GPI 2.0: Optical Designs for the Upgrade of the Gemini Planet Imager Coronagraphic system
Meiji M. Nguyen, Bryony F. Nickson, Emiel H. Por, Remi Soummer, John, G. Hagopian, Bruce Macintosh, Jeffrey Chilcote, Laurent Pueyo, Marshall, Perrin, Quinn Konopacky

TL;DR
This paper presents new optical designs for the GPI 2.0 upgrade, improving contrast and throughput of the coronagraph system using an optimization software, preparing for on-sky deployment in 2023.
Contribution
The paper introduces novel apodizer and Lyot stop designs for GPI 2.0, utilizing a new optimization software to enhance performance metrics.
Findings
Achieved better raw contrast at the dark zone's inner working angle.
Improved core throughput while maintaining robustness to misalignment.
Designs are ready for on-sky use in 2023.
Abstract
The Gemini Planet Imager (GPI) is an integral field spectrograph (IFS) and coronagraph that is one of the few current generation instruments optimized for high-contrast direct imaging of substellar companions. The instrument is in the process of being upgraded and moved from its current mount on the Gemini South Observatory in Cerro Pachon, Chile, to its twin observatory, Gemini North, on Mauna Kea (a process colloquially dubbed 'GPI 2.0'). We present the designs that have been developed for the part of GPI 2.0 that pertains to upgrading various optical components of the GPI coronagraphic system. More specifically, we present new designs for the apodizer and Lyot stop (LS) that achieve better raw contrast at the inner working angle of the dark zone as well as improved core throughput while retaining a similar level of robustness to LS misalignment. To generate these upgraded designs, we…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsStellar, planetary, and galactic studies · Astro and Planetary Science · Astronomy and Astrophysical Research
