Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of 27 December 2004 with the AMANDA-II detector.
Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20 giant flare of 27 December 2004 with the AMANDA-II detector.
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DOI：
10.1103/physrevlett.97.221101
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发表时间：
2006-11
影响因子：
8.6
通讯作者：
A. Achterberg;M. Ackermann;J. Adams;J. Ahrens;K. Andeen;D. Atlee;J. Bahcall;X. Bai;B. Baret;M. Bartelt;S. Barwick;R. Bay;K. Beattie;T. Becka;J. Becker;K. Becker;P. Berghaus;D. Berley;E. Bernardini;D. Bertrand;D. Besson;E. Blaufuss;D. Boersma;C. Bohm;J. Bolmont;S. Böser;O. Botner;A. Bouchta;J. Braun;C. Burgess;T. Burgess;T. Castermans;D. Chirkin;B. Christy;J. Clem;D. Cowen;M. D'Agostino;A. Davour;C. Day;C. De Clercq;L. Demirörs;F. Descamps;P. Desiati;T. DeYoung;J. C. Díaz-Vélez;J. Dreyer;J. Dumm;M. Duvoort;W. Edwards;R. Ehrlich;J. Eisch;R. Ellsworth;P. Evenson;O. Fadiran;A. Fazely;T. Feser;K. Filimonov;B. Fox;T. Gaisser;J. Gallagher;R. Ganugapati;H. Geenen;L. Gerhardt;A. Goldschmidt;J. Goodman;R. Gozzini;S. Grullon;A. Gross;R. Gunasingha;M. Gurtner;A. Hallgren;F. Halzen;K. Han;K. Hanson;D. Hardtke;R. Hardtke;T. Harenberg;J. Hart;T. Hauschildt;D. Hays;J. Heise;K. Helbing;M. Hellwig;P. Herquet;G. Hill;J. Hodges;K. Hoffman;B. Hommez;K. Hoshina;Daan Hubert;B. Hughey;P. O. Hulth;K. Hultqvist;S. Hundertmark;J. Hülß;A. Ishihara;J. Jacobsen;G. Japaridze;A. Jones;J. Joseph;K. Kampert;A. Karle;H. Kawai;J. Kelley;M. Kestel;N. Kitamura;S. Klein;S. Klepser;G. Kohnen;H. Kolanoski;L. Köpke;M. Krasberg;K. Kuehn;H. Landsman;H. Leich;I. Liubarsky;J. Lundberg;J. Madsen;K. Mase;H. Matis;T. McCauley;C. Mcparland;A. Meli;T. Messarius;P. Mészáros;H. Miyamoto;A. Mokhtarani;T. Montaruli;A. Morey;R. Morse;S. Movit;K. Münich;R. Nahnhauer;J. Nam;P. Niessen;D. Nygren;H. Ogelman;P. Olbrechts;A. Olivas;S. Patton;C. Peña-Garay;C. Pérez de los Heros;A. Piegsa;D. Pieloth;A. Pohl;R. Porrata;J. Pretz;P. Price;G. Przybylski;K. Rawlins;S. Razzaque;F. Refflinghaus;E. Resconi;W. Rhode;M. Ribordy;A. Rizzo;S. Robbins;P. Roth;C. Rott;D. Rutledge;D. Ryckbosch;H. Sander;S. Sarkar;S. Schlenstedt;T. Schmidt;D. Schneider;D. Seckel;S. Seo;S. Seunarine;A. Silvestri;A. Smith;M. Solarz;C. Song;J. Sopher;G. Spiczak;C. Spiering;M. Stamatikos;T. Stanev;P. Steffen;T. Stezelberger;R. Stokstad;M. Stoufer;S. Stoyanov;E. Strahler;T. Straszheim;K. Sulanke;G. Sullivan;T. Sumner;I. Taboada;O. Tarasova;A. Tepe;L. Thollander;S. Tilav;P. Toale;D. Turcan;N. van Eijndhoven;J. Vandenbroucke;A. Van Overloop;B. Voigt;W. Wagner;C. Walck;H. Waldmann;M. Walter;Y.-R. Wang;C. Wendt;C. Wiebusch;G. Wikström;D. Williams;R. Wischnewski;H. Wissing;K. Woschnagg;X. Xu;G. Yodh;S. Yoshida;J. Zornoza
中科院分区：
文献类型：
--
作者：
A. Achterberg;M. Ackermann;J. Adams;J. Ahrens;K. Andeen;D. Atlee;J. Bahcall;X. Bai;B. Baret;M. Bartelt;S. Barwick;R. Bay;K. Beattie;T. Becka;J. Becker;K. Becker;P. Berghaus;D. Berley;E. Bernardini;D. Bertrand;D. Besson;E. Blaufuss;D. Boersma;C. Bohm;J. Bolmont;S. Böser;O. Botner;A. Bouchta;J. Braun;C. Burgess;T. Burgess;T. Castermans;D. Chirkin;B. Christy;J. Clem;D. Cowen;M. D'Agostino;A. Davour;C. Day;C. De Clercq;L. Demirörs;F. Descamps;P. Desiati;T. DeYoung;J. C. Díaz-Vélez;J. Dreyer;J. Dumm;M. Duvoort;W. Edwards;R. Ehrlich;J. Eisch;R. Ellsworth;P. Evenson;O. Fadiran;A. Fazely;T. Feser;K. Filimonov;B. Fox;T. Gaisser;J. Gallagher;R. Ganugapati;H. Geenen;L. Gerhardt;A. Goldschmidt;J. Goodman;R. Gozzini;S. Grullon;A. Gross;R. Gunasingha;M. Gurtner;A. Hallgren;F. Halzen;K. Han;K. Hanson;D. Hardtke;R. Hardtke;T. Harenberg;J. Hart;T. Hauschildt;D. Hays;J. Heise;K. Helbing;M. Hellwig;P. Herquet;G. Hill;J. Hodges;K. Hoffman;B. Hommez;K. Hoshina;Daan Hubert;B. Hughey;P. O. Hulth;K. Hultqvist;S. Hundertmark;J. Hülß;A. Ishihara;J. Jacobsen;G. Japaridze;A. Jones;J. Joseph;K. Kampert;A. Karle;H. Kawai;J. Kelley;M. Kestel;N. Kitamura;S. Klein;S. Klepser;G. Kohnen;H. Kolanoski;L. Köpke;M. Krasberg;K. Kuehn;H. Landsman;H. Leich;I. Liubarsky;J. Lundberg;J. Madsen;K. Mase;H. Matis;T. McCauley;C. Mcparland;A. Meli;T. Messarius;P. Mészáros;H. Miyamoto;A. Mokhtarani;T. Montaruli;A. Morey;R. Morse;S. Movit;K. Münich;R. Nahnhauer;J. Nam;P. Niessen;D. Nygren;H. Ogelman;P. Olbrechts;A. Olivas;S. Patton;C. Peña-Garay;C. Pérez de los Heros;A. Piegsa;D. Pieloth;A. Pohl;R. Porrata;J. Pretz;P. Price;G. Przybylski;K. Rawlins;S. Razzaque;F. Refflinghaus;E. Resconi;W. Rhode;M. Ribordy;A. Rizzo;S. Robbins;P. Roth;C. Rott;D. Rutledge;D. Ryckbosch;H. Sander;S. Sarkar;S. Schlenstedt;T. Schmidt;D. Schneider;D. Seckel;S. Seo;S. Seunarine;A. Silvestri;A. Smith;M. Solarz;C. Song;J. Sopher;G. Spiczak;C. Spiering;M. Stamatikos;T. Stanev;P. Steffen;T. Stezelberger;R. Stokstad;M. Stoufer;S. Stoyanov;E. Strahler;T. Straszheim;K. Sulanke;G. Sullivan;T. Sumner;I. Taboada;O. Tarasova;A. Tepe;L. Thollander;S. Tilav;P. Toale;D. Turcan;N. van Eijndhoven;J. Vandenbroucke;A. Van Overloop;B. Voigt;W. Wagner;C. Walck;H. Waldmann;M. Walter;Y.-R. Wang;C. Wendt;C. Wiebusch;G. Wikström;D. Williams;R. Wischnewski;H. Wissing;K. Woschnagg;X. Xu;G. Yodh;S. Yoshida;J. Zornoza
2004 年 12 月 27 日，软伽马射线中继器 1806-20 发出的巨大伽马耀斑使许多卫星伽马射线探测器饱和，成为银河系有史以来观测到的最亮的瞬态事件。 AMANDA-II 用于搜索表明该天体中存在高能伽马和/或中微子的下行 μ 子。数据显示没有显着信号，因此设置归一化常数的上限（在 90% C.L. 时）：0.05(0.5) TeV-1 m;{-2} s;{-1}（对于伽马通量中 gamma=-1.47 (-2)）和 0.4(6.1) TeV-1 m;{-2} s;{-1}（对于高能伽马=-1.47 (-2)）中微子通量。
On 27 December 2004, a giant gamma flare from the Soft Gamma-Ray Repeater 1806-20 saturated many satellite gamma-ray detectors, being the brightest transient event ever observed in the Galaxy. AMANDA-II was used to search for down-going muons indicative of high-energy gammas and/or neutrinos from this object. The data revealed no significant signal, so upper limits (at 90% C.L.) on the normalization constant were set: 0.05(0.5) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the gamma flux and 0.4(6.1) TeV-1 m;{-2} s;{-1} for gamma=-1.47 (-2) in the high-energy neutrino flux.