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High-Contrast Testbeds for Future Space-Based Direct Imaging Exoplanet Missions

Mazoyer, Johan and Baudoz, Pierre and Belikov, Ruslan and Crill, Brendan and Fogarty, Kevin and Galicher, Raphael and Groff, Tyler and Guyon, Olivier and Juanola-Parramon, Roser and Kasdin, Jeremy and Leboulleux, Lucie and Llop Sayson, Jorge and Mawet, Dimitri and Prada, Camilo Mejia and Mennesson, Bertrand and N'Diaye, Mamadou and Perrin, Marshall and Pueyo, Laurent and Roberge, Aki and Ruane, Garreth and Serabyn, Eugene and Shaklan, Stuart and Siegler, Nicholas and Sirbu, Dan and Soummer, Remi and Stark, Chris and Trauger, John and Zimmerman, Neil (2019) High-Contrast Testbeds for Future Space-Based Direct Imaging Exoplanet Missions. Astro2020 APC White Paper, . (Unpublished) https://resolver.caltech.edu/CaltechAUTHORS:20191126-132654179

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Abstract

Instrumentation techniques in the field of direct imaging of exoplanets have greatly advanced over the last two decades. Two of the four NASA-commissioned large concept studies involve a high-contrast instrument for the imaging and spectral characterization of exo-Earths from space: LUVOIR and HabEx. This whitepaper describes the status of 8 optical testbeds in the US and France currently in operation to experimentally validate the necessary technologies to image exo-Earths from space. They explore two complementary axes of research: (i) coronagraph designs and manufacturing and (ii) active wavefront correction methods and technologies. Several instrument architectures are currently being analyzed in parallel to provide more degrees of freedom for designing the future coronagraphic instruments. The necessary level of performance has already been demonstrated in-laboratory for clear off-axis telescopes (HabEx-like) and important efforts are currently in development to reproduce this accomplishment on segmented and/or on-axis telescopes (LUVOIR-like) over the next two years.


Item Type:Report or Paper (White Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1907.09508arXivDiscussion Paper
ORCID:
AuthorORCID
Mazoyer, Johan0000-0002-9133-3091
Crill, Brendan0000-0002-4650-8518
Fogarty, Kevin0000-0002-2691-2476
Mawet, Dimitri0000-0002-8895-4735
Mennesson, Bertrand0000-0003-4205-4800
N'Diaye, Mamadou0000-0002-1721-3294
Ruane, Garreth0000-0003-4769-1665
Soummer, Remi0000-0003-2753-2819
Additional Information:© 2019. Johan Mazoyer acknowledges support for this work was provided by NASA through the NASA Hubble Fellowship grant #HST-HF2-51414 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. The research was carried out at the Jet Propulsion Laboratory, California Institute of Technology.
Group:Astronomy Department
Funders:
Funding AgencyGrant Number
NASA Hubble FellowshipHST-HF2-51414
NASANAS5-26555
JPL/CaltechUNSPECIFIED
Series Name:Astro2020 APC White Paper
Record Number:CaltechAUTHORS:20191126-132654179
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20191126-132654179
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:100069
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:26 Nov 2019 23:13
Last Modified:26 Nov 2019 23:13

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