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

A. Achterberg,M. Ackermann,J. Adams,J. Ahrens,K. Andeen,D. W. Atlee,J. N. Bahcall,X. Bai,B. Baret,M. Bartelt,S. W. Barwick,R. Bay,K. Beattie,T. Becka, J. K. Becker,K. -H. Becker,P. Berghaus,D. Berley,E. Bernardini,D. Bertrand,D. Z. Besson,E. Blaufuss,D. J. Boersma,C. Bohm,J. Bolmont,S. Boeser,O. Botner,A. Bouchta,J. Braun,C. Burgess,T. Burgess,T. Castermans,D. Chirkin,B. Christy,J. Clem,D. F. Cowen, M. V. D'Agostino,A. Davour,C. T. Day,C. De Clercq,L. Demirors, F. Descamps,P. Desiati,T. DeYoung,J. C. Diaz-Velez,J. Dreyer,J. P. Dumm,M. R. Duvoort,W. R. Edwards,R. Ehrlich,J. Eisch,R. W. Ellsworth,P. A. Evenson,O. Fadiran,A. R. Fazely, T. Feser,K. Filimonov,B. D. Fox,T. K. Gaisser,J. Gallagher,R. Ganugapati,H. Geenen,L. Gerhardt,A. Goldschmidt,J. A. Goodman,R. Gozzini,S. Grullon,A. Gross,R. M. Gunasingha,M. Gurtner,A. Hallgren,F. Halzen,K. Han,K. Hanson,D. Hardtke,R. Hardtke,T. Harenberg,J. E. Hart,T. Hauschildt, D. Hays,J. Heise,K. Helbing,M. Hellwig,P. Herquet,G. C. Hill,J. Hodges,K. D. Hoffman,B. Hommez,K. Hoshina,D. Hubert,B. Hughey,P. O. Hulth,K. Hultqvist,S. Hundertmark, J.-P. Huelss,A. Ishihara,J. Jacobsen,G. S. Japaridze,A. Jones,J. M. Joseph,K. -H. Kampert,A. Karle,H. Kawai,J. L. Kelley,M. Kestel,N. Kitamura,S. R. Klein,S. Klepser,G. Kohnen,H. Kolanoski,L. Koepke,M. Krasberg,K. Kuehn,H. Landsman,H. Leich,I. Liubarsky,J. Lundberg,J. Madsen,K. Mase,H. S. Matis,T. McCauley,C. P. McParland,A. Meli,T. Messarius,P. Meszaros,H. Miyamoto,A. Mokhtarani,T. Montaruli,A. Morey,R. Morse,S. M. Movit,K. Muenich,R. Nahnhauer,J. W. Nam,P. Niessen,D. R. Nygren,H. Ogelman,Ph. Olbrechts,A. Olivas,S. Patton,C. Pena-Garay,C. Perez de los Heros,A. Piegsa, D. Pieloth,A. C. Pohl,R. Porrata,J. Pretz,P. B. Price,G. T. 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. -G. Sander,S. Sarkar,S. Schlenstedt,T. Schmidt,D. Schneider,D. Seckel,S. H. Seo,S. Seunarine,A. Silvestri,A. J. Smith,M. Solarz,C. Song,J. E. Sopher,G. M. Spiczak,C. Spiering,M. Stamatikos,T. Stanev,P. Steffen,T. Stezelberger,R. G. Stokstad, M. C. Stoufer,S. Stoyanov,E. A. Strahler,T. Straszheim,K. -H. Sulanke,G. W. Sullivan,T. J. Sumner,I. Taboada,O. Tarasova,A. Tepe,L. Thollander,S. Tilav,P. A. 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. H. Wiebusch,G. Wikstrom, D. R. Williams,R. Wischnewski,H. Wissing,K. Woschnagg,X. W. Xu,G. Yodh,S. Yoshida,J. D. Zornoza

Physical Review Letters（2006）

引用 36|浏览54

暂无评分

摘要

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.

查看译文

关键词

Gamma-Ray Bursts

AI 理解论文

溯源树

样例

生成溯源树，研究论文发展脉络

Chat Paper

正在生成论文摘要