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[ascl:2408.008] HaloFlow: Simulation-Based Inference (SBI) using forward modeled galaxy photometry

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.

Code site:
https://github.com/changhoonhahn/haloflow
Described in:
https://ui.adsabs.harvard.edu/abs/2024ApJ...968...90H
Bibcode:
2024ascl.soft08008H

Views: 411

ascl:2408.008
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