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Hybrid summary statistics: neural weak lensing inference beyond the power spectrum

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arxiv 2407.18909 v1 pith:HEEVJ25L submitted 2024-07-26 astro-ph.CO cs.LGphysics.comp-phstat.MLstat.OT

classification astro-ph.COcs.LGphysics.comp-phstat.MLstat.OT
keywords statisticsinferenceinformationsummariessummarynetworksneuralpower
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abstract

In inference problems, we often have domain knowledge which allows us to define summary statistics that capture most of the information content in a dataset. In this paper, we present a hybrid approach, where such physics-based summaries are augmented by a set of compressed neural summary statistics that are optimised to extract the extra information that is not captured by the predefined summaries. The resulting statistics are very powerful inputs to simulation-based or implicit inference of model parameters. We apply this generalisation of Information Maximising Neural Networks (IMNNs) to parameter constraints from tomographic weak gravitational lensing convergence maps to find summary statistics that are explicitly optimised to complement angular power spectrum estimates. We study several dark matter simulation resolutions in low- and high-noise regimes. We show that i) the information-update formalism extracts at least $3\times$ and up to $8\times$ as much information as the angular power spectrum in all noise regimes, ii) the network summaries are highly complementary to existing 2-point summaries, and iii) our formalism allows for networks with smaller, physically-informed architectures to match much larger regression networks with far fewer simulations needed to obtain asymptotically optimal inference.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations

    astro-ph.CO 2025-01 conditional novelty 6.0 of 10

    JERALD uses a few fitted Lagrangian displacement layers to convert FastPM outputs into DM, stellar mass and HI maps whose power spectra match a full-hydro simulation at up to 8x higher resolution.

  2. Deep Needlet: A CNN based full sky component separation method in Needlet space

    astro-ph.CO 2025-01 conditional novelty 5.0 of 10

    A CNN trained on needlet-filtered Planck-like simulations recovers CMB temperature maps with lower foreground residuals than NILC and power spectra accurate to ell about 1100.

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