel
  • George Mason University
  • Southern University and A&M College
  • Clark Atlanta University
  • Chiba University
  • Imperial College London
  • University of Wisconsin-River Falls
  • Universidad Simón Bolívar
  • Utrecht University

Research output: Contribution to journalShort surveypeer-review

20 Citations (Scopus)

Abstract

The IceCube neutrino telescope, to be constructed near the Antarctic South Pole, represents the next generation of neutrino telescope. Its large 1 km3 size will make it uniquely sensitive to the detection of neutrinos from astrophysical sources. The current design of the detector is presented. The basic performance of the detector and its ability to search for neutrinos from various astrophysical sources has been studied using detailed simulations and is discussed.

Original languageEnglish
Pages (from-to)519-525
Number of pages7
JournalNew Astronomy Reviews
Volume48
Issue number5-6
DOIs
Publication statusPublished - Apr 2004
Externally publishedYes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Status of the IceCube neutrino observatory'. Together they form a unique fingerprint.

Cite this