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  • 标题:The Single-mode Complex Amplitude Refinement (SCAR) coronagraph
  • 其他标题:I. Concept, theory, and design
  • 本地全文:下载
  • 作者:E. H. Por ; S. Y. Haffert
  • 期刊名称:Astronomy & Astrophysics
  • 印刷版ISSN:0004-6361
  • 电子版ISSN:1432-0746
  • 出版年度:2020
  • 卷号:635
  • 页码:1-13
  • DOI:10.1051/0004-6361/201731616
  • 语种:English
  • 出版社:EDP Sciences
  • 摘要:Context.The recent discovery of an Earth-mass exoplanet around the nearby star Proxima Centauri provides a prime target for the search for life on planets outside our solar system. Atmospheric characterization of these planets has been proposed by blocking the starlight with a stellar coronagraph and using a high-resolution spectrograph to search for reflected starlight off the planet.Aims.Due to the large flux ratio and small angular separation between Proxima b and its host star (≲10−7and ≲2.2λ/Drespectively; at 750 nm for an 8 m-class telescope) the coronagraph requires high starlight suppression at extremely-low inner working angles. Additionally, it must operate over a broad spectral bandwidth and under residual telescope vibrations. This allows for efficient use of spectroscopic post-processing techniques. We aim to find the global optimum of an integrated coronagraphic integral-field spectrograph.Methods.We present the Single-mode Complex Amplitude Refinement (SCAR) coronagraph that uses a microlens-fed single-mode fiber array in the focal plane downstream from a pupil-plane phase plate. The mode-filtering property of the single-mode fibers allows for the nulling of starlight on the fibers. The phase pattern in the pupil plane is specifically designed to take advantage of this mode-filtering capability. Second-order nulling on the fibers expands the spectral bandwidth and decreases the tip-tilt sensitivity of the coronagraph.Results.The SCAR coronagraph has a low inner working angle (∼1λ/D) at a contrast of < 3 × 10−5for the six fibers surrounding the star using a sufficiently-good adaptive optics system. It can operate over broad spectral bandwidths (∼20%) and delivers high throughput (> 50% including fiber injection losses). Additionally, it is robust against tip-tilt errors (∼0.1λ/Drms). We present SCAR designs for both an unobstructed and a VLT-like pupil.Conclusions.The SCAR coronagraph is a promising candidate for exoplanet detection and characterization around nearby stars using current high-resolution imaging instruments.
  • 关键词:eninstrumentation: high angular resolutiontechniques: high angular resolutionmethods: numerical
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