An All-Sky Search for Steady VHE Gamma-Ray Sources
Atkins, R. · Benbow, W. · Berley, D. · Chen, M. -L. · Coyne, D. G. · Delay, R. S. · Dingus, B. L. · Dorfan, D. E. · Ellsworth, R. W. · Evans, D. · Falcone, A. · Fleysher, L. · Fleysher, R. · Gisler, G. · Goodman, J. A. · Haines, T. J. · Hoffman, C. M. · Hugenberger, S. · Kelley, L. A. · Leonor, I. · Macri, J. · McConnell, M. · McCullough, J. F. · McEnery, J. E. · Miller, R. S. · Mincer, A. I. · Morales, M. F. · Nemethy, P. · Ryan, J. M. · Schneider, M. · Shen, B. · Shoup, A. · Sinnis, G. · Smith, A. J. · Sullivan, G. W. · Thompson, T. N. · Tumer, O. T. · Wang, K. · Wascko, M. O. · Westerhoff, S. · Williams, D. A. · Yang, T. · Yodh, G. B.
Original · EN
The Milagrito water Cherenkov detector in the Jemez Mountains near Los Alamos, New Mexico took data from February 1997 to April 1998. Milagrito served as a prototype for the larger Milagro detector, which has just begun operations. Milagrito was the first large-aperture gamma-ray detector with sensitivity to gamma rays below 1 TeV. We report here on a search for steady emission from point sources over most of the northern sky using data from Milagrito.
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