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20192026
most citedCombined analysis of stellar and planetary absorption lines via global forward-transit simulations

19 citations · 21 across the 11 of their papers we have counts for

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astro-ph.EP2026

WALTzER: Wide-band Atmospheric Laboratory for Transiting Exoplanet Research

A. G. Sreejith, L. Fossati, M. Lendl +81

Understanding the origin and evolution of planetary atmospheres, and the connection between their lower and upper atmospheric layers, remains a fundamental challenge in exoplanet s…

astro-ph.EP2026

Toward a unified framework for helium observations and interpretation of atmospheric escape

Carteret Yann, Bourrier Vincent

Atmospheric escape is considered a key process in shaping exoplanet demographics and evolution. The near-infrared metastable helium triplet (HeI at ~10833Å) is one of the most powe…

astro-ph.EP2026

Probing Atmospheric Escape Through the Near-Infrared Helium Triplet

C. Farret Jentink, V. Bourrier, Y. Carteret

The most productive tracer of exoplanetary atmospheric escape is the measurement of excess absorption in the near-infrared metastable helium triplet during transits. Atmospheric es…

astro-ph.EP2026

TOI-3862 b: A dense super-Neptune deep in the hot Neptune desert

Ilaria Carleo, Amadeo Castro-González, Enric Pallé +61

The structure and evolution of close-in exoplanets are shaped by atmospheric loss and migration processes, which give rise to key population features such as the hot Neptune desert…

astro-ph.EP2023★ 19 cited

Combined analysis of stellar and planetary absorption lines via global forward-transit simulations

William Dethier, Vincent Bourrier

We characterise the planet-occulted line distortions (POLDs) in absorption spectra of transiting planets, that arise from proxies used for the occulted stellar lines and investigat…

astro-ph.EP2019

EUV influences on exoplanet atmospheric stability and evolution

Allison Youngblood, Kevin France, Tommi Koskinen +15

The planetary effective surface temperature alone is insufficient to characterize exoplanet atmospheres and their stability or evolution. Considering the star-planet system as a wh…