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Record W2895694673 · doi:10.1051/0004-6361/201834379

Consistent cosmic shear in the face of systematics: a <i>B</i>-mode analysis of KiDS-450, DES-SV and CFHTLenS

2019· article· en· W2895694673 on OpenAlexfundaboutno aff
Marika Asgari, Catherine Heymans, H. Hildebrandt, L. Miller, Peter Schneider, A. Amon, T. Erben, Christos Georgiou, Joachim Harnois-Déraps, Konrad Kuijken

Bibliographic record

VenueAstronomy and Astrophysics · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilArgonne National LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityINAF-Osservatorio Astronomico di PadovaScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaUniversity of Illinois at Urbana-ChampaignInstitut de Física d'Altes EnergiesCentre National de la Recherche ScientifiqueCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoDeutsche ForschungsgemeinschaftUniversity of EdinburghUniversity of SussexUniversity of NottinghamUniversity of TorontoNational Aeronautics and Space AdministrationUniversity College LondonUniversity of CambridgeGovernment of OntarioWestern Canada Research GridUniversity of PortsmouthAspen Center for PhysicsOhio State UniversityMinistério da Ciência, Tecnologia e InovaçãoFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroCanada Foundation for InnovationLawrence Berkeley National LaboratoryCanadian Space AgencyFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaAlexander von Humboldt-StiftungInstitut national des sciences de l'UniversUniversity of ChicagoCompute CanadaSimons FoundationUniversity of MichiganU.S. Department of EnergyFermilabNational Science Foundation
KeywordsPhysicsWeak gravitational lensingAstrophysicsRedshiftGalaxyCOSMIC cancer database

Abstract

fetched live from OpenAlex

We analyse three public cosmic shear surveys; the Kilo-Degree Survey (KiDS-450), the Dark Energy Survey (DES-SV) and the Canada France Hawaii Telescope Lensing Survey (CFHTLenS). Adopting the “COSEBIs” statistic to cleanly and completely separate the lensing E -modes from the non-lensing B -modes, we detect B -modes in KiDS-450 and CFHTLenS at the level of ∼2.7 σ . For DES-SV we detect B -modes at the level of 2.8 σ in a non-tomographic analysis, increasing to a 5.5 σ B -mode detection in a tomographic analysis. In order to understand the origin of these detected B -modes we measure the B -mode signature of a range of different simulated systematics including PSF leakage, random but correlated PSF modelling errors, camera-based additive shear bias and photometric redshift selection bias. We show that any correlation between photometric-noise and the relative orientation of the galaxy to the point-spread-function leads to an ellipticity selection bias in tomographic analyses. This work therefore introduces a new systematic for future lensing surveys to consider. We find that the B -modes in DES-SV appear similar to a superposition of the B -mode signatures from all of the systematics simulated. The KiDS-450 and CFHTLenS B -mode measurements show features that are consistent with a repeating additive shear bias.

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: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.015
Threshold uncertainty score0.031

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.007
GPT teacher head0.205
Teacher spread0.198 · 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

Citations42
Published2019
Admission routes2
Has abstractyes

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