Kilonova Light Curve Parameter Estimation Using Likelihood-Free Inference

TL;DR

This paper introduces a fast, likelihood-free inference method with a pre-trained embedding network for estimating kilonova parameters from light curves, achieving accuracy comparable to traditional methods but with less computational effort.

Contribution

The authors develop a novel inference algorithm combining likelihood-free methods with a pre-trained embedding network, enabling efficient and accurate parameter estimation of kilonovae.

Findings

Achieves parameter estimation accuracy comparable to nested sampling.

Reduces training time and model size compared to likelihood-free inference alone.

Successfully marginalizes over nuisance parameters like distance and time of arrival.

Abstract

Rapid parameter estimation is critical when dealing with short lived signals such as kilonovae. We present a parameter estimation algorithm that combines likelihood-free inference with a pre-trained embedding network, optimized to efficiently process kilonova light curves. Our method is capable of retrieving the mass, velocity, and lanthanide fraction of the neutron star ejecta with an accuracy and precision on par with nested sampling methods while taking significantly less computational time. Our inference uniquely utilizes a pre-trained embedding network that marginalizes the time of arrival and the luminosity distance of the signal, allowing inference of signals at distances up to 200 Mpc. We find that including a pre-trained embedding outperforms the use of likelihood-free inference alone, reducing training time, model size, and offering the capability to marginalize over certain nuisance parameters. This framework has been integrated into the publicly available Nuclear Multi-Messenger Astronomy codebase, enabling the broader scientific community to deploy the model for their inference purposes. Our algorithm is broadly applicable to parameterized or simulated light curves of other transient objects, and can be adapted for quick sky localization.