Angelis, NicolasGascón Fora, DavidGomez, SergioHeller, MatthieuMontaruli, TeresaNagai, Andrii2024-03-082024-03-082023-01-011748-0221https://hdl.handle.net/2445/208546Large-area silicon photomultipliers (SiPMs) are desired in many applications where large surfaces have to be covered. For instance, a large area SiPM has been developed by Hamamatsu Photonics in collaboration with the University of Geneva, to equip gamma-ray cameras employed in imaging atmospheric Cherenkov telescopes. The sensor being about 1 cm2, a suitable preamplification electronics has been investigated in this work, which can deal with long pulses induced by the large capacitance of the sensor. The so-called Multiple Use SiPM Integrated Circuit (MUSIC), developed by the ICCUB (University of Barcelona), is investigated as a potential front-end ASIC, suitable to cover large area photodetection planes of gamma-ray telescopes. The ASIC offers an interesting pole-zero cancellation (PZC) that allows dealing with long SiPM signals, the feature of active summation of up to 8 input channels into a single differential output and it can offer a solution for reducing power consumption compared to discrete solutions. Measurements and simulations of MUSIC coupled to two SiPMs developed by Hamamatsu are considered and the ASIC response is characterized.15 p.application/pdfengcc-by (c) Angelis, N. et al., 2023http://creativecommons.org/licenses/by/4.0/Astronomia de raigs gammaSiliciCircuits integratsGamma ray astronomySiliconIntegrated circuitsCharacterisation of the MUSIC ASIC for large-area silicon photomultipliers for gamma-ray astronomyinfo:eu-repo/semantics/article7417742024-03-08info:eu-repo/semantics/openAccess