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Record W4394029306 · doi:10.1088/1475-7516/2025/02/021

DESI 2024 VI: cosmological constraints from the measurements of baryon acoustic oscillations

2025· article· en· W4394029306 on OpenAlexaff
A. G. Adame, José Edgar Madriz Aguilar, S. Ahlen, Shadab Alam, D. M. Alexander, M. A. Álvarez, O. Alves, Abhijeet Anand, U. Andrade, S. Àvila, Alejandro Avilés, H. Awan, Benedict Bahr-Kalus, S. Bailey, C. Baltay, A. Bault, J. Behera, S. BenZvi, Apurba Bera, Florian Beutler, Davide Bianchi, Chris Blake, Robert Blum, S. Brieden, A. Brodzeller, D. Brooks, E. Buckley‐Geer, E. Burtin, R. Calderón, R. Canning, A. Carnero Rosell, R. Cereskaite, Jorge L. Cervantes–Cota, Solène Chabanier, E. Chaussidon, J. Chaves-Montero, Shi-Fan Chen, X. Chen, T. Claybaugh, Shaun Cole, Andrei Cuceu, T. M. Davis, Kyle Dawson, Axel de la Macorra, Arnaud de Mattia, N. Deiosso, A. Dey, Biprateep Dey, Z. Ding, P. Doel, J. Edelstein, Sarah Eftekharzadeh, Daniel J. Eisenstein, A. Elliott, P. Fagrelius, J. Ereza, N. Findlay, B. Flaugher, Andreu Font-Ribera, D. Forero-Sánchez, J. E. Forero-Romero, Carlos S. Frenk, C. García-Quintero, E. Gaztañaga, Héctor Gil-Marín, Satya Gontcho A Gontcho, Alma X. González‐Morales, Violeta González-Pérez, D. Green, D. Gruen, Rafaela Gsponer, G. Gutierrez, J. Guy, Boryana Hadzhiyska, Chang Hoon Hahn, M. Hanif, H. K. Herrera-Alcantar, K. Honscheid, Cullan Howlett, Dragan Huterer, Vid Iršič, Mustapha Ishak, S. Juneau, Naim Göksel Karaçaylı, R. Kehoe, S. Kent, D. Kirkby, Anthony Kremin, Alex Krolewski, Ying‐Cheng Lai, Ting-Wen Lan, M. Landriau, Dustin Lang, J. Lasker, J.M. Le Goff, L. Le Guillou, A. Leauthaud, M. E. Levi, Ting S. Li, E. Linder, K. Lodha, C. Magneville, Marc Manera, Daniel Margala, Paul Martini, M. Maus, Patrick McDonald, L. Medina-Varela, Aaron Meisner, J. Mena-Fernández, R. Miquel, J. Moon, S. Moore, John Moustakas, Eva-Maria Mueller, A. Muñoz-Gutiérrez, S. Nadathur, L. Napolitano, Richard Neveux, Jundan Nie, G. Niz, Nikhil Padmanabhan, E. Paillas, N. Palanque‐Delabrouille, S. Penmetsa, Michele Pinon, C. Poppett, A. Porredon, Francisco Prada, Ignasi Pérez-Ràfols, D. Rabinowitz, A. Raichoor, C. Ramírez-Pérez, S. Ramírez-Solano, M. Rashkovetskyi, C. Ravoux, Mehdi Rezaie, J. Rich, A. Rocher, Constance M. Rockosi, A. Rosado-Marin, Graziano Rossi, Rossana Ruggeri, V. Ruhlmann-Kleider, Lado Samushia, E. Sánchez, Christoph Saulder, David J. Schlegel, M. Schubnell, Hee‐Jong Seo, Arman Shafieloo, R. M. Sharples, J. Silber, A. Slosar, A. G. Smith, D. Sprayberry, T. Tan, G. Tarlé, Peter L. Taylor, S. Trusov, R. Vaisakh, D. Valcin, F. Valdés, M. Vargas-Magaña, Licia Verde, Michael Walther, B. Wang, N. Weaverdyck, Martin White, Jiaxi Yu, Y. Yu, Sihan Yuan, Christophe Yèche, Pauline Zarrouk, Hanyu Zhang, Cheng Zhao, Rongpu Zhou, Ting Zhuang, Hu Zou

Bibliographic record

VenueJournal of Cosmology and Astroparticle Physics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsRegional Municipality of WaterlooPerimeter InstituteUniversity of Waterloo
FundersFermilabHigh Energy PhysicsInstitut de Ciències del CosmosDivision of Astronomical SciencesScience and Technology Facilities CouncilOffice of ScienceCommissariat à l'Énergie Atomique et aux Énergies AlternativesUniversitat de BarcelonaMinisterio de Ciencia e InnovaciónIntegrated Electronics Engineering Center, Binghamton UniversityGordon and Betty Moore FoundationU.S. Department of EnergyInstituto de Astrofísica de AndalucíaNational Science Foundation
KeywordsPhysicsCosmic microwave backgroundDark energyBaryon acoustic oscillationsHubble's lawAstrophysicsRedshiftPlanckEquation of stateBaryonOmegaGalaxyHorizonCosmologyAnisotropyAstronomyQuantum mechanics

Abstract

fetched live from OpenAlex

Abstract We present cosmological results from the measurement of baryon acoustic oscillations (BAO) in galaxy, quasar and Lyman- α forest tracers from the first year of observations from the Dark Energy Spectroscopic Instrument (DESI), to be released in the DESI Data Release 1. DESI BAO provide robust measurements of the transverse comoving distance and Hubble rate, or their combination, relative to the sound horizon, in seven redshift bins from over 6 million extragalactic objects in the redshift range 0.1 < z < 4.2. To mitigate confirmation bias, a blind analysis was implemented to measure the BAO scales. DESI BAO data alone are consistent with the standard flat ΛCDM cosmological model with a matter density Ω m =0.295±0.015. Paired with a baryon density prior from Big Bang Nucleosynthesis and the robustly measured acoustic angular scale from the cosmic microwave background (CMB), DESI requires H 0 =(68.52±0.62) km s -1 Mpc -1 . In conjunction with CMB anisotropies from Planck and CMB lensing data from Planck and ACT, we find Ω m =0.307± 0.005 and H 0 =(67.97±0.38) km s -1 Mpc -1 . Extending the baseline model with a constant dark energy equation of state parameter w , DESI BAO alone require w =-0.99 +0.15 -0.13 . In models with a time-varying dark energy equation of state parametrised by w 0 and w a , combinations of DESI with CMB or with type Ia supernovae (SN Ia) individually prefer w 0 > -1 and w a < 0. This preference is 2.6 σ for the DESI+CMB combination, and persists or grows when SN Ia are added in, giving results discrepant with the ΛCDM model at the 2.5 σ , 3.5 σ or 3.9 σ levels for the addition of the Pantheon+, Union3, or DES-SN5YR supernova datasets respectively. For the flat ΛCDM model with the sum of neutrino mass ∑ m ν free, combining the DESI and CMB data yields an upper limit ∑ m ν < 0.072 (0.113) eV at 95% confidence for a ∑ m ν > 0 (∑ m ν > 0.059) eV prior. These neutrino-mass constraints are substantially relaxed if the background dynamics are allowed to deviate from flat ΛCDM.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.003
metaresearch head score (Gemma)0.003
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.009
Threshold uncertainty score0.031

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.003
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0090.005

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.024
GPT teacher head0.282
Teacher spread0.258 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations953
Published2025
Admission routes1
Has abstractyes

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