ROBIN-PIP: Robust Bayesian Field-Level Inference with Physics-Informed Priors
astro-ph.CO, astro-ph.IM
Submitted: 2026-09-30
Updated: 2026-09-30
Terminology
Sources
- Planck 2018 results. VI. Cosmological parameters
- Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
- Anticipated Performance of the Square Kilometre Array -- Phase 1 (SKA1)
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Euclid. I. Overview of the Euclid mission
- Wide-Field InfraRed Survey Telescope (WFIRST) Final Report
- Full-shape analysis with simulation-based priors: cosmological parameters and the structure growth anomaly
- Field-level Emulation of Cosmic Structure Formation with Cosmology and Redshift Dependence
- Metric Gaussian Variational Inference
- Euclid Definition Study Report
- Systematic-free inference of the cosmic matter density field from SDSS3-BOSS data
- A Latent Slice Sampling Algorithm
- LSST Science Book, Version 2.0
- Field-level inference of cosmic shear with intrinsic alignments and baryons
- Cosmological inference from Bayesian forward modelling of deep galaxy redshift surveys
- Field-level inference of galaxy intrinsic alignment from the SDSS-III BOSS survey
- From Dark Matter to Galaxies with Convolutional Networks
Related papers
- Angular clustering and bias of photometric quasars in the Kilo-Degree Survey Data Release 4
- A Novel kinetic Sunyaev-Zel'dovich Estimator for Electron-Electron Correlations
- Magnetic fields at the dawn of structure formation I. The CARLA J1510+5958 proto-cluster
- Dark Energy Survey Year 6 Results: Weak Lensing and Galaxy Clustering Cosmological Analysis Framework
- Exploring the Impact of Systematic Bias in Type Ia Supernova Cosmology Across Diverse Dark Energy Parametrizations
- Non-Gaussian Galaxy Stochasticity and the Noise-Field Formulation