Event Date/Time
Location
Please contact the MAE Department for the zoom information.
Series/Event Type
Direct imaging of exoplanets has rapidly matured and is now providing invaluable data that is highly complementary to other planet detection and characterization techniques. In this talk, I will discuss two direct imaging projects currently being worked on at the Space Imaging and Optical Systems Lab at Cornell University: the upgrade of the Gemini Planet Imager (GPI 2.0), and the development of the Coronagraphic Instrument (CGI) technology demonstration mission for the Nancy Grace Roman Space Telescope. GPI, a facility instrument at the Gemini South observatory, is one of the world's most advanced extreme adaptive optics coronagraphy systems, capable of spectral-polarimetric imaging of young, giant, self-luminous planets in the near-IR. Over the next two years, a large, multidisciplinary group at institutions spanning the US and Canada will work to make GPI even more sensitive and efficient, after which it will be re-commissioned at Gemini North as GPI 2.0. The Roman CGI will be the first dedicated exoplanet coronagraph on a space mission, scheduled to launch in the mid-2020s. It will initially operate as a technology demonstration, which, if successful, will be followed by a participating scientist program. I will discuss my group's work on the modeling and optimization of exoplanet imaging surveys and our advances in the control of autonomous optical systems.