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Record W2894725121 · doi:10.1093/mnras/sty2755

The age of the Galactic stellar halo from<i>Gaia</i>white dwarfs

2018· article· en· W2894725121 on OpenAlexafffund
Mukremin Kilic, P. Bergeron, Kyra Dame, N. C. Hambly, N. Rowell, Courtney L. Crawford

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversité de Montréal
FundersLawrence Berkeley National LaboratoryBrookhaven National LaboratoryPlanetary Science DivisionScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryEötvös Loránd TudományegyetemNational Central UniversityQueen's University BelfastOffice of ScienceMax-Planck-Institut für AstronomieUniversity of EdinburghNatural Sciences and Engineering Research Council of CanadaDurham UniversityYork UniversitySpace Telescope Science InstituteUniversity of Hawai'iNational Science FoundationDunlap Institute for Astronomy and Astrophysics, University of TorontoCarnegie Mellon UniversityUniversity of ArizonaCollege of Engineering, Michigan State UniversityUniversity of WashingtonEuropean Space AgencyPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityQueen's UniversityHarvard UniversityOhio State UniversityNational Aeronautics and Space AdministrationLockheed MartinSmithsonian InstitutionU.S. Department of EnergyNew Mexico State UniversityUniversity of PortsmouthVanderbilt UniversityScience Mission DirectorateYale University
KeywordsPhysicsWhite dwarfAstrophysicsAstronomyGalactic haloHaloMassive compact halo objectMilky WayBrown dwarfGlobular clusterPhotometry (optics)StarsGalaxy

Abstract

fetched live from OpenAlex

We use 156 044 white dwarf candidates with ≥5σ significant parallax measurements from the Gaia mission to measure the velocity dispersion of the Galactic disc; (σ U , σ V , σ W ) = (30.8,23.9, 20.0) km s -1 .We identify 142 objects that are inconsistent with disc membership at the >5σ level.This is the largest sample of field halo white dwarfs identified to date.We perform a detailed model atmosphere analysis using optical and near-infrared photometry and parallaxes to constrain the mass and cooling age of each white dwarf.The white dwarf cooling ages of our targets range from 7 Myr for J1657+2056 to 10.3 Gyr for J1049-7400.The latter provides a firm lower limit of 10.3 Gyr for the age of the inner halo based on the well-understood physics of white dwarfs.Including the pre-white dwarf evolutionary lifetimes, and limiting our sample to the recently formed white dwarfs with cooling ages of <500 Myr, we estimate an age of 10.9 ± 0.4 Gyr (internal errors only) for the Galactic inner halo.The coolest white dwarfs in our sample also give similar results.For example, J1049-7400 has a total age of 10.9-11.1 Gyr.Our age measurements are consistent with other measurements of the age of the inner halo, including the white dwarf based measurements of the globular clusters M4, NGC 6397, and 47 Tuc.

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)0.001
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 score0.008
Threshold uncertainty score0.016

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0010.000
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.001

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 head0.008
GPT teacher head0.200
Teacher spread0.192 · 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

Citations54
Published2018
Admission routes2
Has abstractyes

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