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Record W2789087330 · doi:10.1093/mnras/sty1740

Detection significance of baryon acoustic oscillations peaks in galaxy and quasar clustering

2018· article· en· W2789087330 on OpenAlexfundno aff
Behzad Ansarinejad, T. Shanks

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratoryLeibniz-GemeinschaftSmithsonian Astrophysical ObservatoryMax-Planck-Institut für AstronomieMinistério da Ciência, Tecnologia e InovaçãoScience and Technology Facilities CouncilInstituto de Astrofísica de CanariasCarnegie Mellon UniversityOffice of ScienceJohns Hopkins UniversityOhio State UniversityCarnegie Institution of WashingtonNew Mexico State UniversityUniversity of Notre DameSmithsonian InstitutionAlfred P. Sloan FoundationMax-Planck-Institut für AstrophysikU.S. Department of EnergyYork UniversityNational Science Foundation
KeywordsPhysicsSigmaQuasarAstrophysicsBaryonRedshiftGalaxyCovariance matrixCorrelation function (quantum field theory)LambdaBaryon acoustic oscillationsRange (aeronautics)CovarianceStatistical physicsStatisticsQuantum mechanics

Abstract

fetched live from OpenAlex

We compare our analysis of the baryon acoustic oscillations (BAO) feature in the correlation functions of SDSS BOSS DR12 LOWZ and CMASS galaxy samples with previous literature results.Using subsets of the data we obtain an empirical estimate of the errors on the correlation functions that are in agreement with the simulated errors of previous works.We find that the significance of BAO detection is the quantity most sensitive to the choice of the fitting range with the CMASS value decreasing from 8.0σ to 5.3σ as the fitting range is reduced.Although our measurements of D V (z) are in agreement with previous studies, we note that their CMASS 8.0σ (LOWZ 4.0σ ) detection significance reduces to 4.7σ (2.8σ ) in fits with their diagonal covariance terms only.We extend our BAO analysis to higher redshifts by fitting to the weighted mean of 2QDESp, SDSS DR5 UNIFORM, 2QZ, and 2SLAQ quasar correlation functions, obtaining a 7.6 per cent measurement compared to 3.9 per cent achieved by eBOSS DR14.Unlike for the LRG surveys, the larger error on quasar correlation functions implies a smaller role for nuisance parameters (accounting for scale-dependent clustering) in providing a good fit to the fiducial cold dark matter model.Again we find that the eBOSS peak significance reduces from 2.8 to 1.4σ if we ignore the off-diagonal covariance matrix terms in our fitting.We conclude that for both LRGs and quasars, the reported BAO peak significances from the SDSS surveys depend sensitively on the accuracy of the covariance matrix at large separations.

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)0.007
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 score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.007
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.001
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 head0.007
GPT teacher head0.200
Teacher spread0.193 · 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

Citations4
Published2018
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→