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<i>Gaia</i> Early Data Release 3

2020· article· en· 330 citations· W3109423373 on OpenAlex· 10.1051/0004-6361/202039498

Why is this work in the frame?

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

Canadian funderA Canadian agency funded it. The work may carry no Canadian affiliation at all.

No Canadian affiliation. An affiliation-only frame, the usual design, would never have seen this work. It is one of the works that make the case for inverting the frame.

Full frame distilled prediction

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.

Candidate categories
Meta-epidemiology (narrow)
Consensus categories
none
Domain
Candidate signal: noneConsensus signal: none
Study design
Candidate signal: ObservationalConsensus signal: none
Genre
Candidate signal: EmpiricalConsensus signal: Empirical
Teacher disagreement score
0.634
Threshold uncertainty score
1.000
Validation status
machine_predicted_unvalidated · codex-gemma-dda1882f352a

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 studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

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.

Opus teacher head0.019
GPT teacher head0.212
Teacher spread
0.192 · how far apart the two teachers sit on this one work
Validation status
score_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Abstract

Aims. We produce a clean and well-characterised catalogue of objects within 100 pc of the Sun from the Gaia Early Data Release 3. We characterise the catalogue through comparisons to the full data release, external catalogues, and simulations. We carry out a first analysis of the science that is possible with this sample to demonstrate its potential and best practices for its use. Methods. Theselection of objects within 100 pc from the full catalogue used selected training sets, machine-learning procedures, astrometric quantities, and solution quality indicators to determine a probability that the astrometric solution is reliable. The training set construction exploited the astrometric data, quality flags, and external photometry. For all candidates we calculated distance posterior probability densities using Bayesian procedures and mock catalogues to define priors. Any object with reliable astrometry and a non-zero probability of being within 100 pc is included in the catalogue. Results. We have produced a catalogue of 331 312 objects that we estimate contains at least 92% of stars of stellar type M9 within 100 pc of the Sun. We estimate that 9% of the stars in this catalogue probably lie outside 100 pc, but when the distance probability function is used, a correct treatment of this contamination is possible. We produced luminosity functions with a high signal-to-noise ratio for the main-sequence stars, giants, and white dwarfs. We examined in detail the Hyades cluster, the white dwarf population, and wide-binary systems and produced candidate lists for all three samples. We detected local manifestations of several streams, superclusters, and halo objects, in which we identified 12 members of Gaia Enceladus. We present the first direct parallaxes of five objects in multiple systems within 10 pc of the Sun. Conclusions. We provide the community with a large, well-characterised catalogue of objects in the solar neighbourhood. This is a primary benchmark for measuring and understanding fundamental parameters and descriptive functions in astronomy.

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.

The record

Venue
Astronomy and Astrophysics
Topic
Stellar, planetary, and galactic studies
Field
Physics and Astronomy
Canadian institutions
not available
Funders
Los Alamos National LaboratoryAustralian Research CouncilUniversity of Colorado BoulderOffice of ScienceMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikLeibniz-Institut für Astrophysik PotsdamEötvös Loránd TudományegyetemNatural Sciences and Engineering Research Council of CanadaNational Central UniversityChina Scholarship CouncilHrvatska Zaklada za ZnanostJavna Agencija za Raziskovalno Dejavnost RSFonds Wetenschappelijk OnderzoekBelgian Federal Science Policy OfficeFonds De La Recherche Scientifique - FNRSAustrian Science FundUniversidad Nacional Autónoma de MéxicoIstituto Nazionale di AstrofisicaCoordenação de Aperfeiçoamento de Pessoal de Nível SuperiorEuropean CommissionFundação de Amparo à Pesquisa do Estado de São PauloYale UniversityU.S. Department of EnergyUniversity of QueenslandInstituto de Astrofísica de CanariasCarnegie Institution for ScienceUniversity of MelbourneLawrence Berkeley National LaboratoryJet Propulsion LaboratoryMonash UniversityÉcole Polytechnique Fédérale de LausanneDeutsche ForschungsgemeinschaftQueen's UniversityUniversity of EdinburghUniversity of OxfordAustralian National Data ServiceDurham UniversityScience and Technology Facilities CouncilMinistério da Ciência, Tecnologia e InovaçãoSchweizerischer Nationalfonds zur Förderung der Wissenschaftlichen ForschungYork UniversityLeibniz-GemeinschaftScience Mission DirectorateNational Computational InfrastructureAgence Nationale de la RechercheGordon and Betty Moore FoundationUniversity of SydneyAustralian GovernmentAustralian National UniversityUniversity of PortsmouthUniversity of UtahNew Mexico State UniversityNational Cancer InstituteAustralian Astronomical Optics-MacquarieAstronomy Australia LimitedUniversity of Notre DameSmithsonian Astrophysical ObservatoryEuropean Space AgencyUniversity of California, Los AngelesCurtin University of TechnologyUniversity of WashingtonAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Mellon UniversityPlanetary Science DivisionCarnegie Institution of WashingtonNational Natural Science Foundation of ChinaOhio State UniversityVanderbilt UniversitySmithsonian InstitutionNational Aeronautics and Space AdministrationSwinburne University of TechnologyQueen's University BelfastSpace Telescope Science InstituteMacquarie UniversityW. M. Keck FoundationCalifornia Institute of TechnologyNational Science Foundation
Keywords
PhysicsAstrophysicsAstronomy
Has abstract in OpenAlex
yes