Constraining in-situ vs. ex-situ stellar mass in nearby galaxies with simulation-based inference
Understanding the complexities of galaxy evolution and the role of mergers therein remains a fundamental challenge in astrophysics. Since galaxies can only be observed at a single point in cosmic time, tracing their merging history and its impact on a galaxy's mass assembly is heavily dependent on models or cosmological simulations. However, while
Angeloudi, Eirini et al.
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2024