English

GNO Solar Neutrino Observations: Results for GNOI

High Energy Physics - Experiment 2009-10-31 v1 Astrophysics

Abstract

We report the first GNO solar neutrino results for the measuring period GNOI, solar exposure time May 20, 1998 till January 12, 2000. In the present analysis, counting results for solar runs SR1 - SR19 were used till April 4, 2000. With counting completed for all but the last 3 runs (SR17 - SR19), the GNO I result is [65.8 +10.2 -9.6 (stat.) +3.4 -3.6 (syst.)]SNU (1sigma) or [65.8 + 10.7 -10.2 (incl. syst.)]SNU (1sigma) with errors combined. This may be compared to the result for Gallex(I-IV), which is [77.5 +7.6 -7.8 (incl. syst.)] SNU (1sigma). A combined result from both GNOI and Gallex(I-IV) together is [74.1 + 6.7 -6.8 (incl. syst.)] SNU (1sigma).

Keywords

Cite

@article{arxiv.hep-ex/0006034,
  title  = {GNO Solar Neutrino Observations: Results for GNOI},
  author = {GNO Collaboration and M. Altmann and M. Balata and P. Belli and E. Bellotti and R. Bernabei and E. Burkert and C. Cattadori and G. Cerichelli and M. Chiarini and M. Cribier and S. d'Angelo and G. Del Re and K. H. Ebert and F. v. Feilitzsch and N. Ferrari and W. Hampel and J. Handt and E. Henrich and G. Heusser and J. Kiko and T. Kirsten and T. Lachenmaier and J. Lanfranchi and M. Laubenstein and D. Motta and W. Rau and H. Richter and S. Waenninger and M. Wojcik and L. Zanotti},
  journal= {arXiv preprint arXiv:hep-ex/0006034},
  year   = {2009}
}

Comments

submitted to Physics Letters B, June 2000. PACS: 26.65. +t ; 14.60 Pq. Corresponding author: [email protected] ; [email protected]