JWST NIRSpec PRISM transmission spectroscopy detects CH4, other hydrocarbons, and aerosols in WD 1856 b's atmosphere, with evidence for recent reheating and a carbon-enriched composition.
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JWST transmission spectrum of WASP-80 b yields log10 X_CS2 = -2.25 with evidence for carbon-sulfur chemical coupling via CH2S networks.
citing papers explorer
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Aerosols and hydrocarbons in the atmosphere of a white dwarf planet
JWST NIRSpec PRISM transmission spectroscopy detects CH4, other hydrocarbons, and aerosols in WD 1856 b's atmosphere, with evidence for recent reheating and a carbon-enriched composition.
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The Identification of CS2 and Evidence for Carbon-Sulfur Chemical Coupling in a Warm Giant Exoplanet Atmosphere
JWST transmission spectrum of WASP-80 b yields log10 X_CS2 = -2.25 with evidence for carbon-sulfur chemical coupling via CH2S networks.