14–24 Jul 2025
CICG - International Conference Centre - Geneva, Switzerland
Europe/Zurich timezone
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Performance of the SiPMs and Beta ASIC in the FIT Scintillating Fiber Tracker

Not scheduled
20m
Levels -1 & 0

Levels -1 & 0

Poster Cosmic-Ray Direct & Acceleration PO-1

Speaker

Keerthana Rajan Lathika (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain)

Description

The scintillating FIber Tracker (FIT) has been designed as a tracking detector for the upcoming High Energy cosmic-Radiation Detection (HERD) facility. The FIT combines excellent angular resolution with precise charge reconstruction measurements for cosmic-rays detection. The tracker consists of multiple tracking planes made of fiber mats, arranged in two orthogonal directions, and read out with Hamamatsu S13552-10 SiPM arrays. A custom-made ASIC, the BETA ASIC, has been developed, in order to fulfill the stringent requirements for noise, linearity, dynamic range, and power consumption of space applications.
This work reports the performance of the SiPMs and the BETA read-out system used in FIT. Our setup has been optimized, characterized, and calibrated using an LED light source. Additionally, we discuss the system’s performance in generating efficient triggers for the identification of ionizing particles.

Collaboration(s) HERD

Author

Keerthana Rajan Lathika (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain)

Co-authors

Albert Espinya (ICCUB (Department of Física Quàntica i Astrofísica, Institut de Ciències Del Cosmos, Universidad de Barcelona, E-08007, Barcelona, Spain)) Andreu Sanuy (ICCUB (Department of Física Quàntica i Astrofísica, Institut de Ciències Del Cosmos, Universidad de Barcelona, E-08007, Barcelona, Spain)) Chiara Perrina (Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Bâtiment PH, Station 3, CH-1015 Lausanne, Switzerland) Daniel Guberman (ICCUB (Department of Física Quàntica i Astrofísica, Institut de Ciències Del Cosmos, Universidad de Barcelona, E-08007, Barcelona, Spain)) David Gascon (ICCUB (Department of Física Quàntica i Astrofísica, Institut de Ciències Del Cosmos, Universidad de Barcelona, E-08007, Barcelona, Spain)) Giulio Lucchetta (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain) Javier Rico (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain) Jennifer Maria Frieden (Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Bâtiment PH, Station 3, CH-1015 Lausanne, Switzerland) Joan Mauricio (ICCUB (Department of Física Quàntica i Astrofísica, Institut de Ciències Del Cosmos, Universidad de Barcelona, E-08007, Barcelona, Spain)) Juan Boix (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain) Kimberly Sarah Keyser (Institute of Physics, Ecole Polytechnique Fédérale de Lausanne (EPFL), Bâtiment PH, Station 3, CH-1015 Lausanne, Switzerland) Laia Cardiel Sas (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain) Manel Martinez (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain) Marina Orta (ICCUB (Department of Física Quàntica i Astrofísica, Institut de Ciències Del Cosmos, Universidad de Barcelona, E-08007, Barcelona, Spain)) Oscar Blanch (Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology (BIST), E-08193 Bellaterra, Barcelona, Spain) Philipp Azzarello (Département de Physique Nucléaire et Corpusculaire (DPNC), Université de Genève, 24 quai Ernest-Ansermet, CH-1211 Genève 4, Switzerland)

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