activity
20242026
most citedObserving bright pulsating white dwarfs with PLATO: A new window into the late stages of stellar evolution

1 citations · 1 across the 5 of their papers we have counts for

collaborators
Showing 2025Show all

18 papers · 1 filter

astro-ph.IM2025

The supernova Ia progenitor problem in the 2040s

Thomas Kupfer, Simone Scaringi, Ingrid Pelisoli +8

Type Ia supernovae (SNe Ia) are fundamental to cosmology and galactic chemical evolution, yet the nature of their progenitor systems remains unresolved. Multiple evolutionary pathw…

astro-ph.IM2025

The final stages of binary evolution using multi-messenger studies

Thomas Kupfer, Simone Scaringi, Paul Groot +11

Ultracompact Galactic binaries with orbital periods below an hour are among the strongest persistent gravitational-wave (GW) sources in the mHz band and will constitute the dominan…

astro-ph.IM2025

Asteroseismology of white dwarfs in the 2040s

Murat Uzundag, Ingrid Pelisoli, Stephane Charpinet +6

White dwarfs, the final evolutionary stage of the vast majority of stars, serve as critical tools for cosmochronology, studies of planetary system evolution, and laboratories for n…

astro-ph.EP2025

Giant Outer Transiting Exoplanet Mass (GOTEM) Survey.VII. TOI-6041: a multi-planet system including a warm Neptune exhibiting strong TTVs

N. Heidari, A. Alnajjarine, H. P. Osborn +101

We present the characterization of the TOI-6041 system, a bright () G7-type star hosting at least two planets. The inner planet, TOI-6041b, is a warm Neptune wit…

astro-ph.EP2025

HARPS-N, TESS, and CHEOPS discover a transiting sub-Neptune and two outer companions around the bright solar analogue HD 85426

F. Lienhard, A. Mortier, A. Collier Cameron +96

We provide a detailed characterisation of the planetary system orbiting HD 85426 (TOI-1774). This bright G-type star (: 0.99 ; : 1.13 $\text{R…

astro-ph.SR2025

The Arizona-Montréal spectroscopic survey of hot subluminous stars

M. Latour, E. M. Green, M. Dorsch +6

Hot subdwarf B (sdB) and O (sdO) type stars are evolved helium-burning objects that lost their hydrogen envelope before the helium flash when their progenitors were close to the ti…