Background light in potential sites for the ANTARES undersea neutrino telescope

P. Amram; S. Anvar; E. Aslanides; J. J. Aubert; R. Azoulay; S. Basa; Y. Benhammou; F. Bernard; V. Bertin; M. Billault; P. E. Blanc; F. Blanc; R. W. Bland; F. Blondeau; N. Bottu; J. Boulesteix; B. Brooks; J. Brunner; A. Calzas; C. Carloganu; E. Carmona; J. Carr; P. H. Carton; S. Cartwright; R. Cases; F. Cassol; C. Compere; S. Cooper; G. Coustillier; N. de Botton; P. Deck; F. E. Desages; J. J. Destelle; G. Dispau; J. F. Drogou; F. Drouhin; P. Y. Duval; F. Feinstein; D. Festy; J. Fopma; J. L. Fuda; P. Goret; L. Gosset; J. F. Gournay; J. J. Hernández; G. Herrouin; F. Hubaut; J. R. Hubbard; D. Huss; M. Jaquet; N. Jelley; E. Kajfasz; M. Karolak; A. Kouchner; V. Kudryavtsev; D. Lachartre; H. Lafoux; P. Lamare; J. C. Languillat; D. Laugier; J. P. Laugier; Y. le Guen; H. le Provost; A. le van Suu; L. Lemoine; P. L. Liotard; S. Loucatos; P. Magnier; M. Macelin; L. Martin; A. Massol; B. Mazeau; A. Mazure; F. Mazéas; J. McMillan; C. Millot; P. Mols; F. Montanet; J. P. Morel; L. Moscoso; S. Navas; C. Olivetto; N. Palanque-Delabrouille; A. Pallares; P. Payre; P. Perrin; A. Pohl; J. Poinsignon; R. Potheau; Y. Queinec; C. Racca; M. Raymond; J. F. Rolin; Y. Sacquin; J. P. Schuller; W. Schuster; N. Spooner; T. Stolarczyk; A. Tabary; M. Talby; C. Tao; Y. Tayalati; L. F. Thompson; R. Triay; T. Tzvetanov; P. Valdy; P. Vernin; E. Vigeolas; D. Vignaud; D. Vilanova; D. Wark; A. Zghiche; J. Zuniga

doi:10.1016/S0927-6505(99)00118-8

Background light in potential sites for the ANTARES undersea neutrino telescope

P. Amram
, S. Anvar
, E. Aslanides
, J. J. Aubert
, R. Azoulay
, S. Basa
, Y. Benhammou
, F. Bernard
, V. Bertin
, M. Billault
, P. E. Blanc
, F. Blanc
, R. W. Bland
, F. Blondeau
, N. Bottu
, J. Boulesteix
, B. Brooks
, J. Brunner
, A. Calzas
, C. Carloganu

E. Carmona, J. Carr, P. H. Carton, S. Cartwright, R. Cases, F. Cassol, C. Compere, S. Cooper, G. Coustillier, N. de Botton, P. Deck, F. E. Desages, J. J. Destelle, G. Dispau, J. F. Drogou, F. Drouhin, P. Y. Duval, F. Feinstein, D. Festy, J. Fopma, J. L. Fuda, P. Goret, L. Gosset, J. F. Gournay, J. J. Hernández, G. Herrouin, F. Hubaut, J. R. Hubbard, D. Huss, M. Jaquet, N. Jelley, E. Kajfasz, M. Karolak, A. Kouchner, V. Kudryavtsev, D. Lachartre, H. Lafoux, P. Lamare, J. C. Languillat, D. Laugier, J. P. Laugier, Y. le Guen, H. le Provost, A. le van Suu, L. Lemoine, P. L. Liotard, S. Loucatos, P. Magnier, M. Macelin, L. Martin, A. Massol, B. Mazeau, A. Mazure, F. Mazéas, J. McMillan, C. Millot, P. Mols, F. Montanet, J. P. Morel, L. Moscoso, S. Navas, C. Olivetto, N. Palanque-Delabrouille, A. Pallares, P. Payre, P. Perrin, A. Pohl, J. Poinsignon, R. Potheau, Y. Queinec, C. Racca, M. Raymond, J. F. Rolin, Y. Sacquin, J. P. Schuller, W. Schuster, N. Spooner, T. Stolarczyk, A. Tabary, M. Talby, C. Tao, Y. Tayalati, L. F. Thompson, R. Triay, T. Tzvetanov, P. Valdy, P. Vernin, E. Vigeolas, D. Vignaud, D. Vilanova, D. Wark, A. Zghiche, J. Zuniga

Observatoire Astronomique Marseille-Provence
Institut Pierre Simon Laplace, CNRS and CEA
Aix-Marseille Université
Université de Haute Alsac
USTV
University of Oxford
University of Valencia
The University of Sheffield
Département Ressources
CNRS
Université de Strasbourg

Résultats de recherche: Contribution à un journal › Article › Revue par des pairs

75 Citations (Scopus)

Résumé

The ANTARES collaboration has performed a series of in-situ measurements to study the background light for a planned undersea neutrino telescope. Such background can be caused by ⁴⁰K decays or by biological activity. We report on measurements at two sites in the Mediterranean Sea at depths of 2400 m and 2700 m, respectively. Three photomultiplier tubes were used to measure single counting rates and coincidence rates for pairs of tubes at various distances. The background rate is seen to consist of three components: a constant rate due to ⁴⁰K decays, a continuum rate that varies on a time scale of several hours simultaneously over distances up to at least 40 m, and random bursts a few seconds long that are only correlated in time over distances of the order of a meter. A trigger requiring coincidences between nearby photomultiplier tubes should reduce the trigger rate for a neutrino telescope to a manageable level with only a small loss in efficiency.

langue originale	Anglais
Pages (de - à)	127-136
Nombre de pages	10
journal	Astroparticle Physics
Volume	13
Numéro de publication	2-3
Les DOIs	https://doi.org/10.1016/S0927-6505(99)00118-8
état	Publié - 1 janv. 2000
Modification externe	Oui

Accès au document

10.1016/S0927-6505(99)00118-8

Contient cette citation

Amram, P., Anvar, S., Aslanides, E., Aubert, J. J., Azoulay, R., Basa, S., Benhammou, Y., Bernard, F., Bertin, V., Billault, M., Blanc, P. E., Blanc, F., Bland, R. W., Blondeau, F., Bottu, N., Boulesteix, J., Brooks, B., Brunner, J., Calzas, A., ... Zuniga, J. (2000). Background light in potential sites for the ANTARES undersea neutrino telescope. Astroparticle Physics, 13(2-3), 127-136. https://doi.org/10.1016/S0927-6505(99)00118-8

@article{dae8a17c73bb46c68479a793dac579c1,

title = "Background light in potential sites for the ANTARES undersea neutrino telescope",

abstract = "The ANTARES collaboration has performed a series of in-situ measurements to study the background light for a planned undersea neutrino telescope. Such background can be caused by 40K decays or by biological activity. We report on measurements at two sites in the Mediterranean Sea at depths of 2400 m and 2700 m, respectively. Three photomultiplier tubes were used to measure single counting rates and coincidence rates for pairs of tubes at various distances. The background rate is seen to consist of three components: a constant rate due to 40K decays, a continuum rate that varies on a time scale of several hours simultaneously over distances up to at least 40 m, and random bursts a few seconds long that are only correlated in time over distances of the order of a meter. A trigger requiring coincidences between nearby photomultiplier tubes should reduce the trigger rate for a neutrino telescope to a manageable level with only a small loss in efficiency.",

keywords = "29.40.Ka, 92.10.Bf, 95.55.Vj, Luminescence, Neutrino telescope, Sea water properties, Undersea Cherenkov detectors",

author = "P. Amram and S. Anvar and E. Aslanides and Aubert, \{J. J.\} and R. Azoulay and S. Basa and Y. Benhammou and F. Bernard and V. Bertin and M. Billault and Blanc, \{P. E.\} and F. Blanc and Bland, \{R. W.\} and F. Blondeau and N. Bottu and J. Boulesteix and B. Brooks and J. Brunner and A. Calzas and C. Carloganu and E. Carmona and J. Carr and Carton, \{P. H.\} and S. Cartwright and R. Cases and F. Cassol and C. Compere and S. Cooper and G. Coustillier and \{de Botton\}, N. and P. Deck and Desages, \{F. E.\} and Destelle, \{J. J.\} and G. Dispau and Drogou, \{J. F.\} and F. Drouhin and Duval, \{P. Y.\} and F. Feinstein and D. Festy and J. Fopma and Fuda, \{J. L.\} and P. Goret and L. Gosset and Gournay, \{J. F.\} and Hern{\'a}ndez, \{J. J.\} and G. Herrouin and F. Hubaut and Hubbard, \{J. R.\} and D. Huss and M. Jaquet and N. Jelley and E. Kajfasz and M. Karolak and A. Kouchner and V. Kudryavtsev and D. Lachartre and H. Lafoux and P. Lamare and Languillat, \{J. C.\} and D. Laugier and Laugier, \{J. P.\} and \{le Guen\}, Y. and \{le Provost\}, H. and \{le van Suu\}, A. and L. Lemoine and Liotard, \{P. L.\} and S. Loucatos and P. Magnier and M. Macelin and L. Martin and A. Massol and B. Mazeau and A. Mazure and F. Maz{\'e}as and J. McMillan and C. Millot and P. Mols and F. Montanet and Morel, \{J. P.\} and L. Moscoso and S. Navas and C. Olivetto and N. Palanque-Delabrouille and A. Pallares and P. Payre and P. Perrin and A. Pohl and J. Poinsignon and R. Potheau and Y. Queinec and C. Racca and M. Raymond and Rolin, \{J. F.\} and Y. Sacquin and Schuller, \{J. P.\} and W. Schuster and N. Spooner and T. Stolarczyk and A. Tabary and M. Talby and C. Tao and Y. Tayalati and Thompson, \{L. F.\} and R. Triay and T. Tzvetanov and P. Valdy and P. Vernin and E. Vigeolas and D. Vignaud and D. Vilanova and D. Wark and A. Zghiche and J. Zuniga",

year = "2000",

month = jan,

day = "1",

doi = "10.1016/S0927-6505(99)00118-8",

language = "English",

volume = "13",

pages = "127--136",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier B.V.",

number = "2-3",

}

Amram, P, Anvar, S, Aslanides, E, Aubert, JJ, Azoulay, R, Basa, S, Benhammou, Y, Bernard, F, Bertin, V, Billault, M, Blanc, PE, Blanc, F, Bland, RW, Blondeau, F, Bottu, N, Boulesteix, J, Brooks, B, Brunner, J, Calzas, A, Carloganu, C, Carmona, E, Carr, J, Carton, PH, Cartwright, S, Cases, R, Cassol, F, Compere, C, Cooper, S, Coustillier, G, de Botton, N, Deck, P, Desages, FE, Destelle, JJ, Dispau, G, Drogou, JF, Drouhin, F, Duval, PY, Feinstein, F, Festy, D, Fopma, J, Fuda, JL, Goret, P, Gosset, L, Gournay, JF, Hernández, JJ, Herrouin, G, Hubaut, F, Hubbard, JR, Huss, D, Jaquet, M, Jelley, N, Kajfasz, E, Karolak, M, Kouchner, A, Kudryavtsev, V, Lachartre, D, Lafoux, H, Lamare, P, Languillat, JC, Laugier, D, Laugier, JP, le Guen, Y, le Provost, H, le van Suu, A, Lemoine, L, Liotard, PL, Loucatos, S, Magnier, P, Macelin, M, Martin, L, Massol, A, Mazeau, B, Mazure, A, Mazéas, F, McMillan, J, Millot, C, Mols, P, Montanet, F, Morel, JP, Moscoso, L, Navas, S, Olivetto, C, Palanque-Delabrouille, N, Pallares, A, Payre, P, Perrin, P, Pohl, A, Poinsignon, J, Potheau, R, Queinec, Y, Racca, C, Raymond, M, Rolin, JF, Sacquin, Y, Schuller, JP, Schuster, W, Spooner, N, Stolarczyk, T, Tabary, A, Talby, M, Tao, C, Tayalati, Y, Thompson, LF, Triay, R, Tzvetanov, T, Valdy, P, Vernin, P, Vigeolas, E, Vignaud, D, Vilanova, D, Wark, D, Zghiche, A & Zuniga, J 2000, 'Background light in potential sites for the ANTARES undersea neutrino telescope', Astroparticle Physics, VOL. 13, Numéro 2-3, p. 127-136. https://doi.org/10.1016/S0927-6505(99)00118-8

TY - JOUR

T1 - Background light in potential sites for the ANTARES undersea neutrino telescope

AU - Amram, P.

AU - Anvar, S.

AU - Aslanides, E.

AU - Aubert, J. J.

AU - Azoulay, R.

AU - Basa, S.

AU - Benhammou, Y.

AU - Bernard, F.

AU - Bertin, V.

AU - Billault, M.

AU - Blanc, P. E.

AU - Blanc, F.

AU - Bland, R. W.

AU - Blondeau, F.

AU - Bottu, N.

AU - Boulesteix, J.

AU - Brooks, B.

AU - Brunner, J.

AU - Calzas, A.

AU - Carloganu, C.

AU - Carmona, E.

AU - Carr, J.

AU - Carton, P. H.

AU - Cartwright, S.

AU - Cases, R.

AU - Cassol, F.

AU - Compere, C.

AU - Cooper, S.

AU - Coustillier, G.

AU - de Botton, N.

AU - Deck, P.

AU - Desages, F. E.

AU - Destelle, J. J.

AU - Dispau, G.

AU - Drogou, J. F.

AU - Drouhin, F.

AU - Duval, P. Y.

AU - Feinstein, F.

AU - Festy, D.

AU - Fopma, J.

AU - Fuda, J. L.

AU - Goret, P.

AU - Gosset, L.

AU - Gournay, J. F.

AU - Hernández, J. J.

AU - Herrouin, G.

AU - Hubaut, F.

AU - Hubbard, J. R.

AU - Huss, D.

AU - Jaquet, M.

AU - Jelley, N.

AU - Kajfasz, E.

AU - Karolak, M.

AU - Kouchner, A.

AU - Kudryavtsev, V.

AU - Lachartre, D.

AU - Lafoux, H.

AU - Lamare, P.

AU - Languillat, J. C.

AU - Laugier, D.

AU - Laugier, J. P.

AU - le Guen, Y.

AU - le Provost, H.

AU - le van Suu, A.

AU - Lemoine, L.

AU - Liotard, P. L.

AU - Loucatos, S.

AU - Magnier, P.

AU - Macelin, M.

AU - Martin, L.

AU - Massol, A.

AU - Mazeau, B.

AU - Mazure, A.

AU - Mazéas, F.

AU - McMillan, J.

AU - Millot, C.

AU - Mols, P.

AU - Montanet, F.

AU - Morel, J. P.

AU - Moscoso, L.

AU - Navas, S.

AU - Olivetto, C.

AU - Palanque-Delabrouille, N.

AU - Pallares, A.

AU - Payre, P.

AU - Perrin, P.

AU - Pohl, A.

AU - Poinsignon, J.

AU - Potheau, R.

AU - Queinec, Y.

AU - Racca, C.

AU - Raymond, M.

AU - Rolin, J. F.

AU - Sacquin, Y.

AU - Schuller, J. P.

AU - Schuster, W.

AU - Spooner, N.

AU - Stolarczyk, T.

AU - Tabary, A.

AU - Talby, M.

AU - Tao, C.

AU - Tayalati, Y.

AU - Thompson, L. F.

AU - Triay, R.

AU - Tzvetanov, T.

AU - Valdy, P.

AU - Vernin, P.

AU - Vigeolas, E.

AU - Vignaud, D.

AU - Vilanova, D.

AU - Wark, D.

AU - Zghiche, A.

AU - Zuniga, J.

PY - 2000/1/1

Y1 - 2000/1/1

N2 - The ANTARES collaboration has performed a series of in-situ measurements to study the background light for a planned undersea neutrino telescope. Such background can be caused by 40K decays or by biological activity. We report on measurements at two sites in the Mediterranean Sea at depths of 2400 m and 2700 m, respectively. Three photomultiplier tubes were used to measure single counting rates and coincidence rates for pairs of tubes at various distances. The background rate is seen to consist of three components: a constant rate due to 40K decays, a continuum rate that varies on a time scale of several hours simultaneously over distances up to at least 40 m, and random bursts a few seconds long that are only correlated in time over distances of the order of a meter. A trigger requiring coincidences between nearby photomultiplier tubes should reduce the trigger rate for a neutrino telescope to a manageable level with only a small loss in efficiency.

AB - The ANTARES collaboration has performed a series of in-situ measurements to study the background light for a planned undersea neutrino telescope. Such background can be caused by 40K decays or by biological activity. We report on measurements at two sites in the Mediterranean Sea at depths of 2400 m and 2700 m, respectively. Three photomultiplier tubes were used to measure single counting rates and coincidence rates for pairs of tubes at various distances. The background rate is seen to consist of three components: a constant rate due to 40K decays, a continuum rate that varies on a time scale of several hours simultaneously over distances up to at least 40 m, and random bursts a few seconds long that are only correlated in time over distances of the order of a meter. A trigger requiring coincidences between nearby photomultiplier tubes should reduce the trigger rate for a neutrino telescope to a manageable level with only a small loss in efficiency.

KW - 29.40.Ka

KW - 92.10.Bf

KW - 95.55.Vj

KW - Luminescence

KW - Neutrino telescope

KW - Sea water properties

KW - Undersea Cherenkov detectors

U2 - 10.1016/S0927-6505(99)00118-8

DO - 10.1016/S0927-6505(99)00118-8

M3 - Article

AN - SCOPUS:0000436090

SN - 0927-6505

VL - 13

SP - 127

EP - 136

JO - Astroparticle Physics

JF - Astroparticle Physics

IS - 2-3

ER -

Background light in potential sites for the ANTARES undersea neutrino telescope

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