Nancy Grace Roman Space Telescope Coronagraph Instrument Overview and Status
Author
Bailey, V.P.Bendek, E.
Monacelli, B.
Baker, C.
Bedrosian, G.
Cady, E.
Douglas, E.S.
Groff, T.
Hildebrandt, S.R.
Kasdin, N.J.
Krist, J.
Macintosh, B.
Mennesson, B.
Morrissey, P.
Poberezhskiy, I.
Subedi, H.B.
Rhodes, J.
Roberge, A.

Ygouf, M.
Zellem, R.T.
Zhao, F.
Zimmerman, N.T.
Affiliation
Steward Observatory, The Department of Astronomy, The University of ArizonaIssue Date
2023-10-05Keywords
circumstellar diskscoronagraphy
deformable mirrors
electron multiplying CCDs
exoplanets
high-contrast imaging
Roman Space Telescope
Metadata
Show full item recordPublisher
SPIECitation
Vanessa P. Bailey, Eduardo Bendek, Brian Monacelli, Caleb Baker, Gasia Bedrosian, Eric Cady, Ewan S. Douglas, Tyler Groff, Sergi R. Hildebrandt, N. Jeremy Kasdin, John Krist, Bruce Macintosh, Bertrand Mennesson, Patrick Morrissey, Ilya Poberezhskiy, Hari B. Subedi, Jason Rhodes, Aki Roberge, Marie Ygouf, Robert T. Zellem, Feng Zhao, Neil T. Zimmerman, "Nancy Grace Roman Space Telescope coronagraph instrument overview and status," Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126800T (5 October 2023); https://doi.org/10.1117/12.2679036Rights
© 2023 SPIE. (2023) Published by SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
The Nancy Grace Roman Space Telescope Coronagraph Instrument is a critical technology demonstrator for NASA’s Habitable Worlds Observatory. With a predicted visible-light flux ratio detection limit of 10−8 or better, it will be capable of reaching new areas of parameter space for both gas giant exoplanets and circumstellar disks. It is in the final stages of integration and test at the Jet Propulsion Laboratory, with an anticipated delivery to payload integration in the coming year. This paper will review the instrument systems, observing modes, potential observing applications, and overall progress toward instrument integration and test. © 2023 SPIE.Note
Immediate accessISSN
0277-786XISBN
978-151066574-3Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/12.2679036