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    The Pandora SmallSat: A Mission to spectroscopically study exoplanet atmospheres

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    Author
    Hoffman, K.
    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.
    Kostov, V.B.
    Lewis, N.K.
    Morris, B.M.
    Mullally, S.E.
    Newton, E.R.
    Schlieder, J.E.
    Youngblood, A.
    Foote, T.
    Mansfield, M.
    Stevenson, K.B.
    Villanueva, S.
    Pepper, J.
    Show allShow less
    Affiliation
    University of Arizona
    Issue Date
    2022-08-27
    Keywords
    astronomy
    exoplanets
    Infrared
    Optical
    photometer
    spectrograph
    stars
    stellar activity
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    Kelsey Hoffman, 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 Gilbert, Veselin B. Kostov, Nikole K. Lewis, Brett M. Morris, Susan E. Mullally, Elisabeth R. Newton, Joshua E. Schlieder, Allison Youngblood, Trevor Foote, Megan Mansfield, Kevin B. Stevenson, Steven Villanueva, and Joshua Pepper "The Pandora SmallSat: a mission to spectroscopically study exoplanet atmospheres", Proc. SPIE 12180, Space Telescopes and Instrumentation 2022: Optical, Infrared, and Millimeter Wave, 121800C (27 August 2022); https://doi.org/10.1117/12.2629546
    Journal
    Proceedings of SPIE - The International Society for Optical Engineering
    Rights
    © 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 low-cost space telescope designed to measure the composition of distant transiting planets. The Pandora observatory is designed with the capability of measuring precision photometry simultaneously with near-infrared spectroscopy, enabling scientists to disentangle stellar activity from the subtle signature of a planetary atmosphere. The broad-wavelength coverage will provide constraints on the spot and faculae covering fractions of low-mass exoplanet host stars and the impact of these active regions on exoplanetary transmission spectra. Pandora will subsequently identify exoplanets with hydrogen- or water-dominated atmospheres, and robustly determine which planets are covered by clouds and hazes. Pandora observations will also contribute to the study of transit timing variations and phase curve photometry. With a launch readiness date of early-2025, the Pandora mission represents a new class of low-cost space missions that will achieve out-of-this-world science. © 2022 SPIE.
    Note
    Immediate access
    ISSN
    0277-786X
    DOI
    10.1117/12.2629546
    Version
    Final Published Version
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2629546
    Scopus Count
    Collections
    UA Faculty Publications

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