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On Linking Planet Formation Models, Protoplanetary Disk Properties, and Mature Gas Giant Exoplanet Atmospheres

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←A Precise Metallicity and Carbon-to-Oxygen Ratio for a Warm Giant Exoplanet from its Panchromatic JWST Emission Spectrum
The NASA Exoplanet Archive and Exoplanet Follow-up Observing Program: Data, Tools, and Usage→

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