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Record W4394007104 · doi:10.1088/1475-7516/2025/01/145

Semi-analytical covariance matrices for two-point correlation function for DESI 2024 data

2025· article· en· W4394007104 on OpenAlexaff
M. Rashkovetskyi, D. Forero-Sánchez, Arnaud de Mattia, Daniel J. Eisenstein, Nikhil Padmanabhan, Hee‐Jong Seo, Ashley J. Ross, J. Aguilar, S. P. Ahlen, O. Alves, U. Andrade, David J. Brooks, E. Burtin, T. Claybaugh, Shaun Cole, Axel de la Macorra, Z. Ding, P. Doel, K. Fanning, Simone Ferraro, Andreu Font-Ribera, C. García-Quintero, Héctor Gil-Marín, G. Gutiérrez, K. Honscheid, Cullan Howlett, S. Juneau, Anthony Kremin, L. Le Guillou, Marc Manera, L. Medina-Varela, J. Mena-Fernández, R. Miquel, Eva-Maria Mueller, A. Muñoz-Gutiérrez, Jundan Nie, Gustavo Niz, E. Paillas, Claire Poppett, Mehdi Rezaie, A.J Rosado-Marín, Graziano Rossi, Rossana Ruggeri, E. Sánchez, Christoph Saulder, David J. Schlegel, M. Schubnell, David Sprayberry, G. Tarlé, Jiaxi Yu, Cheng Zhao, Hu Zou

Bibliographic record

VenueJournal of Cosmology and Astroparticle Physics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsRegional Municipality of WaterlooPerimeter InstituteUniversity of Waterloo
FundersLawrence Berkeley National LaboratoryDivision of Astronomical SciencesScience and Technology Facilities CouncilCommissariat à l'Énergie Atomique et aux Énergies AlternativesMinisterio de Ciencia e InnovaciónFermilabHigh Energy PhysicsSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungU.S. Department of EnergyGordon and Betty Moore FoundationOffice of ScienceNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPhysicsCovarianceCovariance matrixCorrelation function (quantum field theory)Covariance functionDark energyGaussianGalaxyStatistical physicsEstimation of covariance matricesCosmologyAlgorithmStatisticsAstrophysicsMathematicsQuantum mechanics

Abstract

fetched live from OpenAlex

Abstract We present an optimized way of producing the fast semi-analytical covariance matrices for the Legendre moments of the two-point correlation function, taking into account survey geometry and mimicking the non-Gaussian effects. We validate the approach on simulated (mock) catalogs for different galaxy types, representative of the Dark Energy Spectroscopic Instrument (DESI) Data Release 1, used in 2024 analyses. We find only a few percent differences between the mock sample covariance matrix and our results, which can be expected given the approximate nature of the mocks, although we do identify discrepancies between the shot-noise properties of the DESI fiber assignment algorithm and the faster approximation (emulator) used in the mocks. Importantly, we find a close agreement (≤ 8% relative differences) in the projected errorbars for distance scale parameters for the baryon acoustic oscillation measurements. This confirms our method as an attractive alternative to simulation-based covariance matrices, especially for non-standard models or galaxy sample selections, making it particularly relevant to the broad current and future analyses of DESI data.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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: none
Teacher disagreement score0.536
Threshold uncertainty score0.396

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.001
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.022
GPT teacher head0.284
Teacher spread0.262 · 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 teacher head, 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

Citations27
Published2025
Admission routes1
Has abstractyes

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