Abstract
The Gemini Planet Imager is an instrument designed for the Gemini South Telescope to image young Jupiter-mass planets in the infrared. To achieve the high contrast needed for this, it employs an apodized pupil Lyot coronagraph (APLC) to remove most of the starlight. Current designs use a partially transmitting apodizer in the pupil; we examine the use of binary apodizations in the form of star-shaped pupils and present a design that could achieve comparable performance, along with a series of design guidelines for creating shaped pupil versions of APLCs in other systems.
Original language | English (US) |
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Pages (from-to) | 938-943 |
Number of pages | 6 |
Journal | Astrophysical Journal |
Volume | 698 |
Issue number | 1 |
DOIs | |
State | Published - 2009 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science
Keywords
- Instrumentation: high angular resolution
- Planetary systems