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Phase-mask coronagraph holds the ability to detect exoplanets very close to their parent star. We report a new kind of phase mask that performs the contrast ratio of more than the tenth power of 10 for a circular aperture with shades of a secondary mirror and spiders. The phase distribution of the phase mask is numerically obtained by making the leaked light distribute outside the transparent part of the pupil. We applied the hybrid input-output algorithm, one of phase retrieval methods, to find the phase distribution of the phase mask. We show the characteristics of thus obtained phase mask.
Conference Title : Techniques and Instrumentation for Detection of Exoplanets VII
Conference Chair : Stuart Shaklan
Place : San Diego, California, United States
Date : August 09, 2015
収録刊行物
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- Proceedings of SPIE - the International Society for Optical Engineering
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Proceedings of SPIE - the International Society for Optical Engineering 9605 2015
Society of Photo-optical Instrumentation Engineers
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詳細情報 詳細情報について
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- CRID
- 1050574047083895680
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- NII論文ID
- 120006671845
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- NII書誌ID
- AA10619755
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- HANDLE
- 10258/3841
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- ISSN
- 0277786X
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- 本文言語コード
- en
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- 資料種別
- conference paper
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- データソース種別
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- IRDB
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