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Record W3216802950 · doi:10.1093/mnras/stab3311

Dark Energy Survey Year 3 Results: clustering redshifts – calibration of the weak lensing source redshift distributions with <i>redMaGiC</i> and BOSS/eBOSS

2021· article· en· W3216802950 on OpenAlexafffund
M. Gatti, G. Giannini, G. M. Bernstein, A. Alarcon, J. Myles, A. Amon, R. Cawthon, M. A. Troxel, Joseph DeRose, S. Everett, Ashley J. Ross, E. S. Rykoff, J. Elvin-Poole, J. Cordero, I. Harrison, C. Sánchez, J. Prat, D. Gruen, H. Lin, M. Crocce, Eduardo Rozo, T. M. C. Abbott, M. Aguena, S. Allam, J. Annis, S. Àvila, David Bacon, E. Bertin, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, A. Choi, Christopher J. Conselice, M. Costanzi, L. N. da Costa, M. E. S. Pereira, Kyle Dawson, S Desai, H. T. Diehl, K. Eckert, T. F. Eifler, A E Evrard, I. Ferrero, B. Flaugher, P. Fosalba, J Frieman, J. García-Bellido, E. Gaztañaga, T. Giannantonio, R. A. Gruendl, J. Gschwend, S. R. Hinton, Klaus Honscheid, B Hoyle, Dragan Huterer, D. J. James, K. Kuehn, N. Kuropatkin, O. Lahav, M. Lima, N MacCrann, M. A. G. Maia, M. March, J. L. Marshall, P. Melchior, F. Menanteau, R Miquel, J J Mohr, R. Morgan, R. L. C. Ogando, A. Palmese, F. Paz-Chinchón, Will J. Percival, M Rodriguez-Monroy, A. Roodman, Graziano Rossi, S Samuroff, E. Sánchez, V. Scarpine, L F Secco, S. Serrano, I. Sevilla-Noarbe, M. Smith, M. Soares-Santos, E. Suchyta, M E C Swanson, G. Tarlé, D. Thomas, C. To, T N Varga, J. Weller, R. D. Wilkinson

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstronomy and Astrophysical Research
Canadian institutionsPerimeter InstituteUniversity of Waterloo
FundersSLAC National Accelerator LaboratoryH2020 European Research CouncilLawrence Berkeley National LaboratoryArgonne National LaboratoryHigh Energy PhysicsCentro de Investigaciones Energéticas, Medioambientales y TecnológicasEuropean Regional Development FundLeibniz-GemeinschaftUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstrophysikUniversity College LondonFundación Bancaria Caixa d'Estalvis i Pensions de BarcelonaUniversidad Nacional Autónoma de MéxicoYale UniversityU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoScience and Technology Facilities CouncilYork UniversityMinistério da Ciência, Tecnologia e InovaçãoMinisterio de Economía y CompetitividadUniversity of SussexInstitut de Física d'Altes EnergiesEidgenössische Technische Hochschule ZürichGeneralitat de CatalunyaDeutsche ForschungsgemeinschaftUniversity of Colorado BoulderOffice of ScienceFermilabTexas A and M UniversityMax-Planck-Institut für AstronomieIntegrated Electronics Engineering Center, Binghamton UniversityUniversity of EdinburghUniversity of NottinghamEuropean CommissionCarnegie Institution for ScienceAlfred P. Sloan FoundationCentres de Recerca de CatalunyaUniversity of OxfordCarnegie Institution of WashingtonUniversity of VirginiaCarnegie Mellon UniversityVanderbilt UniversityUniversity of ChicagoUniversity of Notre DameHigher Education Funding Council for EnglandUniversity of TokyoUniversity of ArizonaUniversity of WashingtonJohns Hopkins UniversityUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahOhio State UniversityFinanciadora de Estudos e ProjetosStanford UniversitySmithsonian InstitutionNational Science FoundationUniversity of Pennsylvania
KeywordsPhysicsRedshiftWeak gravitational lensingBossDark energyAstrophysicsCluster analysisCalibrationAstronomyPhotometric redshiftRedshift surveyCosmologyGalaxyStatistics

Abstract

fetched live from OpenAlex

ABSTRACT We present the calibration of the Dark Energy Survey Year 3 (DES Y3) weak lensing (WL) source galaxy redshift distributions n(z) from clustering measurements. In particular, we cross-correlate the WL source galaxies sample with redMaGiC galaxies (luminous red galaxies with secure photometric redshifts) and a spectroscopic sample from BOSS/eBOSS to estimate the redshift distribution of the DES sources sample. Two distinct methods for using the clustering statistics are described. The first uses the clustering information independently to estimate the mean redshift of the source galaxies within a redshift window, as done in the DES Y1 analysis. The second method establishes a likelihood of the clustering data as a function of n(z), which can be incorporated into schemes for generating samples of n(z) subject to combined clustering and photometric constraints. Both methods incorporate marginalization over various astrophysical systematics, including magnification and redshift-dependent galaxy-matter bias. We characterize the uncertainties of the methods in simulations; the first method recovers the mean z of tomographic bins to RMS (precision) of ∼0.014. Use of the second method is shown to vastly improve the accuracy of the shape of n(z) derived from photometric data. The two methods are then applied to the DES Y3 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)0.003
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 score0.038
Threshold uncertainty score0.076

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.004
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.000
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 head0.009
GPT teacher head0.214
Teacher spread0.205 · 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".

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Citations77
Published2021
Admission routes2
Has abstractyes

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