The AMANDA neutrino telescope

E. C. Andrés; P. Askebjer; S. W. Barwick; R. C. Bay; L. Bergström; A. Biron; J. Booth; O. Botner; A. Bouchta; S. Carius; M. Carlson; W. Chinowsky; D. Chirkin; J. Conrad; C. G.S. Costa; D. Cowen; E. Dalberg; T. DeYoung; J. Edsjö; P. Ekström; A. Goobar; L. Gray; A. Hallgren; F. Halzen; R. Hardtke; S. Hart; Y. He; C. P. De Los Heros; G. Hill; P. O. Hulth; S. Hundertmark; J. Jacobsen; A. Jones; V. Kandhadai; A. Karle; J. Kim; H. Leich; M. Leuthold; P. Lindahl; I. Liubarsky; P. Loaiza; D. Lowder; P. Marciniewski; T. C. Miller; P. Miocinovic; P. C. Mock; R. Morse; M. Newcomer; P. Niessen; D. Nygren; R. Porrata; D. Potter; P. B. Price; G. Przybylski; W. Rhode; S. Richter; J. Rodriguez; P. Romenesko; D. Ross; H. Rubinstein; T. Schmidt; E. Schneider; R. Schwarz; U. Schwendicke; G. Smoot; M. Solarz; V. Sorin; C. Spiering; P. Steffen; R. Stokstad; O. Streicher; I. Taboada; T. Thon; S. Tilav; C. Walck; C. H. Wiebusch; R. Wischnewski; K. Woschnagg; W. Wu; G. Yodh; S. Young

doi:10.1016/S0920-5632(99)00469-7

The AMANDA neutrino telescope

E. C. Andrés, P. Askebjer, S. W. Barwick, R. C. Bay, L. Bergström, A. Biron, J. Booth, O. Botner, A. Bouchta, S. Carius, M. Carlson, W. Chinowsky, D. Chirkin, J. Conrad, C. G.S. Costa, D. Cowen, E. Dalberg, T. DeYoung, J. Edsjö, P. EkströmA. Goobar, L. Gray, A. Hallgren, F. Halzen, R. Hardtke, S. Hart, Y. He, C. P. De Los Heros, G. Hill, P. O. Hulth, S. Hundertmark, J. Jacobsen, A. Jones, V. Kandhadai, A. Karle, J. Kim, H. Leich, M. Leuthold, P. Lindahl, I. Liubarsky, P. Loaiza, D. Lowder, P. Marciniewski, T. C. Miller, P. Miocinovic, P. C. Mock, R. Morse, M. Newcomer, P. Niessen, D. Nygren, R. Porrata, D. Potter, P. B. Price, G. Przybylski, W. Rhode, S. Richter, J. Rodriguez, P. Romenesko, D. Ross, H. Rubinstein, T. Schmidt, E. Schneider, R. Schwarz, U. Schwendicke, G. Smoot, M. Solarz, V. Sorin, C. Spiering, P. Steffen, R. Stokstad, O. Streicher, I. Taboada, T. Thon, S. Tilav, C. Walck, C. H. Wiebusch, R. Wischnewski, K. Woschnagg, W. Wu, G. Yodh, S. Young

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Abstract

With an effective telescope area of order 10⁴ m² for TeV neutrinos, a threshold near ∼50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope.

Original language	English (US)
Pages (from-to)	474-485
Number of pages	12
Journal	Nuclear Physics B - Proceedings Supplements
Volume	77
Issue number	1-3
DOIs	https://doi.org/10.1016/S0920-5632(99)00469-7
State	Published - May 1999

All Science Journal Classification (ASJC) codes

Atomic and Molecular Physics, and Optics
Nuclear and High Energy Physics

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10.1016/S0920-5632(99)00469-7

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Andrés, E. C., Askebjer, P., Barwick, S. W., Bay, R. C., Bergström, L., Biron, A., Booth, J., Botner, O., Bouchta, A., Carius, S., Carlson, M., Chinowsky, W., Chirkin, D., Conrad, J., Costa, C. G. S., Cowen, D., Dalberg, E., DeYoung, T., Edsjö, J., ... Young, S. (1999). The AMANDA neutrino telescope. Nuclear Physics B - Proceedings Supplements, 77(1-3), 474-485. https://doi.org/10.1016/S0920-5632(99)00469-7

@article{057c37f757ea4b159b1adfc3f4734188,

title = "The AMANDA neutrino telescope",

abstract = "With an effective telescope area of order 104 m2 for TeV neutrinos, a threshold near ∼50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope.",

author = "Andr{\'e}s, {E. C.} and P. Askebjer and Barwick, {S. W.} and Bay, {R. C.} and L. Bergstr{\"o}m and A. Biron and J. Booth and O. Botner and A. Bouchta and S. Carius and M. Carlson and W. Chinowsky and D. Chirkin and J. Conrad and Costa, {C. G.S.} and D. Cowen and E. Dalberg and T. DeYoung and J. Edsj{\"o} and P. Ekstr{\"o}m and A. Goobar and L. Gray and A. Hallgren and F. Halzen and R. Hardtke and S. Hart and Y. He and {De Los Heros}, {C. P.} and G. Hill and Hulth, {P. O.} and S. Hundertmark and J. Jacobsen and A. Jones and V. Kandhadai and A. Karle and J. Kim and H. Leich and M. Leuthold and P. Lindahl and I. Liubarsky and P. Loaiza and D. Lowder and P. Marciniewski and Miller, {T. C.} and P. Miocinovic and Mock, {P. C.} and R. Morse and M. Newcomer and P. Niessen and D. Nygren and R. Porrata and D. Potter and Price, {P. B.} and G. Przybylski and W. Rhode and S. Richter and J. Rodriguez and P. Romenesko and D. Ross and H. Rubinstein and T. Schmidt and E. Schneider and R. Schwarz and U. Schwendicke and G. Smoot and M. Solarz and V. Sorin and C. Spiering and P. Steffen and R. Stokstad and O. Streicher and I. Taboada and T. Thon and S. Tilav and C. Walck and Wiebusch, {C. H.} and R. Wischnewski and K. Woschnagg and W. Wu and G. Yodh and S. Young",

note = "Funding Information: *Work supported by the Department of Energy under grant DE-FG02-91 ER40690.",

year = "1999",

month = may,

doi = "10.1016/S0920-5632(99)00469-7",

language = "English (US)",

volume = "77",

pages = "474--485",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier B.V.",

number = "1-3",

}

Andrés, EC, Askebjer, P, Barwick, SW, Bay, RC, Bergström, L, Biron, A, Booth, J, Botner, O, Bouchta, A, Carius, S, Carlson, M, Chinowsky, W, Chirkin, D, Conrad, J, Costa, CGS, Cowen, D, Dalberg, E, DeYoung, T, Edsjö, J, Ekström, P, Goobar, A, Gray, L, Hallgren, A, Halzen, F, Hardtke, R, Hart, S, He, Y, De Los Heros, CP, Hill, G, Hulth, PO, Hundertmark, S, Jacobsen, J, Jones, A, Kandhadai, V, Karle, A, Kim, J, Leich, H, Leuthold, M, Lindahl, P, Liubarsky, I, Loaiza, P, Lowder, D, Marciniewski, P, Miller, TC, Miocinovic, P, Mock, PC, Morse, R, Newcomer, M, Niessen, P, Nygren, D, Porrata, R, Potter, D, Price, PB, Przybylski, G, Rhode, W, Richter, S, Rodriguez, J, Romenesko, P, Ross, D, Rubinstein, H, Schmidt, T, Schneider, E, Schwarz, R, Schwendicke, U, Smoot, G, Solarz, M, Sorin, V, Spiering, C, Steffen, P, Stokstad, R, Streicher, O, Taboada, I, Thon, T, Tilav, S, Walck, C, Wiebusch, CH, Wischnewski, R, Woschnagg, K, Wu, W, Yodh, G & Young, S 1999, 'The AMANDA neutrino telescope', Nuclear Physics B - Proceedings Supplements, vol. 77, no. 1-3, pp. 474-485. https://doi.org/10.1016/S0920-5632(99)00469-7

TY - JOUR

T1 - The AMANDA neutrino telescope

AU - Andrés, E. C.

AU - Askebjer, P.

AU - Barwick, S. W.

AU - Bay, R. C.

AU - Bergström, L.

AU - Biron, A.

AU - Booth, J.

AU - Botner, O.

AU - Bouchta, A.

AU - Carius, S.

AU - Carlson, M.

AU - Chinowsky, W.

AU - Chirkin, D.

AU - Conrad, J.

AU - Costa, C. G.S.

AU - Cowen, D.

AU - Dalberg, E.

AU - DeYoung, T.

AU - Edsjö, J.

AU - Ekström, P.

AU - Goobar, A.

AU - Gray, L.

AU - Hallgren, A.

AU - Halzen, F.

AU - Hardtke, R.

AU - Hart, S.

AU - He, Y.

AU - De Los Heros, C. P.

AU - Hill, G.

AU - Hulth, P. O.

AU - Hundertmark, S.

AU - Jacobsen, J.

AU - Jones, A.

AU - Kandhadai, V.

AU - Karle, A.

AU - Kim, J.

AU - Leich, H.

AU - Leuthold, M.

AU - Lindahl, P.

AU - Liubarsky, I.

AU - Loaiza, P.

AU - Lowder, D.

AU - Marciniewski, P.

AU - Miller, T. C.

AU - Miocinovic, P.

AU - Mock, P. C.

AU - Morse, R.

AU - Newcomer, M.

AU - Niessen, P.

AU - Nygren, D.

AU - Porrata, R.

AU - Potter, D.

AU - Price, P. B.

AU - Przybylski, G.

AU - Rhode, W.

AU - Richter, S.

AU - Rodriguez, J.

AU - Romenesko, P.

AU - Ross, D.

AU - Rubinstein, H.

AU - Schmidt, T.

AU - Schneider, E.

AU - Schwarz, R.

AU - Schwendicke, U.

AU - Smoot, G.

AU - Solarz, M.

AU - Sorin, V.

AU - Spiering, C.

AU - Steffen, P.

AU - Stokstad, R.

AU - Streicher, O.

AU - Taboada, I.

AU - Thon, T.

AU - Tilav, S.

AU - Walck, C.

AU - Wiebusch, C. H.

AU - Wischnewski, R.

AU - Woschnagg, K.

AU - Wu, W.

AU - Yodh, G.

AU - Young, S.

N1 - Funding Information: *Work supported by the Department of Energy under grant DE-FG02-91 ER40690.

PY - 1999/5

Y1 - 1999/5

N2 - With an effective telescope area of order 104 m2 for TeV neutrinos, a threshold near ∼50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope.

AB - With an effective telescope area of order 104 m2 for TeV neutrinos, a threshold near ∼50 GeV and a pointing accuracy of 2.5 degrees per muon track, the AMANDA detector represents the first of a new generation of high energy neutrino telescopes, reaching a scale envisaged over 25 years ago. We describe early results on the calibration of natural deep ice as a particle detector as well as on AMANDA's performance as a neutrino telescope.

UR - http://www.scopus.com/inward/record.url?scp=0033130149&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=0033130149&partnerID=8YFLogxK

U2 - 10.1016/S0920-5632(99)00469-7

DO - 10.1016/S0920-5632(99)00469-7

M3 - Article

AN - SCOPUS:0033130149

SN - 0920-5632

VL - 77

SP - 474

EP - 485

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

IS - 1-3

ER -

The AMANDA neutrino telescope

Abstract

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