Pith. sign in

REVIEW

Population-Level Inference of Strong Gravitational Lenses with Neural Network-Based Selection Correction

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 2207.04123 v1 pith:H4M2JBLO submitted 2022-07-08 astro-ph.IM astro-ph.CO

classification astro-ph.IMastro-ph.CO
keywords inferencepopulation-levelsystemslensingneuralparametersselectionstrong
verification ladder T0 review T1 audit T2 compute T3 formal
0 comments
read the original abstract

A new generation of sky surveys is poised to provide unprecedented volumes of data containing hundreds of thousands of new strong lensing systems in the coming years. Convolutional neural networks are currently the only state-of-the-art method that can handle the onslaught of data to discover and infer the parameters of individual systems. However, many important measurements that involve strong lensing require population-level inference of these systems. In this work, we propose a hierarchical inference framework that uses the inference of individual lensing systems in combination with the selection function to estimate population-level parameters. In particular, we show that it is possible to model the selection function of a CNN-based lens finder with a neural network classifier, enabling fast inference of population-level parameters without the need for expensive Monte Carlo simulations.

Discussion (0). Continue with ORCID to comment.

Pith tools