Mass Estimation of Galaxy Clusters with Deep Learning. I. Sunyaev-Zel'dovich Effect
Author
Gupta, N; Reichardt, CLDate
2020-09-07Source Title
Astrophysical Journal Supplement SeriesPublisher
American Astronomical SocietyAffiliation
School of PhysicsMetadata
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Journal ArticleCitations
Gupta, N. & Reichardt, C. L. (2020). Mass Estimation of Galaxy Clusters with Deep Learning. I. Sunyaev-Zel'dovich Effect. Astrophysical Journal, 900 (2), https://doi.org/10.3847/1538-4357/aba694.Access Status
This item is embargoed and will be available on 2021-09-07. Access full text via the Open Access locationOpen Access URL
https://arxiv.org/abs/2003.06135v2ARC Grant code
ARC/DP150103208Abstract
We present a new application of deep learning to infer the masses of galaxy clusters directly from images of the microwave sky. Effectively, this is a novel approach to determining the scaling relation between a cluster's Sunyaev–Zel'dovich (SZ) effect signal and mass. The deep-learning algorithm used is mResUNet, which is a modified feed-forward deep-learning algorithm that broadly combines residual learning, convolution layers with different dilation rates, image regression activation, and a U-Net framework. We train and test the deep-learning model using simulated images of the microwave sky that include signals from the cosmic microwave background, dusty and radio galaxies, and instrumental noise as well as the cluster's own SZ signal. The simulated cluster sample covers the mass range 1 × 1014 M ⊙ < M 200c < 8 × 1014 M ⊙ at z = 0.7. The trained model estimates the cluster masses with a 1σ uncertainty ΔM/M ≤ 0.2, consistent with the input scatter on the SZ signal of 20%. We verify that the model works for realistic SZ profiles even when trained on azimuthally symmetric SZ profiles by using the Magneticum hydrodynamical simulations.
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