First results of the instrumentation line for the deep-sea ANTARES neutrino telescope

被引:87
作者
Aguilar, J. A.
Albert, A.
Ameli, F.
Anghinolfi, M.
Anton, G.
Anvar, S.
Aslanides, E.
Aubert, J. -J.
Barbarito, E.
Basa, S.
Battaglieri, M.
Becherini, Y.
Bellotti, R.
Beltramelli, J.
Bertin, V.
Bigi, A.
Billault, M.
Blaes, R.
de Botton, N.
Bouwhuis, M. C.
Bradbury, S. M.
Bruijn, R.
Brunner, J.
Burgio, G. F.
Busto, J.
Cafagna, F.
Caillat, L.
Calzas, A.
Capone, A.
Caponetto, L.
Carmona, E.
Carr, J.
Cartwright, S. L.
Castel, D.
Castorina, E.
Cavasinni, V.
Cecchini, S.
Ceres, A.
Charvis, P.
Chauchot, P.
Chiarusi, T.
Circella, M.
Colnard, C.
Compere, C.
Coniglione, R.
Cottini, N.
Coyle, P.
Cuneo, S.
Cussatlegras, A. -S.
Damy, G.
机构
[1] CNRS, CPPM, IN2P3, F-13288 Marseille 9, France
[2] Univ Mediterranee, F-13288 Marseille, France
[3] Univ Paris 07, APC, CNRS, UMR 7164,CEA,Observ Paris, F-75231 Paris 05, France
[4] Dept Interateneo Fis, I-70126 Bari, Italy
[5] Sez INFN, I-70126 Bari, Italy
[6] Sez INFN, I-40127 Bologna, Italy
[7] Univ Bologna, I-40127 Bologna, Italy
[8] INSU, CNRS, COM, F-13288 Marseille 9, France
[9] Univ Mediterranee, F-13288 Marseille 9, France
[10] Sez INFN, I-95125 Catania, Italy
[11] Univ Catania, Dipartimento Fis & Astron, I-95125 Catania, Italy
[12] Univ Erlangen Nurnberg, Inst Phys, D-91058 Erlangen, Germany
[13] Univ Paris 06, Observ Oceanol Villefranche, Geosci Azur, CNRS,INSU,IRD, F-06235 Villefranche Sur Mer, France
[14] Sez INFN, Dipartimento Fis, I-16146 Genoa, Italy
[15] Univ Valencia, CSIC, IFIC, Edificios Invest Paterna, Valencia 46071, Spain
[16] IFREMER, Ctr Brest, F-29280 Plouzane, France
[17] IFREMER, Ctr Toulon La Seyne Sur Mer, F-83500 La Seyne Sur Mer, France
[18] IASF, INAF, I-40129 Bologna, Italy
[19] Univ Strasbourg 1, IPHC, F-67037 Strasbourg 2, France
[20] CNRS, IN2P3, F-67037 Strasbourg 2, France
[21] Inst Space Sci, Bucharest 77125, Magurele, Romania
[22] ITEP, Moscow 117259, Russia
[23] Univ Groningen, KVI, NL-9747 AA Groningen, Netherlands
[24] CNRS, INSU, LAM, F-13012 Marseille 12, France
[25] Univ Aix Marseille 1, F-13012 Marseille 12, France
[26] LNS, Ist Nazl Fis Nucl, I-95123 Catania, Italy
[27] Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, W Yorkshire, England
[28] Univ Haute Alsace, GRPHE, F-68093 Mulhouse, France
[29] NIKHEF H, NL-1098 SJ Amsterdam, Netherlands
[30] Univ Pisa, Dipartimento Fis, I-56127 Pisa, Italy
[31] Sez INFN, I-56127 Pisa, Italy
[32] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[33] Sez INFN, I-00185 Rome, Italy
[34] CEA Saclay, Direct Sci Matiere, Lab Rech Lois Fondamentales, F-91191 Gif Sur Yvette, France
[35] DSM Dapnia, F-91191 Gif Sur Yvette, France
[36] Univ Sheffield, Dept Phys & Astron, Sheffield S3 7RH, S Yorkshire, England
[37] Univ Utrecht, Fac Betawetenschappen, NL-3584 CC Utrecht, Netherlands
[38] Univ Amsterdam, Inst Hoge Energiefys, NL-1098 SJ Amsterdam, Netherlands
基金
俄罗斯基础研究基金会;
关键词
neutrino astronomy; underwater detector; photon detection;
D O I
10.1016/j.astropartphys.2006.07.004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
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. Crown Copyright (c) 2006 Published by Elsevier B.V. All rights reserved.
引用
收藏
页码:314 / 324
页数:11
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