Abstract
Dark matter simulations require statistical techniques to properly identify and classify their halos and structures. Nonparametric solutions provide catalogs of these structures but lack the additional learning of a model-based algorithm and might misclassify particles in merging situations. With mixture models, we can simultaneously fit multiple density profiles to the halos that are found in a dark matter simulation. In this work, we use the Einasto profile to model the halos found in a sample of the Bolshoi simulation, and we obtain their location, size, shape, and mass. Our code is implemented in the R statistical software environment and can be accessed on https://github.com/LluisHGil/darkmix.
Original language | English |
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Article number | 34 |
Journal | The Astrophysical Journal |
Volume | 939 |
DOIs | |
Publication status | Published - 1 Nov 2022 |
Keywords
- Dark matter distribution
- Galaxy dark matter halos
- Spatial point processes
- Mixture model
- 356
- 1880
- 1915
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- Astrophysics - Astrophysics of Galaxies