Retrieval of atmospheric structure and composition of exoplanets from transit spectroscopy
Recent spectroscopic observations of transiting exoplanets have permitted the derivation of the thermal structure and molecular abundances of H2O, CO, CO2, CH4, metallic oxides and alkali metals in these extreme atmospheres. Here, for the first time, a fully-fledged retrieval algorithm has been applied to exoplanet spectra to determine the thermal ...
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An Informational-Entropic Approach to Exoplanet Characterization. [PDF]
Vannah S, Stiehl ID, Gleiser M.
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Biological, Equilibrium and Photochemical Signatures of C, N and S Isotopes in the Early Earth and Exoplanet Atmospheres. [PDF]
Lyons JR.
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Tracing the inner edge of the habitable zone with sulfur chemistry. [PDF]
Jordan S, Shorttle O, Rimmer PB.
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Revealing the atmospheres of highly irradiated exoplanets: from ultra-hot Jupiters to rocky worlds. [PDF]
Mansfield M.
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Instrumentation prospects for rocky exoplanet atmospheres studies with high resolution spectroscopy. [PDF]
Rukdee S.
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Magma Ocean Evolution at Arbitrary Redox State. [PDF]
Nicholls H+3 more
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How the James Webb Space Telescope Is Revealing the Weather and Chemistry on Planets around Other Stars. [PDF]
Extance A.
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Stability of hydrides in sub-Neptune exoplanets with thick hydrogen-rich atmospheres. [PDF]
Kim T+6 more
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Early Release Science of the exoplanet WASP-39b with JWST NIRCam. [PDF]
Ahrer EM+98 more
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