2000
DOI: 10.1016/s0370-2693(00)00915-1
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GNO solar neutrino observations: results for GNO I

Abstract: We report the first GNO solar neutrino results for the measuring period GNO I, 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 ± 10.29.6 (stat.) ± 3.43.6 (syst.)] SNU (1σ) or [65.8 ± 10.710.2 (incl. syst.)] SNU (1σ) with errors combined. This may be compared to the result for Gallex (I–IV), which is [77.5 ± 7.67.8 (inc… Show more

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Cited by 474 publications
(248 citation statements)
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“…In χ 2 Rates , we include the CC event rate measured at SNO [7], the Chlorine [1] and Gallium [2,3,4] event rates and the Super-Kamiokande [5] total event rate. The matrixσ R,ij contains the theoretical uncertainties, as well as the experimental statistical and systematic errors, for the total rates.…”
Section: Methods Of Analysismentioning
confidence: 99%
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“…In χ 2 Rates , we include the CC event rate measured at SNO [7], the Chlorine [1] and Gallium [2,3,4] event rates and the Super-Kamiokande [5] total event rate. The matrixσ R,ij contains the theoretical uncertainties, as well as the experimental statistical and systematic errors, for the total rates.…”
Section: Methods Of Analysismentioning
confidence: 99%
“…(2.1) was used. The input data include the neutrino fluxes and uncertainties predicted by the BP00 solar model [12] and the total measured event rates from the SNO [7], Chlorine [1], and Gallium (averaged) [2,3,4] experiments, as well as the recoil electron energy spectrum measured by Super-Kamiokande [5] during the day and separately the energy spectrum measured at night. The C.L.…”
Section: Global Oscillation Solution: Three Different Analysesmentioning
confidence: 99%
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“…The strategies corresponding to panels (b) and (c) include the theoretical uncertainty in the 8 B neutrino flux, but differ in how they treat the total rate measured in the Super-Kamiokande experiment. The input data used in constructing figure 1 include the neutrino fluxes and uncertainties predicted by the BP00 solar model [8] and the total measured CC and NC event rates from the SNO experiment [1], the SNO day-night asymmetry [2], the Chlorine [10] and Gallium (averaged) [6,11,12,13] event rates, as well as the zenith angle-recoil energy spectrum data presented by Super-Kamiokande [14]. The rates from the GALLEX/GNO and SAGE experiments have been averaged to provide a unique data point (72.4 ± 4.7 SNU).…”
Section: Global Oscillation Solutionsmentioning
confidence: 99%
“…In the "Before" case, we use all the solar neutrino data (see refs. [9,10,11,12,13,14,15]) that were published or had appeared publicly before April 20, 2002, the date that the SNO NC and day-night asymmetry were first published. In the "After" case, we include in addition measurements reported in the two recent papers [1,2] by the Sudbury Neutrino Observatory (SNO) collaboration.…”
Section: Introductionmentioning
confidence: 99%