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Record W4399837726 · doi:10.1093/mnras/stae2654

Dark energy survey year 3 results: cosmology from galaxy clustering and galaxy–galaxy lensing in harmonic space

2024· article· en· W4399837726 on OpenAlexaff
L Faga, F. Andrade-Oliveira, H. Camacho, R G Rosenfeld, M. Lima, C. Doux, Xiao Fang, J. Prat, A. Porredon, M. Aguena, A. Alarcon, S Allam, O. Alves, A. Amon, S. Àvila, D. Bacon, K Bechtol, M. R. Becker, G. M. Bernstein, J. Blazek, S. Bocquet, D. Brooks, E. Buckley‐Geer, A. Campos, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, R. Cawthon, C. Chang, R Chen, A. Choi, J. Cordero, M. Crocce, L. N. da Costa, M. E. S. Pereira, Joseph DeRose, H. T. Diehl, Scott Dodelson, A. Drlica-Wagner, J. Elvin-Poole, S. Everett, I. Ferrero, A. Ferté, B. Flaugher, P. Fosalba, J. Frieman, J. García-Bellido, M. Gatti, E. Gaztañaga, G. Giannini, D. Gruen, R. A. Gruendl, G Gutierrez, I Harrison, S. R. Hinton, K. Honscheid, Dragan Huterer, D. J. James, Mike Jarvis, T. Jeltema, K. Kuehn, O. Lahav, S Lee, C. Lidman, N. MacCrann, J. L. Marshall, J. McCullough, J. Mena-Fernández, R. Miquel, J Myles, A Navarro-Alsina, A Palmese, Shivam Pandey, M. Paterno, A. Pieres, A A Plazas Malagón, M Raveri, M. Rodriguez-Monroy, R. P. Rollins, Ashley J. Ross, E. S. Rykoff, S. Samuroff, C. Sánchez, E. Sánchez, D Sanchez Cid, M. Schubnell, L F Secco, I. Sevilla-Noarbe, E. Sheldon, T. Shin, M. Smith, M. Soares-Santos, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, M. A. Troxel, B. Tucker, I. Tutusaus, N. Weaverdyck, P. Wiseman, B. Yanny, B. Yin

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of Waterloo
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundScience and Technology Facilities CouncilOffice of ScienceUniversity of Illinois at Urbana-ChampaignInstitut de Física d'Altes EnergiesInstituto Nacional de Ciência e Tecnologia de AstrofísicaUniversidade Estadual PaulistaFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoMinisterio de Economía y CompetitividadGeneralitat de CatalunyaUniversity of SussexUniversity College LondonNational Energy Research Scientific Computing CenterHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaFundação de Amparo à Pesquisa do Estado de São PauloMinistério da Ciência, Tecnologia e InovaçãoCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorLawrence Berkeley National LaboratoryFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaHigher Education Funding Council for EnglandUniversity of PortsmouthUniversity of ChicagoTexas A and M UniversitySchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungOhio State UniversityStanford UniversityChinese Academy of Agricultural SciencesUniversity of Illinois SystemEuropean CommissionU.S. Department of EnergyUniversity of CaliforniaFermilabNational Science Foundation
KeywordsPhysicsAstrophysicsDark energyGalaxyWeak gravitational lensingCosmologyAstronomyRedshift

Abstract

fetched live from OpenAlex

ABSTRACT We present the joint tomographic analysis of galaxy-galaxy lensing and galaxy clustering in harmonic space (HS), using galaxy catalogues from the first three years of observations by the Dark Energy Survey (DES Y3). We utilize the redMaGiC and MagLim catalogues as lens galaxies and the metacalibration catalogue as source galaxies. The measurements of angular power spectra are performed using the pseudo-$C_\ell$ method, and our theoretical modelling follows the fiducial analyses performed by DES Y3 in configuration space, accounting for galaxy bias, intrinsic alignments, magnification bias, shear magnification bias and photometric redshift uncertainties. We explore different approaches for scale cuts based on non-linear galaxy bias and baryonic effects contamination. Our fiducial covariance matrix is computed analytically, accounting for mask geometry in the Gaussian term, and including non-Gaussian contributions and super-sample covariance terms. To validate our HS pipelines and covariance matrix, we used a suite of 1800 log-normal simulations. We also perform a series of stress tests to gauge the robustness of our HS analysis. In the $\Lambda$CDM model, the clustering amplitude $S_8 =\sigma _8(\Omega _m/0.3)^{0.5}$ is constrained to $S_8 = 0.704\pm 0.029$ and $S_8 = 0.753\pm 0.024$ (68 per cent C.L.) for the redMaGiC and MagLim catalogues, respectively. For the wCDM, the dark energy equation of state is constrained to $w = -1.28 \pm 0.29$ and $w = -1.26^{+0.34}_{-0.27}$, for redMaGiC and MagLim catalogues, respectively. These results are compatible with the corresponding DES Y3 results in configuration space and pave the way for HS analyses using the DES Y6 data.

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)0.002
metaresearch head score (Gemma)0.004
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 score0.045
Threshold uncertainty score0.090

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0020.004
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
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 head0.010
GPT teacher head0.206
Teacher spread0.196 · 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

Citations18
Published2024
Admission routes1
Has abstractyes

Explore more

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