Weak-lensing Mass Reconstruction of Galaxy Clusters with a Convolutional Neural Network -- II: Application to Next-Generation Wide-Field Surveys
Sangjun Cha, M. James Jee, Sungwook E. Hong, Sangnam Park, Dongsu Bak,, Taehwan kim

TL;DR
This paper demonstrates that a convolutional neural network can effectively reconstruct galaxy cluster mass maps from weak-lensing data, outperforming traditional methods, especially for next-generation wide-field surveys like the Rubin Observatory.
Contribution
The paper introduces an improved CNN-based method for weak-lensing mass reconstruction, tailored for next-generation surveys, showing high accuracy and cluster detection efficiency.
Findings
High-fidelity mass reconstructions consistent with true convergence fields.
Achieved ~75% completeness for clusters down to 10^14 solar masses.
Effective reconstruction of both small and large-scale structures.
Abstract
Traditional weak-lensing mass reconstruction techniques suffer from various artifacts, including noise amplification and the mass-sheet degeneracy. In Hong et al. (2021), we demonstrated that many of these pitfalls of traditional mass reconstruction can be mitigated using a deep learning approach based on a convolutional neural network (CNN). In this paper, we present our improvements and report on the detailed performance of our CNN algorithm applied to next-generation wide-field observations. Assuming the field of view () and depth (27 mag at ) of the Vera C. Rubin Observatory, we generated training datasets of mock shear catalogs with a source density of 33 arcmin from cosmological simulation ray-tracing data. We find that the current CNN method provides high-fidelity reconstructions consistent with the true convergence field, restoring both…
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Taxonomy
TopicsAstronomy and Astrophysical Research · Stellar, planetary, and galactic studies · Gamma-ray bursts and supernovae
