57 citations · 79 across the 5 of their papers we have counts for
5 papers
An unidentified absorption feature at 5.11 m on the surface of Titan and Pluto from JWST spectroscopy
B. Bézard, E. Lellouch, M. Camarca +14
Titan possesses a thick N-CH atmosphere that makes it difficult to study its surface spectroscopically. The chemical composition of the solid surface of Titan thus remains…
The atmosphere of K2-18 b: The role of hazes, clouds and photoelectrons
P. Lavvas, R. Liu, G. Tinetti +3
The atmospheric characterisation of temperate exoplanets is becoming accessible with JWST, providing a critical connection between Solar System planets and the more commonly observ…
Seasonal variation of Saturn's Lyman- brightness
P. Stephenson, T. T. Koskinen, Z. Brown +5
We examine Saturn's non-auroral (dayglow) emissions at Lyman- observed by the {Cassini/UVIS} instrument from 2004 until 2016, to constrain meridional and seasonal trends in the…
Titan's lakes chemical composition: sources of uncertainties and variability
D. Cordier, O. Mousis, J. I. Lunine +5
Between 2004 and 2007 the instruments of the CASSINI spacecraft discovered hydrocarbon lakes in the polar regions of Titan. We have developed a lake-atmosphere equilibrium model al…
About the possible role of hydrocarbon lakes in the origin of Titan's noble gas atmospheric depletion
D. Cordier, O. Mousis, J. I. Lunine +4
An unexpected feature of Titan's atmosphere is the strong depletion in primordial noble gases revealed by the Gas Chromatograph Mass Spectrometer aboard the Huygens probe during it…