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Record W2898444044 · doi:10.3847/1538-4357/ab01ca

Mass Calibration of Optically Selected DES Clusters Using a Measurement of CMB-cluster Lensing with SPTpol Data

2019· article· en· W2898444044 on OpenAlexaff
S. Raghunathan, S. Patil, Eric J. Baxter, B. A. Benson, L. E. Bleem, T.-L. Chou, T. M. Crawford, G. P. Holder, Thomas McClintock, C. L. Reichardt, Eduardo Rozo, T N Varga, T. M. C. Abbott, P. A. R. Ade, S. Allam, A. J. Anderson, J. Annis, Jason E. Austermann, S. Àvila, James A. Beall, K. Bechtol, A. N. Bender, G. M. Bernstein, E. Bertin, F. Bianchini, D. Brooks, D. L. Burke, J. E. Carlstrom, J. Carretero, C. L. Chang, H. C. Chiang, H. M. Cho, R. Citron, A. T. Crites, C. E. Cunha, L. N. da Costa, C. Davis, S. Desai, H. T. Diehl, J. P. Dietrich, M. Dobbs, P. Doel, T. F. Eifler, W. Everett, A. E. Evrard, B. Flaugher, P. Fosalba, J. Frieman, Jason Gallicchio, J. García-Bellido, E. Gaztañaga, E. M. George, A. Gilbert, D. Gruen, R. A. Gruendl, J. Gschwend, N. Gupta, G. Gutiérrez, T. de Haan, N. W. Halverson, N. L. Harrington, W. G. Hartley, J. W. Henning, G. C. Hilton, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, Z. Hou, B. Hoyle, J. D. Hrubes, N. Huang, Johannes Hubmayr, K. D. Irwin, D. J. James, T. Jeltema, Alex Kim, M. Carrasco Kind, L. Knox, András Kovács, K. Kuehn, N. Kuropatkin, A. T. Lee, T S Li, M. Lima, M. A. G. Maia, J. L. Marshall, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, C. J. Miller, R. Miquel, L. Mocanu, J. Montgomery, Andrew Nadolski, T. Natoli, J. P. Nibarger, V. Novosad, S. Padin, C. Pryke, David Rapetti, A. K. Romer, A. Carnero Rosell, J. E. Ruhl, B. R. Saliwanchik, E. Sánchez, J. T. Sayre, V. Scarpine, K. K. Schaffer, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, G. Smecher, R. C. Smith, M. Soares-Santos, F. Sobreira, A. A. Stark, K. T. Story, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, C. Tucker, K. Vanderlinde, J. De Vicente, J. D. Vieira, G. Wang, N. Whitehorn, W. L. K. Wu, Y. Zhang

Bibliographic record

VenueThe Astrophysical Journal · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsThree-Speed Logic (Canada)Canadian Institute for Theoretical AstrophysicsUniversity of TorontoMcGill UniversityCanadian Institute for Advanced Research
FundersScience and Technology Facilities CouncilOffice of ScienceNational Energy Research Scientific Computing CenterGordon and Betty Moore FoundationU.S. Department of EnergyUniversity of ChicagoNational Science Foundation
KeywordsCosmic microwave backgroundPhysicsWeak gravitational lensingAstrophysicsGalaxy clusterGravitational lensGalaxyEstimatorRedshiftAnisotropyStatisticsOpticsMathematics

Abstract

fetched live from OpenAlex

Abstract We use cosmic microwave background (CMB) temperature maps from the 500 deg2 SPTpol survey to measure the stacked lensing convergence of galaxy clusters from the Dark Energy Survey (DES) Year-3 redMaPPer (RM) cluster catalog. The lensing signal is extracted through a modified quadratic estimator designed to be unbiased by the thermal Sunyaev–Zel’dovich (tSZ) effect. The modified estimator uses a tSZ-free map, constructed from the SPTpol 95 and 150 GHz data sets, to estimate the background CMB gradient. For lensing reconstruction, we employ two versions of the RM catalog: a flux-limited sample containing 4003 clusters and a volume-limited sample with 1741 clusters. We detect lensing at a significance of 8.7σ(6.7σ) with the flux (volume)–limited sample. By modeling the reconstructed convergence using the Navarro–Frenk–White profile, we find the average lensing masses to be and for the volume- and flux-limited samples, respectively. The systematic error budget is much smaller than the statistical uncertainty and is dominated by the uncertainties in the RM cluster centroids. We use the volume-limited sample to calibrate the normalization of the mass-richness scaling relation, and find a result consistent with the galaxy weak-lensing measurements from DES.

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)0.001
metaresearch head score (Gemma)0.003
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.017

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.002
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.001
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 head0.023
GPT teacher head0.222
Teacher spread0.199 · 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

Citations39
Published2019
Admission routes1
Has abstractyes

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