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astro-ph.IM2026

ESO User Support and Observation Preparation for VLTI Science Operations

M. Wittkowski, G. Beccari, A. Corporaal +16

The paper describes recent user‑focused upgrades to the VLTI, including new guiding and instrument modes, enhanced observation‑planning tools, and the availability of reduced GRAVI…

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

Nova Explosions in 2040

Alessandro Ederoclite, Domitilla De Martino, Paul Groot +7

Novae are thermonuclear explosions on the surface of accreting white dwarfs and are key laboratories for studying explosive nucleosynthesis, particle acceleration, shock physics, a…

astro-ph.IM2025

Spectroscopic Alerts for the Time-Domain Era

Alejandra Melo, Paula Sanchez-Saez, Valentin D. Ivanov +13

Time-domain astronomy is entering an era of unprecedented discovery driven by wide-field, high-cadence surveys such as LSST, Roman, Euclid, SKA, and PLATO. While some of these faci…

astro-ph.IM2025

White Dwarf Binaries: Probes of Future Astrophysics

Anna F. Pala, Roberto Raddi, Alberto Rebassa-Mansergas +25

White dwarf binaries are fundamental astrophysical probes. They represent ideal laboratories to test the models of binary evolution, which also apply to the sources of gravitationa…