Built on

M. A. Markov, International Conference on High-Energy Physics
1960
Earlier work this paper cites.
K. S. Hirata et al
1987
Earlier work this paper cites.
J. Holder ( Veritas
2003
Earlier work this paper cites.
E. G. Berezhko & H. J. Völk, arXiv:0707.4647v1
Original
2007
Earlier work this paper cites.

Similar

Pierre Auger Collaboration
2007
Cited alongside, same era.
M. Bouwhuis, for Antares
2009
Cited alongside, same era.
D. Dornic, for Antares
2009
Cited alongside, same era.
G. Guillard for Antares
2009
Cited alongside, same era.
J. Petrovic, arXiv:astro-ph/0908.1235
Cited in the paper.

Then

Th. Pradier, Nuclear Instruments and Methods in Physics Research
Original
2009
Later among the works it cites.
F. Halzen, for IceCube
2010
Closest in time.
E. Chassande-Mottin, for Antares
2010
Closest in time.

Beyond the bibliography

alphaXiv searches the wider corpus for related work and actual follow-ups.

Open on alphaXiv

alphaXiv is searching for related work…

Reading the bibliography…

2010

The Antares Neutrino Telescope and Multi-Messenger Astronomy

Pradier, Thierry

Understand

Antares is currently the largest neutrino telescope operating in the Northern Hemisphere, aiming at the detection of high-energy neutrinos from astrophysical sources.

Such observations would provide important clues about the processes at work in those sources, and possibly help solve the puzzle of ultra-high energy cosmic rays.
In this context, Antares is developing several programs to improve its capabilities of revealing possible spatial and/or temporal correlations of neutrinos with other cosmic messengers: photons, cosmic rays and gravitational waves.
The neutrino telescope and its most recent results are presented, together with these multi-messenger programs.