255 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Centre National de la Recherche ScientifiqueFR18 papers
- Université de LorraineFR13 papers
- Université Paris CitéFR6 papers
- Laboratoire Interuniversitaire des Systèmes AtmosphériquesFR5 papers
- Université Paris-Est CréteilFR5 papers
- Laboratoire d'Astrophysique de BordeauxFR4 papers
- Laboratoire d’études spatiales et d’instrumentation en astrophysiqueFR4 papers
- Sorbonne UniversitéFR4 papers
- Université de BordeauxFR4 papers
- Délégation Paris 7FR3 papers
- Institut de Chimie PhysiqueFR3 papers
- Observatoire de ParisFR3 papers
7 papers · 1 filter
Inclusion of sulfur chemistry in a validated C/H/O/N chemical network: identification of key C/S coupling pathways
R. Veillet, O. Venot, B. Sirjean +6
The detection of SO2 in both WASP-39 b and WASP-107 b recently brought more attention to the modeling of photochemistry in exoplanets. However, sulfur kinetics data is lacking in t…
An extensively validated C/H/O/N chemical network for hot exoplanet disequilibrium chemistry
R. Veillet, O. Venot, B. Sirjean +4
We aimed to build a new and updated C0-C2 chemical network to study the CHON disequilibrium chemistry of warm and hot exoplanet atmospheres that relies on extensively validated and…
The deep composition of Uranus and Neptune from in situ exploration and thermochemical modeling
Thibault Cavalié, Olivia Venot, Yamila Miguel +7
The distant ice giants of the Solar System, Uranus and Neptune, have only been visited by one space mission, Voyager 2. The current knowledge on their composition remains very limi…
A new chemical scheme for giant planet thermochemistry. Update of the methanol chemistry and new reduced chemical scheme
Olivia Venot, Thibault Cavalié, Roda Bounaceur +3
Several chemical networks have been developed to study warm (exo)planetary atmospheres. The kinetics of the reactions related to the methanol chemistry included in these schemes ha…
A reduced chemical scheme for modelling warm to hot hydrogen-dominated atmospheres
Olivia Venot, Roda Bounaceur, Michel Dobrijevic +5
Three dimensional models that account for chemistry are useful tools to predict the chemical composition of (exo)planet and brown dwarf atmospheres and interpret observations of fu…
New chemical scheme for studying carbon-rich exoplanet atmospheres
Olivia Venot, Eric Hébrard, Marcelino Agúndez +2
Atmospheres with a high C/O ratio are expected to contain an important quantity of hydrocarbons, including heavy molecules (with more than 2 carbon atoms). To study correctly these…
A chemical model for the atmosphere of hot Jupiters
Olivia Venot, Eric Hébrard, Marcelino Agùndez +5
Our purpose is to release a chemical network, and the associated rate coefficients, developed for the temperature and pressure range relevant to hot Jupiters atmospheres. Using thi…