论文标题

伽马射线天文学的大面积硅光电层流的音乐表征

Characterisation of the MUSIC ASIC for large-area silicon photomultipliers for gamma-ray astronomy

论文作者

De Angelis, Nicolas, Gascón, David, Gómez, Sergio, Heller, Matthieu, Montaruli, Teresa, Nagai, Andrii

论文摘要

在必须覆盖大型表面的许多应用中,都需要大面积硅光电层流(SIPM)。例如,Hamamatsu Photonics与日内瓦大学合作开发了大面积的SIPM,以配备用于成像大气Cherenkov望远镜中的伽马射相机。作为传感器约1厘米$^2 $,已经在这项工作中研究了合适的前置电子设备,可以处理传感器的较大电容引起的长脉冲。由ICCUB(巴塞罗那大学)开发的所谓多重用途SIPM集成电路(音乐)被研究为潜在的前端ASIC,适合覆盖伽马射线望远镜的大面积光检测平面。 ASIC提供了有趣的极点取消(PZC),该取消(PZC)允许处理长长的SIPM信号,该信号的功能最多可将8个输入通道求和到单个微分输出中,并且与离散解决方案相比,它可以为减少功耗提供解决方案。考虑了对Hamamatsu开发的两个sipms的音乐的测量和模拟,并表征了ASIC响应。 5 $^{th} $低横切技术的发电传感器与音乐结合起来是伽马射相机的一个很好的解决方案。

Large-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. Being the sensor about 1 cm$^2$, 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. The 5$^{th}$ generation sensor of the Low Cross Talk technology coupled to MUSIC turns out to be a good solution for gamma-ray cameras.

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