activity
20242026
collaborators

10 papers

astro-ph.EP2026

ESCAPE: a small explorer mission to study the stellar drivers of exoplanet evolution

Allison Youngblood, Kevin France, Brian Fleming +37

The long-term stability of exoplanetary atmospheres depends critically on the extreme-ultraviolet (EUV) photon and high-energy particle fluxes from the host star, which are poorly…

astro-ph.EP2026

The atmosphere of the warm Neptune GJ 436 b probed with ESPRESSO

E. Herrero-Cisneros, M. R. Zapatero Osorio, J. Sanz-Forcada +21

Aims. We aim to identify the presence of atomic and molecular species in the upper atmosphere of the warm Neptune-sized transiting planet GJ 436 b, which has a radiative equilibriu…

astro-ph.SR2026

The dusty envelopes of asymptotic giant branch stars with ultraviolet excesses

Jaime Alonso-Hernández, Carmen Sánchez Contreras, Raghvendra Sahai +1

Aims. In a first study, we characterised the properties of the gas component in the circumstellar envelopes surrounding a sample of 29 AGB stars with UV excesses. Now we intend to…

astro-ph.EP2025

Revisiting the atmosphere of HAT-P-70b with CARMENES high-resolution transmission spectroscopy

Tianjun Gan, Jaume Orell-Miquel, Fei Yan +19

Owing to hot and inflated envelopes that facilitate atmospheric studies, ultra-hot Jupiters (UHJs) have attracted much attention. Significant progress has been achieved, from enlar…

astro-ph.SR2025

Empirical prediction of plasma emission measure distributions and X-EUV spectra of late-type stars

Antonio Maggio, Ignazio Pillitteri, Jorge Sanz-Forcada +1

High-energy emission spectra from the outer atmospheres of late-type stars represent an important feature of the stellar activity in several contexts, such as the photoevaporation…

astro-ph.EP2025

The effects of stellar activity cycles on planetary atmospheric escape and the HeI 1083nm transit signature

Andrew P. Allan, Aline A. Vidotto, Jorge Sanz-Forcada +1

The HeI 1083nm transit signature is commonly used in tracing escaping planetary atmospheres. However, it can be affected by stellar activity, complicating detections and interpreta…