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Author
Foote, T.O.Quintana, E.V.
Dotson, J.L.
Colón, K.D.
Barclay, T.
Supsinskas, P.
Karburn, J.
Apai, D.
Hedges, C.
Rackham, B.V.
Rowe, J.F.
Christiansen, J.L.
Greene, T.P.
Mason, J.
Mosby, G.
Espinoza, N.
Gilbert, E.A.
Hoffman, K.
Kostov, V.B.
Lewis, N.K.
Morris, B.M.
Mullally, S.E.
Newton, E.R.
Schlieder, J.E.
Youngblood, A.
Mansfield, M.
Stevenson, K.B.
Villanueva, S.
Affiliation
University of ArizonaIssue Date
2022-08-27
Metadata
Show full item recordPublisher
SPIECitation
Trevor O. Foote, Elisa V. Quintana, Jessie L. Dotson, Knicole D. Colón, Thomas Barclay, Pete Supsinskas, Jordan Karburn, Dániel Apai, Christina Hedges, Benjamin V. Rackham, Jason F. Rowe, Jessie L. Christiansen, Thomas P. Greene, James Mason, Gregory Mosby, Néstor Espinoza, Emily A. Gilbert, Kelsey Hoffman, Veselin B. Kostov, Nikole K. Lewis, Brett M. Morris, Susan E. Mullally, Elisabeth R. Newton, Joshua E. Schlieder, Allison Youngblood, Megan Mansfield, Kevin B. Stevenson, and Steven Villanueva "Pandora SmallSat data simulation and target selection", Proc. SPIE 12180, Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave, 121802X (27 August 2022); https://doi.org/10.1117/12.2630131Rights
© 2022 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
Pandora is a SmallSat mission, designed to study the atmospheres of exoplanets using transmission spectroscopy and to investigate the impact that stellar contamination and variability has on observing the spectra of these worlds. Pandora's initial science operation lifetime is one year, so optimizing the science return is critical. Here we present two tools created to assist in the design process. The first is a 2-D spectrum simulator being developed to help refine target selection, optimize observation strategies, and assist in the creation of a data reduction pipeline. The second is a pseudo-retrieval framework that provides a quantifiable method for comparing potential targets against a handful of exoplanetary atmospheric parameters important to the Pandora mission. Preliminary results show Pandora will place tighter constraints on atmospheric properties like water abundance compared to HST and answering its mission objectives will help to inform targets for missions like JWST. © 2022 SPIE.Note
Immediate accessISSN
0277-786XVersion
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/12.2630131