Cited by 38Cosmology and Gravitation TheoriesImage and Signal Denoising MethodsGalaxies: Formation, Evolution, Phenomena

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

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Shirasaki, Masato, Moriwaki, Kana, Oogi, Taira, Yoshida, Naoki, Ikeda, Shiro, Nishimichi, Takahiro·2021·Monthly Notices of the Royal Astronomical Society

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.

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Crossref · 10.1093/mnras/stab982

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  • Shirasaki et al. (2021) found that about 60% of peaks identified on denoised maps have significant clusters counterparts, against about 85% of positive matches on true maps.

    “On simulations the authors find that about 60% of the peaks identified on the denoised maps have significant clusters counterparts, against about 85% of positive matches on true maps”

    From The Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys (2023) · cites this paper as Shirasaki et al. (2021)

  • The adversarial model in Shirasaki et al. is not a generative model; the denoiser does not take random variables as input and is therefore deterministic.

    “It is to be noted here that this adversarial model is not a generative model, the denoiser does not take random variables as an input and is therefore deterministic.”

    From The Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys (2023) · cites this paper as Shirasaki et al. (2021)

  • Shirasaki et al. (2021) showed that the 1-point statistics of the recovered map shows stronger cosmological dependence than the noisy maps.

    “the authors further show that the 1-point statistics of the recovered map shows stronger cosmological dependence than the noisy maps”

    From The Dawes Review 10: The impact of deep learning for the analysis of galaxy surveys (2023) · cites this paper as Shirasaki et al. (2021)

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Authors
Shirasaki, M., Moriwaki, K., Oogi, T., Yoshida, N., Ikeda, S., & Nishimichi, T.
Affiliations
  • The Institute of Statistical Mathematics (JP)
  • The University of Tokyo (JP)
  • Chiba University (JP)
  • Kavli Institute for the Physics and Mathematics of the Universe (JP)
  • The Graduate University for Advanced Studies, SOKENDAI (JP)
Corresponding author
Shirasaki, Masato
Venue
Monthly Notices of the Royal Astronomical Society
Published
2021-04-09
Volume
504
Issue
2
Pages
1825-1839
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W3151390452
Cited by
38
References
4
Citations by year
2026: 5 · 2025: 9 · 2024: 8 · 2023: 8 · 2022: 6 · 2021: 1 · 2020: 1
FWCI
3.09
Type
journal article
Language
en
Open access
Locations
  • Monthly Notices of the Royal Astronomical Society (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • MEXT (18H04358, 19K14767)
  • Japan Science and Technology Agency (JPMJCR1414, JP20317829, JP17K14273, JP19H00677)
  • National Astronomical Observatory of Japan
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Computer Science › Computer Vision and Pattern Recognition › Image and Signal Denoising Methods
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Keywords
weak gravitational lensing, generative adversarial networks, conditional generative adversarial networks, image-to-image translation, cluster matching, multiplicative bias, Hyper Suprime-Cam, mock catalogues

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