TY - JOUR
T1 - The LED calibration systems for the mDOM and D-Egg sensor modules of the IceCube Upgrade
T2 - Design, production, testing and use in module calibration
AU - Icecube Collaboration
AU - Abbasi, R.
AU - Ackermann, M.
AU - Adams, J.
AU - Agarwalla, S. K.
AU - Aguilar, J. A.
AU - Ahlers, M.
AU - Alameddine, J. M.
AU - Ali, S.
AU - Amin, N. M.
AU - Andeen, K.
AU - Argüelles, C.
AU - Ashida, Y.
AU - Athanasiadou, S.
AU - Axani, S. N.
AU - Babu, R.
AU - Bai, X.
AU - Baines-Holmes, J.
AU - Balagopal, A.
AU - Barwick, S. W.
AU - Bash, S.
AU - Basu, V.
AU - Bay, R.
AU - Beatty, J. J.
AU - Becker Tjus, J.
AU - Behrens, P.
AU - Beise, J.
AU - Bellenghi, C.
AU - Benkel, B.
AU - BenZvi, S.
AU - Berley, D.
AU - Bernardini, E.
AU - Besson, D. Z.
AU - Blaufuss, E.
AU - Bloom, L.
AU - Blot, S.
AU - Bodo, I.
AU - Bontempo, F.
AU - Book Motzkin, J. Y.
AU - Boscolo Meneguolo, C.
AU - Böser, S.
AU - Botner, O.
AU - Böttcher, J.
AU - Braun, J.
AU - Brinson, B.
AU - Brisson-Tsavoussis, Z.
AU - Burley, R. T.
AU - Butterfield, D.
AU - Campana, M. A.
AU - Carloni, K.
AU - Kiryluk, J.
N1 - Publisher Copyright:
© 2025 Institute of Physics. All rights reserved.
PY - 2025/11/1
Y1 - 2025/11/1
N2 - The IceCube Neutrino Observatory, instrumenting about 1 km3 of deep, glacial ice at the geographic South Pole, is due to be enhanced with the IceCube Upgrade. The IceCube Upgrade, to be deployed during the 2025/26 Antarctic summer season, will consist of seven new strings of photosensors, densely embedded near the bottom center of the existing array. Aside from a world-leading sensitivity to neutrino oscillations, a primary goal is the improvement of the calibration of the optical properties of the instrumented ice. This calibration will be applied to the entire archive of IceCube data, improving the angular and energy resolution of the detected neutrino events. For this purpose, the Upgrade strings include a host of new calibration devices. Aside from dedicated calibration modules, several thousand LED flashers have been incorporated into the photosensor modules. We describe the design, production, and testing of these LED flashers before their integration into the sensor modules as well as the use of the LED flashers during lab testing of assembled sensor modules.
AB - The IceCube Neutrino Observatory, instrumenting about 1 km3 of deep, glacial ice at the geographic South Pole, is due to be enhanced with the IceCube Upgrade. The IceCube Upgrade, to be deployed during the 2025/26 Antarctic summer season, will consist of seven new strings of photosensors, densely embedded near the bottom center of the existing array. Aside from a world-leading sensitivity to neutrino oscillations, a primary goal is the improvement of the calibration of the optical properties of the instrumented ice. This calibration will be applied to the entire archive of IceCube data, improving the angular and energy resolution of the detected neutrino events. For this purpose, the Upgrade strings include a host of new calibration devices. Aside from dedicated calibration modules, several thousand LED flashers have been incorporated into the photosensor modules. We describe the design, production, and testing of these LED flashers before their integration into the sensor modules as well as the use of the LED flashers during lab testing of assembled sensor modules.
KW - Analogue electronic circuits; Detector alignment and calibration methods (lasers, sources, particle-beams)
KW - Instrumentation
KW - methods for time-of-flight (TOF) spectroscopy
UR - https://www.scopus.com/pages/publications/105034905558
U2 - 10.1088/1748-0221/20/11/P11026
DO - 10.1088/1748-0221/20/11/P11026
M3 - Article
AN - SCOPUS:105034905558
SN - 1748-0221
VL - 20
JO - Journal of Instrumentation
JF - Journal of Instrumentation
IS - 11
M1 - P11026
ER -