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Detection of CMB-Cluster Lensing using Polarization Data from SPTpol

2019· article· en· W2982718457 on OpenAlexaff
S. Raghunathan, S. Patil, Eric J. Baxter, B. A. Benson, L. E. Bleem, T. M. Crawford, G. P. Holder, Thomas McClintock, C. L. Reichardt, T. N. Varga, N. Whitehorn, P. A. R. Ade, S. Allam, A. J. Anderson, Jason E. Austermann, S. Àvila, J. S. Avva, D. Bacon, James A. Beall, A. N. Bender, F. Bianchini, S. Bocquet, D. Brooks, D. L. Burke, J. E. Carlstrom, J. Carretero, F. J. Castander, C. L. Chang, H. C. Chiang, R. Citron, M. Costanzi, A. T. Crites, L. N. da Costa, S. Desai, H. T. Diehl, J. P. Dietrich, M. Dobbs, P. Doel, S. Everett, A. E. Evrard, C. Feng, B. Flaugher, P. Fosalba, J. Frieman, Jason Gallicchio, J. García-Bellido, E. Gaztañaga, E. M. George, T. Giannantonio, A. Gilbert, R. A. Gruendl, J. Gschwend, N. Gupta, G. Gutiérrez, T. de Haan, N. W. Halverson, N. L. Harrington, J. W. Henning, G. C. Hilton, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, N. Huang, Johannes Hubmayr, K. D. Irwin, T. Jeltema, M. Carrasco Kind, L. Knox, N. Kuropatkin, O. Lahav, A. T. Lee, D. Li, M. Lima, A. E. Lowitz, M. A. G. Maia, J. L. Marshall, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, R. Miquel, L. Mocanu, J. J. Mohr, J. Montgomery, C. Corbett Moran, A. Nadolski, T. Natoli, J. P. Nibarger, G. I. Noble, V. Novosad, R. L. C. Ogando, S. Padin, C. Pryke, David Rapetti, A. K. Romer, A. Roodman, A. Carnero Rosell, Eduardo Rozo, J. E. Ruhl, E. S. Rykoff, B. R. Saliwanchik, E. Sánchez, J. T. Sayre, V. Scarpine, K. K. Schaffer, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, C. Sievers, G. Smecher, M. Smith, M. Soares-Santos, A. A. Stark, K. T. Story, E. Suchyta, M. E. C. Swanson, G. Tarlé, C. Tucker, K. Vanderlinde, Todd Veach, J. De Vicente, J. D. Vieira, V. Vikram, G. Wang, W. L. K. Wu, V. Yefremenko, Y. Zhang

Bibliographic record

VenuePhysical Review Letters · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsThree-Speed Logic (Canada)Canadian Institute for Theoretical AstrophysicsUniversity of TorontoMcGill UniversityCanadian Institute for Advanced Research
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundAustralian Research CouncilScience and Technology Facilities CouncilUniversity of Illinois at Urbana-ChampaignLudwig-Maximilians-Universität MünchenFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoMinistério da Ciência, Tecnologia e InovaçãoMinisterio de Economía y CompetitividadInstitut de Física d'Altes EnergiesEidgenössische Technische Hochschule ZürichGeneralitat de CatalunyaOffice of ScienceUniversity of EdinburghUniversity College LondonARC Centre of Excellence for All-Sky AstrophysicsUniversity of CambridgeNational Energy Research Scientific Computing CenterUniversity of PortsmouthUniversity of MichiganTexas A and M UniversityUniversity of ChicagoUniversity of California, Santa CruzOhio State UniversityHigher Education Funding Council for EnglandLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaUniversity of NottinghamStanford UniversityHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaU.S. Department of EnergyKavli FoundationUniversity of SussexSeventh Framework ProgrammeGordon and Betty Moore FoundationEuropean CommissionFermilabNational Science Foundation
KeywordsCosmic microwave backgroundPolarization (electrochemistry)PhysicsCluster (spacecraft)AstrophysicsAstronomyOpticsAnisotropyComputer science

Abstract

fetched live from OpenAlex

We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole signature from stacked images formed by rotating the cluster-centered Stokes QU map cutouts along the direction of the locally measured background CMB polarization gradient. Using data from the SPTpol 500 deg^{2} survey at the locations of roughly 18 000 clusters with richness λ≥10 from the Dark Energy Survey (DES) Year-3 full galaxy cluster catalog, we detect lensing at 4.8σ. The mean stacked mass of the selected sample is found to be (1.43±0.40)×10^{14}M_{⊙} which is in good agreement with optical weak lensing based estimates using DES data and CMB-lensing based estimates using SPTpol temperature data. This measurement is a key first step for cluster cosmology with future low-noise CMB surveys, like CMB-S4, for which CMB polarization will be the primary channel for cluster lensing measurements.

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)0.000
metaresearch head score (Gemma)0.001
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 score0.004
Threshold uncertainty score0.008

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.025
GPT teacher head0.303
Teacher spread0.278 · 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

Citations27
Published2019
Admission routes1
Has abstractyes

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