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Record W3215249984 · doi:10.1093/mnras/stab3586

Lensing without borders – I. A blind comparison of the amplitude of galaxy–galaxy lensing between independent imaging surveys

2021· preprint· en· W3215249984 on OpenAlexafffund
A. Leauthaud, A. Amon, Sukhdeep Singh, D. Gruen, J. Lange, Song Huang, N. C. Robertson, T N Varga, Yifei Luo, Catherine Heymans, H. Hildebrandt, Chris Blake, M. Aguena, S. Allam, F. Andrade-Oliveira, J. Annis, E. Bertin, S Bhargava, J. Blazek, Sarah Bridle, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, R. Cawthon, A. Choi, M. Costanzi, L. N. da Costa, M. E. S. Pereira, C. Davis, J. De Vicente, J. DeRose, H. T. Diehl, J. P. Dietrich, P. Doel, K. Eckert, S. Everett, A. E. Evrard, I. Ferrero, B. Flaugher, P. Fosalba, J. García-Bellido, M. Gatti, E. Gaztañaga, R. A. Gruendl, J. Gschwend, W G Hartley, Klaus Honscheid, Bhuvnesh Jain, D. J. James, M. J. Jarvis, B. Joachimi, Arun Kannawadi, A. G. Kim, E. Krause, K. Kuehn, Konrad Kuijken, N. Kuropatkin, M. Lima, N. MacCrann, M. A. G. Maia, Martı́n Makler, M. March, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, Hironao Miyatake, J. J. Mohr, Bruno Moraes, Surhud More, More Surhud, R. Morgan, J. Myles, R. L. C. Ogando, A. Palmese, F. Paz-Chinchón, A. A. Plazas, J. Prat, Markus Michael Rau, Jason Rhodes, M. Rodríguez-Monroy, A. Roodman, Ashley J. Ross, S. Samuroff, C. Sánchez, E. Sánchez, V. Scarpine, David J. Schlegel, M. Schubnell, S. Serrano, I. Sevilla-Noarbe, Cristobál Sifón, M. Smith, Joshua S. Speagle, E. Suchyta, G. Tarlé

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typepreprint
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsUniversity of British ColumbiaCanadian Institute for Theoretical AstrophysicsUniversity of Toronto
FundersSLAC National Accelerator LaboratoryLos Alamos National LaboratoryLawrence Berkeley National LaboratoryArgonne National LaboratoryPlanetary Science DivisionHigh Energy PhysicsJapan Science and Technology AgencyScience and Technology Facilities CouncilScience Mission DirectorateSmithsonian Astrophysical ObservatoryOffice of ScienceToray Science FoundationEötvös Loránd TudományegyetemNational Astronomical Observatory of JapanU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroEidgenössische Technische Hochschule ZürichImperial College LondonGeneralitat de CatalunyaUniversity of Illinois at Urbana-ChampaignCabinet Office, Government of JapanNational Central UniversityMinistry of Education, Culture, Sports, Science and TechnologyBundesministerium für Bildung und ForschungAcademia SinicaIntegrated Electronics Engineering Center, Binghamton UniversityJapan Society for the Promotion of ScienceUniversity of EdinburghQueen's UniversityDeutsche ForschungsgemeinschaftNederlandse Organisatie voor Wetenschappelijk OnderzoekUniversity of PennsylvaniaConsejo Nacional de Investigaciones Científicas y TécnicasDurham UniversityInstitut de Física d'Altes EnergiesSpace Telescope Science InstituteUniversity of SussexMaterials Research Institute, Pennsylvania State UniversityUniversity of Hawai'iUniversity of NottinghamEuropean CommissionConselho Nacional de Desenvolvimento Científico e TecnológicoUniversity of CambridgeAlfred P. Sloan FoundationCentres de Recerca de CatalunyaUniversity of PortsmouthRoyal SocietyUniversity of ChicagoFermilabMax-Planck-Institut für AstronomieTexas A and M UniversityUniversità degli Studi di PadovaPrinceton UniversityMinisterio de Ciencia e InnovaciónJohns Hopkins UniversityNational Science FoundationUniversity of MichiganFinanciadora de Estudos e ProjetosStanford UniversitySmithsonian InstitutionUniversity of TokyoHigher Education Funding Council for EnglandUniversity of California, Santa CruzUniversity College LondonNational Aeronautics and Space AdministrationOhio State UniversityQueen's University BelfastGordon and Betty Moore FoundationCentro de Investigaciones Energéticas, Medioambientales y TecnológicasAlexander von Humboldt-StiftungEuropean Regional Development FundMax-Planck-Gesellschaft
KeywordsWeak gravitational lensingPhysicsAstrophysicsGalaxyAmplitudeSigmaPhotometric redshiftRedshiftLens (geology)CalibrationAstronomyOptics

Abstract

fetched live from OpenAlex

ABSTRACT Lensing without borders is a cross-survey collaboration created to assess the consistency of galaxy–galaxy lensing signals (ΔΣ) across different data sets and to carry out end-to-end tests of systematic errors. We perform a blind comparison of the amplitude of ΔΣ using lens samples from BOSS and six independent lensing surveys. We find good agreement between empirically estimated and reported systematic errors which agree to better than 2.3σ in four lens bins and three radial ranges. For lenses with zL > 0.43 and considering statistical errors, we detect a 3–4σ correlation between lensing amplitude and survey depth. This correlation could arise from the increasing impact at higher redshift of unrecognized galaxy blends on shear calibration and imperfections in photometric redshift calibration. At zL > 0.54, amplitudes may additionally correlate with foreground stellar density. The amplitude of these trends is within survey-defined systematic error budgets that are designed to include known shear and redshift calibration uncertainty. Using a fully empirical and conservative method, we do not find evidence for large unknown systematics. Systematic errors greater than 15 per cent (25 per cent) ruled out in three lens bins at 68 per cent (95 per cent) confidence at z < 0.54. Differences with respect to predictions based on clustering are observed to be at the 20–30 per cent level. Our results therefore suggest that lensing systematics alone are unlikely to fully explain the ‘lensing is low’ effect at z < 0.54. This analysis demonstrates the power of cross-survey comparisons and provides a promising path for identifying and reducing systematics in future lensing 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 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)0.011
metaresearch head score (Gemma)0.026
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 score0.011
Threshold uncertainty score0.057

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0110.026
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0040.003
Science and technology studies0.0010.001
Scholarly communication0.0020.002
Open science0.0010.003
Research integrity0.0010.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.026
GPT teacher head0.300
Teacher spread0.274 · 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".

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Citations1
Published2021
Admission routes2
Has abstractyes

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