Abstract
This paper presents analytical results on the anatomy of nested sampling, from which a technique is developed to estimate the run-time of the algorithm that works for any nested sampling implementation. We test these methods on both toy models and true cosmological nested sampling runs. The method gives an order-of-magnitude prediction of the endpoint at all times, forecasting the true endpoint within standard error around the halfway point.
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CITATION STYLE
Hu, Z., Baryshnikov, A., & Handley, W. (2024). aeons: approximating the end of nested sampling. Monthly Notices of the Royal Astronomical Society, 532(4), 4035–4049. https://doi.org/10.1093/mnras/stae1754
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