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A super-massive Neptune-sized planet
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Mantle mineralogy limits to rocky planet water inventories
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A mineralogical reason why all exoplanets cannot be equally oxidizing
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TOI-332 b: a super dense Neptune found deep within the Neptunian desert
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Magnesium oxide-water compounds at megabar pressure and implications on planetary interiors
Company for the Ultra-high Density, Ultra-short Period Sub-Earth GJ 367 b: Discovery of Two Additional Low-mass Planets at 11.5 and 34 Days*
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Removing biases on the density of sub-Neptunes characterised via transit timing variations
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A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS
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A detailed analysis of the Gl 486 planetary system
Chemical Abundances for 25 JWST Exoplanet Host Stars with KeckSpec
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Dust formation in the outflows of catastrophically evaporating planets
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Elemental Abundances of nearby M Dwarfs Based on High-resolution Near-infrared Spectra Obtained by the Subaru/IRD Survey: Proof of Concept
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The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution
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Demographics of Exoplanetary Systems
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A Transiting, Temperate Mini-Neptune Orbiting the M Dwarf TOI-1759 Unveiled by TESS
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Understanding the interior structure of gaseous giant exoplanets with machine learning techniques
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Chenliang Huang(黄辰亮), David R Rice and Jason H Steffen Monthly Notices of the Royal Astronomical Society 513(4) 5256 (2022) https://doi.org/10.1093/mnras/stac1133
The importance of silicate vapour in determining the structure, radii, and envelope mass fractions of sub-Neptunes