Calibration systems and methods for the ANTARES neutrino telescope

TL;DR

The paper describes the calibration systems of the ANTARES neutrino telescope, demonstrating successful in situ operation and sub-nanosecond time resolution for accurate neutrino detection.

Contribution

It introduces the calibration methods for time and position measurements in the ANTARES detector, ensuring precise neutrino event reconstruction.

Findings

Calibration systems operate successfully in situ.

Time resolution reaches sub-nanosecond accuracy.

Position and orientation measurements are reliable.

Abstract

The ANTARES neutrino telescope is currently being constructed in the Mediterranean Sea. The complete detector will consist of 12 strings, supplemented by an additional instrumentation line. Nine strings are at present deployed of which five are already connected to the shore and operating. Each string is equipped with 75 Optical Modules (OMs) housing the photomultipliers to detect the Cherenkov light induced by the charged particles produced in neutrino reactions. An accurate measurement of the Cherenkov photon arrival times as well as the positions and orientations of the OMs is required for a precise reconstruction of the direction of the detected neutrinos. For this purpose the ANTARES detector is provided with several system s to facilitate the calibration of the detector. The time calibration is performed using light pulses emitted from LED and laser devices. The positioning is done via acoustic triangulation using hydrophones. Additionally, local tilt angles and the orientations of the modules are measured with a set of tiltmeters and compasses. In this paper, it is demonstrated that the ANTARES time and alignment calibration systems operate successfully in situ. In particular, it is shown that the ANTARES read-out electronics is capable of reaching a sub-nanosecond time resolution.