Results from SAGE

V. M. Vermul, Institute for Nuclear Research of the Russian Academy of Sciences
J. N. Abdurashitov, Institute for Nuclear Research of the Russian Academy of Sciences
T. J. Bowles, Los Alamos National Laboratory
M. L. Cherry, Louisiana State University
B. T. Cleveland, University of Washington
R. Davis, University of Pennsylvania
S. R. Elliott, University of Washington
V. N. Gavrin, Institute for Nuclear Research of the Russian Academy of Sciences
S. V. Girin, Institute for Nuclear Research of the Russian Academy of Sciences
V. V. Gorbachev, Institute for Nuclear Research of the Russian Academy of Sciences
T. V. Ibragimova, Institute for Nuclear Research of the Russian Academy of Sciences
A. V. Kalikhov, Institute for Nuclear Research of the Russian Academy of Sciences
N. G. Khairnasov, Institute for Nuclear Research of the Russian Academy of Sciences
T. V. Knodel, Institute for Nuclear Research of the Russian Academy of Sciences
K. Lande, University of Pennsylvania
J. N. Mirmov, Institute for Nuclear Research of the Russian Academy of Sciences
J. S. Nico, National Institute of Standards and Technology
A. A. Shikhin, Institute for Nuclear Research of the Russian Academy of Sciences
W. A. Teasdale, Los Alamos National Laboratory
E. P. Veretenkin, Institute for Nuclear Research of the Russian Academy of Sciences
D. L. Wark, Los Alamos National Laboratory
P. S. Wildenhain, University of Pennsylvania
J. F. Wilkerson, University of Washington
V. E. Yants, Institute for Nuclear Research of the Russian Academy of Sciences
G. T. Zatsepin, Institute for Nuclear Research of the Russian Academy of Sciences

Abstract

We report the results of 11 years of solar neutrino observation by the Russian-American Gallium solar neutrino Experiment (SAGE). The overall result of 84 runs during the measurement period January 1990 through March 2001 is 75.6 +5.9/-5.8 (stat.) +3.5/-3.0 (syst.) SNU. This represents only slightly more than half of the predicted standard solar model rate of 129 SNU. The individual results of each run, as well as the results of combined analysis of all runs are presented.