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Record W2786929267 · doi:10.1103/physrevd.99.023508

Dark Energy Survey Year 1 results: Methodology and projections for joint analysis of galaxy clustering, galaxy lensing, and CMB lensing two-point functions

2019· article· en· W2786929267 on OpenAlexaff
Eric J. Baxter, Y. Omori, C. Chang, T. Giannantonio, D. Kirk, E. Krause, J. Blazek, L. E. Bleem, A. Choi, T. M. Crawford, Scott Dodelson, T. F. Eifler, O. Friedrich, D. Gruen, G. P. Holder, Bhuvnesh Jain, Mike Jarvis, N. MacCrann, Andrina Nicola, Shivam Pandey, J. Prat, C. L. Reichardt, S. Samuroff, C. Sánchez, L. F. Secco, E. Sheldon, M. A. Troxel, J. Zuntz, T. M. C. Abbott, F. B. Abdalla, J. Annis, S. Àvila, K. Bechtol, B. A. Benson, E. Bertin, D. Brooks, E. Buckley‐Geer, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, R. Cawthon, C. E. Cunha, C. B. D’Andrea, L. N. da Costa, C. Davis, J. De Vicente, D. L. DePoy, H. T. Diehl, P. Doel, J. Estrada, A. E. Evrard, B. Flaugher, P. Fosalba, J. García-Bellido, E. Gaztañaga, D. W. Gerdes, R. A. Gruendl, J. Gschwend, G. Gutiérrez, W. G. Hartley, B. Hoyle, D. J. James, S. Kent, K. Kuehn, N. Kuropatkin, O. Lahav, M. Lima, M. A. G. Maia, M. March, J. L. Marshall, P. Melchior, F. Menanteau, R. Miquel, A. Roodman, E. S. Rykoff, E. Sánchez, R. Schindler, M. Schubnell, I. Sevilla-Noarbe, M. Smith, Rory Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, M. E. C. Swanson, G. Tarlé, A. R. Walker, W. L. K. Wu, J. Weller

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Advanced ResearchMcGill University
FundersSLAC National Accelerator LaboratoryUniversity of EdinburghIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundAustralian Research CouncilMinistério da Ciência, Tecnologia e InovaçãoScience and Technology Facilities CouncilGordon and Betty Moore FoundationH2020 European Research CouncilSmithsonian Astrophysical ObservatoryArmstrong Flight Research CenterUniversity of Illinois at Urbana-ChampaignU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoMinisterio de Economía y CompetitividadGeneralitat de CatalunyaOffice of ScienceUniversity of NottinghamSmithsonian InstitutionARC Centre of Excellence for All-Sky AstrophysicsUniversity of CambridgeNational Aeronautics and Space AdministrationUniversity College LondonUniversity of SussexInstitut de Física d'Altes EnergiesEidgenössische Technische Hochschule ZürichNational Centre for Supercomputing ApplicationsUniversity of PortsmouthFermilabTexas A and M UniversityUniversity of ChicagoOhio State UniversityHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryAlfred P. Sloan FoundationCentres de Recerca de CatalunyaKavli FoundationNational Science FoundationUniversity of MichiganHigher Education Funding Council for EnglandLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaSeventh Framework ProgrammeEuropean Commission
KeywordsPhysicsWeak gravitational lensingCosmic microwave backgroundPlanckDark energyAstrophysicsGravitational lensStrong gravitational lensingCosmologyGalaxyGravitational lensing formalismSouth Pole TelescopeAstronomyGalaxy clusterRedshiftAnisotropy

Abstract

fetched live from OpenAlex

Optical imaging surveys measure both the galaxy density and the gravitational lensing-induced shear fields across the sky. Recently, the Dark Energy Survey (DES) Collaboration used a joint fit to two-point correlations between these observables to place tight constraints on cosmology (T. M. C. Abbott et al. (Dark Energy Survey Collaboration), Phys. Rev. D 98, 043526 (2018)). In this work, we develop the methodology to extend the DES Year 1 joint probes analysis to include cross-correlations of the optical survey observables with gravitational lensing of the cosmic microwave background as measured by the South Pole Telescope (SPT) and Planck. Using simulated analyses, we show how the resulting set of five two-point functions increases the robustness of the cosmological constraints to systematic errors in galaxy lensing shear calibration. Additionally, we show that contamination of the SPT+Planck cosmic microwave background lensing map by the thermal Sunyaev-Zel'dovich effect is a potentially large source of systematic error for two-point function analyses but show that it can be reduced to acceptable levels in our analysis by masking clusters of galaxies and imposing angular scale cuts on the two-point functions. The methodology developed here will be applied to the analysis of data from the DES, the SPT, and Planck in a companion work.

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)0.023
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Simulation or modeling · Consensus signal: none
GenreCandidate signal: Methods · Consensus signal: Methods
Teacher disagreement score0.014
Threshold uncertainty score0.061

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0110.023
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0050.004
Science and technology studies0.0010.001
Scholarly communication0.0020.001
Open science0.0010.002
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0060.002

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 head0.043
GPT teacher head0.384
Teacher spread0.341 · 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 designSimulation or modeling
Domainnot available
GenreMethods

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

Citations52
Published2019
Admission routes1
Has abstractyes

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