AI summary · DOI: 10.1117/1.jatis.12.4.041044 · Physics and Astronomy

Science potential of characterizing gas giant exoplanets with HWO

Beck Dacus (University of California San Diego), Jean-Baptiste Ruffio (University of California San Diego), Quinn Konopacky (University of California San Diego), Tyler Robinson (University of Arizona), Mary Anne Limbach (University of Michigan), Kielan K. Hoch (Space Telescope Science Institute), Katelyn Horstman (California Institute of Technology), Dimitri P. Mawet (California Institute of Technology, Jet Propulsion Laboratory),
and 11 more authorsMichael W. McElwain (California Institute of Technology, Jet Propulsion Laboratory), Bertrand P. Mennesson (Goddard Space Flight Center), Marshall Perrin (Space Telescope Science Institute), Laurent Pueyo (Space Telescope Science Institute), Dmitry Savransky (Cornell University), Corey Spohn (Goddard Space Flight Center), Sarah Steiger (Space Telescope Science Institute), Connor Vancil (University of California, Santa Barbara), Ji Wang (The Ohio State University), Nicole Wolff (University of California, Santa Cruz), Shelley Wright (University of California San Diego)
Original paper Published on 24 Oct. 2026 Journal of Astronomical Telescopes Instruments and Systems License: not stated (all rights reserved)

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