Paper
11 July 2008 The Gemini Planet Imager: from science to design to construction
Author Affiliations +
Abstract
The Gemini Planet Imager (GPI) is a facility instrument under construction for the 8-m Gemini South telescope. It combines a 1500 subaperture AO system using a MEMS deformable mirror, an apodized-pupil Lyot coronagraph, a high-accuracy IR interferometer calibration system, and a near-infrared integral field spectrograph to allow detection and characterization of self-luminous extrasolar planets at planet/star contrast ratios of 10-7. I will discuss the evolution from science requirements through modeling to the final detailed design, provide an overview of the subsystems and show models of the instrument's predicted performance.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
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Cited by 208 scholarly publications.
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KEYWORDS
Gemini Planet Imager

Adaptive optics

Planets

Coronagraphy

Wavefronts

Gemini Observatory

Stars

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