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Record W4414487633 · doi:10.1088/1475-7516/2025/11/049

Enhancing DESI DR1 full-shape analyses using HOD-informed priors

2025· article· en· W4414487633 on OpenAlexafffund
Marco Bonici, A. Rocher, Will J. Percival, Arnaud de Mattia, J. Aguilar, S. P. Ahlen, Otávio Alves, Alejandro Avilés, Antón Baleato Lizancos, D. Bianchi, David J. Brooks, Andrei Cuceu, Axel de la Macorra, P. Doel, Simone Ferraro, N. Findlay, Andreu Font-Ribera, J. E. Forero-Romero, Satya Gontcho A Gontcho, G. Gutiérrez, ChangHoon Hahn, Cullan Howlett, Mustapha Ishak, Minas Karamanis, R. Kehoe, D. Kirkby, Anthony Kremin, O. Lahav, Yan Lai, Martin Landriau, L. Le Guillou, M. E. Levi, Marc Manera, M Maus, Aaron Meisner, Ramon Miquel, James Morawetz, John Moustakas, S. Nadathur, Jeffrey A. Newman, Gustavo Niz, H. E. Noriega, N. Palanque‐Delabrouille, Mathilde Pinon, Francisco Prada, Ignasi Pérez-Ràfols, Graziano Rossi, Shun Saito, Lado Samushia, E. Sánchez, David J. Schlegel, M. Schubnell, Hee‐Jong Seo, David Sprayberry, G. Tarlé, Benjamin Alan Weaver, Ruiyang Zhao, Rongpu Zhou

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
FundersDivision of Astronomical SciencesAgencia Estatal de InvestigaciónScience and Technology Facilities CouncilCanadian Space AgencyOffice of ScienceAlliance de recherche numérique du CanadaSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungU.S. Department of EnergyGordon and Betty Moore FoundationMinisterio de Ciencia, Innovación y UniversidadesNational Aeronautics and Space AdministrationNatural Sciences and Engineering Research Council of CanadaInstitut Périmètre de physique théoriqueCommissariat à l'Énergie Atomique et aux Énergies AlternativesInnovation, Science and Economic Development CanadaMinistry of Colleges and UniversitiesGovernment of CanadaNational Science Foundation
KeywordsPrior probabilityDark energyCosmologyBaryon acoustic oscillationsSpectral densityPosterior probabilityGaussianBayesian probabilityPerturbation (astronomy)

Abstract

fetched live from OpenAlex

Abstract We present an analysis of DESI Data Release 1 (DR1) that incorporates Halo Occupation Distribution (HOD)-informed priors into Full-Shape (FS) modeling of the power spectrum based on cosmological perturbation theory (PT). By leveraging physical insights from the galaxy-halo connection, these HOD-informed priors on nuisance parameters substantially mitigate projection effects in extended cosmological models that allow for dynamical dark energy. The resulting credible intervals now encompass the posterior maximum from the baseline analysis using gaussian priors, eliminating a significant posterior shift observed in baseline studies. In the ΛCDM framework, a combined DESI DR1 FS information and constraints from the DESI DR1 baryon acoustic oscillations (BAO) — including Big Bang Nucleosynthesis (BBN) constraints and a weak prior on the scalar spectral index — yields Ω m = 0.2994 ± 0.0090 and σ 8 = 0.836 +0.024 -0.027 , representing improvements of approximately 4% and 23% over the baseline analysis, respectively. For the w 0 w a CDM model, our results from various data combinations are highly consistent, with all configurations converging to a region with w 0 > -1 and w a < 0. This convergence not only suggests intriguing hints of dynamical dark energy but also underscores the robustness of our HOD-informed prior approach in delivering reliable cosmological constraints.

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)0.010
metaresearch head score (Gemma)0.026
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: Simulation or modeling
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.011
Threshold uncertainty score0.053

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0100.026
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.002
Bibliometrics0.0020.002
Science and technology studies0.0010.001
Scholarly communication0.0020.002
Open science0.0020.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0060.002

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 head0.028
GPT teacher head0.351
Teacher spread0.323 · 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 designSimulation or modeling
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

Citations7
Published2025
Admission routes2
Has abstractyes

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