MétaCan
Menu
Back to cohort
Record W4377121463 · doi:10.3847/1538-3881/ace35d

Performance of the Quasar Spectral Templates for the Dark Energy Spectroscopic Instrument

2023· article· en· W4377121463 on OpenAlexafffund
A. Brodzeller, Kyle Dawson, S. Bailey, Jiaxi Yu, Ashley J. Ross, A. Bault, S. Filbert, J. Aguilar, S. P. Ahlen, D. M. Alexander, E. Armengaud, A. Berti, D. Brooks, E. Chaussidon, Axel de la Macorra, P. Doel, K. Fanning, Victoria A. Fawcett, Andreu Font-Ribera, Satya Gontcho A Gontcho, J. Guy, K. Honscheid, S. Juneau, R. Kehoe, Theodore Kisner, Ting-Wen Lan, Martin Landriau, M. E. Levi, C. Magneville, Aaron Meisner, R. Miquel, John Moustakas, N. Palanque‐Delabrouille, Will J. Percival, Francisco Prada, C. Ravoux, Graziano Rossi, Christoph Saulder, M. Siudek, G. Tarlé, B. A. Weaver, Samantha Youles, Zheng Zheng, Rongpu Zhou, Zhimin Zhou

Bibliographic record

VenueThe Astronomical Journal · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsPerimeter InstituteUniversity of Waterloo
FundersHigh Energy PhysicsLawrence Berkeley National LaboratoryDivision of Astronomical SciencesScience and Technology Facilities CouncilUniversity of Colorado BoulderInstituto de Astrofísica de CanariasOffice of ScienceMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikCommissariat à l'Énergie Atomique et aux Énergies AlternativesMinistério da Ciência, Tecnologia e InovaçãoVanderbilt UniversityConsejo Nacional de Ciencia y TecnologíaUniversity of OxfordYork UniversityLeibniz-GemeinschaftUniversity of Notre DameCarnegie Mellon UniversityUniversidad Nacional Autónoma de MéxicoAlfred P. Sloan FoundationUniversity of WashingtonJohns Hopkins UniversityMinisterio de Ciencia e InnovaciónCarnegie Institution of WashingtonUniversity of UtahOhio State UniversitySmithsonian InstitutionU.S. Department of EnergyGordon and Betty Moore FoundationNational Science FoundationNew Mexico State UniversityUniversity of PortsmouthYale University
KeywordsPhysicsQuasarAstrophysicsAstronomyDark energyTemplateEnergy (signal processing)CosmologyGalaxyNanotechnology

Abstract

fetched live from OpenAlex

Abstract Millions of quasar spectra will be collected by the Dark Energy Spectroscopic Instrument (DESI), leading to a fourfold increase in the number of known quasars. High-accuracy quasar classification is essential to tighten constraints on cosmological parameters measured at the highest redshifts DESI observes ( z > 2.0). We present spectral templates for identification and redshift estimation of quasars in the DESI Year 1 data release. The quasar templates are comprised of two quasar eigenspectra sets, trained on spectra from the Sloan Digital Sky Survey. The sets are specialized to reconstruct quasar spectral variation observed over separate yet overlapping redshift ranges and, together, are capable of identifying DESI quasars from 0.05 < z < 7.0. The new quasar templates show significant improvement over the previous DESI quasar templates regarding catastrophic failure rates, redshift precision and accuracy, quasar completeness, and the contamination fraction in the final quasar sample.

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)0.006
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.008
Threshold uncertainty score0.015

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.006
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0000.001
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0010.001
Open science0.0010.001
Research integrity0.0010.000
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 head0.011
GPT teacher head0.214
Teacher spread0.204 · 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 designBench or experimental
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

Citations54
Published2023
Admission routes2
Has abstractyes

Explore more

Same venueThe Astronomical JournalSame topicGalaxies: Formation, Evolution, PhenomenaFrench-language works237,207