Measurement of the atmospheric muon flux with the NEMO Phase-1 detector,
S. Aiello et al.(The NEMO),
Astropart. Phys. 33 (2010) 263-273,
arXiv:0910.1269.
Sensitivity of an underwater Cerenkov km3 telescope to TeV neutrinos from Galactic Microquasars,
C. Distefano et al.(NEMO),
Astropart. Phys. 28 (2007) 1-9,
arXiv:astro-ph/0608053.
NEMO: A Project for a km^3 Underwater Detector for Astrophysical Neutrinos in the Mediterranean Sea,
I. Amore(NEMO),
IJMPA, Vol. 22, No. 21 (2007) 2007,
arXiv:0709.3991.
ISCRA 2006,
Erice 20-27 June 2006.
Implementation of the trigger algorithm for the NEMO project,
G. d'Angelo, G. Riccio, M. Brescia,
arXiv:astro-ph/0701622, 2007.
I Workshop of Astronomy and Astrophysics for Students,
Naples,
19-20 April 2006.
Statistical analysis of the trigger algorithm for the NEMO project,
G. Riccio, G. D'Angelo, M. Brescia,
arXiv:astro-ph/0701621, 2007.
I Workshop of Astronomy and Astrophysics for Students,
Naples,
19-20 April 2006.
Sensitivity of the NEMO telescope to neutrinos from microquasars,
C. Distefano(NEMO),
Nucl. Phys. Proc. Suppl. 165 (2007) 181-187,
arXiv:astro-ph/0608515.
CRIS06 proceedings (Catania,
Italy,
May 29 - June 2,
2006).
Detection of point-like neutrino sources with the NEMO-km3 telescope,
C. Distefano(NEMO),
Astrophys. Space Sci. 309 (2007) 415-420,
arXiv:astro-ph/0608514.
BCN06 proceedings (Barcelona,
July 4-7,
2006).
Effects of architectural issues on a km3 scale detector,
R. Coniglione et al.(NEMO),
Nucl. Instrum. Meth. A567 (2006) 489-491,
arXiv:astro-ph/0605068.
VVVNT2 proceedings (Catania,
Italy,
November 8-11,
2005).
Sensitivity and pointing accuracy of the NEMO km3 telescope,
C. Distefano et al.(NEMO),
Nucl. Instrum. Meth. A567 (2006) 495-497,
arXiv:astro-ph/0605067.
VLVNT2 (Catania,
Italy,
November 8-11,
2005).