Noise reduction for weak lensing mass mapping: an application of generative adversarial networks to Subaru Hyper Suprime-Cam first-year data

Author:

Shirasaki Masato12,Moriwaki Kana3,Oogi Taira4,Yoshida Naoki3567,Ikeda Shiro28ORCID,Nishimichi Takahiro59

Affiliation:

1. National Astronomical Observatory of Japan, Mitaka, Tokyo 181-8588, Japan

2. The Institute of Statistical Mathematics, Tachikawa, Tokyo 190-8562, Japan

3. Department of Physics, University of Tokyo, Tokyo 113-0033, Japan

4. Institute of Management and Information Technologies, Chiba University, Chiba 263-8522, Japan

5. Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba 277-8583, Japan

6. Institute for Physics of Intelligence, University of Tokyo, Tokyo 113-0033, Japan

7. Research Center for the Early Universe, Faculty of Science, University of Tokyo, Tokyo 113-0033, Japan

8. Department of Statistical Science, Graduate University for Advanced Studies, 10-3 Midori-cho, Tachikawa, Tokyo 190-8562, Japan

9. Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan

Abstract

ABSTRACT We propose a deep-learning approach based on generative adversarial networks (GANs) to reduce noise in weak lensing mass maps under realistic conditions. We apply image-to-image translation using conditional GANs to the mass map obtained from the first-year data of Subaru Hyper Suprime-Cam (HSC) Survey. We train the conditional GANs by using 25 000 mock HSC catalogues that directly incorporate a variety of observational effects. We study the non-Gaussian information in denoised maps using one-point probability distribution functions (PDFs) and also perform matching analysis for positive peaks and massive clusters. An ensemble learning technique with our GANs is successfully applied to reproduce the PDFs of the lensing convergence. About $60{{\ \rm per\ cent}}$ of the peaks in the denoised maps with height greater than 5σ have counterparts of massive clusters within a separation of 6 arcmin. We show that PDFs in the denoised maps are not compromised by details of multiplicative biases and photometric redshift distributions, nor by shape measurement errors, and that the PDFs show stronger cosmological dependence compared to the noisy counterpart. We apply our denoising method to a part of the first-year HSC data to show that the observed mass distribution is statistically consistent with the prediction from the standard ΛCDM model.

Funder

MEXT

Japan Science and Technology Agency

National Astronomical Observatory of Japan

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

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