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Record W2965744020 · doi:10.1103/physrevd.100.043501

Dark Energy Survey Year 1 Results: Tomographic cross-correlations between Dark Energy Survey galaxies and CMB lensing from South Pole <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>Telescope</mml:mi><mml:mo>+</mml:mo><mml:mi>Planck</mml:mi></mml:mrow></mml:math>

2019· article· en· W2965744020 on OpenAlexafffund
Y. Omori, T. Giannantonio, A. Porredon, Eric J. Baxter, C. Chang, M. Crocce, P. Fosalba, A. Alarcon, Nilanjan Banik, J. Blazek, L. E. Bleem, S. L. Bridle, R. Cawthon, A. Choi, Ryan Chown, Thomas O. Crawford, Scott Dodelson, A. Drlica-Wagner, T. F. Eifler, J. Elvin-Poole, O. Friedrich, D. Gruen, G. P. Holder, Dragan Huterer, Bhuvnesh Jain, Mike Jarvis, D. Kirk, Nickolas Kokron, E. Krause, N. MacCrann, J. Muir, J. Prat, C. L. Reichardt, Ashley J. Ross, Eduardo Rozo, E. S. Rykoff, C. Sánchez, L. F. Secco, G. Simard, Risa H. Wechsler, J. Zuntz, T. M. C. Abbott, F. B. Abdalla, S. Allam, S. Àvila, K. Aylor, B. A. Benson, G. M. Bernstein, E. Bertin, F. Bianchini, D. Brooks, E. Buckley-Geer, D. L. Burke, J. E. Carlstrom, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, C. L. Chang, H-M. Cho, A. T. Crites, Carlos E. Cunha, L. N. da Costa, T. de Haan, C. Davis, J. De Vicente, S. Desai, H. T. Diehl, J. P. Dietrich, M. Dobbs, W. Everett, Peter Doel, J. Estrada, B. Flaugher, J. Frieman, J. García-Bellido, E. Gaztañaga, D. W. Gerdes, E. M. George, R. A. Gruendl, J. Gschwend, G. Gutierrez, N. W. Halverson, N. L. Harrington, W. G. Hartley, W. L. Holzapfel, K. Honscheid, Z. Hou, B. Hoyle, J. D. Hrubes, D. J. James, T. Jeltema, K. Kuehn, N. Kuropatkin, A. T. Lee, E. M. Leitch, M. Lima, D. Luong-Van, A. Manzotti, Daniel P. Marrone, J. L. Marshall, J. J. McMahon, P. Melchior, F. Menanteau, S. S. Meyer, C. J. Miller, R. Miquel, L. M. Mocanu, J. J. Mohr, T. Natoli, S. Padin, A. A. Plazas, C. Pryke, A. K. Romer, A. Roodman, J. E. Ruhl, E. Sánchez, V. Scarpine, K. K. Schaffer, M. Schubnell, S. Serrano, I Sevilla-Noarbe, E. Shirokoff, M. Smith, M. Soares-Santos, F. Sobreira, Z. Staniszewski, A. A. Stark, K. T. Story, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, M. A. Troxel, K. Vanderlinde, J. D. Vieira, A. R. Walker, W. L. K. Wu, O. Zahn

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of TorontoMcMaster UniversityCanadian Institute for Advanced ResearchMcGill University
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundAustralian Research CouncilScience and Technology Facilities CouncilNatural Sciences and Engineering Research Council of CanadaOffice of ScienceUniversity of Illinois at Urbana-ChampaignInstitut de Física d'Altes EnergiesARC Centre of Excellence for All-Sky AstrophysicsFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroMinistério da Ciência, Tecnologia e InovaçãoMinisterio de Economía y CompetitividadGeneralitat de CatalunyaNational Aeronautics and Space AdministrationUniversity College LondonHigh Energy PhysicsMcGill UniversityDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaJet Propulsion LaboratoryMinistère de l'Économie, de la Science et de l'Innovation - QuébecUniversity of Illinois SystemUniversity of California, Los AngelesUniversity of PortsmouthTexas A and M UniversityUniversity of ChicagoCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoCanada Research ChairsOhio State UniversityCalifornia Institute of TechnologyHigher Education Funding Council for EnglandLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaEuropean CommissionU.S. Department of EnergyUniversity of SussexSeventh Framework ProgrammeGordon and Betty Moore FoundationCompute CanadaFermilabNational Science Foundation
KeywordsPhysicsCosmic microwave backgroundDark energyAstrophysicsSouth Pole TelescopeGalaxyPlanckRedshiftWeak gravitational lensingCosmologyOmegaGravitational lensPhotometric redshiftRedshift surveyAstronomy

Abstract

fetched live from OpenAlex

We measure the cross-correlation between redMaGiC galaxies selected from the Dark Energy Survey (DES) year 1 data and gravitational lensing of the cosmic microwave background (CMB) reconstructed from South Pole Telescope (SPT) and Planck data over $1289\text{ }\text{ }{\mathrm{deg}}^{2}$. When combining measurements across multiple galaxy redshift bins spanning the redshift range of $0.15<z<0.90$, we reject the hypothesis of no correlation at $19.9\ensuremath{\sigma}$ significance. When removing small-scale data points where thermal Sunyaev-Zel'dovich signal and nonlinear galaxy bias could potentially bias our results, the detection significance is reduced to $9.9\ensuremath{\sigma}$. We perform a joint analysis of galaxy-CMB lensing cross-correlations and galaxy clustering to constrain cosmology, finding ${\mathrm{\ensuremath{\Omega}}}_{\mathrm{m}}=0.27{6}_{\ensuremath{-}0.030}^{+0.029}$ and ${S}_{8}={\ensuremath{\sigma}}_{8}\sqrt{{\mathrm{\ensuremath{\Omega}}}_{\mathrm{m}}/0.3}=0.80{0}_{\ensuremath{-}0.094}^{+0.090}$. We also perform two alternate analyses aimed at constraining only the growth rate of cosmic structure as a function of redshift, finding consistency with predictions from the concordance $\mathrm{\ensuremath{\Lambda}}\mathrm{CDM}$ model. The measurements presented here are part of a joint cosmological analysis that combines galaxy clustering, galaxy lensing and CMB lensing using data from DES, SPT and Planck.

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 score0.027
Threshold uncertainty score0.054

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.003
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0040.003
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0060.001

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 head0.015
GPT teacher head0.287
Teacher spread0.271 · 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

Citations54
Published2019
Admission routes2
Has abstractyes

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