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

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

PHYSICAL REVIEW LETTERS（2006）

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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.

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physical sciences,solar flare,gamma ray,solar radiation,elementary particles,gamma radiation,astroparticle physics,physics

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