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Record W4399283172 · doi:10.1093/mnras/stae1316

DESI complete calibration of the colour–redshift relation (DC3R2): results from early DESI data

2024· article· en· W4399283172 on OpenAlexaff
J. McCullough, D. Gruen, A. Amon, A. Roodman, Daniel Masters, Anand Raichoor, David J. Schlegel, Rebecca Canning, F. J. Castander, Joseph DeRose, R. Miquel, J. Myles, Jeffrey A. Newman, Anže Slosar, Joshua S. Speagle, M. J. Wilson, J. Aguilar, S. P. Ahlen, S. Bailey, D. Brooks, T. Claybaugh, Shaun Cole, Kyle Dawson, P. Doel, J. E. Forero-Romero, Satya Gontcho A Gontcho, J. Guy, R. Kehoe, Martin Landriau, L. Le Guillou, M. E. Levi, Marc Manera, Paul Martini, Aaron Meisner, John Moustakas, Jundan Nie, Will J. Percival, Claire Poppett, Francisco Prada, Mehdi Rezaie, Graziano Rossi, E. Sánchez, Hee‐Jong Seo, G. Tarlé, B. A. Weaver, Zhiming Zhou, Hu Zou

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsCanadian Institute for Theoretical AstrophysicsUniversity of WaterlooUniversity of Toronto
FundersLawrence Berkeley National LaboratoryHigh Energy PhysicsDivision of Astronomical SciencesJet Propulsion LaboratoryOffice of ScienceCommissariat à l'Énergie Atomique et aux Énergies AlternativesDeutscher Akademischer AustauschdienstUniversità degli Studi di PadovaNederlandse Organisatie voor Wetenschappelijk OnderzoekDeutsche ForschungsgemeinschaftChinese Academy of SciencesNational Energy Research Scientific Computing CenterNational Aeronautics and Space AdministrationU.S. Department of EnergyCalifornia Institute of TechnologyBayerisch-Kalifornischen HochschulzentrumGordon and Betty Moore FoundationNational Science Foundation
KeywordsPhysicsRedshiftAstrophysicsPhotometry (optics)GalaxyWeak gravitational lensingAstronomyPhotometric redshiftDark energyRedshift surveyCosmologyStars

Abstract

fetched live from OpenAlex

ABSTRACT We present initial results from the Dark Energy Spectroscopic Instrument (DESI) complete calibration of the colour–redshift relation (DC3R2) secondary target survey. Our analysis uses 230 k galaxies that overlap with KiDS-VIKING ugriZYJHKs photometry to calibrate the colour–redshift relation and to inform photometric redshift (photo-z) inference methods of future weak lensing surveys. Together with emission line galaxies (ELGs), luminous red galaxies (LRGs), and the Bright Galaxy Survey (BGS) that provide samples of complementary colour, the DC3R2 targets help DESI to span 56 per cent of the colour space visible to Euclid and LSST with high confidence spectroscopic redshifts. The effects of spectroscopic completeness and quality are explored, as well as systematic uncertainties introduced with the use of common Self-Organizing Maps trained on different photometry than the analysis sample. We further examine the dependence of redshift on magnitude at fixed colour, important for the use of bright galaxy spectra to calibrate redshifts in a fainter photometric galaxy sample. We find that noise in the KiDS-VIKING photometry introduces a dominant, apparent magnitude dependence of redshift at fixed colour, which indicates a need for carefully chosen deep drilling fields, and survey simulation to model this effect for future weak lensing surveys.

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)0.004
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 score0.022
Threshold uncertainty score0.043

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0040.004
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.003
Science and technology studies0.0010.000
Scholarly communication0.0010.001
Open science0.0010.002
Research integrity0.0010.001
Insufficient payload (model declined to judge)0.0030.003

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 head0.019
GPT teacher head0.214
Teacher spread0.195 · 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

Citations10
Published2024
Admission routes1
Has abstractyes

Explore more

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