Accelerating Posterior Inference from Pulsar Light Curves via Learned Latent Representations and Local Simulator-Guided Optimization
Farhana Taiyebah, Abu Bucker Siddik, Indronil Bhattacharjee, Diane Oyen, Soumi De, Greg Olmschenk, Constantinos Kalapotharakos

TL;DR
This paper presents a novel framework that combines learned latent representations with local simulator-guided optimization to significantly accelerate posterior inference from pulsar light curves, maintaining accuracy while reducing computation time by over 120 times.
Contribution
The authors introduce a method that uses a pretrained U-Net for latent embedding and local optimization to efficiently approximate posteriors, outperforming traditional MCMC in speed.
Findings
Achieves 120x faster inference than MCMC.
Maintains high accuracy in posterior estimation.
Effectively uses learned embeddings for initialization.
Abstract
Posterior inference from pulsar observations in the form of light curves is commonly performed using Markov chain Monte Carlo methods, which are accurate but computationally expensive. We introduce a framework that accelerates posterior inference while maintaining accuracy by combining learned latent representations with local simulator-guided optimization. A masked U-Net is first pretrained to reconstruct complete light curves from partial observations and to produce informative latent embeddings. Given a query light curve, we identify similar simulated light curves from the simulation bank by measuring similarity in the learned embedding space produced by pretrained U-Net encoder, yielding an initial empirical approximation to the posterior over parameters. This initialization is then refined using a local optimization procedure using hill-climbing updates, guided by a forward…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Gaussian Processes and Bayesian Inference
