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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Bibliographic Details
Main Authors: Cady, Eric, Mejia Prada, Camilo, Rizzo, Maxime J., Gong, Qian, Groff, Tyler D., Krist, John E., Mandell, Avi M., McElwain, Michael W., Riggs, A. J. Eldorado, Saxena, Prabal, Zimmermann, Neil T., Brandt, Timothy, Roberge, Aki, Douglas, Ewan S., Cahoy, Kerri
Other Authors: Massachusetts Institute of Technology. Department of Aeronautics and Astronautics
Format: Article
Published: SPIE-Intl Soc Optical Eng 2018
Online Access:http://hdl.handle.net/1721.1/116760
https://orcid.org/0000-0002-2989-3725
https://orcid.org/0000-0002-0813-4308
https://orcid.org/0000-0002-7791-5124

Internet

http://hdl.handle.net/1721.1/116760
https://orcid.org/0000-0002-2989-3725
https://orcid.org/0000-0002-0813-4308
https://orcid.org/0000-0002-7791-5124

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