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Record W2979088950 · doi:10.3847/1538-4357/ab8f24

A Measurement of the Degree-scale CMB B-mode Angular Power Spectrum with Polarbear

2020· article· en· W2979088950 on OpenAlexafffund
S. Adachi, M. A. O. Aguilar Faúndez, Kam Arnold, C. Baccigalupi, Darcy Barron, D. Beck, S. Beckman, F. Bianchini, D. Boettger, J. Borrill, Julien Carron, S. C. Chapman, K. Cheung, Y. Chinone, Kevin T. Crowley, A. Cukierman, M. Dobbs, T. Elleflot, Josquin Errard, Giulio Fabbian, Chang Feng, T. Fujino, N. Galitzki, N. Goeckner-Wald, J. C. Groh, G. Hall, N. W. Halverson, T. Hamada, M. Hasegawa, M. Hazumi, C. A. Hill, L. Howe, Yuki Inoue, G. Jaehnig, O. Jeong, Daisuke Kaneko, N. Katayama, Brian Keating, Reijo Keskitalo, S. Kikuchi, Theodore Kisner, N. Krachmalnicoff, A. Kusaka, A. T. Lee, D. Leon, Eric V. Linder, L. N. Lowry, Aashrita Mangu, Frederick Matsuda, Y. Minami, M. Navaroli, H. Nishino, A. T. P. Pham, D. Poletti, Giuseppe Puglisi, C. L. Reichardt, Y. Segawa, Maximiliano Silva-Feaver, P. Siritanasak, N. Stebor, R. Stompor, Aritoki Suzuki, O. Tajima, S. Takakura, S. Takatori, D. Tanabe, G. P. Teply, Calvin Tsai, C. Vergès, Benjamin Westbrook, Y. Zhou

Bibliographic record

VenueThe Astrophysical Journal · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsMcGill UniversityCanadian Institute for Advanced ResearchDalhousie University
FundersLawrence Berkeley National LaboratoryHigh Energy PhysicsLabex UnivEarthSComisión Nacional de Investigación Científica y TecnológicaJapan Society for the Promotion of ScienceScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaUniversity of California, San DiegoUniversity of MelbourneOffice of ScienceMinistry of Education, Culture, Sports, Science and TechnologyAgence Nationale de la RechercheU.S. Department of EnergyEuropean CommissionNational Energy Research Scientific Computing CenterJohn Templeton FoundationGordon and Betty Moore FoundationSimons FoundationNational Science Foundation
KeywordsPhysicsCosmic microwave backgroundSpectral densityPlanckPolarization (electrochemistry)AstrophysicsSpectral lineSpectral indexLambdaCosmic background radiationAnisotropyOpticsQuantum mechanicsStatistics

Abstract

fetched live from OpenAlex

Abstract We present a measurement of the B -mode polarization power spectrum of the cosmic microwave background (CMB) using data taken from 2014 July to 2016 December with the Polarbear experiment. The CMB power spectra are measured using observations at 150 GHz with an instantaneous array sensitivity of on a 670 square degree patch of sky centered at (R.A., decl.) = (+0 h 12 m 0 s , −59°18′). A continuously rotating half-wave plate is used to modulate polarization and to suppress low-frequency noise. We achieve 32 μ K arcmin effective polarization map noise with a knee in sensitivity of ℓ = 90, where the inflationary gravitational-wave signal is expected to peak. The measured B -mode power spectrum is consistent with a ΛCDM lensing and single dust component foreground model over a range of multipoles 50 ≤ ℓ ≤ 600. The data disfavor zero at 2.2 σ using this ℓ range of Polarbear data alone. We cross-correlate our data with Planck full mission 143, 217, and 353 GHz frequency maps and find the low- ℓ B -mode power in the combined data set to be consistent with thermal dust emission. We place an upper limit on the tensor-to-scalar ratio r < 0.90 at the 95% confidence level after marginalizing over foregrounds.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. 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.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.408
Threshold uncertainty score0.221

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
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)

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 head0.013
GPT teacher head0.219
Teacher spread0.205 · 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 teacher head, not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designTheoretical or conceptual
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

Citations71
Published2020
Admission routes2
Has abstractyes

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