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Dynamical Constraints on the HR 8799 Planets with GPI
UploadLessons for WFIRST CGI from ground-based high-contrast systems
UploadThe Gemini Planet Imager: looking back over five years and forward to the future
UploadGPI Spectra of HR 8799 c, d, and e from 1.5 to 2.4 μm with KLIP Forward Modeling
UploadAutomated data processing architecture for the Gemini Planet Imager Exoplanet Survey
UploadTheδScuti pulsations ofβPictoris as observed by ASTEP from Antarctica
UploadEvidence That the Directly Imaged Planet HD 131399 Ab Is a Background Star
UploadCharacterizing 51 Eri b from 1 to 5μm: A Partly Cloudy Exoplanet
UploadComplex Spiral Structure in the HD 100546 Transitional Disk as Revealed by GPI and MagAO
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