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WST探测器基础设施的概念架构

Conceptual architecture of the detector infrastructure for WST

A. Meoli, O. Iwert, E. George, O. Squalli, M. Richerzhagen, A. Rüde, M. Seidel, S. Lévêque

arXiv 2608.00734首次发表:更新:

AI 中文总结

本文针对需大量探测器的12米WST,提出含系统级、配电及数据处理的探测器控制器与基础设施概念架构,勾勒出基于近探测器模块化单元和网络化后端电子的分布式控制器架构。

AI 中文摘要

广角光谱望远镜(Wide-field Spectroscopic Telescope, WST)是拟议中的12米广角光谱设施,它结合了多个多目标摄谱仪,需要数量空前的探测器。本文针对WST所需的大量探测器,提出了探测器控制器及基础设施的概念架构,重点关注系统级、配电及相关数据处理,还考虑了这些要素在该设施预期开发周期内的演变。基于问题规模,我们勾勒出一种可能的分布式探测器控制器架构,该架构基于靠近探测器的模块化单元和网络化后端电子设备构建。

英文摘要

The Wide-field Spectroscopic Telescope (WST) is a proposed 12 m wide-field spectroscopic facility combining several multi-object spectrographs. It requires a yet unprecedented number of detectors. In this paper we present conceptual architecture for the detector controller and infrastructure required to operate a large number of detectors, potentially applicable to WST, focusing on the system-level, power distribution, and the associated data handling. We also consider how these elements may evolve over the expected development timeline of such a facility. Motivated by the scale of the problem, we outline a possible distributed detector-controller architecture, based on modular units placed close to the detectors and networked backend electronics.

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