activity
20162022
most citedNon-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b

66 citations · 148 across the 4 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2025

Transit-timing variations in the AU Mic system observed with CHEOPS

Á. Boldog, Gy. M. Szabó, L. Kriskovics +86

AU Mic is a very active M dwarf with an edge-on debris disk and two transiting sub-Neptunes with a possible third planetary companion. The two transiting planets exhibit significan…

astro-ph.EP202222 cited

A retrieval challenge exercise for the Ariel mission

Joanna K. Barstow, Quentin Changeat, Katy L. Chubb +5

The Ariel mission, due to launch in 2029, will obtain spectroscopic information for 1000 exoplanets, providing an unprecedented opportunity for comparative exoplanetology. Retrieva…

astro-ph.EP202166 cited

Non-local thermodynamic equilibrium effects determine the upper atmospheric temperature structure of the ultra-hot Jupiter KELT-9b

L. Fossati, M. E. Young, D. Shulyak +5

Several results indicate that the atmospheric temperature of the ultra-hot Jupiter KELT-9b in the main line formation region is a few thousand degrees higher than predicted by self…

astro-ph.EP2020

A data-driven approach to constraining the atmospheric temperature structure of KELT-9b

L. Fossati, D. Shulyak, A. G. Sreejith +10

Context. Observationally constraining the atmospheric temperature-pressure (TP) profile of exoplanets is an important step forward for improving planetary atmosphere models, furthe…

astro-ph.EP202015 cited

Non-Local Thermodynamic Equilibrium Transmission Spectrum Modelling of HD209458b

Mitchell E. Young, Luca Fossati, Tommi T. Koskinen +3

Context - Exoplanetary upper atmospheres are low density environments where radiative processes can compete with collisional ones and introduce non-local thermodynamic equilibrium…

astro-ph.EP201945 cited

The Kepler-11 system: evolution of the stellar high-energy emission and {initial planetary} atmospheric mass fractions

D. Kubyshkina, L. Fossati, A. J. Mustill +8

The atmospheres of close-in planets are strongly influenced by mass loss driven by the high-energy (X-ray and extreme ultraviolet, EUV) irradiation of the host star, particularly d…