activity
20242026
collaborators
Showing astro-ph.EPShow all

6 papers · 1 filter

astro-ph.EP2026

C, N, O, S, and photochemistry in a temperate giant planet orbiting a late M dwarf

Michael Zhang, Qiao Xue, Jeehyun Yang +20

We report the JWST NIRSpec/PRISM transit spectrum of TOI-6894b, an exceptional 420 K sub-Saturn that is the only known giant planet transiting a late M dwarf. Remarkably, both the…

astro-ph.EP2025

A Cold and Super-Puffy Planet on a Prograde Orbit

Juan I. Espinoza-Retamal, Rafael Brahm, Cristobal Petrovich +36

We report the discovery of TOI-4507 b, a transiting sub-Saturn with a density 0.2 g/cm on a 105-day prograde orbit around a 700 Myr old F star. The transits were detected u…

astro-ph.EP2025

Ten Aligned Orbits: Planet Migration in the Era of JWST and Ariel

J. Zak, H. M. J. Boffin, A. Bocchieri +3

Understanding the diverse formation and migration pathways that shape exoplanetary systems requires characterizing both their atmospheric properties and their orbital dynamics. A k…

astro-ph.EP2025

Stellar obliquities of eight close-in gas giant exoplanets

J. Zak, H. M. J. Boffin, E. Sedaghati +4

The Rossiter-McLaughlin effect allows us to measure the projected stellar obliquity of exoplanets. From the spin-orbit alignment, planet formation and migration theories can be tes…

astro-ph.EP2024

Detection of faculae in the transit and transmission spectrum of WASP-69b

D. J. M. Petit dit de la Roche, H. Chakraborty, M. Lendl +9

Context: Transmission spectroscopy is a powerful tool for understanding exoplanet atmospheres. At optical wavelengths, it makes it possible to infer the composition and the presenc…

astro-ph.EP2024

HD 110067 c has an aligned orbit

J. Zak, H. M. J. Boffin, E. Sedaghati +25

Planetary systems in mean motion resonances hold a special place among the planetary population. They allow us to study planet formation in great detail as dissipative processes ar…