MétaCan
Menu
← Back to cohort
Record W3117471256 · doi:10.1093/mnras/stac1160

Dark Energy Survey Year 3 results: calibration of lens sample redshift distributions using clustering redshifts with BOSS/eBOSS

2022· article· en· W3117471256 on OpenAlexafffund
R. Cawthon, J. Elvin-Poole, A. Porredon, M. Crocce, G. Giannini, M. Gatti, Ashley J. Ross, E.S. Rykoff, A. Carnero Rosell, Joseph DeRose, S. Lee, M Rodriguez-Monroy, A. Amon, K. Bechtol, J. De Vicente, D. Gruen, R. Morgan, E. Sánchez, J Sanchez, I. Sevilla-Noarbe, T. M. C. Abbott, M. Aguena, S. Allam, J Annis, S. Àvila, D Bacon, E. Bertin, David J. Brooks, D L Burke, M. Carrasco Kind, J. Carretero, F. J. Castander, A. Choi, M. Costanzi, L. N. da Costa, M. E. S. Pereira, Kyle Dawson, S. Desai, H. T. Diehl, K Eckert, S Everett, I. Ferrero, P Fosalba, J Frieman, J. García-Bellido, E. Gaztañaga, R. A. Gruendl, J Gschwend, G Gutierrez, S R Hinton, K Honscheid, Dragan Huterer, D. J. James, Alex Kim, K. Kuehn, N. Kuropatkin, O. Lahav, M. Lima, H. Lin, M A G Maia, P Melchior, F. Menanteau, R. Miquel, J. J. Mohr, J. Muir, J. Myles, A. Palmese, Sahil Pandey, F. Paz-Chinchón, Will J. Percival, A. Roodman, Graziano Rossi, V. Scarpine, S. Serrano, M. Smith, M Soares-Santos, E. Suchyta, M. E. C. Swanson, G. Tarlé, C. To, M. A. Troxel, R. D. Wilkinson

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2022
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsUniversity of Waterloo
FundersSLAC National Accelerator LaboratoryLawrence Berkeley National LaboratoryArgonne National LaboratoryHigh Energy PhysicsCentro de Investigaciones Energéticas, Medioambientales y TecnológicasEuropean Regional Development FundLeibniz-GemeinschaftUniversity of Colorado BoulderOffice of ScienceUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstrophysikUniversity of SussexInstitut de Física d'Altes EnergiesUniversidad Nacional Autónoma de MéxicoYale UniversityU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroNew York UniversityConselho Nacional de Desenvolvimento Científico e TecnológicoScience and Technology Facilities CouncilYork UniversityMinistério da Ciência, Tecnologia e InovaçãoMinisterio de Economía y CompetitividadGeneralitat de CatalunyaDeutsche ForschungsgemeinschaftFermilabTexas A and M UniversityMax-Planck-Institut für AstronomieIntegrated Electronics Engineering Center, Binghamton UniversityUniversity of EdinburghUniversity of NottinghamEuropean CommissionUniversity College LondonCarnegie Institution for ScienceInstituto de Astrofísica de CanariasUniversity of CambridgeAlfred P. Sloan FoundationCentres de Recerca de CatalunyaUniversity of TokyoUniversity of ArizonaHigher Education Funding Council for EnglandUniversity of OxfordPennsylvania State UniversityCarnegie Institution of WashingtonUniversity of VirginiaCarnegie Mellon UniversityVanderbilt UniversityUniversity of ChicagoNational Science FoundationUniversity of MichiganUniversity of Notre DameUniversity of WashingtonJohns Hopkins UniversityUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahOhio State UniversitySmithsonian InstitutionFinanciadora de Estudos e ProjetosUniversity of Pennsylvania
KeywordsRedshiftPhysicsAstrophysicsDark energyPhotometric redshiftGalaxyGravitational lensBaryonRedshift surveyRedshift-space distortionsWeak gravitational lensingCluster analysisCosmologyAstronomyStatistics

Abstract

fetched live from OpenAlex

ABSTRACT We present clustering redshift measurements for Dark Energy Survey (DES) lens sample galaxies used in weak gravitational lensing and galaxy clustering studies. To perform these measurements, we cross-correlate with spectroscopic galaxies from the Baryon Acoustic Oscillation Survey (BOSS) and its extension, eBOSS. We validate our methodology in simulations, including a new technique to calibrate systematic errors that result from the galaxy clustering bias, and we find that our method is generally unbiased in calibrating the mean redshift. We apply our method to the data, and estimate the redshift distribution for 11 different photometrically selected bins. We find general agreement between clustering redshift and photometric redshift estimates, with differences on the inferred mean redshift found to be below |Δz| = 0.01 in most of the bins. We also test a method to calibrate a width parameter for redshift distributions, which we found necessary to use for some of our samples. Our typical uncertainties on the mean redshift ranged from 0.003 to 0.008, while our uncertainties on the width ranged from 4 to 9 per cent. We discuss how these results calibrate the photometric redshift distributions used in companion papers for DES Year 3 results.

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)0.005
metaresearch head score (Gemma)0.008
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 score0.029
Threshold uncertainty score0.057

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0050.008
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0020.002
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0010.001
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 head0.013
GPT teacher head0.206
Teacher spread0.193 · 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

Citations53
Published2022
Admission routes2
Has abstractyes

Explore more

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