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The population of hot subdwarf stars studied with

2022· article· en· W6940685925 on OpenAlexfundno aff

Bibliographic record

VenueSpringer Link (Chiba Institute of Technology) · 2022
Typearticle
Languageen
FieldAgricultural and Biological Sciences
TopicMycorrhizal Fungi and Plant Interactions
Canadian institutionsnot available
FundersLos Alamos National LaboratoryU.S. Naval ObservatoryINAF-Osservatorio Astronomico di PadovaCollege of Engineering, Michigan State UniversityUniversity of Colorado BoulderOffice of ScienceFermilabMax-Planck-Institut für AstronomieNational Development and Reform CommissionEötvös Loránd TudományegyetemUniversidad Nacional Autónoma de MéxicoBrookhaven National LaboratoryMax-Planck-GesellschaftScience and Technology Facilities CouncilYork UniversityMinistério da Ciência, Tecnologia e InovaçãoNederlandse Organisatie voor Wetenschappelijk OnderzoekChinese Academy of SciencesLawrence Berkeley National LaboratoryAstrophysics DivisionJet Propulsion LaboratoryMonash UniversityUniversity of OxfordAustralian National Data ServiceDurham UniversityUniversity of California, Los AngelesUniversity of WashingtonCurtin University of TechnologyInstituto de Astrofísica de CanariasCarnegie Institution for ScienceGordon and Betty Moore FoundationAustralian GovernmentNational Central UniversityEuropean Southern ObservatorySpace Telescope Science InstituteAustralian National UniversityNational Cancer InstituteAustralian Astronomical Optics-MacquarieAstronomy Australia LimitedUniversity of UtahNew Mexico State UniversityUniversity of PortsmouthUniversität BaselNational Science FoundationCase Western Reserve UniversityCarnegie Mellon UniversityUniversity of PittsburghUniversity of Notre DameUniversity of ArizonaMax-Planck-Institut für AstrophysikUniversità degli Studi di PadovaSmithsonian Astrophysical ObservatoryEuropean Space AgencyPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityPlanetary Science DivisionCarnegie Institution of WashingtonQueen's UniversityHarvard UniversityOhio State UniversityLeibniz-GemeinschaftScience Mission DirectorateNational Computational InfrastructureVanderbilt UniversityDrexel UniversityYale UniversityU.S. Department of EnergySmithsonian InstitutionNational Aeronautics and Space AdministrationSwinburne University of TechnologyQueen's University BelfastNational Astronomical Observatories, Chinese Academy of SciencesCalifornia Institute of Technology
KeywordsSubdwarfStarsAstrometryGalactic planePhotometry (optics)PopulationStellar populationMetallicity

Abstract

fetched live from OpenAlex

In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the Gaia mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data release 3 (DR3) catalogue of the known hot subdwarf stars contains 6616 unique sources and provides multi-band photometry, and astrometry from Gaia EDR3 as well as classifications based on spectroscopy and colours. This is an increase of 742 objects over the DR2 catalogue. This new catalogue provides atmospheric parameters for 3087 stars and radial velocities for 2791 stars from the literature. In addition, we have updated the Gaia Data Release 2 (DR2) catalogue of hot subluminous stars using the improved accuracy of the Gaia EDR3 data set together with updated quality and selection criteria to produce the Gaia EDR3 catalogue of 61 585 hot subluminous stars, representing an increase of 21 785 objects. The improvements in Gaia EDR3 astrometry and photometry compared to Gaia DR2 have enabled us to define more sophisticated selection functions. In particular, we improved hot subluminous star detection in the crowded regions of the Galactic plane as well as in the direction of the Magellanic Clouds by including sources with close apparent neighbours but with flux levels that dominate the neighbourhood.

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)0.000
metaresearch head score (Gemma)0.001
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 score0.002
Threshold uncertainty score0.005

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.001
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.001
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 head0.012
GPT teacher head0.210
Teacher spread0.198 · 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".

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Citations0
Published2022
Admission routes1
Has abstractyes

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