Pith. sign in

REVIEW 1 cited by

Density Deconvolution with Normalizing Flows

Not yet reviewed by Pith; the record is open.

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 2006.09396 v2 pith:63IXTKBX submitted 2020-06-16 stat.ML cs.LG

classification stat.MLcs.LG
keywords densitydeconvolutionflowsdemonstrategaussianlikelihoodnoisenormalizing
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

Density deconvolution is the task of estimating a probability density function given only noise-corrupted samples. We can fit a Gaussian mixture model to the underlying density by maximum likelihood if the noise is normally distributed, but would like to exploit the superior density estimation performance of normalizing flows and allow for arbitrary noise distributions. Since both adjustments lead to an intractable likelihood, we resort to amortized variational inference. We demonstrate some problems involved in this approach, however, experiments on real data demonstrate that flows can already out-perform Gaussian mixtures for density deconvolution.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

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

  1. Denoising Milky Way stellar survey data with normalizing flow models

    astro-ph.GA 2025-05 conditional novelty 5.0 of 10

    A normalizing flow with importance-sampling denoising partially recovers kinematic substructures (Hercules stream, phase spiral) from mock Gaia data with amplified errors.

Pith tools