Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
Robert McGibbon, Sadegh Khochfar

TL;DR
This paper introduces a machine learning model using extremely randomized trees to predict baryonic properties of dark matter subhalos from simulations, revealing nurture's dominant role over nature in galaxy properties.
Contribution
The study develops a novel ERT-based model trained on IllustrisTNG data, outperforming previous models and providing insights into the physical drivers of galaxy properties.
Findings
Model significantly outperforms baseline and mass-history models.
Feature importance varies across properties, indicating different physical influences.
Galaxies' properties are primarily driven by nurture, with some properties influenced by nature.
Abstract
We present a novel machine learning method for predicting the baryonic properties of dark matter only subhalos from N-body simulations. Our model is built using the extremely randomized tree (ERT) algorithm and takes subhalo properties over a wide range of redshifts as its input features. We train our model using the IllustrisTNG simulations to predict blackhole mass, gas mass, magnitudes, star formation rate, stellar mass, and metallicity. We compare the results of our method with a baseline model from previous works, and against a model that only considers the mass history of the subhalo. We find that our new model significantly outperforms both of the other models. We then investigate the predictive power of each input by looking at feature importance scores from the ERT algorithm. We produce feature importance plots for each baryonic property, and find that they differ…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Gaussian Processes and Bayesian Inference · Astronomy and Astrophysical Research
