activity
20242026
most citedOptimized HDBSCAN clustering for reconstructing the merger history of the Milky Way: applications and limitations

1 citations · 1 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.GA2026

A simulation-based inference of the Milky Way merger history

Andrea Sante, Andreea S. Font, Daisuke Kawata +2

Accreted stars in the Milky Way (MW) preserve information about the progenitor galaxies where they formed in their chemical and kinematic properties. In this study, we use the chem…

astro-ph.GA20261 cited

Optimized HDBSCAN clustering for reconstructing the merger history of the Milky Way: applications and limitations

Andrea Sante, Andreea S. Font, Dharmesh Mistry +2

Clustering algorithms can help reconstruct the assembly history of the Milky Way by identifying groups of stars sharing similar properties in a kinematical or chemical abundance sp…

astro-ph.GA2025

Measuring and modelling the Splash with APOGEE/Gaia and ARTEMIS

Shobhit Kisku, Ricardo P. Schiavon, Andreea S. Font +6

Using combined data from SDSS-IV/APOGEE and Gaia, we study the chemo-dynamical properties of the Splash population in comparison with those of the high-alpha disc. We investigate a…

astro-ph.GA2025

GalactiKit: reconstructing mergers from debris using simulation-based inference in Auriga

Andrea Sante, Daisuke Kawata, Andreea S. Font +1

We present GalactiKit, a data-driven methodology for estimating the lookback infall time, stellar mass, halo mass and mass ratio of the disrupted progenitors of Milky Way-like gala…

astro-ph.GA2024

Applying machine learning to Galactic Archaeology: how well can we recover the origin of stars in Milky Way-like galaxies?

Andrea Sante, Andreea S. Font, Sandra Ortega-Martorell +2

We present several machine learning (ML) models developed to efficiently separate stars formed in-situ in Milky Way-type galaxies from those that were formed externally and later a…