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Record W2048747575 · doi:10.1088/2041-8205/755/2/l25

THE APACHE POINT OBSERVATORY GALACTIC EVOLUTION EXPERIMENT: FIRST DETECTION OF HIGH-VELOCITY MILKY WAY BAR STARS

2012· article· en· W2048747575 on OpenAlexfundno aff
David L. Nidever, Gail Zasowski, Steven R. Majewski, Jonathan C. Bird, A. C. Robin, Inma Martínez-Valpuesta, Rachael L. Beaton, Ralph Schönrich, M. Schultheis, John C. Wilson, Michael F. Skrutskie, R. W. O’Connell, Matthew Shetrone, Ricardo P. Schiavon, Jennifer A. Johnson, Benjamin J. Weiner, Ortwin Gerhard, Donald P. Schneider, Carlos Allende Prieto, K. Sellgren, Dmitry Bizyaev, H. Brewington, J. Brinkmann, Daniel J. Eisenstein, Peter M. Frinchaboy, A. E. García Pérez, Jon A. Holtzman, Fred Hearty, Elena Malanushenko, Viktor Malanushenko, Demitri Muna, Daniel Oravetz, Kaike Pan, Audrey Simmons, Stephanie A. Snedden, Benjamin Alan Weaver

Bibliographic record

VenueThe Astrophysical Journal Letters · 2012
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratoryUniversity of PortsmouthUniversity of California, Los AngelesAgence Nationale de la RechercheYork UniversityCarnegie Mellon UniversityUniversity of ArizonaOffice of SciencePrinceton UniversityAlfred P. Sloan FoundationUniversity of WashingtonJohns Hopkins UniversityCollege of Engineering, Michigan State UniversityHarvard UniversityOhio State UniversityNew Mexico State UniversityYale UniversityVanderbilt UniversityNational Science FoundationBrookhaven National LaboratoryU.S. Department of EnergyCalifornia Institute of TechnologyNational Aeronautics and Space AdministrationJet Propulsion Laboratory
KeywordsPhysicsMilky WayAstrophysicsStarsBulgeAstronomyGalactic CenterRed clumpGalaxySkyObservatoryGiant starSagittarius

Abstract

fetched live from OpenAlex

Commissioning observations with the Apache Point Observatory Galactic Evolution Experiment (APOGEE), part of the Sloan Digital Sky Survey III, have produced radial velocities (RVs) for ∼4700 K/M-giant stars in the Milky Way (MW) bulge. These high-resolution ( R ∼ 22, 500), high-S/N (>100 per resolution element), near-infrared (NIR; 1.51–1.70 μm) spectra provide accurate RVs ( V ∼ 0.2 km s −1 ) for the sample of stars in 18 Galactic bulge fields spanning −1° < l < 20°, | b | < 20°, and δ > −32°. This represents the largest NIR high-resolution spectroscopic sample of giant stars ever assembled in this region of the Galaxy. A cold (σ V ∼ 30 km s −1 ), high-velocity peak ( V GSR ≈ +200 km s −1 ) is found to comprise a significant fraction (∼10%) of stars in many of these fields. These high RVs have not been detected in previous MW surveys and are not expected for a simple, circularly rotating disk. Preliminary distance estimates rule out an origin from the background Sagittarius tidal stream or a new stream in the MW disk. Comparison to various Galactic models suggests that these high RVs are best explained by stars in orbits of the Galactic bar potential, although some observational features remain unexplained.

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 score0.022
Threshold uncertainty score0.043

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
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)0.0010.000

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 head0.012
GPT teacher head0.205
Teacher spread0.193 · 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

Citations67
Published2012
Admission routes1
Has abstractyes

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