GALLEX results from the first 30 solar neutrino runs
References (34)
Phys. Lett. B
(1992)Phys. Lett. B
(1993)Phys. Rev. D
(1991)- et al.
Phys. Rev. Lett.
(1993) - et al.
Ap. J.
(1993) - et al.
Rev. Mod. Phys.
(1992) - et al.
Angew. Chem., Int. Ed. (Engl.)
(1992) - et al.
Statistical treatment of the low-level counting data in GALLEX
Status of the GALLEX solar neutrino experiment with emphasis on error treatment and on blank runs
Phys. Rev. Lett.
Recent results from SAGE
Phys. Rep.
Ap. J. Lett.
Neutrino Astrophysics
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This work has been supported by the German Federal Minister for Research and Technology (BMFT). This work has been generously supported by the ALFRIED KRUPP von BOHLEN und HALBACH-Foundation, Germany.
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This work has been supported by Istituto Nazionale di Fisica Nucleare (INFN), Italy.
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This work has been supported by the Commissariat à l'énergie atomique (CEA), France.
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This work has been supported by the Office of High Energy and Nuclear Physics of the U.S. Department of Energy, United States.
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Permanent address: Instytut Fizyki, Uniwersytet Jagiellonski, ul. Reymonta 4, PL-30059 Kraków, Poland.