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Record W4399115505 · doi:10.1088/1475-7516/2025/01/146

Forward modeling fluctuations in the DESI LRGs target sample using image simulations

2025· article· en· W4399115505 on OpenAlexaff
Hui Kong, Ashley J. Ross, K. Honscheid, Dustin Lang, A. Porredon, Arnaud de Mattia, Mehdi Rezaie, E. F. Schlafly, John Moustakas, A. Rosado-Marin, S. P. Ahlen, D. Brooks, E. Chaussidon, T. Claybaugh, Shaun Cole, Axel de la Macorra, Arjun Dey, Biprateep Dey, Peter Doel, J. E. Forero-Romero, E. Gaztañaga, Satya Gontcho A Gontcho, G. Gutierrez, Cullan Howlett, S. Juneau, M. Landriau, M. E. Levi, Marc Manera, Paul Martini, Aaron Meisner, R Miquel, Eva-Maria Mueller, A. D. Myers, J. A. Newman, Jundan Nie, G. Niz, Will J. Percival, Claire Poppett, F. Prada, E. Sanchez, D. Schlegel, M. Schubnell, D. Sprayberry, G. Tarlé, M. Vargas-Magaña, B. A. Weaver, Hu Zou

Bibliographic record

VenueJournal of Cosmology and Astroparticle Physics · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGamma-ray bursts and supernovae
Canadian institutionsRegional Municipality of WaterlooPerimeter InstituteUniversity of Waterloo
FundersLawrence Berkeley National LaboratoryHigh Energy PhysicsDivision of Astronomical SciencesAgencia Estatal de InvestigaciónScience and Technology Facilities CouncilHORIZON EUROPE Framework ProgrammeJet Propulsion LaboratoryMinisterio de Ciencia e InnovaciónCommissariat à l'Énergie Atomique et aux Énergies AlternativesChinese Academy of SciencesU.S. Department of EnergyCalifornia Institute of TechnologyEuropean CommissionNational Energy Research Scientific Computing CenterOffice of ScienceNational Aeronautics and Space AdministrationGordon and Betty Moore FoundationNational Science Foundation
KeywordsSample (material)Image (mathematics)Computer scienceArtificial intelligenceAcousticsPhysics

Abstract

fetched live from OpenAlex

Abstract We use the forward modeling pipeline, Obiwan, to study the imaging systematics of the Luminous Red Galaxies (LRGs) targeted by the Dark Energy Spectroscopic Instrument (DESI). Imaging systematics refers to the false fluctuation of galaxy densities due to varying observing conditions and astrophysical foregrounds corresponding to the imaging surveys from which DESI LRG target galaxies are selected. We update the Obiwan pipeline, which we previously developed to simulate the optical images used to target DESI data, to further simulate WISE images in the infrared. This addition allows simulating the DESI LRGs sample, which utilizes WISE data in the target selection. Deep DESI imaging data combined with a method to account for biases in their shapes is used to define a truth sample of potential LRG targets. We inject these data evenly throughout the DESI Legacy Imaging Survey footprint at declinations between -30 and 32.375 degrees. We simulate a total of 15 million galaxies to obtain a simulated LRG sample (Obiwan LRGs) that predicts the variations in target density due to imaging properties. We find that the simulations predict the trends with depth observed in the data, including how they depend on the intrinsic brightness of the galaxies. We observe that faint LRGs are the main contributing source of the imaging systematics trend induced by depth. We also find significant trends in the data against Galactic extinction that are not predicted by Obiwan. These trends depend strongly on the particular map of Galactic extinction chosen to test against, implying systematic contamination in the Galactic extinction maps is a likely root cause (e.g., Cosmic-Infrared Background, dust temperature correction). We additionally observe a morphological change of the DESI LRGs population evidenced by a correlation between OII emission line average intensity and the size of the z-band PSF. This effect most likely results from uncertainties in background subtraction. The detailed findings we present should be used to guide any observational systematics mitigation treatment for the clustering of the DESI LRGs sample.

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)0.001
metaresearch head score (Gemma)0.006
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 score0.060
Threshold uncertainty score0.119

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.006
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0010.001
Open science0.0020.001
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0020.000

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 head0.024
GPT teacher head0.293
Teacher spread0.269 · 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

Citations9
Published2025
Admission routes1
Has abstractyes

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