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Impact of photochemical hazes on the thermal structure of exoplanet atmospheres
Transit observations reveal that a significant population of the detected exoplanets has hazy atmospheres (Sing et al. 2016). Although the relative contribution of clouds and photochemical aerosols is not yet fully clarified, the impact of haze particles on the thermal structure could be significant, as such particles can efficiently scatter and absorbPanayotis Lavvas, Anthony Arfaux
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Impact of photochemical hazes and gases on exoplanet atmospheric thermal structure
Monthly Notices of the Royal Astronomical Society, 2021Panayotis Lavvas
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Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres?
Life, 2023Shuhei Ono +2 more
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Possibilities for an Aerial Biosphere in Temperate Sub Neptune-Sized Exoplanet Atmospheres
Universe, 2021Thomas M Evans +2 more
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Internal structure and mineralogy of low-mass terrestrial exoplanets
Structure interne et minéralogie des exoplanètes terrestres de faible masse La modélisation d'intérieurs exoplanétaires fait le lien entre deux domaines : la détection et caractérisation d'exoplanètes, en plein essor avec le lancement de nouvelles missions telles que PLATO ou CHEOPS, et la géophysique, permettant l'étude des corps du ...openaire +1 more source
Phosphine as a Biosignature Gas in Exoplanet Atmospheres
Astrobiology, 2020William Bains +2 more
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Transit search: An optimization algorithm based on exoplanet exploration
Results in Control and Optimization, 2022Hosein Naderpour, Masoomeh Mirrashid
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