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Characterisation and testing of CHEC-M-A camera prototype for the small-sized telescopes of the Cherenkov telescope array

机译:切伦科夫望远镜阵列小型望远镜的CHEC-M-A相机原型的特性测试

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摘要

The Compact High Energy Camera (CHEC) is a camera design for the Small-Sized Telescopes (SSTs; 4 m diameter mirror) of the Cherenkov Telescope Array (CTA). The SSTs are focused on very-high-energyγ-ray detection via atmospheric Cherenkov light detection over a very large area. This implies many individual units and hence cost-effective implementation, as well as shower detection at large impact distance, and hence large field of view (FoV), and efficient image capture in the presence of large time gradients in the shower image detected by the camera. CHEC relies on dual-mirror optics to reduce the plate-scale and make use of 6 × 6 mm2pixels, leading to a low-cost (∼150 k€), compact (0.5 m × 0.5 m), and light (∼45 kg) camera with 2048 pixels providing a camera FoV of∼9 degrees. The CHEC electronics are based on custom TARGET (TeV array readout with GSa/s sampling and event trigger) application-specific integrated circuits (ASICs) and field programmable gate arrays (FPGAs) sampling incoming signals at a gigasample per second, with flexible camera-level triggering within a single backplane FPGA. CHEC is designed to observe in theγ-ray energy range of 1–300 TeV, and at impact distances up to∼500 m. To accommodate this and provide full flexibility for later data analysis, full waveforms with 96 samples for all 2048 pixels can be read out at rates up to∼900 Hz. The first prototype, CHEC-M, based on multi-anode photomultipliers (MAPMs) as photosensors, was commissioned and characterised in the laboratory and during two measurement campaigns on a telescope structure at the Paris Observatory in Meudon. In this paper, the results and conclusions from the laboratory and on-site testing of CHEC-M are presented. They have provided essential input on the system design and on operational and data analysis procedures for a camera of this type. A second full-camera prototype based on Silicon photomultipliers (SiPMs), addressing the drawbacks of CHEC-M identified during the first prototype phase, has already been built and is currently being commissioned and tested in the laboratory.
机译:紧凑型高能相机(CHEC)是为Cherenkov望远镜阵列(CTA)的小型望远镜(SST;直径为4 m的镜子)设计的相机。 SST专注于通过很大面积上的大气Cherenkov光检测进行非常高能量的γ射线检测。这意味着需要很多独立的单元,因此具有成本效益,并且在较大的冲击距离下进行淋浴检测,因此在较大的视场(FoV)下进行拍摄,并且在由淋浴器检测到的淋浴图像中存在较大时间梯度的情况下,可以有效捕获图像。相机。 CHEC依靠双镜光学元件来减小板块尺寸并使用6×6 mm2像素,从而实现了低成本(〜150 k€),紧凑型(0.5 m×0.5 m)和轻型(〜45 kg) )2048像素的相机,可提供约9度的相机FoV。 CHEC电子产品基于定制的TARGET(具有GSa / s采样和事件触发功能的TeV阵列读数),专用集成电路(ASIC)和现场可编程门阵列(FPGA),以每秒千兆采样的速率采样输入信号,并具有灵活的摄像头-单个背板FPGA中的电平触发。 CHEC设计用于在1–300 TeV的γ射线能量范围内观察,并且冲击距离最远约为500 m。为了适应这种情况并为以后的数据分析提供完全的灵活性,可以以高达〜900 Hz的速率读取所有2048个像素的96个样本的完整波形。第一个原型是基于多阳极光电倍增管(MAPMs)作为光传感器的CHEC-M,已在实验室以及Meudon巴黎天文台的望远镜结构的两次测量活动中进行调试和表征。本文介绍了CHEC-M实验室和现场测试的结果和结论。他们为这类摄像机的系统设计以及操作和数据分析程序提供了重要的信息。解决基于第一个原型阶段发现的CHEC-M缺点的第二个基于硅光电倍增管(SiPM)的全相机原型已经建立,目前正在实验室中进行调试和测试。

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