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P. Amram et al (ANTARES Collab.), Nucl. Instrum. Meth., 2002, A484, 369
2002
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M. Ageron et al., (ANTARES Collab.), Nucl. Instr. Meth., 2007, A578, 498
2007
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2009

Brown, Anthony M.

Completed in May 2008, the ANTARES neutrino telescope is located 40 km off the coast of Toulon, at a depth of about 2500 m.

The telescope consists of 12 detect or lines housing a total of 884 optical modules.
Each line is anchored to the seabed and pulled taught by the buoyancy of the individual optical modules and a top buoy.
Due to the fluid nature of the sea-water detecting medium and the flexible nature of the detector lines, the optical modules of the ANTARES telescope can suffer from deviations of up to several meters from the vertical and as such, real time positioning is needed.

P. Amram et al (ANTARES Collab.), Nucl. Instrum. Meth., 2002, A484, 369
2002
Earlier work this paper cites.
M. Ageron et al., (ANTARES Collab.), Nucl. Instr. Meth., 2007, A578, 498
2007
Earlier work this paper cites.

P. Keller (ANTARES Collab.), Proc. SENSORCOMM Conf., 2007, 243
2007
Cited alongside, same era.
P. Coyle (ANTARES Collab.), 2009, submitted to this issue
2009
Cited alongside, same era.
M. Spurio (ANTARES Collab.), arXiv:0904.3836v1
Original
Cited in the paper.
http://www.km3net.org
Original
Cited in the paper.

J.P. Gomez (ANTARES Collab.), 2009, submitted to this issue
2009
Closest in time.
M. Ardid (ANTARES Collab.), Nucl. Instr. and Meth., 2009, A602, 174
2009
Closest in time.

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

alphaXiv is searching for related work…