Imperial College London

ProfessorTimothySumner

Faculty of Natural SciencesDepartment of Physics

Professor of Experimental Astrophysics
 
 
 
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Contact

 

+44 (0)20 7594 7552t.sumner

 
 
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Location

 

1108Blackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@inproceedings{Achterberg:2006,
author = {Achterberg, A and Ackermann, M and Adams, J and Ahrens, J and Andeen, K and Atlee, DW and Bahcall, JN and Bai, X and Baret, B and Bartelt, M and Barwick, SW and Bay, R and Beattie, K and Becka, T and Becker, JK and Becker, KH and Berghaus, P and Berley, D and Bernardini, E and Bertrand, D and Besson, DZ and Blaufuss, E and Boersma, DJ and Bohm, C and Bolmont, J and Böser, S and Botner, O and Bouchta, A and Braun, J and Burgess, C and Burgess, T and Castermans, T and Chirkin, D and Clem, J and Cowen, DF and D'Agostino, MV and Davour, A and Day, CT and De, Clercq C and Demirörs, L and Descamps, F and Desiati, P and DeYoung, T and Diaz-Velez, JC and Dreyer, J and Duvoort, MR and Edwards, WR and Ehrlich, R and Eisch, J and Ellsworth, RW and Evenson, PA and Fadiran, O and Fazely, AR and Feser, T and Filimonov, K and Fox, BD and Gaisser, TK and Gallagher, J and Ganugapati, R and Geenen, H and Gerhardt, L and Goldschmidt, A and Goodman, JA and Gozzini, R and Grullon, S and Groß},
pages = {87--101},
title = {Neutrino detectors in ICE: Results and perspectives},
year = {2006}
}

RIS format (EndNote, RefMan)

TY  - CPAPER
AB - The AMANDA neutrino detector has been in operation at the South Pole for several years. A number of searches for extraterrestrial sources of high energy neutrinos have been performed. A selection of results is presented in this paper. The much larger IceCube detector will extend the instrumented ice volume to a cubic kilometer and 9 out of 80 planned IceCube strings have been deployed to date. We present the status for both detectors.
AU - Achterberg,A
AU - Ackermann,M
AU - Adams,J
AU - Ahrens,J
AU - Andeen,K
AU - Atlee,DW
AU - Bahcall,JN
AU - Bai,X
AU - Baret,B
AU - Bartelt,M
AU - Barwick,SW
AU - Bay,R
AU - Beattie,K
AU - Becka,T
AU - Becker,JK
AU - Becker,KH
AU - Berghaus,P
AU - Berley,D
AU - Bernardini,E
AU - Bertrand,D
AU - Besson,DZ
AU - Blaufuss,E
AU - Boersma,DJ
AU - Bohm,C
AU - Bolmont,J
AU - Böser,S
AU - Botner,O
AU - Bouchta,A
AU - Braun,J
AU - Burgess,C
AU - Burgess,T
AU - Castermans,T
AU - Chirkin,D
AU - Clem,J
AU - Cowen,DF
AU - D'Agostino,MV
AU - Davour,A
AU - Day,CT
AU - De,Clercq C
AU - Demirörs,L
AU - Descamps,F
AU - Desiati,P
AU - DeYoung,T
AU - Diaz-Velez,JC
AU - Dreyer,J
AU - Duvoort,MR
AU - Edwards,WR
AU - Ehrlich,R
AU - Eisch,J
AU - Ellsworth,RW
AU - Evenson,PA
AU - Fadiran,O
AU - Fazely,AR
AU - Feser,T
AU - Filimonov,K
AU - Fox,BD
AU - Gaisser,TK
AU - Gallagher,J
AU - Ganugapati,R
AU - Geenen,H
AU - Gerhardt,L
AU - Goldschmidt,A
AU - Goodman,JA
AU - Gozzini,R
AU - Grullon,S
AU - Groß,A
AU - Gunasingha,RM
AU - Gurtner,M
AU - Hallgren,A
AU - Halzen,F
AU - Han,K
AU - Hanson,K
AU - Hardtke,D
AU - Hardtke,R
AU - Harenberg,T
AU - Hart,JE
AU - Hauschildt,T
AU - Hays,D
AU - Heise,J
AU - Helbing,K
AU - Hellwig,M
AU - Herquet,P
AU - Hill,GC
AU - Hodges,J
AU - Hoffman,KD
AU - Hommez,B
AU - Hoshina,K
AU - Hubert,D
AU - Hughey,B
AU - Hulth,PO
AU - Hultqvist,K
AU - Hundertmark,S
AU - Hülß,JP
AU - Ishihara,A
AU - Jacobsen,J
AU - Japaridze,GS
AU - Jones,A
AU - Joseph,JM
AU - Kampert,KH
AU - Karle,A
EP - 101
PY - 2006///
SN - 1122-5157
SP - 87
TI - Neutrino detectors in ICE: Results and perspectives
ER -