%0 Journal Article
%T Determination of neutrino incoming direction in the CHOOZ experiment and Supernova explosion location by scintillator detectors
%A M. Apollonio
%A A. Baldini
%A C. Bemporad
%A E. Caffau
%A F. Cei
%A Y. Declais
%A H. de Kerret
%A B. Dieterle
%A A. Etenko
%A L. Foresti
%A J. George
%A G. Giannini
%A M. Grassi
%A Y. Kozlov
%A W. Kropp
%A D. Kryn
%A M. Laiman
%A C. E. Lane
%A B. Lefievre
%A I. Machulin
%A A. Martemyanov
%A V. Martemyanov
%A L. Mikaelyan
%A D. Nicolo
%A M. Obolensky
%A R. Pazzi
%A G. Pieri
%A L. Price
%A S. Riley
%A R. Reeder
%A A. Sabelnikov
%A G. Santin
%A M. Skorokhvatov
%A H. Sobel
%A J. Steele
%A R. Steinberg
%A S. Sukhotin
%A S. Tomshaw
%A D. Veron
%A V. Vyrodov
%J Physics
%D 1999
%I arXiv
%R 10.1103/PhysRevD.61.012001
%X The CHOOZ experiment measured the antineutrino flux at a distance of about 1 Km from two nuclear reactors in order to detect possible neutrino oscillations with squared mass differences as low as 10**-3 eV**2 for full mixing. We show that the data analysis of the electron antineutrino events, collected by our liquid scintillation detector, locates the antineutrino source within a cone of half-aperture of about 18 degrees at the 68% C.L.. We discuss the implications of this experimental result for tracking down a supernova explosion.
%U http://arxiv.org/abs/hep-ex/9906011v1