Time calibration of the ANTARES neutrino telescope
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Time calibration of the ANTARES neutrino telescope

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Time calibration of the ANTARES neutrino telescope

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ANTARES Collaboration; Aguilar Sánchez, Juan Antonio; Bigongiari, C.; Dornic, Damien; Emanuele, U.; Gómez González, Juan Pablo; Hernández Rey, Juan José Perfil; Mangano, Salvatore; Salesa Greus, Francisco; Toscano, S.; Yepes Ramírez, Harold; Zornoza Gómez, Juan de Dios Perfil; Zúñiga Román, Juan
Aquest document és un/a article, creat/da en: 2011
The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of similar to 1 ns. The methods developed to attain this level of precision are described.

    ANTARES Collaboration Aguilar Sánchez, Juan Antonio Bigongiari, C. Dornic, Damien Emanuele, U. Gómez González, Juan Pablo Hernández Rey, Juan José Mangano, Salvatore Salesa Greus, Francisco Toscano, S. Yepes Ramírez, Harold Zornoza Gómez, Juan de Dios Zúñiga Román, Juan 2011 Time calibration of the ANTARES neutrino telescope Astroparticle Physics 34 7 539 549
http://dx.doi.org/10.1016/j.astropartphys.2010.12.004
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