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Record W4394007100 · doi:10.1088/1475-7516/2025/01/133

HOD-dependent systematics for luminous red galaxies in the DESI 2024 BAO analysis

2025· article· en· W4394007100 on OpenAlexaff
J. Mena-Fernández, C. García-Quintero, Sihan Yuan, Boryana Hadzhiyska, O. Alves, M. Rashkovetskyi, Hee‐Jong Seo, Nikhil Padmanabhan, S. Nadathur, Cullan Howlett, Shadab Alam, A. Rocher, Ashley J. Ross, E. Sánchez, M Ishak, J. Aguilar, S. P. Ahlen, U. Andrade, S. BenZvi, D. Brooks, E. Burtin, S. Chen, Xinyi Chen, T. Claybaugh, Shaun Cole, Axel de la Macorra, Arnaud de Mattia, Arjun Dey, Biprateep Dey, Z. Ding, P. Doel, K. Fanning, J. E. Forero-Romero, E. Gaztañaga, Héctor Gil-Marín, Satya Gontcho A Gontcho, G. Gutierrez, J. Guy, ChangHoon Hahn, K. Honscheid, S. Juneau, Anthony Kremin, M. Landriau, L. Le Guillou, M. E. Levi, Marc Manera, Paul Martini, L. Medina-Varela, Aaron Meisner, R. Miquel, John Moustakas, Eva-Maria Mueller, A. Muñoz-Gutiérrez, Adam D. Myers, Jeffrey A. Newman, J. Nie, Gustavo Niz, E. Paillas, N. Palanque‐Delabrouille, Will J. Percival, Claire Poppett, A. Rosado-Marin, Graziano Rossi, Rossana Ruggeri, Christoph Saulder, David J. Schlegel, M. Schubnell, David Sprayberry, G. Tarlé, M. Vargas-Magaña, B. A. Weaver, Jiaxi Yu, H. Zhang, 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
FundersDivision of Astronomical SciencesScience and Technology Facilities CouncilOffice of ScienceMinisterio de Ciencia e InnovaciónFermilabHigh Energy PhysicsGordon and Betty Moore FoundationU.S. Department of EnergyLawrence Berkeley National LaboratoryCommissariat à l'Énergie Atomique et aux Énergies AlternativesNational Science Foundation
KeywordsSystematicsGalaxyAstrophysicsPhysicsAstronomyBiologyEcologyTaxonomy (biology)

Abstract

fetched live from OpenAlex

Abstract In this paper, we present the estimation of systematics related to the halo occupation distribution (HOD) modeling in the baryon acoustic oscillations (BAO) distance measurement of the Dark Energy Spectroscopic Instrument (DESI) 2024 analysis. This paper focuses on the study of HOD systematics for luminous red galaxies (LRG). We consider three different HOD models for LRGs, including the base 5-parameter vanilla model and two extensions to it, that we refer to as baseline and extended models. The baseline model is described by the 5 vanilla HOD parameters, an incompleteness factor and a velocity bias parameter, whereas the extended one also includes a galaxy assembly bias and a satellite profile parameter. We utilize the 25 dark matter simulations available in the AbacusSummit simulation suite at z=0.8 and generate mock catalogs for our different HOD models. To test the impact of the HOD modeling in the position of the BAO peak, we run BAO fits for all these sets of simulations and compare the best-fit BAO-scaling parameters α iso and α AP between every pair of HOD models. We do this for both Fourier and configuration spaces independently, using post-reconstruction measurements. We find a 3.3σ detection of HOD systematic for α AP in configuration space with an amplitude of 0.19%. For the other cases, we did not find a 3σ detection, and we decided to compute a conservative estimation of the systematic using the ensemble of shifts between all pairs of HOD models. By doing this, we quote a systematic with an amplitude of 0.07% in α iso for both Fourier and configuration spaces; and of 0.09% in α AP for Fourier space.

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)0.002
metaresearch head score (Gemma)0.004
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.016

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.004
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.011
GPT teacher head0.249
Teacher spread0.238 · 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

Citations16
Published2025
Admission routes1
Has abstractyes

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