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Normalized Point Source Sensitivity for Off-Axis Optical Performance Evaluation of the Thirty Meter Telescope

机译:三十米望远镜离轴光学性能评估的归一化点源灵敏度

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The Normalized Point Source Sensitivity (PSSN) has previously been defined and analyzed as an On-Axis seeing-limited telescope performance metric. In this paper, we expand the scope of the PSSN definition to include Off-Axis field of view (FoV) points and apply this generalized metric for performance evaluation of the Thirty Meter Telescope (TMT). We first propose various possible choices for the PSSN definition and select one as our baseline. We show that our baseline metric has useful properties including the multiplicative feature even when considering Off-Axis FoV points, which has proven to be useful for optimizing the telescope error budget. Various TMT optical errors are considered for the performance evaluation including segment alignment and phasing, segment surface figures, temperature, and gravity, whose On-Axis PSSN values have previously been published by our group.
机译:归一化点源灵敏度(PSSN)先前已被定义和分析为同轴可见受限望远镜性能指标。在本文中,我们将PSSN定义的范围扩展到包括离轴视场(FoV)点,并将此通用度量应用于30米望远镜(TMT)的性能评估。我们首先为PSSN定义提出各种可能的选择,然后选择一个作为我们的基准。我们表明,即使考虑离轴FoV点,我们的基准度量标准也具有包括乘性在内的有用属性,事实证明,这对于优化望远镜误差预算非常有用。性能评估考虑了各种TMT光学误差,包括节段对齐和定相,节段表面图形,温度和重力,其轴上PSSN值先前已由我们小组发布。

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