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Record W3187241039 · doi:10.1093/mnras/stab2325

Uncovering fossils of the distant Milky Way with UNIONS: NGC 5466 and its stellar stream

2021· article· en· W3187241039 on OpenAlexafffundabout
Jaclyn Jensen, Guillaume F. Thomas, Alan W. McConnachie, Else Starkenburg, Khyati Malhan, Julio F. Navarro, Nicolas F. Martin, Benoît Famaey, Rodrigo Ibata, S. C. Chapman, Jean‐Charles Cuillandre, Stephen Gwyn

Bibliographic record

VenueMonthly Notices of the Royal Astronomical Society · 2021
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsDalhousie UniversityHerzberg Institute of AstrophysicsUniversity of Victoria
FundersEuropean Space AgencyLos Alamos National LaboratoryAgencia Estatal de InvestigaciónHorizon 2020 Framework ProgrammeH2020 European Research CouncilSmithsonian Astrophysical ObservatoryEötvös Loránd TudományegyetemCentre National de la Recherche ScientifiqueDurham UniversityNatural Sciences and Engineering Research Council of CanadaNemzeti Fejlesztési MinisztériumUniversity of MarylandMinisterio de Ciencia e InnovaciónUniversity of EdinburghAgence Nationale de la RechercheSpace Telescope Science InstituteCalifornia Earthquake AuthorityNational Science FoundationNational Aeronautics and Space AdministrationUniversity of Hawai'iNational Central UniversityGordon and Betty Moore FoundationNational Research Council CanadaAssociation for Women in Mathematics
KeywordsPhysicsAstrophysicsMilky WayGlobular clusterStarsAstronomyGalaxyLocal GroupStar clusterOpen cluster

Abstract

fetched live from OpenAlex

ABSTRACT We examine the spatial clustering of blue horizontal branch (BHB) stars from the u-band of the Canada–France Imaging Survey (CFIS, a component of the Ultraviolet Near-Infrared Optical Northern Survey, or UNIONS). All major groupings of stars are associated with previously known satellites, and among these is NGC 5466, a distant (16 kpc) globular cluster. NGC 5466 reportedly possesses a long stellar stream, although no individual members of the stream have previously been identified. Using both BHBs and more numerous red giant branch stars cross-matched to Gaia Data Release 2, we identify extended tidal tails from NGC 5466 that are both spatially and kinematically coherent. Interestingly, we find that this stream does not follow the same path as the previous detection at large distances from the cluster. We trace the stream across 31° of sky and show that it exhibits a very strong distance gradient in the range 10 < Rhelio < 30 kpc. We compare our observations to simple dynamical models of the stream and find that they are able to broadly reproduce the overall path and kinematics. The fact that NGC 5466 is so distant, traces a wide range of Galactic distances, has an identified progenitor, and appears to have recently had an interaction with the Galaxy’s disc makes it a unique test-case for dynamical modelling of the Milky Way.

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 score0.014
Threshold uncertainty score0.029

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 studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0010.000

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 head0.007
GPT teacher head0.192
Teacher spread0.185 · 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

Citations17
Published2021
Admission routes3
Has abstractyes

Explore more

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