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Record W2742923777 · doi:10.1093/mnras/sty305

A measurement of CMB cluster lensing with SPT and DES year 1 data

2018· article· en· W2742923777 on OpenAlexaff
Eric J. Baxter, S. Raghunathan, T. M. Crawford, P. Fosalba, Z. Hou, G. P. Holder, Y. Omori, S. Patil, Eduardo Rozo, T. M. C. Abbott, J. Annis, K. Aylor, A. Benoit-Lévy, B. A. Benson, E. Bertin, L. E. Bleem, E. Buckley‐Geer, D. L. Burke, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, C. L. Chang, H. M. Cho, A. T. Crites, M. Crocce, C. E. Cunha, L. N. da Costa, C. B. D’Andrea, C. Davis, T. de Haan, S. Desai, J. P. Dietrich, M. Dobbs, Scott Dodelson, P. Doel, A. Drlica-Wagner, Juan Estrada, W. Everett, A. Fausti Neto, B. Flaugher, J. Frieman, J. García-Bellido, E. M. George, E. Gaztañaga, T. Giannantonio, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutiérrez, N. W. Halverson, N. L. Harrington, W. G. Hartley, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, Bhuvnesh Jain, D. J. James, Mike Jarvis, T. Jeltema, L. Knox, E. Krause, K. Kuehn, S. Kuhlmann, N. Kuropatkin, O. Lahav, Adrian T. Lee, E. M. Leitch, T. S. Li, M. Lima, D. Luong-Van, A. Manzotti, M. March, Daniel P. Marrone, J. L. Marshall, Paul Martini, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, C. J. Miller, R. Miquel, L. Mocanu, J. J. Mohr, T. Natoli, B. Nord, R. L. C. Ogando, S. Padin, C. Pryke, David Rapetti, C. L. Reichardt, A. K. Romer, A. Roodman, J. E. Ruhl, E Rykoff, M. Šako, E. Sánchez, J. T. Sayre, V Scarpine, K K Schaffer, R. Schindler, M Schubnell, I. Sevilla-Noarbe, E Shirokoff, M. Smith, R C Smith, M. Soares-Santos, F. Sobreira, Z Staniszewski, A. A. Stark, K. T. Story, E. Suchyta, G. Tarlé, D. Thomas, M. A. Troxel, K. Vanderlinde, JEFTÉ DOS SANTOS VIEIRA, A. R. Walker, A. R. Williamson, Y Zhang, J. Zuntz

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoMcGill UniversityCanadian Institute for Advanced Research
FundersArgonne National LaboratoryScience and Technology Facilities CouncilUniversity of ChicagoKavli FoundationU.S. Department of EnergyGordon and Betty Moore FoundationNational Aeronautics and Space AdministrationEuropean Research CouncilMinisterio de Economía y CompetitividadNational Science Foundation
KeywordsPhysicsCosmic microwave backgroundAstrophysicsCluster (spacecraft)Weak gravitational lensingAstronomyGravitational lensGalaxyOpticsAnisotropyRedshift

Abstract

fetched live from OpenAlex

Clusters of galaxies gravitationally lens the cosmic microwave background (CMB) radiation, resulting in a distinct imprint in the CMB on arcminute scales. Measurement of this effect offers a promising way to constrain the masses of galaxy clusters, particularly those at high redshift. We use CMB maps from the South Pole Telescope Sunyaev–Zel'dovich (SZ) survey to measure the CMB lensing signal around galaxy clusters identified in optical imaging from first year observations of the Dark Energy Survey. The cluster catalogue used in this analysis contains 3697 members with mean redshift of z¯=0.45. We detect lensing of the CMB by the galaxy clusters at 8.1σ significance. Using the measured lensing signal, we constrain the amplitude of the relation between cluster mass and optical richness to roughly 17 per cent precision, finding good agreement with recent constraints obtained with galaxy lensing. The error budget is dominated by statistical noise but includes significant contributions from systematic biases due to the thermal SZ effect and cluster miscentring.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.009
Threshold uncertainty score0.289

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 studies0.0000.001
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 head0.018
GPT teacher head0.229
Teacher spread0.211 · 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 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

Citations54
Published2018
Admission routes1
Has abstractyes

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