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

机译:三十米望远镜的离轴光学成本评估的归一化点源极灵敏度

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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:预先定义了归一化点源极灵敏度(PSSN),并分析为轴上的望远镜性能度量。在本文中,我们扩展了PSSN定义的范围,以包括轴外视野(FOV)点,并应用该广义度量,以进行三十米望远镜(TMT)的性能评估。我们首先提出了PSSN定义的各种可能选择,并选择一个作为我们的基线。我们表明,我们的基线度量标准具有有用的属性,包括乘法特征,即使在考虑轴上的FOV点时,也可以证明可以用于优化望远镜错误预算。考虑各种TMT光学误差用于性能评估,包括段对准和分阶段,段表面图,温度和重力,其在轴上PSSN值以前由我们的组发布。

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