astro-ph.COJun 22, 2026

Field-level weak lensing cosmology with 6060 simulations using multifidelity simulation-based inference

Authors: Alex A. SaoulisKiyam LinNiall JeffreyMaximilian von Wietersheim-KramstaDavide PirasAlessio Spurio ManciniAna M. G. FerreiraBenjamin Joachimi

Organizations: Department of Physics & Astronomy, University College London, Gower Street, London, WC1E 6BT, United Kingdom · Department of Earth Sciences, University College London, 5 Gower Place, London, WC1E 6BS, United Kingdom · Department of Physics & King’s Institute for Artificial Intelligence, King’s College London, Strand, London WC2R 2LS, United Kingdom · Institute for Computational Cosmology (ICC) & the Centre for Extragalactic Astronomy (CEA), Durham University, Durham, United Kingdom · Département de Physique Théorique, Université de Genève, 24 quai Ernest Ansermet, 1211 Genève 4, Switzerland · ETH Zurich, Institute for Particle Physics and Astrophysics, Wolfgang-Pauli-Strasse 27, 8093 Zurich, Switzerland

Abstract

We perform a realistic KiDS-Legacy mock analysis with field-level neural compression and simulation-based inference using just 60 NN-body simulations. The weak lensing shear field encodes substantially more cosmological information than standard two-point summary statistics such as the power spectrum. Field-level inference can fully exploit this information, but physical realism at the field-level requires very high-fidelity simulations. This poses a major challenge for simulation-based inference (SBI): accurate empirical density modelling and deep-learning-based neural compression require tens of thousands of training samples, but achieving physical realism at the field level makes each simulation extremely costly. We demonstrate that multifidelity SBI can alleviate this tension by substantially reducing the number of high-fidelity simulations needed for accurate cosmological inference. We pre-train neural inference models on realistic KiDS-Legacy-like shear mocks using fast log-normal \texttt{GLASS} simulations and fine-tune them on a small set of high-fidelity NN-body simulations. We show that 6060 high-fidelity simulations are sufficient to obtain informative and well-calibrated cosmological posteriors, enabling at least an order-of-magnitude reduction in simulation cost for accurate field-level inference in a realistic setting.

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