DECADE+DES Y3 Weak Lensing Mass Map: A 13,000 deg$^2$ View of Cosmic Structure from 270 Million Galaxies

We present the largest galaxy weak lensing mass map of the late-time Universe, reconstructed from 270 million galaxies in the DECADE and DES Year 3 datasets, covering 13,000 square degrees. We validate the map through systematic tests against observational conditions (depth, seeing, etc.), finding the map is statistically consistent with no contamination. The large area covered by the mass map makes it a well-suited tool for cosmological analyses, cross-correlation studies and the identification of large-scale structure features. We demonstrate its potential by detecting cosmic filaments directly from the mass map for the first time and validating them through their association with galaxy clusters selected using the Sunyaev-Zeldovich effect from Planck and ACT DR6.

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ArXiv.org
Published
2025-09-04
Primary Topic
Astronomy and Astrophysical Research
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article

DECADE+DES Y3 Weak Lensing Mass Map: A 13,000 deg$^2$ View of Cosmic Structure from 270 Million Galaxies

Kai Herron, G. E. Medina, M. Gatti, M. Adamów et al.
ArXiv.org
Astronomy and Astrophysical Research
article

DECADE+DES Y3 Weak Lensing Mass Map: A 13,000 deg$^2$ View of Cosmic Structure from 270 Million Galaxies

Kai Herron, G. E. Medina, M. Gatti, M. Adamów, M. R. Becker, D. Gruen, C. E. Martínez-Vázquez, S. Mau, J. Prat, R.A Gruendl, Pol Massana, C. Chang, Rayane Brinck Teixeira, J. A. Carballo-Bello, Nathalie Chicoine, J. McCullough, Andrew B. Pace, D.J James, N Jeffrey, Burçı̇n Mutlu-Pakdı̇l, C.Y. Tan, P. S. Ferguson, L. F. Secco, David Bacon, Dhayaa Anbajagane, G. S. Stringfellow, A. Drlica-Wagner, Noelia E. D. Noël, A. Alarcon, Erik Tollerud, Attila Kovács, L Whiteway, C. Doux, A. Zenteno, G Pollina, Z. Zhang, D Suson, M.A Troxel, A. H. Riley, D. J. Sand
article en

Abstract

We present the largest galaxy weak lensing mass map of the late-time Universe, reconstructed from 270 million galaxies in the DECADE and DES Year 3 datasets, covering 13,000 square degrees. We validate the map through systematic tests against observational conditions (depth, seeing, etc.), finding the map is statistically consistent with no contamination. The large area covered by the mass map makes it a well-suited tool for cosmological analyses, cross-correlation studies and the identification of large-scale structure features. We demonstrate its potential by detecting cosmic filaments directly from the mass map for the first time and validating them through their association with galaxy clusters selected using the Sunyaev-Zeldovich effect from Planck and ACT DR6.

ArXiv.org
Laboratoire de Physique Subatomique et de Cosmologie (FR)
Openalex Percentile: Top 72%
Astronomy and Astrophysical Research
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