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Aggouras, G.; Anassontzis, E.; Ball, A.; Bourlis, G.; Chinowsky, W.; Fahrun, E.; Grammatikakis, G.; Green, C.; Grieder, P.; Katrivanos, P.; Katrivanos, P.; Koske, P.; Leisos, A.; Markopoulos, E.; Minkowsky, P.; Nygren, D.; Papageorgiou, K.; Przybylski, G.; Resvanis, L. K.; Siotis, I.; Sopher, J.;
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Aggouras, G.; Anassontzis, E.G.; Ball, A.E.; Bourlis, G.; Chinowsky, W.; Fahrun, E.; Grammatikakis, G.; Green, C.; Grieder, P.; Katrivanos, P.; Koske, P.; Leisos, A.; Ludvig, J.; Markopoulos, E.; Minkowsky, P.; Nygren, D.; Papageorgiou, K.; Przybylski, G.; Resvanis, L.K.; Siotis, I.; Sopher, J.;
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was selected for the installation of the telescope for several reasons. It combines deep water with close proximity to the shore, a convenient combination for the installation of the NESTOR towers and the communication and power supply cables. It is also located in an anti-diametric point with
169:-collaboration. As such, they are not developing the NESTOR telescope anymore as its own instance, but Km3Net has a planned telescope site off the coast of Pylos (which can thus be seen as a continuation of the NESTOR project to build an underwater telescope off the coast of Pylos).
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Because neutrinos are very weakly interacting, neutrino detectors must be very large to detect a significant number of neutrinos. After completion, NESTOR will consist of a large number of glass balls (the "eyes") containing
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27:(Neutrino Extended Submarine Telescope with Oceanographic Research Project) is an international scientific collaboration whose target is the deployment of a neutrino telescope on the sea floor off
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84:. Since they do not interact with matter via the electromagnetic or gravitational forces, it is extremely difficult to detect them. Since their mass is very small (less than 14
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Staveris-Polikalas, A.; Tsagli, V.; Tsirigotis, A.; Zhukov, V. A. (2005). "A measurement of the cosmic-ray muon flux with a module of the NESTOR neutrino telescope".
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Original surveys of the seafloor were conducted in 1989, 1991, 1992 and scientific conferences of the NESTOR Collaboration were held in the 1990s.
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Nuclear
Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
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Tzamarias, S.E. (2005). "Operation and performance of the NESTOR test detector: A measurement of the atmospheric muon flux".
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frames. Many frames compose a NESTOR tower. The whole construction is placed at the bottom of the sea to reduce noise from
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Staveris, T.; Tsagli, V.; Tsirigotis, A.; Zhukov, V.A. (2005). "Operation and performance of the NESTOR test detector".
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ocean and therefore, it is possible to compare observations and study correlations between the observed neutrino.
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In March 2003, the NESTOR prototype was lowered to the depth of 3800 meters some 30 kilometers off the coast of
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are elementary particles first detected in the 1950s, long after their theoretical prediction by theorist
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In 2014 the project was still applying funding to build the actual telescope.
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This article is about the neutrino observatory. For other projects, see
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and vice versa. Neutrinos do not interact with matter via either the
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XIX International
Conference on Neutrino Physics & Astrophysics
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Feder, T. (2002). "Deep-Sea Km
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forces, since they are electrically neutral leptons and their
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76:is very small. They interact with the
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82:weak nuclear interactions
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18:Nestor (disambiguation)
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60:are transformed into
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560:Neutrino oscillation
157:University of Athens
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403:. 24 October 2002.
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229:: 355–358.
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1260:Categories
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972:Gargamelle
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190:References
1172:Cancelled
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575:Operating
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173:See also
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62:neutrons
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1143:Nucifer
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346:(PDF)
155:from
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