Poster + Paper
5 October 2023 Testing and performance of IFS upgrades for GPI 2.0
Author Affiliations +
Conference Poster
Abstract
The Gemini Planet Imager (GPI), is a facility class instrument for the Gemini Observatory with the primary goal of directly detecting young Jovian planets. After spending 2013 - 2020 at Gemini South, the instrument is currently undergoing maintenance and upgrades before its transition to Gemini North as GPI 2.0. Among the upgrades are significant changes to the Integral Field Spectrograph (IFS), including the installation of new prisms, Lyot stops/apodizers, and filters. The upgrades are expected to improve overall performance in the relevant wavelengths and angular separations needed for GPI 2.0.
(2023) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Dillon Peng, Jeffrey Chilcote, Quinn Konopacky, Randall Hamper, Joel Burke, Brian Sands, Matthew Engstrom, Abigail Karaszewski, Rebecca Boyle, Mary Anne Limbach, Alexandra Greenbaum, Anand Sivaramakrishnan, Alexa Rizika, Saavidra Perera, Clarissa Do Ó, Jayke Nguyen, Bruce Macintosh, Joeleff Fitzsimmons, Christian Marois, Fredrik Rantakyrö, Arlene Aleman, Jérôme Maire, Robert De Rosa, Emiel Por, Dmitry Savransky, Meiji Nguyen, Marshall Perrin, Remi Soummer, Laurent Pueyo, Bryony Nickson, and Eckhart Spalding "Testing and performance of IFS upgrades for GPI 2.0", Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126801Y (5 October 2023); https://doi.org/10.1117/12.2677675
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KEYWORDS
Prisms

Gemini Planet Imager

Iterated function systems

Optical filters

Spectral resolution

Design and modelling

Gemini Observatory

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