Flexible Simulation Based Inference for Galaxy Photometric Fitting with Synthesizer
Thomas Harvey, Christopher C. Lovell, Sophie Newman, Christopher J. Conselice, Duncan Austin, William J. Roper, Aswin P. Vijayan, Stephen M. Wilkins, Patricia Iglesias-Navarro, Vadim Rusakov, Qiong Li, Nathan Adams, Kai Magdwick, Caio M. Goolsby, Marc Huertas-Company, Matthew Ho

TL;DR
Synference is a flexible, simulation-based inference framework for galaxy photometric fitting that enables rapid, accurate parameter estimation and model comparison, significantly accelerating analysis of large galaxy survey datasets.
Contribution
This work introduces Synference, a novel Python framework combining simulation-based inference with flexible galaxy SED modeling, validated on real data and demonstrating substantial speed improvements.
Findings
High accuracy in parameter recovery (e.g., R^2 > 0.99 for stellar mass)
Fast inference speed (~3 minutes for 3,088 galaxies on a single CPU)
Effective simultaneous inference of redshifts and physical parameters
Abstract
We introduce Synference, a new, flexible Python framework for galaxy SED fitting using simulation-based inference (SBI). Synference leverages the Synthesizer package for flexible forward-modelling of galaxy SEDs and integrates the LtU-ILI package to ensure best practices in model training and validation. In this work we demonstrate Synference by training a neural posterior estimator on simulated galaxies, based on a flexible 8-parameter physical model, to infer galaxy properties from 14-band HST and JWST photometry. We validate this model, demonstrating excellent parameter recovery (e.g. R0.99 for M) and accurate posterior calibration against nested sampling results. We apply our trained model to 3,088 spectroscopically-confirmed galaxies in the JADES GOODS-South field. The amortized inference is exceptionally fast, having nearly fixed cost per posterior evaluation…
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