Results from the AMANDA neutrino telescope

C. de los Heros; M. Ackermann; J. Ahrens; H. Albrecht; X. Bai; R. Bay; M. Bartelt; S. W. Barwick; T. Becka; K. H. Becker; J. K. Becker; E. Bernardini; D. Bertrand; D. J. Boersma; S. Böser; O. Botner; A. Bouchta; O. Bouhali; J. Braun; C. Burgess; T. Burgess; T. Castermans; D. Chirkin; B. Collin; J. Conrad; J. Cooley; D. F. Cowen; A. Davour; C. de Clercq; T. DeYoung; P. Desiati; P. Ekström; T. Feser; T. K. Gaisser; R. Ganugapati; H. Geenen; L. Gerhardt; A. Goldschmidt; A. Gross; A. Hallgren; F. Halzen; K. Hanson; R. Hardtke; T. Harenberg; T. Hauschildt; K. Helbing; M. Hellwig; P. Herquet; G. C. Hill; J. Hodges; D. Hubert; B. Hughey; P. O. Hulth; K. Hultqvist; S. Hundertmark; J. Jacobsen; K. H. Kampert; A. Karle; J. Kelley; M. Kestel; L. Köpke; M. Kowalski; M. Krasberg; K. Kuehn; H. Leich; M. Leuthold; I. Liubarsky; J. Madsen; K. Mandli; P. Marciniewski; H. S. Matis; C. P. McParland; T. Messarius; Y. Minaeva; P. Miočinović; R. Morse; K. Munich; R. Nahnhauer; J. W. Nam; T. Neunhöffer; P. Niessen; D. R. Nygren; H. Ögelman; P. Olbrecht; A. C. Pohl; R. Porrata; P. B. Price; G. T. Przybylski; K. Rawlins; E. Resconi; W. Rhode; M. Ribordy; S. Richter; J. Rodríguez Martino; H. G. Sander; K. Schinarakis; S. Schlenstedt; D. Schneider; R. Schwarz; A. Silvestri; M. Solarz; G. M. Spiczak; C. Spiering; M. Stamatikos; D. Steele; P. Steffen; R. G. Stokstad; K. H. Sulanke; I. Taboada; L. Thollander; S. Tilav; W. Wagner; C. Walck; M. Walter; Y. R. Wang; C. H. Wiebusch; R. Wischnewski; H. Wissing; K. Woschnagg; G. Yodh

doi:10.1016/j.nuclphysbps.2004.10.003

Results from the AMANDA neutrino telescope

C. de los Heros, M. Ackermann, J. Ahrens, H. Albrecht, X. Bai, R. Bay, M. Bartelt, S. W. Barwick, T. Becka, K. H. Becker, J. K. Becker, E. Bernardini, D. Bertrand, D. J. Boersma, S. Böser, O. Botner, A. Bouchta, O. Bouhali, J. Braun, C. BurgessT. Burgess, T. Castermans, D. Chirkin, B. Collin, J. Conrad, J. Cooley, D. F. Cowen, A. Davour, C. de Clercq, T. DeYoung, P. Desiati, P. Ekström, T. Feser, T. K. Gaisser, R. Ganugapati, H. Geenen, L. Gerhardt, A. Goldschmidt, A. Gross, A. Hallgren, F. Halzen, K. Hanson, R. Hardtke, T. Harenberg, T. Hauschildt, K. Helbing, M. Hellwig, P. Herquet, G. C. Hill, J. Hodges, D. Hubert, B. Hughey, P. O. Hulth, K. Hultqvist, S. Hundertmark, J. Jacobsen, K. H. Kampert, A. Karle, J. Kelley, M. Kestel, L. Köpke, M. Kowalski, M. Krasberg, K. Kuehn, H. Leich, M. Leuthold, I. Liubarsky, J. Madsen, K. Mandli, P. Marciniewski, H. S. Matis, C. P. McParland, T. Messarius, Y. Minaeva, P. Miočinović, R. Morse, K. Munich, R. Nahnhauer, J. W. Nam, T. Neunhöffer, P. Niessen, D. R. Nygren, H. Ögelman, P. Olbrecht, A. C. Pohl, R. Porrata, P. B. Price, G. T. Przybylski, K. Rawlins, E. Resconi, W. Rhode, M. Ribordy, S. Richter, J. Rodríguez Martino, H. G. Sander, K. Schinarakis, S. Schlenstedt, D. Schneider, R. Schwarz, A. Silvestri, M. Solarz, G. M. Spiczak, C. Spiering, M. Stamatikos, D. Steele, P. Steffen, R. G. Stokstad, K. H. Sulanke, I. Taboada, L. Thollander, S. Tilav, W. Wagner, C. Walck, M. Walter, Y. R. Wang, C. H. Wiebusch, R. Wischnewski, H. Wissing, K. Woschnagg, G. Yodh

Physics and Astronomy (Twin Cities)

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Abstract

We review recent results from AMANDA on the search for cosmic point sources of neutrinos, both in the diffuse and point-like channels. Assuming a E^-2 spectral shape of the neutrino energy at the source, we derive limits on the diffuse ν_μ flux as well as in the all-flavour diffuse flux from the cascade search. We report limits on selected point sources as well as on GRB searches. We present results on primary cosmic CR composition in the range ∼100 TeV-PeV obtained with the help of the SPASE air shower array run in coincidence with AMANDA.

Original language	English (US)
Pages (from-to)	85-92
Number of pages	8
Journal	Nuclear Physics B - Proceedings Supplements
Volume	136
Issue number	1-3 SPEC.ISS.
DOIs	https://doi.org/10.1016/j.nuclphysbps.2004.10.003
State	Published - Nov 2004

Bibliographical note

Funding Information:
This research is supported by the following agencies: National Science Foundation–Office of Polar Programs, National Science Foundation– Physics Division, University of Wisconsin Alumni Research Foundation, Department of Energy, and National Energy Research Scientific Computing Center, UC-Irvine AENEAS Supercomputer Facility, USA; Swedish Research Council, Swedish Polar Research Secretariat and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research, Deutsche Forschungsgemeinschaft (DFG), Germany; Fund for Scientific Research (FNRS-FWO), Flanders Institute to encourage scientific and technological research in industry (IWT) and Belgian Federal Office for Scientific, Technical and Cultural affairs (OSTC), Belgium. D.F.C. acknowledges the support of the NSF CAREER program.

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10.1016/j.nuclphysbps.2004.10.003

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de los Heros, C., Ackermann, M., Ahrens, J., Albrecht, H., Bai, X., Bay, R., Bartelt, M., Barwick, S. W., Becka, T., Becker, K. H., Becker, J. K., Bernardini, E., Bertrand, D., Boersma, D. J., Böser, S., Botner, O., Bouchta, A., Bouhali, O., Braun, J., ... Yodh, G. (2004). Results from the AMANDA neutrino telescope. Nuclear Physics B - Proceedings Supplements, 136(1-3 SPEC.ISS.), 85-92. https://doi.org/10.1016/j.nuclphysbps.2004.10.003

de los Heros, C, Ackermann, M, Ahrens, J, Albrecht, H, Bai, X, Bay, R, Bartelt, M, Barwick, SW, Becka, T, Becker, KH, Becker, JK, Bernardini, E, Bertrand, D, Boersma, DJ, Böser, S, Botner, O, Bouchta, A, Bouhali, O, Braun, J, Burgess, C, Burgess, T, Castermans, T, Chirkin, D, Collin, B, Conrad, J, Cooley, J, Cowen, DF, Davour, A, de Clercq, C, DeYoung, T, Desiati, P, Ekström, P, Feser, T, Gaisser, TK, Ganugapati, R, Geenen, H, Gerhardt, L, Goldschmidt, A, Gross, A, Hallgren, A, Halzen, F, Hanson, K, Hardtke, R, Harenberg, T, Hauschildt, T, Helbing, K, Hellwig, M, Herquet, P, Hill, GC, Hodges, J, Hubert, D, Hughey, B, Hulth, PO, Hultqvist, K, Hundertmark, S, Jacobsen, J, Kampert, KH, Karle, A, Kelley, J, Kestel, M, Köpke, L, Kowalski, M, Krasberg, M, Kuehn, K, Leich, H, Leuthold, M, Liubarsky, I, Madsen, J, Mandli, K, Marciniewski, P, Matis, HS, McParland, CP, Messarius, T, Minaeva, Y, Miočinović, P, Morse, R, Munich, K, Nahnhauer, R, Nam, JW, Neunhöffer, T, Niessen, P, Nygren, DR, Ögelman, H, Olbrecht, P, Pohl, AC, Porrata, R, Price, PB, Przybylski, GT, Rawlins, K, Resconi, E, Rhode, W, Ribordy, M, Richter, S, Martino, JR, Sander, HG, Schinarakis, K, Schlenstedt, S, Schneider, D, Schwarz, R, Silvestri, A, Solarz, M, Spiczak, GM, Spiering, C, Stamatikos, M, Steele, D, Steffen, P, Stokstad, RG, Sulanke, KH, Taboada, I, Thollander, L, Tilav, S, Wagner, W, Walck, C, Walter, M, Wang, YR, Wiebusch, CH, Wischnewski, R, Wissing, H, Woschnagg, K & Yodh, G 2004, 'Results from the AMANDA neutrino telescope', Nuclear Physics B - Proceedings Supplements, vol. 136, no. 1-3 SPEC.ISS., pp. 85-92. https://doi.org/10.1016/j.nuclphysbps.2004.10.003

@article{03effdd00fc746d2b37d5cb2616ebded,

title = "Results from the AMANDA neutrino telescope",

abstract = "We review recent results from AMANDA on the search for cosmic point sources of neutrinos, both in the diffuse and point-like channels. Assuming a E-2 spectral shape of the neutrino energy at the source, we derive limits on the diffuse νμ flux as well as in the all-flavour diffuse flux from the cascade search. We report limits on selected point sources as well as on GRB searches. We present results on primary cosmic CR composition in the range ∼100 TeV-PeV obtained with the help of the SPASE air shower array run in coincidence with AMANDA.",

author = "{de los Heros}, C. and M. Ackermann and J. Ahrens and H. Albrecht and X. Bai and R. Bay and M. Bartelt and Barwick, {S. W.} and T. Becka and Becker, {K. H.} and Becker, {J. K.} and E. Bernardini and D. Bertrand and Boersma, {D. J.} and S. B{\"o}ser and O. Botner and A. Bouchta and O. Bouhali and J. Braun and C. Burgess and T. Burgess and T. Castermans and D. Chirkin and B. Collin and J. Conrad and J. Cooley and Cowen, {D. F.} and A. Davour and {de Clercq}, C. and T. DeYoung and P. Desiati and P. Ekstr{\"o}m and T. Feser and Gaisser, {T. K.} and R. Ganugapati and H. Geenen and L. Gerhardt and A. Goldschmidt and A. Gross and A. Hallgren and F. Halzen and K. Hanson and R. Hardtke and T. Harenberg and T. Hauschildt and K. Helbing and M. Hellwig and P. Herquet and Hill, {G. C.} and J. Hodges and D. Hubert and B. Hughey and Hulth, {P. O.} and K. Hultqvist and S. Hundertmark and J. Jacobsen and Kampert, {K. H.} and A. Karle and J. Kelley and M. Kestel and L. K{\"o}pke and M. Kowalski and M. Krasberg and K. Kuehn and H. Leich and M. Leuthold and I. Liubarsky and J. Madsen and K. Mandli and P. Marciniewski and Matis, {H. S.} and McParland, {C. P.} and T. Messarius and Y. Minaeva and P. Mio{\v c}inovi{\'c} and R. Morse and K. Munich and R. Nahnhauer and Nam, {J. W.} and T. Neunh{\"o}ffer and P. Niessen and Nygren, {D. R.} and H. {\"O}gelman and P. Olbrecht and Pohl, {A. C.} and R. Porrata and Price, {P. B.} and Przybylski, {G. T.} and K. Rawlins and E. Resconi and W. Rhode and M. Ribordy and S. Richter and Martino, {J. Rodr{\'i}guez} and Sander, {H. G.} and K. Schinarakis and S. Schlenstedt and D. Schneider and R. Schwarz and A. Silvestri and M. Solarz and Spiczak, {G. M.} and C. Spiering and M. Stamatikos and D. Steele and P. Steffen and Stokstad, {R. G.} and Sulanke, {K. H.} and I. Taboada and L. Thollander and S. Tilav and W. Wagner and C. Walck and M. Walter and Wang, {Y. R.} and Wiebusch, {C. H.} and R. Wischnewski and H. Wissing and K. Woschnagg and G. Yodh",

note = "Funding Information: This research is supported by the following agencies: National Science Foundation–Office of Polar Programs, National Science Foundation– Physics Division, University of Wisconsin Alumni Research Foundation, Department of Energy, and National Energy Research Scientific Computing Center, UC-Irvine AENEAS Supercomputer Facility, USA; Swedish Research Council, Swedish Polar Research Secretariat and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research, Deutsche Forschungsgemeinschaft (DFG), Germany; Fund for Scientific Research (FNRS-FWO), Flanders Institute to encourage scientific and technological research in industry (IWT) and Belgian Federal Office for Scientific, Technical and Cultural affairs (OSTC), Belgium. D.F.C. acknowledges the support of the NSF CAREER program.",

year = "2004",

month = nov,

doi = "10.1016/j.nuclphysbps.2004.10.003",

language = "English (US)",

volume = "136",

pages = "85--92",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier B.V.",

number = "1-3 SPEC.ISS.",

}

TY - JOUR

T1 - Results from the AMANDA neutrino telescope

AU - de los Heros, C.

AU - Ackermann, M.

AU - Ahrens, J.

AU - Albrecht, H.

AU - Bai, X.

AU - Bay, R.

AU - Bartelt, M.

AU - Barwick, S. W.

AU - Becka, T.

AU - Becker, K. H.

AU - Becker, J. K.

AU - Bernardini, E.

AU - Bertrand, D.

AU - Boersma, D. J.

AU - Böser, S.

AU - Botner, O.

AU - Bouchta, A.

AU - Bouhali, O.

AU - Braun, J.

AU - Burgess, C.

AU - Burgess, T.

AU - Castermans, T.

AU - Chirkin, D.

AU - Collin, B.

AU - Conrad, J.

AU - Cooley, J.

AU - Cowen, D. F.

AU - Davour, A.

AU - de Clercq, C.

AU - DeYoung, T.

AU - Desiati, P.

AU - Ekström, P.

AU - Feser, T.

AU - Gaisser, T. K.

AU - Ganugapati, R.

AU - Geenen, H.

AU - Gerhardt, L.

AU - Goldschmidt, A.

AU - Gross, A.

AU - Hallgren, A.

AU - Halzen, F.

AU - Hanson, K.

AU - Hardtke, R.

AU - Harenberg, T.

AU - Hauschildt, T.

AU - Helbing, K.

AU - Hellwig, M.

AU - Herquet, P.

AU - Hill, G. C.

AU - Hodges, J.

AU - Hubert, D.

AU - Hughey, B.

AU - Hulth, P. O.

AU - Hultqvist, K.

AU - Hundertmark, S.

AU - Jacobsen, J.

AU - Kampert, K. H.

AU - Karle, A.

AU - Kelley, J.

AU - Kestel, M.

AU - Köpke, L.

AU - Kowalski, M.

AU - Krasberg, M.

AU - Kuehn, K.

AU - Leich, H.

AU - Leuthold, M.

AU - Liubarsky, I.

AU - Madsen, J.

AU - Mandli, K.

AU - Marciniewski, P.

AU - Matis, H. S.

AU - McParland, C. P.

AU - Messarius, T.

AU - Minaeva, Y.

AU - Miočinović, P.

AU - Morse, R.

AU - Munich, K.

AU - Nahnhauer, R.

AU - Nam, J. W.

AU - Neunhöffer, T.

AU - Niessen, P.

AU - Nygren, D. R.

AU - Ögelman, H.

AU - Olbrecht, P.

AU - Pohl, A. C.

AU - Porrata, R.

AU - Price, P. B.

AU - Przybylski, G. T.

AU - Rawlins, K.

AU - Resconi, E.

AU - Rhode, W.

AU - Ribordy, M.

AU - Richter, S.

AU - Martino, J. Rodríguez

AU - Sander, H. G.

AU - Schinarakis, K.

AU - Schlenstedt, S.

AU - Schneider, D.

AU - Schwarz, R.

AU - Silvestri, A.

AU - Solarz, M.

AU - Spiczak, G. M.

AU - Spiering, C.

AU - Stamatikos, M.

AU - Steele, D.

AU - Steffen, P.

AU - Stokstad, R. G.

AU - Sulanke, K. H.

AU - Taboada, I.

AU - Thollander, L.

AU - Tilav, S.

AU - Wagner, W.

AU - Walck, C.

AU - Walter, M.

AU - Wang, Y. R.

AU - Wiebusch, C. H.

AU - Wischnewski, R.

AU - Wissing, H.

AU - Woschnagg, K.

AU - Yodh, G.

N1 - Funding Information: This research is supported by the following agencies: National Science Foundation–Office of Polar Programs, National Science Foundation– Physics Division, University of Wisconsin Alumni Research Foundation, Department of Energy, and National Energy Research Scientific Computing Center, UC-Irvine AENEAS Supercomputer Facility, USA; Swedish Research Council, Swedish Polar Research Secretariat and Knut and Alice Wallenberg Foundation, Sweden; German Ministry for Education and Research, Deutsche Forschungsgemeinschaft (DFG), Germany; Fund for Scientific Research (FNRS-FWO), Flanders Institute to encourage scientific and technological research in industry (IWT) and Belgian Federal Office for Scientific, Technical and Cultural affairs (OSTC), Belgium. D.F.C. acknowledges the support of the NSF CAREER program.

PY - 2004/11

Y1 - 2004/11

N2 - We review recent results from AMANDA on the search for cosmic point sources of neutrinos, both in the diffuse and point-like channels. Assuming a E-2 spectral shape of the neutrino energy at the source, we derive limits on the diffuse νμ flux as well as in the all-flavour diffuse flux from the cascade search. We report limits on selected point sources as well as on GRB searches. We present results on primary cosmic CR composition in the range ∼100 TeV-PeV obtained with the help of the SPASE air shower array run in coincidence with AMANDA.

AB - We review recent results from AMANDA on the search for cosmic point sources of neutrinos, both in the diffuse and point-like channels. Assuming a E-2 spectral shape of the neutrino energy at the source, we derive limits on the diffuse νμ flux as well as in the all-flavour diffuse flux from the cascade search. We report limits on selected point sources as well as on GRB searches. We present results on primary cosmic CR composition in the range ∼100 TeV-PeV obtained with the help of the SPASE air shower array run in coincidence with AMANDA.

UR - http://www.scopus.com/inward/record.url?scp=10444256567&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=10444256567&partnerID=8YFLogxK

U2 - 10.1016/j.nuclphysbps.2004.10.003

DO - 10.1016/j.nuclphysbps.2004.10.003

M3 - Article

AN - SCOPUS:10444256567

SN - 0920-5632

VL - 136

SP - 85

EP - 92

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

IS - 1-3 SPEC.ISS.

ER -

Results from the AMANDA neutrino telescope

Abstract

Bibliographical note

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