Ghent University Academic Bibliography

Advanced

Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data

R Abbasi, Yasser Abdou, T Abu-Zayyad, J Adams, JA Aguilar, M Ahlers, K Andeen, J Auffenberg, X Bai, M Baker, et al. (2011) PHYSICAL REVIEW D. 83(9).
abstract
We report on a search for extremely-high energy neutrinos with energies greater than 10(6) GeV using the data taken with the IceCube detector at the South Pole. The data was collected between April 2008 and May 2009 with the half-completed IceCube array. The absence of signal candidate events in the sample of 333.5 days of live time significantly improves model-independent limits from previous searches and allows to place a limit on the diffuse flux of cosmic neutrinos with an E-2 spectrum in the energy range 2.0 x 10(6) - 6.3 x 10(9) GeV to a level of E-2 phi <= 3.6 x 10(-8) GeV cm(-2) sec(-1) sr(-1).
Please use this url to cite or link to this publication:
author
organization
year
type
journalArticle (original)
publication status
published
subject
keyword
SPECTRUM, RAYS
journal title
PHYSICAL REVIEW D
Phys. Rev. D
volume
83
issue
9
article number
092003
pages
9 pages
Web of Science type
Article
Web of Science id
000290897000001
JCR category
ASTRONOMY & ASTROPHYSICS
JCR impact factor
4.558 (2011)
JCR rank
11/56 (2011)
JCR quartile
1 (2011)
ISSN
1550-7998
DOI
10.1103/PhysRevD.83.092003
language
English
UGent publication?
yes
classification
A1
additional info
correction (see uploaded document) published in Phys. Rev. D (2011) 84(7), art. 079902, DOI 10.1103/PhysRevD.84.079902
copyright statement
I have transferred the copyright for this publication to the publisher
id
1317644
handle
http://hdl.handle.net/1854/LU-1317644
date created
2011-06-22 14:21:10
date last changed
2017-02-28 15:45:27
@article{1317644,
  abstract     = {We report on a search for extremely-high energy neutrinos with energies greater than 10(6) GeV using the data taken with the IceCube detector at the South Pole. The data was collected between April 2008 and May 2009 with the half-completed IceCube array. The absence of signal candidate events in the sample of 333.5 days of live time significantly improves model-independent limits from previous searches and allows to place a limit on the diffuse flux of cosmic neutrinos with an E-2 spectrum in the energy range 2.0 x 10(6) - 6.3 x 10(9) GeV to a level of E-2 phi {\textlangle}= 3.6 x 10(-8) GeV cm(-2) sec(-1) sr(-1).},
  articleno    = {092003},
  author       = {Abbasi, R and Abdou, Yasser and Abu-Zayyad, T and Adams, J and Aguilar, JA and Ahlers, M and Andeen, K and Auffenberg, J and Bai, X and Baker, M and Barwick, SW and Bay, R and Alba, JLB and Beattie, K and Beatty, JJ and Bechet, S and Becker, JK and Becker, KH and Benabderrahmane, ML and BenZvi, S and Berdermann, J and Berghaus, P and Berley, D and Bernardini, E and Bertrand, D and Besson, DZ and Bindig, D and Bissok, M and Blaufuss, E and Blumenthal, J and Boersma, DJ and Bohm, C and Bose, D and Boser, S and Botner, O and Braun, J and Brown, AM and Buitink, S and Carson, Michael and Chirkin, D and Christy, B and Clem, J and Clevermann, F and Cohen, S and Colnard, C and Cowen, DF and D'Agostino, MV and Danninger, M and Daughhetee, J and Davis, JC and De Clercq, C and Demirors, L and Denger, T and Depaepe, O and Descamps, Freija and Desiati, P and De Vries-Uiterweerd, Garmt and DeYoung, T and Diaz-Velez, JC and Dierckxsens, M and Dreyer, J and Dumm, JP and Ehrlich, R and Eisch, J and Ellsworth, RW and Engdegard, O and Euler, S and Evenson, PA and Fadiran, O and Fazely, AR and Fedynitch, A and Feusels, Tom and Filimonov, K and Finley, C and Fischer-Wasels, T and Foerster, MM and Fox, BD and Franckowiak, A and Franke, R and Gaisser, TK and Gallagher, J and Geisler, M and Gerhardt, L and Gladstone, L and Glusenkamp, T and Goldschmidt, A and Goodman, JA and Gora, D and Grant, D and Griesel, T and Gross, A and Grullon, S and Gurtner, M and Ha, C and Hallgren, A and Halzen, F and Han, K and Hanson, K and Heinen, D and Helbing, K and Herquet, P and Hickford, S and Hill, GC and Hoffman, KD and Homeier, A and Hoshina, K and Hubert, D and Huelsnitz, W and Hulss, JP and Hulth, PO and Hultqvist, K and Hussain, S and Ishihara, A and Jacobsen, J and Japaridze, GS and Johansson, H and Joseph, JM and Kampert, KH and Kappes, A and Karg, T and Karle, A and Kelley, JL and Kenny, P and Kiryluk, J and Kislat, F and Klein, SR and Kohne, JH and Kohnen, G and Kolanoski, H and Kopke, L and Kopper, S and Koskinen, DJ and Kowalski, M and Kowarik, T and Krasberg, M and Krings, T and Kroll, G and Kuwabara, T and Labare, M and Lafebre, S and Laihem, K and Landsman, H and Larson, MJ and Lauer, R and Lunemann, J and Madsen, J and Majumdar, P and Marotta, A and Maruyama, R and Mase, K and Matis, HS and Meagher, K and Merck, M and Meszaros, P and Meures, T and Middell, E and Milke, N and Miller, J and Montaruli, T and Morse, R and Movit, SM and Nahnhauer, R and Nam, JW and Naumann, U and Niessen, P and Nygren, DR and Odrowski, S and Olivas, A and Olivo, M and O'Murchadha, A and Ono, M and Panknin, S and Paul, L and Heros, CPD and Petrovic, J and Piegsa, A and Pieloth, D and Porrata, R and Posselt, J and Price, PB and Przybylski, GT and Rawlins, K and Redl, P and Resconi, E and Rhode, W and Ribordy, M and Rizzo, A and Rodrigues, JP and Roth, P and Rothmaier, F and Rott, C and Ruhe, T and Rutledge, D and Ruzybayev, B and Ryckbosch, Dirk and Sander, HG and Santander, M and Sarkar, S and Schatto, K and Schmidt, T and Schonwald, A and Schukraft, A and Schultes, A and Schulz, O and Schunck, M and Seckel, D and Semburg, B and Seo, SH and Sestayo, Y and Seunarine, S and Silvestri, A and Slipak, A and Spiczak, GM and Spiering, C and Stamatikos, M and Stanev, T and Stephens, G and Stezelberger, T and Stokstad, RG and Stossl, A and Stoyanov, S and Strahler, EA and Straszheim, T and Stur, M and Sullivan, GW and Swillens, Q and Taavola, H and Taboada, I and Tamburro, A and Tepe, A and Ter-Antonyan, S and Tilav, S and Toale, PA and Toscano, S and Tosi, D and Turcan, D and van Eijndhoven, N and Vandenbroucke, J and Van Overloop, Arne and van Santen, J and Vehring, M and Voge, M and Walck, C and Waldenmaier, T and Wallraff, M and Walter, M and Weaver, C and Wendt, C and Westerhoff, S and Whitehorn, N and Wiebe, K and Wiebusch, CH and Williams, DR and Wischnewski, R and Wissing, H and Wolf, M and Wood, TR and Woschnagg, K and Xu, C and Xu, XW and Yodh, G and Yoshida, S and Zarzhitsky, P},
  issn         = {1550-7998},
  journal      = {PHYSICAL REVIEW D},
  keyword      = {SPECTRUM,RAYS},
  language     = {eng},
  number       = {9},
  pages        = {9},
  title        = {Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data},
  url          = {http://dx.doi.org/10.1103/PhysRevD.83.092003},
  volume       = {83},
  year         = {2011},
}

Chicago
Abbasi, R, Yasser Abdou, T Abu-Zayyad, J Adams, JA Aguilar, M Ahlers, K Andeen, et al. 2011. “Constraints on the Extremely-high Energy Cosmic Neutrino Flux with the IceCube 2008-2009 Data.” Physical Review D 83 (9).
APA
Abbasi, R., Abdou, Y., Abu-Zayyad, T., Adams, J., Aguilar, J., Ahlers, M., Andeen, K., et al. (2011). Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data. PHYSICAL REVIEW D, 83(9).
Vancouver
1.
Abbasi R, Abdou Y, Abu-Zayyad T, Adams J, Aguilar J, Ahlers M, et al. Constraints on the extremely-high energy cosmic neutrino flux with the IceCube 2008-2009 data. PHYSICAL REVIEW D. 2011;83(9).
MLA
Abbasi, R, Yasser Abdou, T Abu-Zayyad, et al. “Constraints on the Extremely-high Energy Cosmic Neutrino Flux with the IceCube 2008-2009 Data.” PHYSICAL REVIEW D 83.9 (2011): n. pag. Print.