271 citations · 3k across the 62 of their papers we have counts for
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A model of scattered thermal radiation for Venus from 3 to 5 m
A. García Muñoz, P. Wolkenberg, A. Sánchez-Lavega +2
Thermal radiation becomes a prominent feature in the continuum spectrum of Venus longwards of 3 m. The emission is traceable to the upper cloud and haze layers in the plan…
Potential Vorticity of the South Polar Vortex of Venus
I. Garate-Lopez, R. Hueso, A. Sánchez-Lavega +1
Venus' atmosphere shows highly variable warm vortices over both of the planet's poles. The nature of the mechanism behind their formation and properties is still unknown. Potential…
Large Interferometer For Exoplanets (LIFE). X. Detectability of currently known exoplanets and synergies with future IR/O/UV reflected-starlight imaging missions
Óscar Carrión-González, Jens Kammerer, Daniel Angerhausen +10
The next generation of space-based observatories will characterize the atmospheres of low-mass, temperate exoplanets with the direct-imaging technique. This will be a major step fo…
Heating and ionization by non-thermal electrons in the upper atmospheres of water-rich exoplanets
A. García Muñoz
Context. The long-term evolution of an atmosphere and the remote detectability of its chemical constituents are susceptible to how the atmospheric gas responds to stellar irradiati…
The Hubble PanCET program: The near-ultraviolet transmission spectrum of WASP-79b
A. Gressier, A. Lecavelier des Etangs, D. K. Sing +11
We present Hubble Space Telescope (HST) transit observations of the Hot-Jupiter WASP-79b acquired with the Space Telescope Imaging Spectrograph (STIS) in the near ultraviolet (NUV)…
An efficient Monte Carlo model for the slowing down of photoelectrons. Application to H- in exoplanet atmospheres
Antonio García Muñoz
Photoelectrons, the fast electrons produced in the photoionization of planetary atmospheres, drive transformations in the atmospheric gas that are often inhibited by energy conside…