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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 OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.
fundA Canadian funder is recorded on the work.

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.

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: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.269
Threshold uncertainty score0.554

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 science0.0000.001
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 head0.009
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