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Record W4414508655 · doi:10.1093/mnras/staf1630

The PAU Survey: measuring intrinsic galaxy alignments in deep wide fields as a function of colour, luminosity, stellar mass, and redshift

2025· article· en· W4414508655 on OpenAlexaboutno aff
D Navarro-Gironés, Anna Wittje, M. Siudek, Henk Hoekstra, H. Hildebrandt, Benjamin Joachimi, Romain Paviot, C. M. Baugh, J. Carretero, Raquel Casas, F. J. Castander, Martin Eriksen, E. Fernández, P. Fosalba, J. García-Bellido, R. Miquel, Pablo Renard, S. Serrano, I. Sevilla-Noarbe, P. Tallada-Crespí

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsnot available
FundersH2020 European Research CouncilIntegrated Electronics Engineering Center, Binghamton UniversityAgencia Estatal de InvestigaciónInstitut de Física d'Altes EnergiesNarodowa Agencja Wymiany AkademickiejUniversitat Autònoma de BarcelonaMinisterio de Economía y CompetitividadNational Key Research and Development Program of ChinaUniversity College LondonEidgenössische Technische Hochschule ZürichDeutsches Zentrum für Luft- und RaumfahrtMinisterio de Ciencia e InnovaciónGeneralitat de CatalunyaDurham UniversityUniversiteit LeidenTsinghua UniversityNederlandse Organisatie voor Wetenschappelijk OnderzoekEuropean Regional Development FundEuropean CommissionCentres de Recerca de CatalunyaDeutsche ForschungsgemeinschaftCentro de Investigaciones Energéticas, Medioambientales y TecnológicasUK Research and Innovation
KeywordsRedshiftGalaxyLuminosity functionLuminosityRedshift surveyPhotometric redshiftUniversePopulationAmplitudeGalaxy formation and evolution

Abstract

fetched live from OpenAlex

ABSTRACT We present the measurements and constraints of intrinsic alignments (IAs) in the Physics of the Accelerating Universe Survey (PAUS) deep wide fields, which include the W1 and W3 fields from the Canada–France–Hawaii Telescope Legacy Survey (CFHTLS) and the G09 field from the Kilo-Degree Survey (KiDS). Our analyses cover 51deg$^{2}$, in the photometric redshift (photo-z) range $0.1 < z_{\mathrm{b}} < 1$ and a magnitude limit $i_{\mathrm{AB}}< 22$. The precise photo-zs and the luminosity coverage of PAUS enable robust IA measurements, which are key for setting informative priors for upcoming stage-IV surveys. For red galaxies, we detect an increase in IA amplitude with both luminosity and stellar mass, extending previous results towards fainter and less massive regimes. As a function of redshift, we observe strong IA signals at intermediate ($z_{\mathrm{b}}\sim 0.55$) and high ($z_{\mathrm{b}}\sim 0.75$) redshift bins. However, we find no significant trend of IA evolution with redshift after accounting for the varying luminosities across redshift bins, consistent with the literature. For blue galaxies, no significant IA signal is detected, with $A_{1}=0.68_{-0.51}^{+0.53}$ when splitting only by galaxy colour, yielding some of the tightest constraints to date for the blue population and constraining a regime of very faint and low-mass galaxies.

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)0.002
Version: metacan-v3-hybrid-931329e0061cValidation 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: Empirical
Teacher disagreement score0.009
Threshold uncertainty score0.019

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
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 head0.009
GPT teacher head0.225
Teacher spread0.216 · 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 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

Citations2
Published2025
Admission routes1
Has abstractyes

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