activity
20092026
most citedA population study of gaseous exoplanets

335 citations · 666 across the 8 of their papers we have counts for

collaborators
Showing astro-ph.EPShow all

6 papers · 1 filter

astro-ph.EP2026

The physical and chemical structure of Titan's upper atmosphere: energy balance, photochemistry and Jeans escape

Sudeshna Boro Saikia, Jonathan Tennyson, Shuchen Ji +7

Titan's upper atmospheric layers provide a unique opportunity to study how photochemistry, photoionisation, haze microphysics and escape processes shape its atmospheric chemical st…

astro-ph.EP2026

Probing Exoplanetary Chemistry with Ariel: Scientific Priorities and Observational Strategies

Olivia Venot, Yamila Miguel, Robin Baeyens +30

Over the past two decades, increasingly precise observations have revealed that exoplanet atmospheres are chemically diverse and often far from equilibrium, with processes such as…

astro-ph.EP2025★ 1 cited

A new look into the atmospheric composition of WASP-39 b

Sushuang Ma, Arianna Saba, Ahmed Faris Al-Refaie +4

Being one of the first exoplanets observed by the James Webb Space Telescope, WASP-39 b has become an iconic target and many transit spectra recorded with different instruments (NI…

astro-ph.EP2017★ 335 cited

A population study of gaseous exoplanets

A. Tsiaras, I. P. Waldmann, T. Zingales +8

We present here the analysis of 30 gaseous extrasolar planets, with temperatures between 600 and 2400 K and radii between 0.35 and 1.9 . The quality of the HST/WFC3…

astro-ph.EP2015★ 224 cited

Detection of an atmosphere around the super-Earth 55 Cancri e

A. Tsiaras, M. Rocchetto, I. P. Waldmann +8

We report the analysis of two new spectroscopic observations of the super-Earth 55 Cancri e, in the near infrared, obtained with the WFC3 camera onboard the HST. 55 Cancri e orbits…

astro-ph.EP2009★ 106 cited

Water in HD 209458b's atmosphere from 3.6 - 8 microns IRAC photometric observations in primary transit

J. P. Beaulieu, D. M. Kipping, V. Batista +15

The hot Jupiter HD 209458b was observed during primary transit at 3.6, 4.5, 5.8 and 8.0 microns using the Infrared Array Camera (IRAC) on the Spitzer Space Telescope. We detail her…