HaloFlow: Simulation-Based Inference (SBI) using forward modeled galaxy photometry
Abstract
HaloFlow uses a machine learning approach to infer Mh and stellar mass, M∗, using grizy band magnitudes, morphological properties quantifying characteristic size, concentration, and asymmetry, total measured satellite luminosity, and number of satellites.
- Publication:
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Astrophysics Source Code Library
- Pub Date:
- August 2024
- Bibcode:
- 2024ascl.soft08008H
- Keywords:
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- Software