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Record W1899149329 · doi:10.1103/physrevd.91.123011

Empirical covariance modeling for 21 cm power spectrum estimation: A method demonstration and new limits from early Murchison Widefield Array 128-tile data

2015· article· en· W1899149329 on OpenAlexfundno aff
Joshua S. Dillon, Abraham R. Neben, Jacqueline N. Hewitt, Max Tegmark, N. Barry, Adam P. Beardsley, Judd D. Bowman, F. Briggs, P. Carroll, A. de Oliveira‐Costa, Aaron Ewall‐Wice, L. Feng, L. J. Greenhill, B. J. Hazelton, Lars Hernquist, N. Hurley‐Walker, Daniel Jacobs, Han-Seek Kim, Piyanat Kittiwisit, E. Lenc, J. Line, Abraham Loeb, B. McKinley, D. A. Mitchell, M. F. Morales, A. R. Offringa, S. Paul, B. Pindor, J. C. Pober, P. Procopio, J. Riding, S. K. Sethi, N. Udaya Shankar, R. Subrahmanyan, Ian Sullivan, Nithyanandan Thyagarajan, S. J. Tingay, Cathryn M. Trott, R. B. Wayth, R. L. Webster, J. Stuart B. Wyithe, G. Bernardi, R. J. Cappallo, A. A. Deshpande, M. Johnston‐Hollitt, D. L. Kaplan, C. J. Lonsdale, S. R. McWhirter, E. Morgan, Divya Oberoi, S. M. Ord, T. Prabu, K. S. Srivani, A. Williams, C. L. Williams

Bibliographic record

VenuePhysical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology · 2015
Typearticle
Languageen
FieldPhysics and Astronomy
TopicRadio Astronomy Observations and Technology
Canadian institutionsnot available
FundersAir Force Office of Scientific ResearchAustralian Research CouncilAustralian National UniversityOntario Ministry of Economic Development and InnovationMassachusetts Institute of TechnologyCommonwealth Scientific and Industrial Research OrganisationInternational Business Machines CorporationNational Science Foundation
KeywordsPhysicsRedshiftCovarianceLimit (mathematics)Spectral densityGalaxyAstrophysicsSubtractionA priori and a posterioriAlgorithmComputer scienceStatisticsMathematicsMathematical analysisTelecommunications

Abstract

fetched live from OpenAlex

The separation of the faint cosmological background signal from bright astrophysical foregrounds remains one of the most daunting challenges of mapping the high-redshift intergalactic medium with the redshifted 21 cm line of neutral hydrogen. Advances in mapping and modeling of diffuse and point source foregrounds have improved subtraction accuracy, but no subtraction scheme is perfect. Precisely quantifying the errors and error correlations due to missubtracted foregrounds allows for both the rigorous analysis of the 21 cm power spectrum and for the maximal isolation of the ``EoR window'' from foreground contamination. We present a method to infer the covariance of foreground residuals from the data itself in contrast to previous attempts at a priori modeling. We demonstrate our method by setting limits on the power spectrum using a 3 h integration from the 128-tile Murchison Widefield Array. Observing between 167 and 198 MHz, we find at 95% confidence a best limit of ${\mathrm{\ensuremath{\Delta}}}^{2}(k)<3.7\ifmmode\times\else\texttimes\fi{}{10}^{4}\text{ }\text{ }{\mathrm{mK}}^{2}$ at comoving scale $k=0.18\text{ }\text{ }h\text{ }{\mathrm{Mpc}}^{\ensuremath{-}1}$ and at $z=6.8$, consistent with existing limits.

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)0.005
metaresearch head score (Gemma)0.022
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: none
Teacher disagreement score0.011
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0050.022
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0010.001
Science and technology studies0.0010.001
Scholarly communication0.0010.002
Open science0.0020.002
Research integrity0.0010.003
Insufficient payload (model declined to judge)0.0020.001

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 head0.064
GPT teacher head0.367
Teacher spread0.303 · 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

Citations122
Published2015
Admission routes1
Has abstractyes

Explore more

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