activity
20242026
collaborators

9 papers

astro-ph.GA2026

Estimating the dynamical masses of dwarf galaxies in the presence of binary-star contamination

José María Arroyo-Polonio, Giuseppina Battaglia, Guillaume F. Thomas

Ultra-faint dwarf galaxies (UFDs) show extreme dynamical mass-to-light ratios of approximately 100-5000 in solar units within the half-light radius, making them critical tests for…

astro-ph.GA2026

HR-GO II: chemical abundances of low- retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure

Renjing Xie, Zhen Yuan, Haining Li +12

Milky Way halo substructures identified in dynamical space are known to suffer from contamination from the Milky Way in-situ stars, which makes their accreted origins uncertain. We…

astro-ph.GA2025

Chronology of our Galaxy from Gaia colour-magnitude diagram fitting (ChronoGal): IV. On the inner Milky Way stellar age distribution

Tomás Ruiz-Lara, David Mirabal, Carme Gallart +15

The Milky Way's inner region is dominated by a stellar bar and a boxy-peanut shaped bulge. However, which stellar populations inhabit the inner Galaxy or how star formation proceed…

astro-ph.GA2025

Chemo-dynamics of the stellar component of the Sculptor dwarf galaxy II: dynamical properties and dark matter halo density

José María Arroyo Polonio, Raffaele Pascale, Giuseppina Battaglia +4

Dwarf galaxies satellite of the Milky Way are excellent laboratories for testing dark matter (DM) models and baryonic feedback implementation in simulations. The Sculptor 'classica…

astro-ph.GA2025

The Pristine survey: XXV. The very metal-poor Galaxy: Chemodynamics through the follow-up of the Pristine-Gaia synthetic catalogue

Akshara Viswanathan, Zhen Yuan, Anke Ardern-Arentsen +27

The Pristine-\textit{Gaia} synthetic catalogue provides reliable photometric metallicities for 30 million FGK stars using the Pristine survey model and Gaia XP spectra. We pe…

astro-ph.GA2025

How well can we unravel the accreted constituents of the Milky Way stellar halo? A test on cosmological hydrodynamical simulations

Guillaume F. Thomas, Giuseppina Battaglia, Robert J. J. Grand +1

Context. One of the primary goals of Galactic Archaeology is to reconstruct the Milky Way's accretion history. To achieve this, significant efforts have been dedicated to identifyi…