Simulation of the final image produced by GPI. A bright star is observed, but the light is greatly diminished due to the adaptive optics system and coronagraph. A faint point of light (circled) simulates the existence of a planet near the star.


Publications


2008

Graham, J.R., Macintosh, B., Doyon, R. et al. 2008, Ground-based direct detection of exoplanets with the Gemini Planet Imager (GPI), B.A.A.S. , in press -- abstract -- poster

Soummer, R., Sivaramkrishnan, A., Oppenheimer B.R. et al. 2008, The Gemini Planet Imager: Coronagraph design & testbed, B.A.A.S. , in press -- pdf


2007

Graham, J. R., Macintosh, B., Doyon, R., et al., 2007, Ground-based direct detection of exoplanets with the Gemini Planet Imager (GPI), Exoplanet Task Force White Paper, http://arxiv.org/abs/0704.1454 -- pdf

Jensen, J. 2007, New Instrumentation for the Gemini Telescopes, Gemini Focus Newsletter (June), pp. 6 - 12 -- pdf




2006

Macintosh, B., Graham, J. R., Palmer, D., et al. 2006, The Gemini Planet Imager, Advances in Adaptive Optics II, Proc. of SPIE Vol 672 (eds. B. L. Ellerbroek and D. B. Calia), pp. 62720L -- pdf

Macintosh, B. and Graham, J. R., 2006, The Gemini Planet Imager, Gemini Focus Newsletter (December), pp. 73 - 76 -- pdf