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Euclid end-to-end straylight performance assessment

机译:Euclid端到端杂散光性能评估

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In the Euclid mission the straylight has been identified at an early stage as the main driver for the final imaging quality of the telescope. The assessment by simulation of the final straylight in the focal plane of both instruments in Euclid's payload have required a complex workflow involving all stakeholders in the mission, from industry to the scientific community. The straylight is defined as a Normalized Detector Irradiance (NDI) which is a convenient definition tool to separate the contributions of the telescope and of the instruments. The end-to-end straylight of the payload is then simply the sum of the NDIs of the telescope and of each instrument. The NDIs for both instruments are presented in this paper for photometry and spectrometry.
机译:在Euclid任务中,杂散光在早期被确定为望远镜最终成像质量的主要驱动力。通过对欧几里得有效载荷中两种仪器焦平面上最终杂散光的仿真评估,需要一个复杂的工作流程,涉及任务的所有利益相关者,从工业界到科学界。杂散光被定义为归一化探测器辐照度(NDI),这是一种方便的定义工具,可以将望远镜和仪器的贡献分开。因此,有效载荷的端到端杂散光只是望远镜和每种仪器的NDI的总和。本文介绍了两种仪器的NDI,用于光度法和光谱法。

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