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The Baikal underwater neutrino telescope: Design, performance, and first resultsby: IA Belolaptikov, LB Bezrukov, BA Borisovets, NM Budnev, EV Bugaev, AG Chensky, IA Danilchenko, Djilkibaev, VI Dobrynin, GV Domogatsky, LA Donskych, AA Doroshenko, GN Dudkin, Egorov, SV Fialkovsky, AA Garus, A Gaponenko, AV Golikov, OA Gress, TA Gress, MN Gushtan, R Heller, VB Kabikov, H Heukenkamp, A Karle, AM Klabukov, AI Klimov, SI Klimushin, AP Koshechkin, J Krabi, VF Kulepov, LA Kuzmichov, Lanin, AL Lopin, BK Lubsandorzhiev, MB Milenin, T Mikolajski, RR Mirgazov, AV Moroz, NI Moseiko, MN Nemchenko, SA Nikiforov, NV Ogievetsky, EA Osipova, AN Padusenko, AI Panfilov, Yu Parfenov, AA Pavlov, DP Petukhov, KA Pocheikin, PG Pokhil, PA Pokolev, MI Rosanov, Rubzov, AV Rzhestshitski, SI Sinegovsky, IA Sokalski, Ch Spiering, O Streicher, AA Sumanov, L Tanko, T Thon, BA Tarashanski, II Trofimenko, Ch Wiebusch, R Wischnewski, VL Zurbanov
Astroparticle Physics, Vol. 7, No. 3. (August 1997), pp. 263-282.
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AbstractA first deep underwater detector for muons and neutrinos, NT-200, is currently under construction in Lake Baikal. Part of the detector, NT-36, with 36 photomultiplier tubes at three strings, has been installed in 1993. This array allowed for the first time a three-dimensional mapping of Cherenkov light deep underwater. Since then, various arrays have been almost continuously taking data. Presently a 96-PMT array is operating. We describe the NT-200 detector design and present results obtained with NT-36.
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