Nancy Grace Roman Space Telescope Coronagraph Instrument Observation Calibration Plan
- Creators
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Zellem, Robert T.
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Nemati, Bijan
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Bailey, Vanessa P.
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Cady, Eric J.
- Colavita, M. Mark
- Gonzalez, Guillermo
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Hildebrandt, Sergi R.
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Maier, Erin R.
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Mennesson, Bertrand
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Ygouf, Marie
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Zimmerman, Neil
- Belikov, Ruslan
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Debes, John
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de Rosa, Robert J.
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Douglas, Ewan S.
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Girard, Julien
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Groff, Tyler
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Kasdin, Jeremy
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Lowrance, Patrick J.
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Macintosh, Bruce
- Payne, Lindsey
- Ryan, Daniel
- Weisberg, Carey
Abstract
NASA's next flagship mission, the Nancy Grace Roman Space Telescope, is a 2.4-meter observatory set to launch no later than May 2027. Roman features two instruments: the Wide Field Imager and the Coronagraph Instrument. Roman's Coronagraph is a Technology Demonstration that will push the current capabilities of direct imaging to smaller contrast ratios (∼10−9) and inner-working angles (3~λ/D). In order to achieve this high precision, Roman Coronagraph data must be calibrated to remove as many potential sources of error as possible. Here we present a detailed overview of the Nancy Grace Roman Space Telescope Coronagraph Instrument Observation Calibration Plan including identifying potential sources of error and how they will be mitigated via on-sky calibrations.
Additional Information
Part of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Copyright 2022. All rights reserved. The authors would like to thank Bala Balasubramanian, Jeremy Kasdin, Nikole Lewis, and Tiffany Meshkat for their helpful discussions.Attached Files
Submitted - 2202.05923.pdf
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Additional details
- Eprint ID
- 115376
- Resolver ID
- CaltechAUTHORS:20220707-170607876
- NASA/JPL/Caltech
- Created
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2022-07-08Created from EPrint's datestamp field
- Updated
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2023-06-02Created from EPrint's last_modified field
- Caltech groups
- Infrared Processing and Analysis Center (IPAC)