Characterisation of the Hamamatsu photomultipliers for the KM3NeT Neutrino Telescope
Characterisation of the Hamamatsu photomultipliers for the KM3NeT Neutrino Telescope
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KM3NeT 中微子望远镜滨松光电倍增管的表征
DOI：
10.1088/1748-0221/13/05/p05035
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发表时间：
2018
影响因子：
1.3
通讯作者：
J. Zúñiga
中科院分区：
文献类型：
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作者：
S. Aiello;S. E. Akrame;F. Ameli;E. Anassontzis;M. André;G. Androulakis;M. Anghinolfi;G. Anton;M. Ardid;J. Aublin;T. Avgitas;M. Baars;C. Bagatelas;G. Barbarino;B. Baret;J. Barrios;A. Belias;E. Berbee;A. Berg;V. Bertin;S. Biagi;A. Biagioni;C. Biernoth;R. Bormuth;J. Boumaaza;S. Bourret;M. Bouwhuis;C. Bozza;H. Brânzaş;N. Briukhanova;R. Bruijn;J. Brunner;E. Buis;R. Buompane;J. Busto;D. Calvo;A. Capone;L. Caramete;S. Celli;M. Chabab;S. Cherubini;V. Chiarella;T. Chiarusi;M. Circella;R. Cocimano;J. Coelho;A. Coleiro;M. C. Molla;R. Coniglione;P. Coyle;A. Creusot;G. Cuttone;A. D'Onofrio;R. Dallier;C. Sio;I. Palma;A. Díaz;C. Distefano;A. Domi;R. Donà;C. Donzaud;D. Dornic;M. Dörr;M. Durocher;T. Eberl;D. Eijk;I. Bojaddaini;D. Elsaesser;A. Enzenhöfer;G. Ferrara;L. Fusco;T. Gál;F. Garufi;S. Gauchery;S. Geißelsöder;L. Gialanella;E. Giorgio;A. Giuliante;S. Gozzini;R. G. Ruiz;K. Graf;D. Grasso;T. Grégoire;G. Grella;S. Hallmann;H. Haren;T. Heid;A. Heijboer;A. Hekalo;J. Hernández;J. Hofestädt;G. Illuminati;C. James;M. Jongen;B. Jongewaard;M. Jong;P. Jong;M. Kadler;P. Kalaczyński;O. Kalekin;U. Katz;N. R. K. Chowdhury;G. Kieft;D. Kiessling;E. Koffeman;P. Kooijman;A. Kouchner;M. Kreter;V. Kulikovskiy;R. Lahmann;R. Breton;F. Leone;E. Leonora;G. Levi;M. Lincetto;A. Lonardo;F. Longhitano;M. Lotze;S. Loucatos;G. Maggi;J. Mańczak;K. Mannheim;A. Margiotta;A. Marinelli;C. Markou;L. Martin;J. Martínez;A. Martini;F. Marzaioli;R. Mele;K. Melis;P. Migliozzi;E. Migneco;P. Mijakowski;L. S. Miranda;C. Mollo;M. Morganti;M. Moser;A. Moussa;R. Muller;M. Musumeci;L. Nauta;S. Navas;C. Nicolau;C. Nielsen;Mukharbek Organokov;A. Orlando;V. Panagopoulos;G. Papalashvili;R. Papaleo;G. Pǎvǎlaş;G. Pellegrini;C. Pellegrino;J. P. Romero;M. Perrin;P. Piattelli;K. Pikounis;O. Pisanti;C. Poirè;G. Polydefki;G. Poma;V. Popa;M. Post;T. Pradier;G. Pühlhofer;S. Pulvirenti;L. Quinn;F. Raffaelli;N. Randazzo;S. Razzaque;D. Real;L. Resvanis;J. Reubelt;G. Riccobene;M. Richer;A. Rovelli;I. Salvadori;D. Samtleben;A. S. Losa;M. Sanguineti;A. Santangelo;P. Sapienza;B. Schermer;V. Sciacca;J. Seneca;I. Sgura;R. Shanidze;A. Sharma;F. Simeone;A. Sinopoulou;B. Spisso;M. Spurio;D. Stavropoulos;J. Steijger;S. Stellacci;B. Strandberg;D. Stransky;T. Stüven;M. Taiuti;F. Tatone;Y. Tayalati;E. Tenllado;T. Thakore;P. Timmer;A. Trovato;S. Tsagkli;E. Tzamariudaki;D. Tzanetatos;C. Valieri;B. Vallage;V. Elewyck;F. Versari;S. Viola;D. Vivolo;M. Volkert;L. D. Waardt;J. Wilms;E. Wolf;D. Zaborov;J. Zornoza;J. Zúñiga
滨松R12199-02 3英寸光电倍增管是KM 3 NeT中微子望远镜第一阶段的光电探测器。大约7000个光电倍增管已被表征为暗计数率，定时扩展和假脉冲。量子效率，增益和峰谷比也已被测量的子样本，以确定所需的参数值作为输入的检测器的数值模拟。
The Hamamatsu R12199-02 3-inch photomultiplier tube is the photodetector chosen for the first phase of the KM3NeT neutrino telescope. About 7000 photomultipliers have been characterised for dark count rate, timing spread and spurious pulses. The quantum efficiency, the gain and the peak-to-valley ratio have also been measured for a sub-sample in order to determine parameter values needed as input to numerical simulations of the detector.