noirlab2603 — Science Release
Four methods for studying dark energy come together in a single experiment for the first time
22 January 2026
The Dark Energy Survey Collaboration collected information on hundreds of millions of galaxies across the Universe using the U.S. Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation Víctor M. Blanco 4-meter Telescope at CTIO, a Program of NSF NOIRLab. Their completed analysis combines all six years of data for the first time and yields constraints on the Universe’s expansion history that are twice as tight as past analyses.
The Dark Energy Survey (DES) is an international, collaborative effort to map hundreds of millions of galaxies, detect thousands of supernovae, and find patterns of cosmic structure that will help reveal the nature of the mysterious dark energy that is accelerating the expansion of our Universe.
From 2013 to 2019, the DES Collaboration carried out a deep, wide-area survey of the sky using the 570-megapixel DOE-fabricated Dark Energy Camera (DECam), mounted on the NSF Víctor M. Blanco 4-meter Telescope at NSF Cerro Tololo Inter-American Observatory (CTIO) in Chile. For 758 nights over six years, the DES Collaboration recorded information from 669 million galaxies that are billions of light-years from Earth, covering an eighth of the sky.
Today, the DES Collaboration is releasing results that, for the first time, combine all six years of data from weak lensing and galaxy clustering probes — two techniques for measuring the Universe’s expansion history. The collaboration also presents the first results found by combining all four methods of measuring the expansion history of the Universe — baryon acoustic oscillations (BAO), Type-Ia supernovae, galaxy clusters, and weak gravitational lensing — as proposed at the inception of DES 25 years ago. The paper, submitted to Physical Review D, represents a summary of 18 supporting papers.
“It is an incredible feeling to see these results based on all the data, and with all four probes that DES had planned. This was something I would have only dared to dream about when DES started collecting data, and now the dream has come true,” says Yuanyuan Zhang, assistant astronomer at NSF NOIRLab and member of the DES Collaboration.
The analysis yields new, tighter constraints that narrow down the possible models for how the Universe behaves. These constraints are more than twice as strong as those from past DES analyses while remaining consistent with previous DES results.
“These results from the Dark Energy Survey shine new light on our understanding of the Universe and its expansion,” said Regina Rameika, Associate Director for the Office of High Energy Physics in the DOE’s Office of Science (DOE/SC). “They demonstrate how long-term investment in research and combining multiple types of analysis can provide insight into some of the Universe’s biggest mysteries.”
The first clue for dark energy was uncovered about a century ago when astronomers noticed that distant galaxies appeared to be moving away from us. In fact, the farther away a galaxy is, the faster it recedes. This provided the first key evidence that the Universe is expanding. But since the Universe is permeated by gravity, a force that pulls matter together, astronomers expected the expansion would slow down over time.
Then, in 1998, two independent teams of cosmologists used distant supernovae to discover that the Universe’s expansion is accelerating rather than slowing. To explain these observations, they proposed a new kind of phenomenon that is responsible for driving the Universe’s accelerated expansion: dark energy. Astrophysicists now believe dark energy makes up about 70% of the mass-energy density of the Universe. Yet, we still know very little about it.
In the following years, scientists began devising experiments to study dark energy, including DES. Today, DES is an international collaboration of over 400 astrophysicists and scientists from 35 institutions in seven countries led by DOE’s Fermi National Accelerator Laboratory.
For the latest results, DES scientists greatly advanced methods using weak lensing to robustly reconstruct the distribution of matter in the Universe. Weak lensing is the distortion of light from distant galaxies due to the gravity of intervening matter, like galaxy clusters. They did this by measuring the probability of two galaxies being a certain distance apart and the probability that they are also distorted similarly by weak lensing. By reconstructing the matter distribution over six billion years of cosmic history, these measurements of weak lensing and galaxy distribution tell scientists how much dark energy and dark matter there is at each moment.
In this analysis, DES tested two models of the Universe against their data. There is the currently accepted standard model of cosmology — Lambda cold dark matter (ΛCDM) — in which the dark energy density is constant. There is also an extended model, in which the dark energy density evolves over time — wCDM.
DES found that their data mostly aligned with the standard model of cosmology. Their data also fit the evolving dark energy model, but no better than they fit the standard model.
However, one parameter is still off. Based on measurements of the early Universe, both the standard and evolving dark energy models predict how matter in the Universe clusters at later times. In previous analyses, galaxy clustering was found to be different from what was predicted. When DES added the most recent data, that gap widened, but not yet to the point of certainty that the standard model of cosmology is incorrect. The difference persisted even when DES combined their data with those of other experiments.
Next, DES will combine this work with the most recent constraints from other dark energy experiments to investigate alternative gravity and dark energy models. This analysis is also important because it paves the way for the new NSF–DOE Vera C. Rubin Observatory, funded by the NSF and DOE/SC, and jointly operated by NSF NOIRLab and SLAC, to collect complementary data during its decade-long Legacy Survey of Space and Time (LSST). LSST is a deep and wide survey that will catalog about 20 billion galaxies across the entire Southern Hemisphere sky. The data can be combined with those from surveys like DES to enable high-accuracy measurements of cosmological parameters that will further refine our understanding of dark energy and the expansion history of the Universe.
“DES has been transformative, and the NSF–DOE Vera C. Rubin Observatory will take us even further,” said Chris Davis, NSF Program Director for NOIRLab. “Rubin’s unprecedented survey of the southern sky will enable new tests of gravity and shed light on dark energy.”
More information
This research is presented in a paper titled “Dark Energy Survey Year 6 Results: Cosmological Constraints from Galaxy Clustering and Weak Lensing,” submitted to Physical Review D and appearing on arXiv.
These results are presented by the DES Collaboration.
NSF NOIRLab, the U.S. National Science Foundation center for ground-based optical-infrared astronomy, operates the International Gemini Observatory (a facility of NSF, NRC–Canada, ANID–Chile, MCTIC–Brazil, MINCyT–Argentina, and KASI–Republic of Korea), NSF Kitt Peak National Observatory (KPNO), NSF Cerro Tololo Inter-American Observatory (CTIO), the Community Science and Data Center (CSDC), and NSF–DOE Vera C. Rubin Observatory (in cooperation with DOE’s SLAC National Accelerator Laboratory). It is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with NSF and is headquartered in Tucson, Arizona.
The scientific community is honored to have the opportunity to conduct astronomical research on I’oligam Du’ag (Kitt Peak) in Arizona, on Maunakea in Hawai‘i, and on Cerro Tololo and Cerro Pachón in Chile. We recognize and acknowledge the very significant cultural role and reverence of I’oligam Du’ag to the Tohono O’odham Nation, and Maunakea to the Kanaka Maoli (Native Hawaiians) community.
This work is supported in part by the U.S. Department of Energy Office of Science. The Dark Energy Survey is a collaboration of more than 400 scientists from 26 institutions in seven countries. Funding for the DES Projects has been provided by the U.S. Department of Energy Office of Science, U.S. National Science Foundation, Ministry of Science and Education of Spain, Science and Technology Facilities Council of the United Kingdom, Higher Education Funding Council for England, ETH Zurich for Switzerland, National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, Kavli Institute of Cosmological Physics at the University of Chicago, Center for Cosmology and AstroParticle Physics at Ohio State University, Mitchell Institute for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and Ministério da Ciência e Tecnologia, Deutsche Forschungsgemeinschaft, and the collaborating institutions in the Dark Energy Survey.
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Contacts
Yuanyuan Zhang
DES Collaboration
NSF NOIRLab
Email: yuanyuan.zhang@noirlab.edu
Josie Fenske
Public Information Officer
NSF NOIRLab
Email: josie.fenske@noirlab.edu
Tracy Marc
Media Relations Manager
Fermilab
Email: tracym@fnal.gov