An ultra-high-resolution map of (dark) matter
Artikel i vetenskaplig tidskrift, 2026
Ordinary matter—including particles such as protons and neutrons—accounts for only about one-sixth of all matter in the Universe. The rest is dark matter, which does not emit or absorb light but plays a fundamental role in galaxy and structure evolution. Because it interacts only through gravity, one of the most direct probes is weak gravitational lensing: the deflection of light from distant galaxies by intervening mass. Here we present an extremely detailed, wide-area weak-lensing mass map covering 0.77° × 0.70°, using high-resolution imaging from the James Webb Space Telescope as part of the COSMOS-Web survey. By measuring the shapes of 129 galaxies per square arcminute—many independently in the F115W and F150W bands—we achieve an angular resolution of 1.00±0.01′. Our map has more than twice the resolution of earlier Hubble Space Telescope maps, revealing how dark and luminous matter co-evolve across filaments, clusters and underdensities. It traces mass features out to z ≈ 2, including the most distant structure at z ≈ 1.1. The sensitivity to high-redshift lensing constrains galaxy environments at the peak of cosmic star formation and sets a high-resolution benchmark for testing theories about the nature of dark matter and the formation of large-scale cosmic structure.
Författare
Diana Scognamiglio
California Institute of Technology (Caltech)
Gavin Leroy
Durham University
David Harvey
Ecole Polytechnique Federale de Lausanne (EPFL)
Richard Massey
Durham University
Jason Rhodes
California Institute of Technology (Caltech)
Hollis B. Akins
University of Texas
Malte Brinch
Millenium Nucleus for Galaxies (MINGAL)
Universidad de Chile (UCH)
Edward Berman
Northeastern University
Caitlin M. Casey
Cosmic Dawn Center (DAWN)
University of Texas
University of California
Nicole E. Drakos
University of Hawaii
A. Faisst
California Institute of Technology (Caltech)
M. Franco
University of Texas
Université Paris-Saclay
Leo W.H. Fung
Durham University
Ghassem Gozaliasl
Aalto-Yliopisto
Helsingin Yliopisto
Qiuhan He
Rijksuniversiteit Groningen
Durham University
Hossein Hatamnia
University of California
Eric Huff
California Institute of Technology (Caltech)
Natalie B. Hogg
University of Cambridge
Laboratoire Univers et Particules de Montpellier
O. Ilbert
Laboratoire d'Astrophysique de Marseille
Jeyhan S. Kartaltepe
Rochester Institute of Technology
Anton M. Koekemoer
Space Telescope Science Institute (STScI)
Shouwen Jin
Danmarks Tekniske Universitet (DTU)
Cosmic Dawn Center (DAWN)
Erini Lambrides
National Aeronautics and Space Administration (NASA)
Alexie Leauthaud
University of California
Zane D. Lentz
Durham University
Daizhong Liu
Chinese Academy of Sciences
Guillaume Mahler
Durham University
Universite de Liège
Claudia Maraston
University of Portsmouth
Crystal L. Martin
University of California
Jacqueline McCleary
Northeastern University
James W. Nightingale
Newcastle University
Bahram Mobasher
University of California
Louise Paquereau
Institut d 'Astrophysique de Paris
Chalmers, Rymd-, geo- och miljövetenskap, Astronomi och plasmafysik
Sandrine Pires
Université Paris-Saclay
Brant Robertson
University of California
D. B. Sanders
University of Hawaii
Claudia Scarlata
University of Minnesota
Marko Shuntov
Niels Bohr Institute
Cosmic Dawn Center (DAWN)
Greta Toni
Universita di Bologna
Universität Heidelberg
Istituto nazionale di astrofisica (INAF)
Maximilian von Wietersheim-Kramsta
Durham University
J. R. Weaver
Massachusetts Institute of Technology (MIT)
University of Massachusetts
Nature Astronomy
23973366 (eISSN)
Vol. 10 4 573-582Infrastruktur
Onsala rymdobservatorium
Ämneskategorier (SSIF 2025)
Astronomi, astrofysik och kosmologi
DOI
10.1038/s41550-025-02763-9