当前与未来地基及天基望远镜高对比度成像系统综述 II. 共路波前传感/控制与相干差分成像
天体物理仪器与方法
2018-07-19 v1
摘要
2017年9月在荷兰莱顿洛伦兹中心举行的最优光学日冕仪(OOC)研讨会聚集了25位从事系外行星仪器研究的多元化研究人员，以激发新思想的产生与共享。在总结OOC研讨会成果的三篇系列论文的第二篇中（另见~\citenum{ruane2018,snik2018}），我们概述了共路波前传感/控制与相干差分成像技术，突出了最新结果，并揭示了它们各自的优缺点。我们为该领域布局了关键里程碑，旨在增强未来的地基/天基高对比度成像平台。此类技术将有助于弥合在空间中围绕G型恒星以反射光成像位于可保留液态水的宜居带内类地行星所需的巨大对比度鸿沟。
引用
@article{arxiv.1807.07043,
title = {Review of high-contrast imaging systems for current and future ground-based and space-based telescopes II. Common path wavefront sensing/control and Coherent Differential Imaging},
author = {Nemanja Jovanovic and Olivier Absil and Pierre Baudoz and Mathilde Beaulieu and Michael Bottom and Eric Cady and Brunella Carlomagno and Alexis Carlotti and David Doelman and Kevin Fogarty and Raphael Galicher and Olivier Guyon and Sebastiaan Haffert and Elsa Huby and Jeffrey Jewell and Christoph Keller and Matthew A. Kenworthy and Justin Knight and Jonas Kuhn and Kelsey Miller and Johan Mazoyer and Mamadou N'Diaye and Emiel Por and Laurent Pueyo and A J Eldorado Riggs and Garreth Ruane and Dan Sirbu and Frans Snik and J. Kent Wallace and Michael Wilby and Marie Ygouf},
journal= {arXiv preprint arXiv:1807.07043},
year = {2018}
}
备注
18 pages, 9 figures