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TeV Observations of Markarian 501 with the Milagrito Water Cerenkov Detector.
Atkins R; Benbow W; Berley D; Chen ML; Coyne DG; Delay RS; Dingus BL; Dorfan DE; Ellsworth RW; Espinoza C; Evans D; Falcone A; Fleysher L; Fleysher R; Gisler G; Goodman JA; Haines TJ; Hoffman CM; Hugenberger S; Kelley LA; Leonor I; McConnell M; McCullough JF; McEnery JE; Miller RS; Mincer AI; Morales MF; Murray MM; Nemethy P; Ryan JM; Schneider M; Shen B; Shoup A; Sinnis C; Smith AJ; Sullivan GW; Thompson TN; Tumer T; Wang K; Wascko MO; Westerhoff S; Williams DA; Yang T; Yodh GB.
Astrophys J ; 525(1): L25-L28, 1999 Nov 01.
Article in English | MEDLINE | ID: mdl-10511505

ABSTRACT

The Milagrito water Cerenkov detector near Los Alamos, New Mexico, was operated as a sky monitor at energies of a few TeV between 1997 February and 1998 May, including the period of the strong, long-lasting 1997 flare of Markarian 501. Milagrito served as a test run for the full Milagro detector. An event excess with a significance of 3.7 sigma from Markarian 501 was observed, in agreement with expectations.

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