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Record W4414685054 · doi:10.1103/3f1p-spfp

Cosmology with second- and third-order shear statistics for the Dark Energy Survey: Methods and simulated analysis

2025· article· en· W4414685054 on OpenAlexaff
Rafael C. H. Gomes, S. Sugiyama, Bhuvnesh Jain, Mike Jarvis, Dhayaa Anbajagane, M. Gatti, D. Gebauer, Zengtai Gong, Ashadul Halder, Gabriela A. Marques, S. Pandey, J. L. Marshall, S. Allam, O. Alves, F. Andrade-Oliveira, D. Bacon, J Blazek, S. Bocquet, D. Brooks, A. Carnero Rosell, J. Carretero, L. N. da Costa, P. Doel, C. Doux, S Everett, B Flaugher, J Frieman, J García-Bellido, E. Gaztañaga, D. Gruen, R. A. Gruendl, G Gutierrez, K. Herner, S. R. Hinton, K Honscheid, Dragan Huterer, D.J James, N Jeffrey, J. Mena-Fernández, Aaron Meisner, J. Muir, R. L. C. Ogando, M. E. S. Pereira, A. Pieres, S Samuroff, E. Sánchez, D. Sanchez Cid, B. Santiago, I Sevilla-Noarbe, M Smith, M. E. C. Swanson, G. Tarlé, C. To, V. Vikram, N. Weaverdyck, J. Weller

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsPerimeter InstituteInstitute of Particle Physics
FundersMitchell InstituteDeutsche ForschungsgemeinschaftHigh Energy PhysicsOffice of ScienceConselho Nacional de Desenvolvimento Científico e TecnológicoInstituto Nacional de Ciência e Tecnologia: Física Nuclear e AplicaçõesCenter for Cosmology and Astroparticle Physics, Ohio State UniversityMinistério da Ciência, Tecnologia e InovaçãoNational Aeronautics and Space AdministrationHigher Education Funding Council for EnglandTexas A and M UniversityUniversity of ChicagoBread and Roses Community FundUniversity of Illinois at Urbana-ChampaignFinanciadora de Estudos e ProjetosFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroMinisterio de Ciencia, Innovación y UniversidadesScience and Technology Facilities CouncilNational Centre for Supercomputing ApplicationsEuropean Regional Development FundU.S. Department of EnergyMinisterio de Ciencia e InnovaciónGeneralitat de CatalunyaFermilabNational Science Foundation
KeywordsDark energyCosmologyShear (geology)ScalingCovariance matrixMeasure (data warehouse)RedshiftStatisticIntensity mapping

Abstract

fetched live from OpenAlex

We present a new pipeline designed for the robust inference of cosmological parameters using both second- and third-order shear statistics. We build a theoretical model for rapid evaluation of three-point correlations using our fastnc code and integrate it into the cosmosis framework. We measure the two-point functions ${\ensuremath{\xi}}_{\ifmmode\pm\else\textpm\fi{}}$ and the full configuration-dependent three-point shear correlation functions across all auto- and cross-redshift bins. We compress the three-point functions into the mass aperture statistic $⟨{\mathcal{M}}_{\mathrm{ap}}^{3}⟩$ for a set of 796 simulated shear maps designed to model the Dark Energy Survey Year 3 data. We estimate from it the full covariance matrix and model the effects of intrinsic alignments, shear calibration biases and photometric redshift uncertainties. We apply scale cuts to minimize the contamination from the baryonic signal as modeled through hydrodynamical simulations. We find a significant improvement of 83% on the figure of merit in the ${\mathrm{\ensuremath{\Omega}}}_{\mathrm{m}}\text{\ensuremath{-}}{S}_{8}$ plane when we add the $⟨{\mathcal{M}}_{\mathrm{ap}}^{3}⟩$ data to ${\ensuremath{\xi}}_{\ifmmode\pm\else\textpm\fi{}}$. We present our findings for all relevant cosmological and systematic uncertainty parameters and discuss the complementarity of third-order and second-order statistics.

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)0.013
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: Methods · Consensus signal: Methods
Teacher disagreement score0.021
Threshold uncertainty score0.042

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.013
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0020.002
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0070.001

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 head0.014
GPT teacher head0.447
Teacher spread0.433 · 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
GenreMethods

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

Citations4
Published2025
Admission routes1
Has abstractyes

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