Applying scale-free mass estimators to the Local Group in Constrained Local Universe Simulations
Arianna Di Cintio (UAM), Alexander Knebe (UAM), Noam I. Libeskind, (AIP), Yehuda Hoffman (Hebrew University), Gustavo Yepes (UAM), Stefan, Gottloeber (AIP)

TL;DR
This study applies scale-free mass estimators to simulated Local Group galaxies, demonstrating their effectiveness in estimating galaxy masses accurately using satellite distributions, with implications for real Milky Way and Andromeda mass measurements.
Contribution
The paper validates the applicability of scale-free mass estimators to binary galaxy systems like the Local Group, linking satellite radial distributions to host mass profiles for improved mass estimation.
Findings
Scale-free estimators work well for simulated Local Group galaxies.
The radial satellite distribution index relates to the host's mass profile.
Estimators can be reliably applied to real MW and M31 systems.
Abstract
We use the recently proposed scale-free mass estimators to determine the masses of the Milky Way (MW) and Andromeda (M31) galaxy in a dark matter only Constrained Local UniversE Simulation (CLUES). While these mass estimators work rather well for isolated spherical host systems, we examine here their applicability to a simulated binary system with a unique satellite population similar to the observed satellites of MW and M31. We confirm that the scale-free estimators work also very well in our simulated Local Group galaxies with the right number of satellites which follow the observed radial distribution. In the isotropic case and under the assumption that the satellites are tracking the total gravitating mass, the power-law index of the radial satellite distribution is directly related to the host's mass profile as…
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