Detection potential to point-like neutrino sources with the NEMO-km3 telescope

Abstract

The NEMO Collaboration is conducting an R&D activity towards the construction of a Mediterranean km3 neutrino telescope. In this work, we present the results of Monte Carlo simulation studies on the capability of the proposed NEMO telescope to detect and identify point-like sources of high energy muon neutrinos.

To be published on BCN06 proceedings (Barcelona, July 4-7, 2006)

References in corpus (4)

• Deep seawater inherent optical properties in the Southern Ionian Sea
• Expected neutrino signal from supernova remnant RX J1713.7-3946 and flavor oscillations
• Sensitivity of an underwater Cerenkov km3 telescope to TeV neutrinos from Galactic Microquasars
• Sensitivity and pointing accuracy of the NEMO km${}^3$ telescope

Cited by in corpus (1)

• Production of gamma rays and neutrinos in the dark jets of the microquasar SS433