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Record W4383046449 · doi:10.1088/1475-7516/2024/01/033

Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4

2024· article· en· W4383046449 on OpenAlexaff
Gabriela A. Marques, Mathew S. Madhavacheril, Omar Darwish, Shabbir Shaikh, M. Aguena, O. Alves, S. Àvila, D. Bacon, Eric J. Baxter, K. Bechtol, M. R. Becker, E. Bertin, J. Blazek, J. Richard Bond, D. Brooks, Haiying Cai, Erminia Calabrese, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, R. Cawthon, M. Crocce, L. N. da Costa, M. E. S. Pereira, J. De Vicente, S. Desai, H. T. Diehl, P. Doel, C. Doux, A. Drlica-Wagner, Jo Dunkley, J. Elvin-Poole, S. Everett, Simone Ferraro, I. Ferrero, B. Flaugher, P. Fosalba, J. García-Bellido, M. Gatti, G. Giannini, Vera Gluscevic, D. Gruen, R. A. Gruendl, G. Gutiérrez, I. Harrison, J. Colin Hill, S. R. Hinton, D.L Hollowood, K. Honscheid, Dragan Huterer, N Jeffrey, Joshua Kim, K. Kuehn, O. Lahav, Pablo Lemos, M. Lima, K. M. Huffenberger, N. MacCrann, J. L. Marshall, J. Mena-Fernández, R. Miquel, J. J. Mohr, Kavilan Moodley, J. Muir, Sigurd Næss, F. Nati, Lyman A. Page, A. Palmese, A. Porredon, J. Prat, Frank J. Qu, Marco Raveri, Ashley J. Ross, E. S. Rykoff, Gerrit S. Farren, S. Samuroff, E. Sánchez, M. Schubnell, Neelima Sehgal, I Sevilla-Noarbe, E. Sheldon, B. D. Sherwin, Cristobál Sifón, M. Smith, David N. Spergel, Suzanne T. Staggs, G. Tarlé, C. To, Alexander van Engelen, N. Weaverdyck, J. Weller, L. Wenzl, P. Wiseman, Edward J. Wollack, B. Yanny

Bibliographic record

VenueJournal of Cosmology and Astroparticle Physics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversité de MontréalCentre for Research in Astrophysics of QuébecUniversity of WaterlooUniversity of TorontoPerimeter Institute
FundersSLAC National Accelerator LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundScience and Technology Facilities CouncilOffice of ScienceUniversity of Illinois at Urbana-ChampaignNational Institute of Standards and TechnologyInstitut de Física d'Altes EnergiesConselho Nacional de Desenvolvimento Científico e TecnológicoEuropean CommissionMinisterio de Ciencia e InnovaciónAgencia Nacional de Investigación y DesarrolloGeneralitat de CatalunyaLawrence Berkeley National LaboratoryUniversity of PennsylvaniaFinanciadora de Estudos e ProjetosFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroUniversity of SussexOhio State UniversityNational Research FoundationNational Aeronautics and Space AdministrationUniversity College LondonNational Energy Research Scientific Computing CenterUniversity of ChicagoSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungMinistério da Ciência, Tecnologia e InovaçãoHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaU.S. Department of EnergyAlfred P. Sloan FoundationPrinceton UniversityUniversity of PortsmouthFermilabNational Science Foundation
KeywordsPhysicsAstrophysicsCosmic microwave backgroundGalaxyRedshiftSouth Pole TelescopePlanckCosmologyDark energyAstronomySpectral densityCorrelation function (quantum field theory)Anisotropy

Abstract

fetched live from OpenAlex

Abstract We present a measurement of the cross-correlation between the MagLim galaxies selected from the Dark Energy Survey (DES) first three years of observations (Y3) and cosmic microwave background (CMB) lensing from the Atacama Cosmology Telescope (ACT) Data Release 4 (DR4), reconstructed over ∼ 436 deg 2 of the sky. Our galaxy sample, which covers ∼ 4143 deg 2 , is divided into six redshift bins spanning the redshift range of 0.20<z<1.05. We adopt a blinding procedure until passing all consistency and systematics tests. After imposing scale cuts for the cross-power spectrum measurement, we reject the null hypothesis of no correlation at 9.1σ. We constrain cosmological parameters from a joint analysis of galaxy and CMB lensing-galaxy power spectra considering a flat ΛCDM model, marginalized over 23 astrophysical and systematic nuisance parameters. We find the clustering amplitude S 8 ≡ σ 8 (Ω m /0.3) 0.5 = 0.75 +0.04 -0.05 . In addition, we constrain the linear growth of cosmic structure as a function of redshift. Our results are consistent with recent DES Y3 analyses and suggest a preference for a lower S 8 compared to results from measurements of CMB anisotropies by the Planck satellite, although at a mild level (< 2 σ ) of statistical significance.

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 distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation 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 score0.100
Threshold uncertainty score0.401

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0000.001
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.012
GPT teacher head0.222
Teacher spread0.209 · 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 teacher head, 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

Citations22
Published2024
Admission routes1
Has abstractyes

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