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Record W4295887012 · doi:10.1093/mnras/stad2945

Dark Energy Survey Year 3 results: redshift calibration of the <scp>MagLim</scp> lens sample from the combination of SOMPZ and clustering and its impact on cosmology

2023· article· en· W4295887012 on OpenAlexfundno aff
G. Giannini, A. Alarcon, M. Gatti, A. Porredon, M. Crocce, G. M. Bernstein, R. Cawthon, C. Sánchez, C. Doux, J. Elvin-Poole, Marco Raveri, J. Myles, Huey-Wen Lin, A. Amon, S. Allam, O. Alves, F. Andrade-Oliveira, Eric J. Baxter, K Bechtol, M. R. Becker, J Blazek, H. Camacho, A. Campos, A. Carnero Rosell, M. Carrasco Kind, A. Choi, J. Cordero, J. De Vicente, Joseph DeRose, H. T. Diehl, Scott Dodelson, A. Drlica-Wagner, K. Eckert, Xiao Fang, Arya Farahi, P. Fosalba, O. Friedrich, D. Gruen, R. A. Gruendl, J. Gschwend, I. Harrison, W.G Hartley, Erica Huff, Mike Jarvis, E. Krause, N. Kuropatkin, Pablo Lemos, N. MacCrann, J. McCullough, J. Muir, Shivam Pandey, J. Prat, M. Rodriguez-Monroy, Ashley J. Ross, E. S. Rykoff, S. Samuroff, L F Secco, I Sevilla-Noarbe, E. Sheldon, M. A. Troxel, D.L. Tucker, N. Weaverdyck, B. Yanny, B. Yin, Y Zhang, T. M. C. Abbott, M. Aguena, David Bacon, E. Bertin, S. Bocquet, D Brooks, D L Burke, J. Carretero, F. J. Castander, M. Costanzi, L. N. da Costa, M. E. S. Pereira, S. Desai, P. Doel, I. Ferrero, B. Flaugher, D. N. Friedel, J. García-Bellido, D. W. Gerdes, G. Gutiérrez, S R Hinton, K. Honscheid, D. J. James, S. Kent, K. Kuehn, O. Lahav, C. Lidman, M. Lima, P. Melchior, J. Mena-Fernández, F. Menanteau, R. Miquel, R. L. C. Ogando, M. Paterno, F. Paz-Chinchón, A. Pieres, A. Roodman, E. Sánchez, V. Scarpine, M. Smith, E. Suchyta, M. E. C. Swanson, G. Tarlé, D. Thomas, C. To, M. Vincenzi

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryLawrence Berkeley National LaboratoryArgonne National LaboratoryUniversity of EdinburghIntegrated Electronics Engineering Center, Binghamton UniversityYork UniversityMinistério da Ciência, Tecnologia e InovaçãoScience and Technology Facilities CouncilOffice of ScienceUniversity of Colorado BoulderUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstrophysikUniversity of SussexInstitut de Física d'Altes EnergiesUniversity College LondonFundación Bancaria Caixa d'Estalvis i Pensions de BarcelonaUniversidad Nacional Autónoma de MéxicoCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoGeneralitat de CatalunyaHigh Energy PhysicsDeutsche ForschungsgemeinschaftFermilabMax-Planck-Institut für AstronomieUniversity of NottinghamEuropean CommissionUniversity of OxfordUniversity of CambridgeCarnegie Institution for ScienceAlfred P. Sloan FoundationCentres de Recerca de CatalunyaLeibniz-GemeinschaftNational Science FoundationUniversity of MichiganUniversity of Notre DameEuropean Regional Development FundCarnegie Mellon UniversityUniversity of WashingtonJohns Hopkins UniversityUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahCarnegie Institution of WashingtonVanderbilt UniversityUniversity of ChicagoOhio State UniversityYale UniversityU.S. Department of EnergySmithsonian InstitutionFinanciadora de Estudos e ProjetosUniversity of Pennsylvania
KeywordsPhysicsRedshiftCosmologyAstrophysicsDark energyGalaxyCalibrationRedshift surveyDark matterPhotometric redshiftWeak gravitational lensingCluster analysisLens (geology)OpticsStatistics

Abstract

fetched live from OpenAlex

ABSTRACT We present an alternative calibration of the MagLim lens sample redshift distributions from the Dark Energy Survey (DES) first 3 yr of data (Y3). The new calibration is based on a combination of a self-organizing-map-based scheme and clustering redshifts to estimate redshift distributions and inherent uncertainties, which is expected to be more accurate than the original DES Y3 redshift calibration of the lens sample. We describe in detail the methodology, and validate it on simulations and discuss the main effects dominating our error budget. The new calibration is in fair agreement with the fiducial DES Y3 n(z) calibration, with only mild differences (<3σ) in the means and widths of the distributions. We study the impact of this new calibration on cosmological constraints, analysing DES Y3 galaxy clustering and galaxy–galaxy lensing measurements, assuming a Lambda cold dark matter cosmology. We obtain Ωm = 0.30 ± 0.04, σ8 = 0.81 ± 0.07, and S8 = 0.81 ± 0.04, which implies a ∼0.4σ shift in the Ω − S8 plane compared to the fiducial DES Y3 results, highlighting the importance of the redshift calibration of the lens sample in multiprobe cosmological analyses.

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)0.005
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 score0.018
Threshold uncertainty score0.036

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.005
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.001

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 head0.012
GPT teacher head0.214
Teacher spread0.202 · 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

Citations11
Published2023
Admission routes1
Has abstractyes

Explore more

Same venueMonthly Notices of the Royal Astronomical Society→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→