The functional form of galaxy and halo luminosity and mass functions
Amelia Ford, Harry Desmond, Deaglan J Bartlett, Pedro G Ferreira

TL;DR
This paper uses symbolic regression to automatically discover optimal functional forms for galaxy and halo luminosity and mass functions, outperforming traditional models and providing a framework for future astrophysical data analysis.
Contribution
It introduces a novel application of symbolic regression to derive better fitting functions for astrophysical quantities, surpassing traditional models.
Findings
Many functions outperform Schechter and double Schechter fits for LF and SMF.
Functions outperform Press--Schechter and Warren/Tinker models for HMF.
Framework enables automated discovery of optimal functions for astrophysical data.
Abstract
The galaxy luminosity and stellar mass function (LF, SMF), and halo mass function (HMF), are fundamental quantities in astrophysics and crucial inputs to a range of astrophysical and cosmological analyses. They are typically parametrised by fitting functions that have been chosen "by eye" to match observed or simulated data. We apply symbolic regression -- specifically the Exhaustive Symbolic Regression (ESR) algorithm -- to automate the search for optimal LF, SMF and HMF functional forms. ESR scores all functions up to a maximum complexity composed of a user-defined basis set of operators using the description length, an approximation to the Bayesian evidence that balances accuracy with complexity. We find many functions outperforming the Schechter and double Schechter functions for the LF and SMF, and that outperform the Press--Schechter and Warren/Tinker functions for the HMF. By…
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