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20212026
most citedTowards multi-dimensional analysis of transmission spectroscopy. Part II: Day-night induced biases in retrievals from hot to ultra-hot Jupiters

38 citations · 117 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.EP2026★ 1 cited

Atmospheric asymmetries in WASP-121 b revealed by rotational transits detected with JWST

Cyril Gapp, Aurélien Falco, Thomas M. Evans-Soma +6

Close-in exoplanets are tidally locked to their host star and thus exhibit extreme atmospheric temperature gradients. It has been theorized that the fraction of star light absorbed…

astro-ph.EP2024★ 6 cited

Signature of the atmospheric asymmetries of hot and ultra-hot Jupiters in lightcurves

Aurélien Falco, Jérémy Leconte, Alexandre Mechineau +1

With the new generation of space telescopes such as the James Webb Space Telescope (JWST), it is possible to better characterize the atmospheres of exoplanets. The atmospheres of H…

astro-ph.EP2024★ 1 cited

Hydrogenated atmospheres of lava planets: atmospheric structure and emission spectra

Aurélien Falco, Pascal Tremblin, Sébastien Charnoz +2

Hot rocky super-Earths are thought to be sufficiently irradiated by their host star to melt their surface and thus allow for long-lasting magma oceans. Some processes have been pro…

astro-ph.EP2024★ 7 cited

ARES VI: Viability of one-dimensional retrieval models for transmission spectroscopy characterization of exo-atmospheres in the era of JWST and Ariel

Adam Yassin Jaziri, William Pluriel, Andrea Bocchieri +10

Observed exoplanet transit spectra are usually retrieved using 1D models to determine atmospheric composition while planetary atmospheres are 3D. With the JWST and future space tel…

astro-ph.EP2023★ 3 cited

The role of interior dynamics and differentiation on the surface and atmosphere of lava planets

Charles-Édouard Boukaré, Daphné Lemasquerier, Nicolas Cowan +5

Lava planets are rocky exoplanets that orbit so close to their host star that their day-side is hot enough to melt silicate rock. Their short orbital periods ensure that lava plane…

astro-ph.EP2023★ 25 cited

The effect of a small amount of hydrogen in the atmosphere of ultrahot magma-ocean planets: atmospheric composition and escape

Sébastien Charnoz, Aurélien Falco, Pascal Tremblin +3

Here we investigate how small amounts of hydrogen (much smaller than the mass of the exoplanet) above a magma ocean on a rocky exoplanet may modify the atmospheric chemistry and at…

astro-ph.EP2022★ 11 cited

Toward a multidimensional analysis of transmission spectroscopy. Part III: Modelling 2D effects in retrievals with TauREx

Tiziano Zingales, Aurélien Falco, William Pluriel +1

New-generation spectrographs dedicated to the study of exoplanetary atmospheres require a high accuracy in the atmospheric models to better interpret the input spectra. Thanks to s…

astro-ph.EP2021★ 25 cited

Toward a multidimensional analysis of transmission spectroscopy. Part I: Computation of transmission spectra using a 1D, 2D, or 3D atmosphere structure

Aurélien Falco, Tiziano Zingales, William Pluriel +1

Considering the relatively high precision that will be reached by future observatories, it has recently become clear that one dimensional (1D) atmospheric models, in which the atmo…

astro-ph.EP2021★ 38 cited

Towards multi-dimensional analysis of transmission spectroscopy. Part II: Day-night induced biases in retrievals from hot to ultra-hot Jupiters

William Pluriel, Jeremy Leconte, Vivien Parmentier +4

Hot Jupiters are very good targets for transmission spectroscopy analysis. Their atmospheres have a large scale height implying a high signal to noise ratio. As these planets orbit…