Deep learning reconstruction of three-dimensional galaxy distributions with intensity mapping observations
Kana Moriwaki, Naoki Yoshida

TL;DR
This paper introduces a deep learning GAN approach to reconstruct three-dimensional galaxy distributions from intensity mapping data, effectively addressing line confusion and enabling accurate galaxy identification at high redshifts.
Contribution
The study develops a novel GAN architecture that decomposes overlapping emission lines in 3D intensity maps, improving galaxy distribution reconstruction from noisy observational data.
Findings
Achieves 84% precision in identifying bright galaxies.
Cross-correlation coefficients reach up to 0.8 between true and reconstructed maps.
Successfully reconstructs galaxy distributions at redshifts 1.3-2.4.
Abstract
Line intensity mapping is emerging as a novel method that can measure the collective intensity fluctuations of atomic/molecular line emission from distant galaxies. Several observational programs with various wavelengths are ongoing and planned, but there remains a critical problem of line confusion; emission lines originating from galaxies at different redshifts are confused at the same observed wavelength. We devise a generative adversarial network that extracts designated emission line signals from noisy three-dimensional data. Our novel network architecture allows two input data, in which the same underlying large-scale structure is traced by two emission lines of H and [OIII], so that the network learns the relative contributions at each wavelength and is trained to decompose the respective signals. After being trained with a large number of realistic mock catalogs, the…
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