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Cosmological Constraints from Multiple Probes in the Dark Energy Survey

2019· article· en· W2900358442 on OpenAlexaff
T. M. C. Abbott, A. Alarcon, S. Allam, Per H. Andersen, F. Andrade-Oliveira, J. Annis, J. Asorey, S. Àvila, D. Bacon, N. Banik, Bruce A. Bassett, Eric J. Baxter, K Bechtol, M. R. Becker, G. M. Bernstein, E. Bertin, J. Blazek, S. L. Bridle, D. Brooks, D. Brout, D. L. Burke, J. Calcino, H. Camacho, A. Campos, A. Carnero Rosell, D. Carollo, M. Carrasco Kind, J. Carretero, F. J. Castander, R. Cawthon, P. Challis, Kwan Chuen Chan, C. Chang, M. Childress, M. Crocce, Carlos E. Cunha, C. B. D’Andrea, L. N. da Costa, C. Davis, T. M. Davis, J. De Vicente, D. L. DePoy, J. DeRose, S. Desai, H. T. Diehl, J. P. Dietrich, Scott Dodelson, Peter Doel, A Drlica-Wagner, T. F. Eifler, J. Elvin-Poole, J. Estrada, A. E. Evrard, Elizabeth R. Fernandez, B. Flaugher, R. J. Foley, P. Fosalba, J. Frieman, L. Galbany, J. García-Bellido, M. Gatti, E. Gaztañaga, D. W. Gerdes, T. Giannantonio, Karl Glazebrook, D. A. Goldstein, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, W G Hartley, S. R. Hinton, Klaus Honscheid, J. K. Hoormann, B. Hoyle, Dragan Huterer, Bhuvnesh Jain, D. J. James, Mike Jarvis, T. Jeltema, E. Kasai, S. Kent, R. Keßler, A. G. Kim, Nickolas Kokron, E. Krause, Richard G. Kron, K. Kuehn, N.P. Kuropatkin, O. Lahav, J. Lasker, Pablo Lemos, Geraint F. Lewis, T. S. Li, C. Lidman, M. Lima, Huey-Wen Lin, E. Macaulay, N. MacCrann, M. A. G. Maia, M. March, J. Marriner, J. L. Marshall, Paul Martini, R. G. McMahon, P. Melchior, F. Menanteau, R. Miquel, J. J. Mohr, E. Morganson, J. Muir, A. Möller, E. Neilsen, R. C. Nichol, B. Nord, R. L. C. Ogando, A. Palmese, Y. C. Pan, Hiranya V. Peiris, Will J. Percival, A. Porredon, J. Prat, A. K. Romer, A. Roodman, R. Rosenfeld, Ashley J. Ross, E. S. Rykoff, S. Samuroff, C. Sánchez, E. Sánchez, V. Scarpine, R. Schindler, M. Schubnell, D. Scolnic, L. F. Secco, S. Serrano, I. Sevilla-Noarbe, R. Sharp, E. Sheldon, M Smith, M. Soares-Santos, F. Sobreira, N. E. Sommer, Elizabeth Swann, M E C Swanson, G. Tarlé, D. Thomas, R. C. Thomas, M. A. Troxel, B. E. Tucker, S. A. Uddin, P Vielzeuf, A. R. Walker, M. Wang, N. Weaverdyck, R. H. Wechsler, J. Weller, B. Yanny, B. Zhang, Y. Zhang, J. Zuntz

Bibliographic record

VenuePhysical Review Letters · 2019
Typearticle
Languageen
FieldPhysics and Astronomy
TopicCosmology and Gravitation Theories
Canadian institutionsPerimeter InstituteUniversity of Waterloo
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilIntegrated Electronics Engineering Center, Binghamton UniversityEuropean Regional Development FundAustralian Research CouncilScience and Technology Facilities CouncilOffice of ScienceUniversity of Illinois at Urbana-ChampaignARC Centre of Excellence for All-Sky AstrophysicsCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoMinisterio de Economía y CompetitividadCenter for Cosmology and Astroparticle Physics, Ohio State UniversityUniversity of SussexMinisterio de Educación, Cultura y DeporteEuropean CommissionMinisterio de Ciencia e InnovaciónGeneralitat de CatalunyaLawrence Berkeley National LaboratoryUniversity of PennsylvaniaFinanciadora de Estudos e ProjetosFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroKavli Institute for Cosmological Physics, University of ChicagoNational Energy Research Scientific Computing CenterUniversity College LondonNational Aeronautics and Space AdministrationHigher Education Funding Council for EnglandUniversity of PortsmouthUniversity of California, Santa CruzInstituto Nacional de Ciência e Tecnologia de Fármacos e MedicamentosOhio State UniversityHigh Energy PhysicsDeutsche ForschungsgemeinschaftArgonne National LaboratoryCentres de Recerca de CatalunyaU.S. Department of EnergyInstitut de Física d'Altes EnergiesEidgenössische Technische Hochschule ZürichNational Centre for Supercomputing ApplicationsFermilabNational Science Foundation
KeywordsDark energyPhysicsDark matterCosmologyAstrophysicsEnergy (signal processing)Particle physicsCosmological modelAstronomyNuclear physicsQuantum mechanics

Abstract

fetched live from OpenAlex

The combination of multiple observational probes has long been advocated as a powerful technique to constrain cosmological parameters, in particular dark energy. The Dark Energy Survey has measured 207 spectroscopically confirmed type Ia supernova light curves, the baryon acoustic oscillation feature, weak gravitational lensing, and galaxy clustering. Here we present combined results from these probes, deriving constraints on the equation of state, w, of dark energy and its energy density in the Universe. Independently of other experiments, such as those that measure the cosmic microwave background, the probes from this single photometric survey rule out a Universe with no dark energy, finding w=-0.80_{-0.11}^{+0.09}. The geometry is shown to be consistent with a spatially flat Universe, and we obtain a constraint on the baryon density of Ω_{b}=0.069_{-0.012}^{+0.009} that is independent of early Universe measurements. These results demonstrate the potential power of large multiprobe photometric surveys and pave the way for order of magnitude advances in our constraints on properties of dark energy and cosmology over the next decade.

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)0.004
metaresearch head score (Gemma)0.017
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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.004
Threshold uncertainty score0.024

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.017
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.000
Bibliometrics0.0010.002
Science and technology studies0.0010.001
Scholarly communication0.0010.002
Open science0.0010.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0030.000

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 head0.017
GPT teacher head0.276
Teacher spread0.259 · 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

Citations110
Published2019
Admission routes1
Has abstractyes

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