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arXiv 2608.24333astro-ph.IMastro-ph.EPastro-ph.SR

采用纳米打印PIAACMC相位掩模的亚衍射极限日冕成像

Sub-diffraction-limited coronagraphic imaging with nano-printed PIAACMC phase masks

Elena Tonucci, Sebastiaan Y. Haffert, Warren B. Foster, Jared R. Males, Olivier Guyon, Laird M. Close, Kyle van Gorkom, Alexander D. Hedglen, Parker T. Johnson,… 展开作者

Elena Tonucci, Sebastiaan Y. Haffert, Warren B. Foster, Jared R. Males, Olivier Guyon, Laird M. Close, Kyle van Gorkom, Alexander D. Hedglen, Parker T. Johnson, Maggie Y. Kautz, Jay K. Kueny, Rico Landman, Jialin Li, Joshua Liberman, Joseph D. Long, Miles Lucas, Jennifer Lumbres, Matthijs Mars, Eden A. McEwen, Avalon McLeod, Tiffany Nguyen, Logan A. Pearce, María Eugenia Redondo González, Lauren Schatz, Katie Twitchell

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中文总结 AI 辅助

该研究采用纳米打印PIAACMC相位掩模,在麦哲伦望远镜的MagAO-X仪器上实现亚衍射极限日冕成像,探测到特定角距的双星伴星,验证了PIAACMC的相关观测能力。

中文摘要 AI 辅助

在其宿主恒星宜居带内成像类地系外行星,是未来地基和空间天文台的主要科学目标之一。然而,当前技术无法达到成像此类行星所需的极高对比度和小角距。相位诱导振幅切趾复合掩模日冕仪(PIAACMC)是实现该目标的一种有前景的日冕仪。PIAACMC采用一组非球面透镜对入射光瞳进行切趾且无通量损失,并使用移相焦平面掩模抑制恒星光,这些特性使其能保持高通量并实现小内工作角(IWA),具备在衍射极限下观测系外行星的能力。该掩模由莱顿大学使用Nanoscribe(一种采用双光子聚合实现亚微米高度精度的微3D打印机)内部制造。我们展示了智利拉斯坎帕纳斯天文台6.5米麦哲伦克莱望远镜的麦哲伦极端自适应光学系统(MagAO-X)仪器上PIAACMC焦平面掩模的首批科学结果,呈现了中心波长908纳米、带宽14%的宽带z'滤光片的实验室和实测对比度曲线。我们使用PIAACMC探测到角距约0.8-5λ/D(约23-144毫角秒)的双星伴星,证明了PIAACMC在亚λ/D IWA下于衍射极限及以下进行观测的能力。未来工作包括探索新型掩模设计以提升宽带光中的对比度,并开展主动焦平面波前传感与控制。

英文摘要

Imaging Earth-like exoplanets in the habitable zone of their host star is among the main science objectives of future ground-based and space-based observatories. However, the extreme contrast and small separations needed to image such planets cannot be reached with current technology. The Phase-Induced Amplitude Apodization Complex Mask Coronagraph (PIAACMC) is a promising coronagraph to reach this goal. The PIAACMC uses a set of aspheric lenses to apodize the entrance pupil without throughput losses and a phase-shifting focal plane mask for starlight suppression. These allow us to maintain high throughput and achieve a small inner-working angle (IWA), unlocking the capability to observe exoplanets at the diffraction limit. The masks are manufactured in-house at Leiden University with Nanoscribe, a micro-3D-printer that uses two-photon polymerization to achieve sub-micron precision in height. We present the first scientific results with a focal plane mask for the PIAACMC on the Magellan Adaptive Optics eXtreme (MagAO-X) instrument for the 6.5-meter Magellan Clay telescope at Las Campanas Observatory, Chile. We show laboratory and on-sky contrast curves with a broadband z' filter centered at 908 nm with a 14% bandwidth. We use the PIAACMC to detect binary companions at separations ~0.8-5 lambda/D (~23-144 mas). This demonstrates the PIAACMC's capability to observe at the diffraction limit and below, with a sub-lambda/D IWA. Future work includes exploring new mask designs to improve the contrast in broadband light and performing active focal plane wavefront sensing and control.

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