Combination of apodized pupil and phase mask coronagraph for SCExAO at Subaru Telescope
Author
Nishikawa, J.Murakami, N.
Lozi, J.
Guyon, O.
Habu, K.
Ichien, H.
Yoneta, K.
Sudo, S.
Kumaki, K.
Kumagaih, S.
Jovanovic, N.
Martinache, F.
Affiliation
Steward Observatory, University of ArizonaCollege of Optical Sciences, University of Arizona
Issue Date
2020
Metadata
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SPIECitation
Nishikawa, J., Murakami, N., Lozi, J., Guyon, O., Habu, K., Ichien, H., Yoneta, K., Sudo, S., Kumaki, K., Kumagaih, S., Jovanovic, N., & Martinache, F. (2020). Combination of apodized pupil and phase mask coronagraph for SCExAO at Subaru Telescope. Proceedings of SPIE - The International Society for Optical Engineering, 11447.Rights
Copyright © 2021 SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Subaru telescope has been operating a high-contrast imaging instruments called Subaru coronagraphic extreme adaptive optics (SCExAO) which is used for exoplanet research. We are developing phase mask coronagraphs using photonic crystal wave plates inside the SCExAO. An eight-octant phase mask (8OPM) of three-layer achromatic structure has been fabricated as a second generation. It was designed for J and H band to reach 10-5 contrast, and Ks band to 10-4. A retardation and a coronagraphic performance of the 8OPM were confirmed almost as designed at 1550nm. An apodised (binary shaped) pupil to be used with the 8OPM was also studied to suppress diffracted light by the secondary shadow and spiders. We confirmed a performance of the combination of the apodizer and the 8OPM at visible wavelengths in a lab. We optimized the apodizer for a pupil of the SCExAO where we obtained a transmission of 50 % and a contrast of 10-4 at the center and 10-6 at outer region. We manufactured the designed apodizer to be installed in SCExAO for infrared observations. © 2020 SPIENote
Immediate accessISSN
0277-786XISBN
9781510636811Version
Final published versionae974a485f413a2113503eed53cd6c53
10.1117/12.2560839
