D
D. Hays
Researcher at Lawrence Berkeley National Laboratory
Publications - 17
Citations - 2561
D. Hays is an academic researcher from Lawrence Berkeley National Laboratory. The author has contributed to research in topics: Neutrino & Muon. The author has an hindex of 12, co-authored 17 publications receiving 2473 citations.
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The IceCube Collaboration
A. Achterberg,Markus Ackermann,J. Ahrens,Xinhua Bai,Bruny Baret,M. Bartelt,R. C. Bay,K. Beattie,T. Becka,P. Berghaus,D. Berley,Elisa Bernardini,D. Bertrand,E. Blaufuss,Olga Botner,Adam Bouchta,James E. Braun,T. Burgess,T. Castermans,Dmitry Chirkin,J. M. Clem,Jan Conrad,Anna Davour,C. De Clercq,Paolo Desiati,Tyce DeYoung,J. Dreyer,R. Ehrlich,T. Feser,Kirill Filimonov,Thomas K. Gaisser,R. Ganugapati,Heiko Geenen,L. Gerhardt,A. Goldschmidt,J. A. Goodman,Allan Hallgren,Francis Halzen,D. Hardtke,R. Hardtke,Torsten Harenberg,T. Hauschildt,D. Hays,John Heise,K. Helbing,M. Hellwig,P. Herquet,D. Hubert,B. Hughey,Klas Hultqvist,S. Hundertmark,Aya Ishihara,Janet Jacobsen,A. W. Jones,Albrecht Karle,H. Kawai,J. L. Kelley,S. Klepser,G. Kohnen,Hermann Kolanoski,M. Krasberg,Kyler Kuehn,E. Kujawski,H. Landsman,R. Lang,H. Leich,I. Liubarsky,Johan Lundberg,James Madsen,Pawel Marciniewski,K. Mase,T. McCauley,A. Meli,T. Messarius,P. Mio,H. Miyamoto,A. Mokhtarani,Teresa Montaruli,A. Morey,R. Morse,R. Nahnhauer,P. Niessen +81 more
TL;DR: The AMANDA-II data collected during the period 2000-2003 have been analysed in a search for a diffuse flux of high-energy extra-terrestrial muon neutrinos from the sum of all sources in the Universe as mentioned in this paper.
Journal ArticleDOI
First year performance of the IceCube neutrino telescope
A. Achterberg,Markus Ackermann,Jenni Adams,J. Ahrens,Karen Andeen,D.W. Atlee,J. Baccus,J.N. Bahcall,Xinhua Bai,B. Baret,M. Bartelt,Steven W. Barwick,R. C. Bay,K. Beattie,T. Becka,J.K. Becker,K. H. Becker,P. Berghaus,D. Berley,Elisa Bernardini,D. Bertrand,D. Z. Besson,E. Blaufuss,D. J. Boersma,Christian Bohm,S. Böser,Olga Botner,Adam Bouchta,James E. Braun,C.P. Burgess,T. Burgess,T. Castermans,J. Cherwinka,Dmitry Chirkin,John Clem,D. F. Cowen,M. V. D'Agostino,Anna Davour,C. T. Day,C. De Clercq,L. Demirörs,Paolo Desiati,T. DeYoung,J. C. Díaz-Vélez,J. Dreyer,M. R. Duvoort,W. R. Edwards,R. Ehrlich,J. Eisch,A. Elcheikh,R. W. Ellsworth,Paul Evenson,O. Fadiran,A. R. Fazely,T. Feser,Kirill Filimonov,B. D. Fox,Thomas K. Gaisser,Jay Gallagher,R. Ganugapati,Heiko Geenen,L. Gerhardt,A. Goldschmidt,J. A. Goodman,R. Gozzini,M.G. Greene,S. Grullon,A. Groß,R. M. Gunasingha,M. Gurtner,Allan Hallgren,Francis Halzen,K. Han,Kael Hanson,D. Hardtke,R. Hardtke,Torsten Harenberg,J. E. Hart,J. Haugen,T. Hauschildt,D. Hays,John Heise,K. Helbing,M. Hellwig,P. Herquet,G. C. Hill,Joseph T. Hodges,Kara Hoffman,K. Hoshina,D. Hubert,B. Hughey,P. O. Hulth,Klas Hultqvist,S. Hundertmark,J.-P. Hülß,Aya Ishihara,Janet Jacobsen,George Japaridze,A. W. Jones,J. M. Joseph,Karl-Heinz Kampert,Albrecht Karle,H. Kawai,J. L. Kelley,M. Kestel,N. Kitamura,Spencer Klein,S. Klepser,G. Kohnen,Hermann Kolanoski,L. Köpke,M. Krasberg,K. Kuehn,H. Landsman,A. Laundrie,H. Leich,I. Liubarsky,Johan Lundberg,C. Mackenzie,James Madsen,K. Mase,H. S. Matis,T. McCauley,C. P. McParland,A. Meli,T. Messarius,Peter Mészáros,H. Miyamoto,A. Mokhtarani,Teresa Montaruli,A. Morey,R. Morse,S. M. Movit,K. Münich,A. Muratas,R. Nahnhauer,J. W. Nam,P. Nießen,Dave Nygren,Hakki Ögelman,Ph. Olbrechts,A. Olivas,S. Patton,Carlos Pena-Garay,C. Pérez de los Heros,Claire Pettersen,A. Piegsa,Damian Pieloth,A. C. Pohl,R. Porrata,J. Pretz,P. B. Price,Gerald Przybylski,K. Rawlins,Soebur Razzaque,F. Refflinghaus,Elisa Resconi,Wolfgang Rhode,M. Ribordy,A. Rizzo,S. Robbins,Carsten Rott,D. Rutledge,H. G. Sander,P. Sandstrom,Subir Sarkar,S. Schlenstedt,David A. Schneider,D. Seckel,S. H. Seo,S. Seunarine,A. Silvestri,A. J. Smith,M. Solarz,C. Song,J. E. Sopher,Glenn Spiczak,Christian Spiering,Michael Stamatikos,Todor Stanev,P. Steffen,T. Stezelberger,R. G. Stokstad,M. C. Stoufer,S. Stoyanov,E. A. Strahler,K.-H. Sulanke,G. W. Sullivan,Ignacio Taboada,O. Tarasova,A. Tepe,L. Thollander,S. Tilav,P. A. Toale,D. Turcan,N. van Eijndhoven,Justin Vandenbroucke,A. Van Overloop,B. Voigt,W. Wagner,C. Walck,H. Waldmann,M. Walter,Yi Wang,Chris Wendt,M. H. Whitney,Christopher Wiebusch,G. Wikström,Dawn Williams,R. Wischnewski,P. Wisniewski,H. Wissing,Kurt Woschnagg,Xianwu Xu,G. B. Yodh,S. Yoshida,J.D. Zornoza +216 more
TL;DR: The first sensors of the IceCube neutrino observatory were deployed at the South Pole during the austral summer of 2004-2005 and have been producing data since February 2005.
Journal ArticleDOI
Sensitivity of the IceCube detector to astrophysical sources of high energy muon neutrinos
J. Ahrens,John N. Bahcall,Xinhua Bai,R. C. Bay,T. Becka,K.-H. Becker,D. Berley,Elisa Bernardini,D. Bertrand,D. Z. Besson,A. Biron,E. Blaufuss,D. J. Boersma,S. Böser,Christian Bohm,Olga Botner,Adam Bouchta,Othmane Bouhali,T. Burgess,William Carithers,T. Castermans,J. Cavin,W. Chinowsky,Dmitry Chirkin,B. Collin,Jan Conrad,Jodi Cooley,D. F. Cowen,Anna Davour,C. De Clercq,T. DeYoung,Paolo Desiati,R. Ehrlich,R. W. Ellsworth,Paul Evenson,A. R. Fazely,T. Feser,Thomas K. Gaisser,Jean Gallagher,R. Ganugapati,Heiko Geenen,A. Goldschmidt,J. A. Goodman,R. M. Gunasingha,Allan Hallgren,Francis Halzen,Kael Hanson,R. Hardtke,T. Hauschildt,D. Hays,K. Helbing,M. Hellwig,Ph. Herquet,G. C. Hill,D. Hubert,B. Hughey,P. O. Hulth,K. Hultqvist,S. Hundertmark,Janet Jacobsen,George Japaridze,A. W. Jones,Albrecht Karle,H. Kawai,M. Kestel,N. Kitamura,R Koch,L. Köpke,Marek Kowalski,J. I. Lamoureux,H. Leich,Matthias Leuthold,I. Liubarsky,James Madsen,H. S. Matis,C. P. McParland,T. Messarius,Peter Mészáros,Y. Minaeva,R. H. Minor,P. Miocinovic,H. Miyamoto,R. Morse,R. Nahnhauer,T. Neunhöffer,P. Niessen,D. R. Nygren,Hakki Ögelman,Ph. Olbrechts,S. Patton,R. Paulos,C. Pérez de los Heros,A. C. Pohl,J. Pretz,P. B. Price,Gerald Przybylski,K. Rawlins,Soebur Razzaque,Elisa Resconi,Wolfgang Rhode,M. Ribordy,S. Richter,H. G. Sander,K. Schinarakis,S. Schlenstedt,T. O. B. Schmidt,David A. Schneider,R. Schwarz,D. Seckel,A. J. Smith,M. Solarz,Glenn Spiczak,Christian Spiering,Michael Stamatikos,Todor 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,Wolfgang Wagner,C. Walck,R.-R Wang,C. H. Wiebusch,C. Wiedemann,R. Wischnewski,H. Wissing,Kurt Woschnagg,S. Yoshida +133 more
TL;DR: In this paper, a Monte Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies is presented.
Journal ArticleDOI
The IceCube data acquisition system: Signal capture, digitization, and timestamping
Rasha Abbasi,Markus Ackermann,Jenni Adams,Markus Ahlers,J. Ahrens,Karen Andeen,J. Auffenberg,Xinhua Bai,M. Baker,Steven W. Barwick,R. C. Bay,J. L. Bazo Alba,K. Beattie,T. Becka,Julia Becker,K. H. Becker,P. Berghaus,D. Berley,Elisa Bernardini,D. Bertrand,D. Z. Besson,B. Bingham,E. Blaufuss,D. J. Boersma,Christian Bohm,J. Bolmont,S. Böser,Olga Botner,James E. Braun,D. Breeder,T. Burgess,W. Carithers,T. Castermans,H. F. Chen,Dmitry Chirkin,B. Christy,John Clem,D. F. Cowen,M. V. D'Agostino,M. Danninger,Anna Davour,C. T. Day,O. Depaepe,C. De Clercq,L. Demirörs,F. Descamps,Paolo Desiati,G. de Vries-Uiterweerd,T. DeYoung,J. C. Díaz-Vélez,J. Dreyer,J. P. Dumm,M. R. Duvoort,W. R. Edwards,R. Ehrlich,J. Eisch,R. W. Ellsworth,O. Engdegård,S. Euler,Paul Evenson,O. Fadiran,A. R. Fazely,T. Feusels,Kirill Filimonov,Chad Finley,M. M. Foerster,B. D. Fox,Anna Franckowiak,R. Franke,Thomas K. Gaisser,Jay Gallagher,R. Ganugapati,L. Gerhardt,L. Gladstone,D. Glowacki,A. Goldschmidt,J. A. Goodman,R. Gozzini,Darren Grant,T. Griesel,A. Groß,A. Groß,S. Grullon,R. M. Gunasingha,M. Gurtner,C. Ha,Allan Hallgren,Francis Halzen,K. Han,Kael Hanson,R. Hardtke,Y. Hasegawa,J. Haugen,D. Hays,John Heise,K. Helbing,M. Hellwig,P. Herquet,S. Hickford,G. C. Hill,Joseph T. Hodges,Kara Hoffman,K. Hoshina,D. Hubert,W. Huelsnitz,B. Hughey,J.-P. Hülß,P. O. Hulth,Klas Hultqvist,S. Hussain,R. L. Imlay,M. Inaba,Aya Ishihara,J. E. Jacobsen,George Japaridze,Henrik J. Johansson,A. W. Jones,J. M. Joseph,Karl-Heinz Kampert,Alexander Kappes,Timo Karg,Albrecht Karle,H. Kawai,J. L. Kelley,Joanna Kiryluk,Joanna Kiryluk,Fabian Kislat,Spencer Klein,Spencer Klein,S. Kleinfelder,S. Klepser,G. Kohnen,Hermann Kolanoski,L. Köpke,Marek Kowalski,T. Kowarik,M. Krasberg,K. Kuehn,E. Kujawski,T. Kuwabara,M. Labare,K. Laihem,H. Landsman,R. J. Lauer,A. Laundrie,H. Leich,D. Leier,Chance W. Lewis,A. Lucke,J. Ludvig,Johan Lundberg,J. Lünemann,James Madsen,Reina H. Maruyama,K. Mase,H. S. Matis,C. P. McParland,K. Meagher,A. Meli,M. Merck,T. Messarius,Peter Mészáros,R.H. Minor,H. Miyamoto,A. Mohr,A. Mokhtarani,Teresa Montaruli,R. Morse,S. M. Movit,K. Münich,A. Muratas,R. Nahnhauer,J. W. Nam,P. Nießen,Dave Nygren,S. Odrowski,A. Olivas,M. Olivo,M. Ono,S. Panknin,S. J. Patton,C. Pérez de los Heros,J. Petrovic,A. Piegsa,Damian Pieloth,A. C. Pohl,R. Porrata,N. Potthoff,J. Pretz,P. B. Price,Gerald Przybylski,K. Rawlins,Soebur Razzaque,P. Redl,Elisa Resconi,Wolfgang Rhode,M. Ribordy,A. Rizzo,W.J. Robbins,J. P. Rodrigues,P. Roth,F. Rothmaier,Carsten Rott,C. Roucelle,C. Roucelle,D. Rutledge,Dirk Ryckbosch,H. G. Sander,Subir Sarkar,Konstancja Satalecka,P. Sandstrom,S. Schlenstedt,T. O. B. Schmidt,David A. Schneider,O. Schulz,D. Seckel,B. Semburg,S. H. Seo,Y. Sestayo,S. Seunarine,A. Silvestri,A. J. Smith,C. Song,J. E. Sopher,Glenn Spiczak,Christian Spiering,Todor Stanev,T. Stezelberger,R. G. Stokstad,M. C. Stoufer,S. Stoyanov,E. A. Strahler,T. Straszheim,Karl-Heinz Sulanke,G. W. Sullivan,Q. Swillens,Ignacio Taboada,O. Tarasova,A. Tepe,Samvel Ter-Antonyan,S. Tilav,M. Tluczykont,P. A. Toale,D. Tosi,D. Turcan,N. van Eijndhoven,Justin Vandenbroucke,A. Van Overloop,V. Viscomi,C. Vogt,B. Voigt,Chinh Vu,D. Wahl,C. Walck,T. Waldenmaier,H. Waldmann,M. Walter,Chris Wendt,S. Westerhof,Nathan Whitehorn,D. Wharton,Christopher Wiebusch,C. Wiedemann,G. Wikström,Dawn Williams,R. Wischnewski,H. Wissing,Kurt Woschnagg,Xianwu Xu,G. B. Yodh,S. Yoshida +270 more
TL;DR: In this paper, the Digital Optical Modules (DOMs) are used to detect, digitize and timestamp the signals from optical Cherenkov-radiation photons at the South Pole.
Journal Article
Sensitivity of the icecube detector to astrophysical sources of high energy muon neutrinos
J. Ahrens,John N. Bahcall,X. Bai,R. C. Bay,T. Becka,K.-H. Becker,D. Berley,Elisa Bernardini,D. Bertrand,D. Z. Besson,E. Blaufuss,D. J. Boersma,S. Böser,C. Bohm,Olga Botner,Adam Bouchta,Othmane Bouhali,T. Burgess,W. Carithers,T. Castermans,J. Cavin,W. Chinowsky,Dmitry Chirkin,B. Collin,Jan Conrad,Jodi Cooley,D. F. Cowen,Anna Davour,C. De Clercq,Tyce DeYoung,Paolo Desiati,R. Ehrlich,R. W. Ellsworth,Paul Evenson,A. R. Fazely,T. Feser,Thomas K. Gaisser,J. S. Gallagher,R. Ganugapati,Heiko Geenen,A. Goldschmidt,J. A. Goodman,R. M. Gunasingha,Allan Hallgren,Francis Halzen,Kael 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,Janet Jacobsen,George Japaridze,A. W. Jones,A. Karle,H. Kawai,M. Kestel,N. Kitamura,R. Koch,L. Köpke,Marek Kowalski,J. I. Lamoureux,H. Leich,I. Liubarsky,James Madsen,H. S. Matis,C. P. McParland,T. Messarius,Peter Mészáros,Y. Minaeva,R.H. Minor,P. Miocinovic,H. Miyamoto,R. Morse,R. Nahnhauer,T. Neunhöffer,P. Niessen,D. R. Nygren,Hakki Ögelman,Ph. Olbrechts,S. J. Patton,R. Paulos,C. Pérez de los Heros,A. C. Pohl,J. Pretz,P. B. Price,Gerald Przybylski,K. Rawlins,Soebur Razzaque,Elisa Resconi,Wolfgang Rhode,M. Ribordy,Stefan Richter,H. G. Sander,K. Schinarakis,S. Schlenstedt,David A. Schneider,R. Schwarz,D. Seckel,A. J. S. Smith,M. Solarz,Glenn Spiczak,Christian Spiering,Michael 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,Wolfgang Wagner,C. Walck,R.-R Wang,C. H. Wiebusch,C. Wiedemann,R. Wischnewski,Henrike Wissing,K. Woschnagg,S. Yoshida +130 more
TL;DR: In this paper, the authors present the results of a Monte-Carlo study of the sensitivity of the planned IceCube detector to predicted fluxes of muon neutrinos at TeV to PeV energies.