Gemini planet imager 2.0: implementing a Zernike wavefront sensor for non-common path aberrations measurement-Reference-Cited by-同舟云学术

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Gemini planet imager 2.0: implementing a Zernike wavefront sensor for non-common path aberrations measurement

Published:2023-10-05 Issue: Volume: Page:
ISSN:
Container-title:Techniques and Instrumentation for Detection of Exoplanets XI
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Author:

Chambouleyron Vincent,Salama Maissa,Guthery Charlotte,Perera Saavi,Konopacky Quinn,Véran Jean-Pierre,Savransky Dmitry,Chilcote Jeffrey K.,Wallace Kent,Dillon Daren,Jensen-Clem Rebecca,Macintosh Bruce

Publisher

SPIE

Reference9 articles.

1. GPI 2.0: pyramid wavefront sensor status;Perera,2022

2. GPI 2.0: Optical Designs for the upgrade of the Gemini Planet Imager coronagraphic system

3. GPI 2.0: Upgrades to the IFS including new spectral modes

4. The Santa Cruz Extreme AO Lab (SEAL): design and first light;Jensen-Clem,2021

5. First light of the gemini planet imager;Macintosh,2014

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Keck Primary Mirror Closed-loop Segment Control Using a Vector-Zernike Wavefront Sensor;The Astrophysical Journal;2024-05-30

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