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Joint Analysis of BICEP2/<i>Keck Array</i>and<i>Planck</i>Data

2015· article· en· 979 citations· W1964777539 on OpenAlex· 10.1103/physrevlett.114.101301

Why is this work in the frame?

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

Canadian affiliationAn author listed a Canadian institution. This is the only route the usual frame has.
Canadian funderA Canadian agency funded it. The work may carry no Canadian affiliation at all.

Full frame distilled prediction

Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

Candidate categories
none
Consensus categories
none
Domain
Candidate signal: noneConsensus signal: none
Study design
Candidate signal: Theoretical or conceptualConsensus signal: Theoretical or conceptual
Genre
Candidate signal: EmpiricalConsensus signal: Empirical
Teacher disagreement score
0.125
Threshold uncertainty score
0.389
Validation status
machine_predicted_unvalidated · codex-gemma-dda1882f352a

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0000.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

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.

Opus teacher head0.044
GPT teacher head0.321
Teacher spread
0.277 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Abstract

We report the results of a joint analysis of data from BICEP2/Keck Array and Planck. BICEP2 and Keck Array have observed the same approximately 400 deg^{2} patch of sky centered on RA 0 h, Dec. -57.5°. The combined maps reach a depth of 57 nK deg in Stokes Q and U in a band centered at 150 GHz. Planck has observed the full sky in polarization at seven frequencies from 30 to 353 GHz, but much less deeply in any given region (1.2 μK deg in Q and U at 143 GHz). We detect 150×353 cross-correlation in B modes at high significance. We fit the single- and cross-frequency power spectra at frequencies ≥150 GHz to a lensed-ΛCDM model that includes dust and a possible contribution from inflationary gravitational waves (as parametrized by the tensor-to-scalar ratio r), using a prior on the frequency spectral behavior of polarized dust emission from previous Planck analysis of other regions of the sky. We find strong evidence for dust and no statistically significant evidence for tensor modes. We probe various model variations and extensions, including adding a synchrotron component in combination with lower frequency data, and find that these make little difference to the r constraint. Finally, we present an alternative analysis which is similar to a map-based cleaning of the dust contribution, and show that this gives similar constraints. The final result is expressed as a likelihood curve for r, and yields an upper limit r_{0.05}<0.12 at 95% confidence. Marginalizing over dust and r, lensing B modes are detected at 7.0σ significance.

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.

The record

Venue
Physical Review Letters
Topic
Cosmology and Gravitation Theories
Field
Physics and Astronomy
Canadian institutions
McGill UniversityUniversity of British ColumbiaUniversity of Toronto
Funders
Faculdade de Ciências e Tecnologia, Universidade Nova de LisboaINAF-Osservatorio Astronomico di PadovaEuropean Research CouncilInstitut National de Physique Nucléaire et de Physique des ParticulesScience and Technology Facilities CouncilCanadian Space AgencyMinisterio de Ciencia e InnovaciónAdvanced Research Projects AgencyW. M. Keck FoundationCentre National de la Recherche ScientifiqueMinisterio de Economía y CompetitividadMax-Planck-GesellschaftDanmarks Tekniske UniversitetCalifornia Institute of TechnologyTekesConsiglio Nazionale delle RicercheDeutsches Zentrum für Luft- und RaumfahrtFundação para a Ciência e a TecnologiaCentre National d’Etudes SpatialesNorges ForskningsrådMinistério da Ciência, Tecnologia e Ensino SuperiorUK Space AgencyAcademy of FinlandNational Aeronautics and Space AdministrationPartnership for Advanced Computing in Europe AISBLConsejo Superior de Investigaciones CientíficasVillum FondenAgenzia Spaziale ItalianaScience Foundation IrelandNational Science FoundationEuropean Space AgencyChina Scholarship CouncilU.S. Department of Energy
Keywords
PlanckPhysicsCosmic microwave backgroundAstrophysicsSkyPolarization (electrochemistry)Gravitational waveStokes parametersParameterized complexityOpticsScattering
Has abstract in OpenAlex
yes