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Rapid parameter estimation for kilonovae using likelihood-free inference
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DOI：10.1093/mnras/staf1045.png)
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Abstract
En 中文
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 Multimessenger Astronomy codebase, enabling the broader scientific community to deploy the model for their inference purposes. Our algorithm is broadly applicable to parametrized or simulated light curves of other transient objects and can be adapted for quick sky localization.
Keywords:
methods: numerical
stars: neutron
neutron star mergers
transients: novae
Journal
IF:
4.8
Papers:
7.0W
Citations:
25.0W