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Record W3085299096 · doi:10.1093/mnras/stab1386

Mass calibration of distant SPT galaxy clusters through expanded weak-lensing follow-up observations with <i>HST</i>, VLT, &amp; Gemini-South

2021· article· en· W3085299096 on OpenAlexaff
T. Schrabback, S. Bocquet, Martin W. Sommer, H. Zohren, Beatriz Hernández-Martín, Henk Hoekstra, Selim Raihan, M. Schirmer, Douglas Applegate, Matthew Bayliss, B. A. Benson, L. E. Bleem, J. P. Dietrich, Benjamin Floyd, Stefan Hilbert, Julie Hlavacek-Larrondo, M. McDonald, A. Saro, A. A. Stark, N Weissgerber

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversité de Montréal
FundersInternational Max Planck Research School for Advanced Methods in Process and Systems EngineeringBundesministerium für Wirtschaft und EnergieMinistero dell’Istruzione, dell’Università e della RicercaSpace Telescope Science InstituteNederlandse Organisatie voor Wetenschappelijk OnderzoekMinisterio de Ciencia, Tecnología e Innovación ProductivaDeutsche ForschungsgemeinschaftHigh Energy PhysicsInternational Max Planck Research School for Environmental, Cellular and Molecular MicrobiologyArgonne National LaboratoryU.S. Department of EnergyGordon and Betty Moore FoundationNational Science FoundationEuropean Space AgencyKorea Astronomy and Space Science InstituteNational Aeronautics and Space AdministrationComisión Nacional de Investigación Científica y TecnológicaUniversity of Chicago
KeywordsPhysicsAstrophysicsSouth Pole TelescopeRedshiftGalaxy clusterWeak gravitational lensingAstronomyGalaxyCosmologyPhotometry (optics)Sunyaev–Zel'dovich effectPhotometric redshiftPlanckStars

Abstract

fetched live from OpenAlex

ABSTRACT Expanding from previous work, we present weak-lensing (WL) measurements for a total sample of 30 distant (zmedian = 0.93) massive galaxy clusters from the South Pole Telescope Sunyaev–Zel’dovich (SPT-SZ) Survey, measuring galaxy shapes in Hubble Space Telescope (HST) Advanced Camera for Surveys images. We remove cluster members and preferentially select z ≳ 1.4 background galaxies via V − I colour, employing deep photometry from VLT/FORS2 and Gemini-South/GMOS. We apply revised calibrations for the WL shape measurements and the source redshift distribution to estimate the cluster masses. In combination with earlier Magellan/Megacam results for lower-redshifts clusters, we infer refined constraints on the scaling relation between the SZ detection significance and the cluster mass, in particular regarding its redshift evolution. The mass scale inferred from the WL data is lower by a factor $0.76^{+0.10}_{-0.14}$ (at our pivot redshift z = 0.6) compared to what would be needed to reconcile a flat Planck νΛCDM cosmology (in which the sum of the neutrino masses is a free parameter) with the observed SPT-SZ cluster counts. In order to sensitively test the level of (dis-)agreement between SPT clusters and Planck, further expanded WL follow-up samples are needed.

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 score0.008
Threshold uncertainty score0.015

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.001
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 head0.015
GPT teacher head0.204
Teacher spread0.189 · 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

Citations40
Published2021
Admission routes1
Has abstractyes

Explore more

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