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1.	Aguilar, J. A., et al. (author) First results of the instrumentation line for the deep-sea ANTARES neutrino telescope 2006 In: Astroparticle physics. - : Elsevier. - 0927-6505 .- 1873-2852. ; 26:4-5, s. 314-324 Journal article (peer-reviewed)abstract In 2005, the ANTARES Collaboration deployed and operated at a depth of 2500 m a so-called Mini Instrumentation Line equipped with Optical Modules (MILOM) at the ANTARES site. The various data acquired during the continuous operation from April to December 2005 of the MILOM confirm the satisfactory performance of the Optical Modules, their front-end electronics and readout system. as well as the calibration devices of the detector. The in situ measurement of the Optical Module time response yields a resolution better than 0.5 ns. The performance of the acoustic positioning system, which enables the spatial reconstruction of the ANTARES detector with a precision of about 10 cm, is verified. These results demonstrate that with the full ANTARES neutrino telescope the design angular resolution of better than 0.3 degrees can be realistically achieved.
2.	Casolino, M., et al. (author) Cosmic-ray observations of the heliosphere with the PAMELA experiment 2006 In: Astrophysics. - : Elsevier BV. ; , s. 1848-1852 Conference paper (peer-reviewed)abstract The PAMELA experiment is a multi-purpose apparatus built around a permanent magnet spectrometer, with the main goal of studying in detail the antiparticle component of cosmic rays. The apparatus will be carried in space by means of a Russian satellite, due to launch in 2005, for a three year-long mission. The characteristics of the detectors composing the instrument, alongside the long lifetime of the mission and the orbital characteristics of the satellite, will allow to address several items of cosmic-ray physics. In this paper, we will focus on the solar and heliospheric observation capabilities of PAMELA.

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Type of publication: conference paper (1); journal article (1)

Type of content: peer-reviewed (2)

Author/Editor: Bellotti, R. (2); Casolino, M. (1); Cavasinni, V. (1); Korolkova, E. V. (1); Roda, C. (1); Petta, C. (1); show more...; Vacchi, A. (1); Bonvicini, V. (1); Zampa, G. (1); Rostovtsev, A. (1); Kooijman, P. (1); Aguilar, J. A. (1); Kappes, A. (1); Karg, T. (1); Kopper, C. (1); Montaruli, T. (1); Shanidze, R. (1); Anton, G. (1); Katz, U. (1); Lucarelli, F. (1); Brunner, J. (1); Bruijn, R. (1); Albert, A. (1); Pearce, Mark (1); Cuneo, S. (1); Colnard, C. (1); Carlson, Per (1); Becherini, Yvonne (1); Carr, J. (1); Ernenwein, J. -P (1); Lamanna, G. (1); Zaborov, D. (1); Giglietto, N. (1); Morselli, A. (1); Spinelli, P. (1); Karkar, S. (1); Stolarczyk, T. (1); Vallage, B. (1); Flaminio, V. (1); Cafagna, F. (1); Campana, D. (1); Marcelli, L. (1); Osteria, G. (1); Picozza, P. (1); Ricci, M. (1); Castellini, G. (1); Kok, H. (1); Naumann-Godo, M. (1); Mongelli, M. (1); Mirizzi, N. (1); show less...

University: Royal Institute of Technology (1); Linnaeus University (1)

Language: English (2)

Research subject (UKÄ/SCB): Natural sciences (2)

Year: 2006 (2)Undo refine

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