001     329829
005     20250731154533.0
024 7 _ |a 10.1103/PhysRevLett.92.071102
|2 doi
024 7 _ |a 0031-9007
|2 ISSN
024 7 _ |a 1079-7114
|2 ISSN
024 7 _ |a 1092-0145
|2 ISSN
024 7 _ |a WOS:000189139500007
|2 WOS
024 7 _ |a pmid:14995836
|2 pmid
024 7 _ |a inspire:628728
|2 inspire
024 7 _ |a 10.3204/PUBDB-2017-06379
|2 datacite_doi
024 7 _ |a openalex:W1482772510
|2 openalex
037 _ _ |a PUBDB-2017-06379
041 _ _ |a English
082 _ _ |a 550
088 1 _ |a astro-ph/0309585
088 _ _ |a astro-ph/0309585
|2 arXiv
100 1 _ |a Ahrens, J.
|b 0
245 _ _ |a Search for extraterrestrial point sources of neutrinos with AMANDA-II
260 _ _ |a College Park, Md.
|c 2004
|b APS
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Report
|0 PUB:(DE-HGF)29
|2 PUB:(DE-HGF)
|m report
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1499064876_21226
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
500 _ _ |a Standort Zeuthen; AMANDA Collaboration
520 _ _ |a We present the results of a search for point sources of high energy neutrinos in the northern hemisphere using AMANDA-II data collected in the year 2000. Included are flux limits on several AGN blazars, microquasars, magnetars and other candidate neutrino sources. A search for excesses above a random background of cosmic-ray-induced atmospheric neutrinos and misreconstructed downgoing cosmic-ray muons reveals no statistically significant neutrino point sources. We show that AMANDA-II has achieved the sensitivity required to probe known TeV gamma-ray sources such as the blazar Markarian 501 in its 1997 flaring state at a level where neutrino and gamma-ray fluxes are equal.
536 _ _ |a 899 - ohne Topic (POF3-899)
|0 G:(DE-HGF)POF3-899
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|f POF III
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588 _ _ |a Dataset connected to CrossRef, INSPIRE
650 _ 7 |a neutrino: cosmic radiation
|2 INSPIRE
650 _ 7 |a cosmic radiation: particle source
|2 INSPIRE
650 _ 7 |a cosmic radiation: flux
|2 INSPIRE
650 _ 7 |a upper limit
|2 INSPIRE
650 _ 7 |a AGN: blazar
|2 INSPIRE
650 _ 7 |a quasar
|2 INSPIRE
650 _ 7 |a matter: magnetic
|2 INSPIRE
650 _ 7 |a Cherenkov counter: water
|2 INSPIRE
650 _ 7 |a photomultiplier
|2 INSPIRE
650 _ 7 |a data management
|2 INSPIRE
650 _ 7 |a muon: cosmic radiation
|2 INSPIRE
650 _ 7 |a numerical methods
|2 INSPIRE
650 _ 7 |a AMANDA
|2 INSPIRE
650 _ 7 |a experimental results
|2 INSPIRE
693 _ _ |0 EXP:(DE-H253)AMANDA-20170101
|5 EXP:(DE-H253)AMANDA-20170101
|e Antarctic Muon And Neutrino Detector Array
|x 0
700 1 _ |a Bai, X.
|b 1
700 1 _ |a Barwick, S. W.
|b 2
700 1 _ |a Becka, T.
|b 3
700 1 _ |a Becker, K. H.
|b 4
700 1 _ |a Bernardini, Elisa
|b 5
700 1 _ |a Bertrand, D.
|b 6
700 1 _ |a Binon, F. G.
|b 7
700 1 _ |a Biron, A.
|b 8
700 1 _ |a Boersma, D. J.
|b 9
700 1 _ |a Boeser, Sebastian
|b 10
700 1 _ |a Botner, O.
|b 11
700 1 _ |a Bouchta, A.
|b 12
700 1 _ |a Bouhali, O.
|b 13
700 1 _ |a Burgess, T.
|b 14
700 1 _ |a Carius, S.
|b 15
700 1 _ |a Castermans, T.
|b 16
700 1 _ |a Chen, A.
|b 17
700 1 _ |a Chirkin, D.
|b 18
700 1 _ |a Collin, B.
|b 19
700 1 _ |a Conrad, J.
|b 20
700 1 _ |a Cooley, J.
|b 21
700 1 _ |a Cowen, D. F.
|b 22
700 1 _ |a Davour, A.
|b 23
700 1 _ |a De Clercq, C.
|b 24
700 1 _ |a DeYoung, T.
|b 25
700 1 _ |a Desiati, P.
|b 26
700 1 _ |a Dewulf, J. P.
|b 27
700 1 _ |a Ekstrom, P.
|b 28
700 1 _ |a Feser, T.
|b 29
700 1 _ |a Gaisser, T. K.
|b 30
700 1 _ |a Ganugapati, R.
|b 31
700 1 _ |a Gaug, M.
|b 32
700 1 _ |a Geenen, Heiko
|b 33
700 1 _ |a Gerhardt, L.
|b 34
700 1 _ |a Goldschmidt, A.
|b 35
700 1 _ |a Gross, A.
|b 36
700 1 _ |a Hallgren, A.
|b 37
700 1 _ |a Halzen, F.
|b 38
700 1 _ |a Hanson, K.
|b 39
700 1 _ |a Hardtke, R.
|b 40
700 1 _ |a Harenberg, T.
|b 41
700 1 _ |a Hauschildt, Tonio
|b 42
700 1 _ |a Helbing, K.
|b 43
700 1 _ |a Hellwig, M.
|b 44
700 1 _ |a Herquet, P.
|b 45
700 1 _ |a Hill, G. C.
|b 46
700 1 _ |a Hubert, D.
|b 47
700 1 _ |a Hughey, B.
|b 48
700 1 _ |a Hulth, P. O.
|b 49
700 1 _ |a Hultqvist, K.
|b 50
700 1 _ |a Hundertmark, S.
|b 51
700 1 _ |a Jacobsen, J.
|b 52
700 1 _ |a Karle, A.
|b 53
700 1 _ |a Kestel, M.
|b 54
700 1 _ |a Kopke, L.
|b 55
700 1 _ |a Kowalski, M.
|b 56
700 1 _ |a Kuehn, K.
|b 57
700 1 _ |a Lamoureux, J. I.
|b 58
700 1 _ |a Leich, H.
|b 59
700 1 _ |a Leuthold, M.
|b 60
700 1 _ |a Lindahl, P.
|b 61
700 1 _ |a Liubarsky, I.
|b 62
700 1 _ |a Madsen, J.
|b 63
700 1 _ |a Mandli, K.
|b 64
700 1 _ |a Marciniewski, P.
|b 65
700 1 _ |a Matis, H. S.
|b 66
700 1 _ |a McParland, C. P.
|b 67
700 1 _ |a Messarius, T.
|b 68
700 1 _ |a Minaeva, Y.
|b 69
700 1 _ |a Miocinovic, P.
|b 70
700 1 _ |a Morse, R.
|b 71
700 1 _ |a Munich, K.
|b 72
700 1 _ |a Nahnhauer, R.
|b 73
700 1 _ |a Neunhoffer, T.
|b 74
700 1 _ |a Niessen, P.
|b 75
700 1 _ |a Nygren, D. R.
|b 76
700 1 _ |a Ogelman, H.
|b 77
700 1 _ |a Olbrechts, Ph.
|b 78
700 1 _ |a Perez de los Heros, C.
|b 79
700 1 _ |a Pohl, A. C.
|b 80
700 1 _ |a Porrata, R.
|b 81
700 1 _ |a Price, P. B.
|b 82
700 1 _ |a Przybylski, G. T.
|b 83
700 1 _ |a Rawlins, K.
|b 84
700 1 _ |a Resconi, E.
|b 85
700 1 _ |a Rhode, W.
|b 86
700 1 _ |a Ribordy, M.
|b 87
700 1 _ |a Richter, S.
|b 88
700 1 _ |a Rodriguez Martino, J.
|b 89
700 1 _ |a Sander, H. G.
|b 90
700 1 _ |a Schinarakis, K.
|b 91
700 1 _ |a Schlenstedt, S.
|b 92
700 1 _ |a Schmidt, T.
|b 93
700 1 _ |a Schneider, D.
|b 94
700 1 _ |a Schwarz, R.
|b 95
700 1 _ |a Silvestri, A.
|b 96
700 1 _ |a Solarz, M.
|b 97
700 1 _ |a Spiczak, G.
|b 98
700 1 _ |a Spiering, C.
|b 99
700 1 _ |a Stamatikos, M.
|b 100
700 1 _ |a Steele, D.
|b 101
700 1 _ |a Steffen, P.
|b 102
700 1 _ |a Stokstad, R. G.
|b 103
700 1 _ |a Sulanke, K. H.
|b 104
700 1 _ |a Taboada, I.
|b 105
700 1 _ |a Thollander, L.
|b 106
700 1 _ |a Tilav, S.
|b 107
700 1 _ |a Wagner, W.
|b 108
700 1 _ |a Walck, C.
|b 109
700 1 _ |a Wang, Y. R.
|b 110
700 1 _ |a Wiebusch, C. H.
|b 111
700 1 _ |a Wiedemann, C.
|b 112
700 1 _ |a Wischnewski, R.
|b 113
700 1 _ |a Wissing, H.
|b 114
700 1 _ |a Yodh, G.
|b 115
700 1 _ |a AMANDA Collaboration
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773 _ _ |a 10.1103/PhysRevLett.92.071102
|g Vol. 92, no. 7, p. 071102
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