MétaCan
Menu
Back to cohort

[no title]

2020· article· en· W3103249958 on OpenAlexaff
H. Hildebrandt, F. Köhlinger, Jan Luca van den Busch, Benjamin Joachimi, Catherine Heymans, Arun Kannawadi, Angus H. Wright, Marika Asgari, Chris Blake, Henk Hoekstra, Shahab Joudaki, Konrad Kuijken, L. Miller, Christopher Morrison, Tilman Tröster, A. Amon, Maria Archidiacono, S. Brieden, A. Choi, J. T. A. de Jong, T. Erben, Benjamin Giblin, Alexander Mead, J. A. Peacock, M. Radovich, Peter Schneider, Cristobál Sifón, M. Tewes

Bibliographic record

VenueEdinburgh Research Explorer (University of Edinburgh) · 2020
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of British Columbia
FundersScience and Technology Facilities CouncilBundesministerium für Bildung und ForschungAspen Center for PhysicsSLAC National Accelerator LaboratoryNederlandse Organisatie voor Wetenschappelijk OnderzoekAlexander von Humboldt-StiftungMax-Planck-GesellschaftDeutsche ForschungsgemeinschaftMinistry of Education, Culture, Sports, Science and TechnologyNational Aeronautics and Space AdministrationNational Science Foundation
KeywordsPhysicsRedshiftPhotometric redshiftAstrophysicsWeak gravitational lensingPlanckCosmic microwave backgroundDark energyCOSMIC cancer databaseCosmic infrared backgroundGalaxyCosmic varianceOmegaRedshift surveyLarge Synoptic Survey TelescopeGravitational lensSouth Pole TelescopeAstronomyCosmologyOptics

Abstract

fetched live from OpenAlex

We present a tomographic cosmic shear analysis of the Kilo-Degree Survey (KiDS) combined with the VISTA Kilo-Degree Infrared Galaxy Survey. This is the first time that a full optical to near-infrared data set has been used for a wide-field cosmological weak lensing experiment. This unprecedented data, spanning 450 deg2, allows us to significantly improve the estimation of photometric redshifts, such that we are able to include robustly higher-redshift sources for the lensing measurement, and – most importantly – to solidify our knowledge of the redshift distributions of the sources. Based on a flat ΛCDM model we find $ S_8\equiv\sigma_8\sqrt{\Omega_{\mathrm{m}}/0.3}=0.737_{-0.036}^{+0.040} $ in a blind analysis from cosmic shear alone. The tension between KiDS cosmic shear and the Planck-Legacy CMB measurements remains in this systematically more robust analysis, with S8 differing by 2.3σ. This result is insensitive to changes in the priors on nuisance parameters for intrinsic alignment, baryon feedback, and neutrino mass. KiDS shear measurements are calibrated with a new, more realistic set of image simulations and no significant B-modes are detected in the survey, indicating that systematic errors are under control. When calibrating our redshift distributions by assuming the 30-band COSMOS-2015 photometric redshifts are correct (following the Dark Energy Survey and the Hyper Suprime-Cam Survey), we find the tension with Planck is alleviated. The robust determination of source redshift distributions remains one of the most challenging aspects for future cosmic shear surveys.

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 categoriesInsufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Not applicable · Consensus signal: none
GenreCandidate signal: Other · Consensus signal: none
Teacher disagreement score0.975
Threshold uncertainty score0.000

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0020.002
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0250.010

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 head0.066
GPT teacher head0.270
Teacher spread0.204 · 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.

Study designNot applicable
Domainnot available
GenreOther

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

Citations148
Published2020
Admission routes1
Has abstractyes

Explore more

Same venueEdinburgh Research Explorer (University of Edinburgh)Same topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207