A transformer-based diffusion model learns the joint distribution of convergence maps and cosmology from log-normal weak lensing simulations and generates calibrated posterior samples matching MCMC results.
Posteriorsamplesofsourcegalaxiesinstronggravitationallenseswithscore-based priors.CoRR, abs/2211.03812
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Derives the conditional score exactly from an unconditional score via affine maps for linear inverse problems in infinite dimensions, shifting computation to offline training.
ShuffleFlow is a variational inference framework that partitions images with pixel-unshuffling and models the joint posterior over sub-images using a shared conditional normalizing flow conditioned on neural field features for scalable Bayesian inverse imaging.
MIRA is a new analytic score for conditional distribution accuracy derived from equal probability mass assignment, enabling Bayesian model comparison via direct posterior validation.
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Joint inference of weak lensing convergence map and cosmology with diffusion models
A transformer-based diffusion model learns the joint distribution of convergence maps and cosmology from log-normal weak lensing simulations and generates calibrated posterior samples matching MCMC results.
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