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Record W2980160815 · doi:10.3847/1538-4365/ab6993

The SPTpol Extended Cluster Survey

2020· article· en· W2980160815 on OpenAlexafffund
L. E. Bleem, S. Bocquet, B. Stalder, Michael D. Gladders, P. A. R. Ade, S. W. Allen, A. J. Anderson, J. Annis, M. L. N. Ashby, Jason E. Austermann, S. Àvila, J. S. Avva, Matthew Bayliss, James A. Beall, K. Bechtol, A. N. Bender, B. A. Benson, E. Bertin, F. Bianchini, Chris Blake, M. Brodwin, D. Brooks, E. Buckley‐Geer, D. L. Burke, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, C. L. Chang, H. C. Chiang, R. Citron, C. Corbett Moran, M. Costanzi, T. M. Crawford, A. T. Crites, L. N. da Costa, T. de Haan, J. De Vicente, S. Desai, H. T. Diehl, J. P. Dietrich, M. Dobbs, T. F. Eifler, W. Everett, B. Flaugher, Benjamin Floyd, J. Frieman, Jason Gallicchio, J. García-Bellido, E. M. George, D. W. Gerdes, A. Gilbert, D. Gruen, R. A. Gruendl, J. Gschwend, N. Gupta, G. Gutiérrez, N. W. Halverson, N. L. Harrington, J. W. Henning, Catherine Heymans, G. P. Holder, D. L. Hollowood, W. L. Holzapfel, K. Honscheid, J. D. Hrubes, N. Huang, Johannes Hubmayr, K. D. Irwin, D. J. James, T. Jeltema, Shahab Joudaki, Gourav Khullar, Matthias Klein, L. Knox, N. Kuropatkin, A. T. Lee, D. Li, C. Lidman, A. E. Lowitz, N. MacCrann, Guillaume Mahler, M. A. G. Maia, J. L. Marshall, M. McDonald, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, R. Miquel, L. M. Mocanu, J. J. Mohr, J. Montgomery, Andrew Nadolski, T. Natoli, J. P. Nibarger, G. I. Noble, V. Novosad, S. Padin, A. Palmese, David Parkinson, S. Patil, F. Paz-Chinchón, A. A. Plazas, C. Pryke, Nesar Ramachandra, C. L. Reichardt, J. D. Remolina González, A. K. Romer, A. Roodman, J. E. Ruhl, E. S. Rykoff, B. R. Saliwanchik, E. Sánchez, A. Saro, J. T. Sayre, K. K. Schaffer, T. Schrabback, S. Serrano, Keren Sharon, C. Sievers, G. Smecher, M. Smith, M. Soares-Santos, A. A. Stark, K. T. Story, E. Suchyta, G. Tarlé, C. Tucker, K. Vanderlinde, Todd Veach, J. D. Vieira, G. Wang, J. Weller, N. Whitehorn, W. L. K. Wu, V. Yefremenko, Y. Zhang

Bibliographic record

VenueThe Astrophysical Journal Supplement Series · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoThree-Speed Logic (Canada)Canadian Institute for Advanced ResearchMcGill University
FundersArgonne National LaboratoryPlanetary Science DivisionScience Mission DirectorateSmithsonian Astrophysical ObservatoryScience and Technology Facilities CouncilUniversity of Colorado BoulderJet Propulsion LaboratoryAustralian Astronomical Optics-MacquarieMax-Planck-GesellschaftLos Alamos National LaboratoryJohns Hopkins UniversityMinistero dell’Istruzione, dell’Università e della RicercaSLAC National Accelerator LaboratoryQueen's UniversityBundesministerium für Bildung und ForschungBundesministerium für Wirtschaft und TechnologieGordon and Betty Moore FoundationQueen's University BelfastAustralian Research CouncilSpace Telescope Science InstituteOffice of ScienceDeutsche ForschungsgemeinschaftMcGill UniversityUniversity of ChicagoSmithsonian InstitutionU.S. Department of EnergyKavli FoundationEötvös Loránd TudományegyetemCalifornia Institute of TechnologyNational Central UniversityNational Aeronautics and Space AdministrationAlexander von Humboldt-StiftungNatural Sciences and Engineering Research Council of CanadaDurham UniversityNational Science Foundation
KeywordsPhysicsAstrophysicsGalaxy clusterCluster (spacecraft)RedshiftPlanckCosmologyGalaxyWeak gravitational lensingGravitational lensDark energyAstronomy

Abstract

fetched live from OpenAlex

Abstract We describe the observations and resultant galaxy cluster catalog from the 2770 deg 2 SPTpol Extended Cluster Survey (SPT-ECS). Clusters are identified via the Sunyaev–Zel’dovich (SZ) effect and confirmed with a combination of archival and targeted follow-up data, making particular use of data from the Dark Energy Survey (DES). With incomplete follow-up we have confirmed as clusters 244 of 266 candidates at a detection significance ξ ≥ 5 and an additional 204 systems at 4 < ξ < 5. The confirmed sample has a median mass of and a median redshift of z = 0.49, and we have identified 44 strong gravitational lenses in the sample thus far. Radio data are used to characterize contamination to the SZ signal; the median contamination for confirmed clusters is predicted to be ∼1% of the SZ signal at the ξ > 4 threshold, and <4% of clusters have a predicted contamination >10% of their measured SZ flux. We associate SZ-selected clusters, from both SPT-ECS and the SPT-SZ survey, with clusters from the DES redMaPPer sample, and we find an offset distribution between the SZ center and central galaxy in general agreement with previous work, though with a larger fraction of clusters with significant offsets. Adopting a fixed Planck -like cosmology, we measure the optical richness–SZ mass ( ) relation and find it to be 28% shallower than that from a weak-lensing analysis of the DES data—a difference significant at the 4 σ level—with the relations intersecting at λ = 60. The SPT-ECS cluster sample will be particularly useful for studying the evolution of massive clusters and, in combination with DES lensing observations and the SPT-SZ cluster sample, will be an important component of future cosmological analyses.

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 categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.176
Threshold uncertainty score1.000

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 studies0.0010.000
Scholarly communication0.0000.001
Open science0.0010.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.228
Teacher spread0.216 · 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.

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

Citations202
Published2020
Admission routes2
Has abstractyes

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