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SimSIMS: Simulation-based Supernova Ia Model Selection with thousands of latent variables

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arxiv 2311.15650 v1 pith:WRMABD2B submitted 2023-11-27 astro-ph.CO astro-ph.IM

classification astro-ph.COastro-ph.IM
keywords modelapplieddatademonstratingdustlatentsimulatedsimulation-based
verification ladder T0 review T1 audit T2 compute T3 formal
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We present principled Bayesian model comparison through simulation-based neural classification applied to SN Ia analysis. We validate our approach on realistically simulated SN Ia light curve data, demonstrating its ability to recover posterior model probabilities while marginalizing over >4000 latent variables. The amortized nature of our technique allows us to explore the dependence of Bayes factors on the true parameters of simulated data, demonstrating Occam's razor for nested models. When applied to a sample of 86 low-redshift SNae Ia from the Carnegie Supernova Project, our method prefers a model with a single dust law and no magnitude step with host mass, disfavouring different dust laws for low- and high-mass hosts with odds in excess of 100:1.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 4 citations worldwide. Full citation record

  1. A COMPASS to Model Comparison and Simulation-Based Inference in Galactic Chemical Evolution

    astro-ph.GA 2025-07 conditional novelty 6.0 of 10

    A diffusion-based simulation inference framework selects NuGrid AGB plus IllustrisTNG core-collapse yields as the best explanation for solar-type stellar abundances, and infers a steep IMF slope and high SN Ia normalization.

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