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Record W4417172151 · doi:10.48550/arxiv.2504.20722

Cosmology from LOFAR Two-metre Sky Survey Data Release 2: Cross-correlations with luminous red galaxies from eBOSS

2025· preprint· en· W4417172151 on OpenAlexfundno aff
Jinglan Zheng, Prabhakar Tiwari, Gong‐Bo Zhao, Dominik J. Schwarz, David Bacon, S. Camera, Caroline Heneka, Catherine Hale, Szymon J. Nakoneczny, Morteza Pashapour-Ahmadabadi

Bibliographic record

VenueArXiv.org · 2025
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersLeibniz-GemeinschaftScience and Technology Facilities CouncilUniversity of Colorado BoulderMax-Planck-Institut für AstronomieLeibniz-Institut für Astrophysik PotsdamChina National Textile and Apparel CouncilMinisterium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-WestfalenMinistero degli Affari Esteri e della Cooperazione InternazionaleNational Astronomical Observatories, Chinese Academy of SciencesUniversity of Illinois at Urbana-ChampaignUniversité d'OrléansIstituto Nazionale di AstrofisicaCentre National de la Recherche ScientifiqueYale UniversityUniversity of TorontoBundesministerium für Bildung und ForschungSmithsonian InstitutionNational Natural Science Foundation of ChinaDeutsche ForschungsgemeinschaftÉcole Polytechnique Fédérale de LausanneYunnan UniversityNational Science FoundationScience Foundation IrelandVolkswagen FoundationAlfred P. Sloan FoundationJohns Hopkins UniversityNederlandse Organisatie voor Wetenschappelijk OnderzoekHarvard UniversityEuropean CommissionCalifornia Institute of TechnologyObservatoire de Paris, Université de Recherche Paris Sciences et LettresOhio State UniversityMax-Planck-GesellschaftCarnegie Institution of WashingtonNanjing UniversityNew Mexico State UniversityUniversidad Nacional Autónoma de MéxicoSpace Telescope Science InstituteSmithsonian Astrophysical ObservatoryFlatiron Health
KeywordsRedshiftLOFARGalaxySkyRedshift surveyBaryonCosmologyBaryon acoustic oscillations

Abstract

fetched live from OpenAlex

We cross-correlated galaxies from the LOw-Frequency ARray (LOFAR) Two-metre Sky Survey (LoTSS) second data release (DR2) radio source with the extended Baryon Oscillation Spectroscopic Survey (eBOSS) luminous red galaxy (LRG) sample to extract the baryon acoustic oscillation (BAO) signal and constrain the linear clustering bias of radio sources in LoTSS DR2. In the LoTSS DR2 catalogue, employing a flux density limit of $1.5$ mJy at the central LoTSS frequency of 144 MHz and a signal-to-noise ratio (S/N) of $7.5$, additionally considering eBOSS LRGs with redshifts between 0.6 and 1, we measured both the angular LoTSS-eBOSS cross-power spectrum and the angular eBOSS auto-power spectrum. These measurements were performed across various eBOSS redshift tomographic bins with a width of $Δz=0.06$. By marginalising over the broadband shape of the angular power spectra, we searched for a BAO signal in cross-correlation with radio galaxies, and determine the linear clustering bias of LoTSS radio sources for a constant-bias and an evolving-bias model. Using the cross-correlation, we measured the isotropic BAO dilation parameter as $α=1.01\pm 0.11$ at $z_{\rm eff}=0.63$. By combining four redshift slices at $z_{\rm eff}=0.63, 0.69, 0.75$, and $0.81$, we determined a more constrained value of $α= 0.968^{+0.060}_{-0.095}$. For the entire redshift range of $z_{\rm eff}=0.715$, we measured $b_C = 2.64 \pm 0.20$ for the constant-bias model, $b(z)=b_C$, and then $b_D = 1.80 \pm 0.13$ for the evolving-bias model, $b(z) = b_D / D(z)$, with $D(z)$ denoting the growth rate of linear structures. Additionally, we measured the clustering bias for individual redshift bins.

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 score0.011
Threshold uncertainty score0.022

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.002
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0020.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0050.002

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 head0.041
GPT teacher head0.284
Teacher spread0.243 · 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

Citations0
Published2025
Admission routes1
Has abstractyes

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Same venueArXiv.org→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→