Simulating the WFIRST coronagraph integral field spectrograph

Simulating the WFIRST coronagraph integral field spectrograph

A primary goal of direct imaging techniques is to spectrally characterize the atmospheres of planets around other stars at extremely high contrast levels. To achieve this goal, coronagraphic instruments have favored integral field spectrographs (IFS) as the science cameras to disperse the entire sea...

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Main Authors: Cady, Eric (Author), Mejia Prada, Camilo (Author), Rizzo, Maxime J. (Author), Gong, Qian (Author), Groff, Tyler D. (Author), Krist, John E. (Author), Mandell, Avi M. (Author), McElwain, Michael W. (Author), Riggs, A. J. Eldorado (Author), Saxena, Prabal (Author), Zimmermann, Neil T. (Author), Brandt, Timothy (Author), Roberge, Aki (Contributor), Douglas, Ewan S. (Contributor), Cahoy, Kerri (Contributor)
Other Authors: Massachusetts Institute of Technology. Department of Aeronautics and Astronautics (Contributor), Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences (Contributor), Massachusetts Institute of Technology. Department of Physics (Contributor)
Format: Article
Language:English
Published: SPIE-Intl Soc Optical Eng, 2018-07-03T16:09:13Z.
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