Comparison of symbolic regression algorithms in Star/galaxy/quasar separation
arXiv:2602.24022 · doi:10.1016/j.ascom.2026.101156
Abstract
This work investigates symbolic regression (SR) as an interpretable alternative to black-box machine learning for the classification of stars, galaxies, and quasars in the Sloan Digital Sky Survey Data Release 17 (SDSS DR17). We conduct a systematic comparative study of four state-of-the-art SR frameworks: {\tt PySR}, Exhaustive Symbolic Regression ({\tt ESR}) with MDL-based selection, Physical Symbolic Optimization ({\tt PhySO}) using deep reinforcement learning, and Multi-View Symbolic Regression ({\tt MvSR}). By deriving compact analytic functions (complexity 10) on a representative training subset and subsequently evaluating them via an 80,000-sample 5-fold cross-validation threshold optimization phase and a subsequent 10,000-sample unseen hold-out test set, we map spectroscopic redshift () to continuous classification scores. Our results demonstrate that these low-complexity expressions achieve high predictive reliability, with {\tt MvSR} reaching a cross-validation Cohen's Kappa of 0.8956 (0.8876 on the hold-out set) and {\tt PhySO} achieving exceptional parametric stability (). We note however that the resulting equations returned by Symbolic regression are purely empirical and no physical significance should be ascribed to these equations.
23 pages, 32 figures. Accepted for publication in Astronomy and Computing
References in corpus (14)
- Spectroscopic Target Selection in the Sloan Digital Sky Survey: The Quasar Sample
- The Blanco Cosmology Survey: Data Acquisition, Processing, Calibration, Quality Diagnostics and Data Release
- Deep symbolic regression for physics guided by units constraints: toward the automated discovery of physical laws
- Star/galaxy separation at faint magnitudes: Application to a simulated Dark Energy Survey
- Separation of pulsar signals from noise with supervised machine learning algorithms
- Unsupervised star, galaxy, qso classification: Application of HDBSCAN
- Model Comparison tests of modified gravity from the Eöt-Wash experiment
- The SZ flux-mass (-) relation at low halo masses: improvements with symbolic regression and strong constraints on baryonic feedback
- Photometric identification of compact galaxies, stars and quasars using multiple neural networks
- Morphological Star-Galaxy Separation
- Optimal Inflationary Potentials
- Enhanced Astronomical Source Classification with Integration of Attention Mechanisms and Vision Transformers
- Exploring symbolic regression and genetic algorithms for astronomical object classification
- Approximating neutron-star radii using gravitational-wave only measurements with symbolic regression