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Record W4221145089 · doi:10.1093/mnras/stac1826

Dark energy survey year 3 results: cosmological constraints from the analysis of cosmic shear in harmonic space

2022· article· en· W4221145089 on OpenAlexaff
C. Doux, Bhuvnesh Jain, D Zeurcher, J Lee, Xiao Fang, R. Rosenfeld, A. Amon, H. Camacho, A. Choi, L F Secco, J. Blazek, C. Chang, M. Gatti, E. Gaztañaga, N Jeffrey, Marco Raveri, S. Samuroff, A. Alarcon, O. Alves, F. Andrade-Oliveira, Eric J. Baxter, K. Bechtol, M. R. Becker, G. M. Bernstein, A. Campos, A. Carnero Rosell, M. Carrasco Kind, R. Cawthon, R Chen, J. Cordero, M. Crocce, C. Davis, J. DeRose, Scott Dodelson, A. Drlica-Wagner, K. Eckert, T. F. Eifler, F. Elsner, J. Elvin-Poole, S. Everett, A. Ferté, P. Fosalba, O. Friedrich, G. Giannini, D. Gruen, R. A. Gruendl, I. Harrison, W. G. Hartley, K. Herner, Hung-Jin Huang, Eric Huff, Dragan Huterer, Mike Jarvis, E. Krause, N. Kuropatkin, P-F Leget, Pablo Lemos, Andrew R. Liddle, N. MacCrann, J. McCullough, J. Muir, J. Myles, A Navarro-Alsina, Shivam Pandey, Youngsoo Park, A. Porredon, J. Prat, M. Rodríguez-Monroy, R. P. Rollins, A. Roodman, Ashley J. Ross, E. S. Rykoff, C. Sánchez, Javier Sánchez, I. Sevilla-Noarbe, E. Sheldon, T. Shin, A. Troja, M. A. Troxel, I. Tutusaus, T N Varga, N. Weaverdyck, Risa H. Wechsler, B. Yanny, B. Yin, Y. Zhang, J. Zuntz, T. M. C. Abbott, M. Aguena, S. Allam, J. Annis, David Bacon, E. Bertin, S. Bocquet, D. Brooks, D. L. Burke, J. Carretero, M. Costanzi, L. N. da Costa, M. E. S. Pereira, J. De Vicente, S. Desai, H. T. Diehl, P. Doel, I. Ferrero, B. Flaugher, J. Frieman, J. García-Bellido, D. W. Gerdes, T. Giannantonio, J. Gschwend, G. Gutiérrez, S. R. Hinton, K. Honscheid, D. J. James, Alex Kim, K. Kuehn, O. Lahav, J. L. Marshall, F. Menanteau, R. Miquel, R. Morgan, R. L. C. Ogando, A. Palmese, F. Paz-Chinchón, A. Pieres, A A Plazas Malagón, K Reil, E. Sánchez, V Scarpine, S. Serrano, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarlé, David Thomas, C. To, J. Weller

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsPerimeter Institute
FundersSLAC National Accelerator LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundScience and Technology Facilities CouncilInstitut de Física d'Altes EnergiesUniversity of Illinois at Urbana-ChampaignLawrence Berkeley National LaboratoryUniversity of PennsylvaniaFinanciadora de Estudos e ProjetosFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoEuropean CommissionMinisterio de Ciencia e InnovaciónGeneralitat de CatalunyaOffice of ScienceUniversity of EdinburghUniversity of NottinghamUniversity College LondonNational Aeronautics and Space AdministrationHigher Education Funding Council for EnglandUniversity of PortsmouthUniversity of ChicagoOhio State UniversityUniversity of MichiganHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaU.S. Department of EnergyUniversity of CambridgeFermilabNational Science Foundation
KeywordsPhysicsCosmic microwave backgroundDark energyPlanckSpectral densityEstimatorOmegaAstrophysicsBaryon acoustic oscillationsSigmaGaussianCosmic background radiationCosmologyStatisticsQuantum mechanics

Abstract

fetched live from OpenAlex

ABSTRACT We present cosmological constraints from the analysis of angular power spectra of cosmic shear maps based on data from the first three years of observations by the Dark Energy Survey (DES Y3). Our measurements are based on the pseudo-Cℓ method and complement the analysis of the two-point correlation functions in real space, as the two estimators are known to compress and select Gaussian information in different ways, due to scale cuts. They may also be differently affected by systematic effects and theoretical uncertainties, making this analysis an important cross-check. Using the same fiducial Lambda cold dark matter model as in the DES Y3 real-space analysis, we find ${S_8 \equiv \sigma _8 \sqrt{\Omega _{\rm m}/0.3} = 0.793^{+0.038}_{-0.025}}$, which further improves to S8 = 0.784 ± 0.026 when including shear ratios. This result is within expected statistical fluctuations from the real-space constraint, and in agreement with DES Y3 analyses of non-Gaussian statistics, but favours a slightly higher value of S8, which reduces the tension with the Planck 2018 constraints from 2.3σ in the real space analysis to 1.5σ here. We explore less conservative intrinsic alignments models than the one adopted in our fiducial analysis, finding no clear preference for a more complex model. We also include small scales, using an increased Fourier mode cut-off up to $k_{\rm max}={5}\, {h}\, {\rm Mpc}^{-1}$, which allows to constrain baryonic feedback while leaving cosmological constraints essentially unchanged. Finally, we present an approximate reconstruction of the linear matter power spectrum at present time, found to be about 20 per cent lower than predicted by Planck 2018, as reflected by the lower S8 value.

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)0.003
metaresearch head score (Gemma)0.006
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 score0.016
Threshold uncertainty score0.032

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.006
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 integrity0.0000.001
Insufficient payload (model declined to judge)0.0040.001

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 head0.011
GPT teacher head0.223
Teacher spread0.212 · 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

Citations72
Published2022
Admission routes1
Has abstractyes

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