collaborators

15 papers

astro-ph.GA2026

The open cluster NGC 2509. Stellar rotation and main sequence turnoff extension from FLAMES spectroscopy

C. Boeche, J. Alonso-Santiago, A. Bragaglia +8

NGC 2509 is a distant (~2.5 kpc) and little-studied open cluster located in the third Galactic quadrant. It is a moderately old cluster, whose age has not yet been precisely determ…

astro-ph.SR2026

Asteroseismic ages for 17,000 stars in Kepler, K2 and TESS

Emma Willett, Andrea Miglio, Saniya Khan +9

The availability of asteroseismic constraints for tens of thousands of red giant (RG) stars has opened the door to robust age estimates, enabling time-resolved studies of different…

astro-ph.SR2026

Ariel stellar characterisation IV. Fundamental parameters of 18 hot stars in the Ariel mission candidate sample

H. Ramler, S. P. D. Borthakur, C. P. Folsom +16

The characterisation of exoplanetary systems depends on the accurate determination of host star parameters. The Ariel mission will probe the atmospheres of a statistically signific…

astro-ph.SR2026

The PLATO Science Calibration and Validation Plan: Targets for the First Long-pointing Field

Konstanze Zwintz, Conny Aerts, Andrew Tkachenko +56

In order to meet the science goals of the PLATO space mission, an extensive science calibration and validation plan has been designed. This paper describes this plan, as well as th…

astro-ph.SR2026

A homogeneous view of asymptotic giant branch carbon stars as seen by Gaia

Alessio Liberatori, Despina Hatzidimitriou, Konstantinos Antoniadis +12

Carbon stars on the asymptotic giant branch are major contributors to galactic dust enrichment, with gas mass-loss rates up to 1e-4 Msun/yr. We present a homogeneous spectral energ…

astro-ph.SR2026

Wide binaries without viable bound Newtonian orbits

L. Pasquini, R. Saglia, F. Patat +7

Context. Wide binaries offer a unique opportunity to test gravity in the low acceleration regime, where deviations from Newtonian dynamics may appear. Aims. We use high-resolution…