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Record W2092239968 · doi:10.1086/512726

A Canis Major Overdensity Imaging Survey. I. Stellar Content and Star-Count Maps: A Distinctly Elongated Body of Main-Sequence Stars

2007· article· en· W2092239968 on OpenAlexaff
D. Butler, David Martínez‐Delgado, Hans‐Walter Rix, Jorge Peñarrubia, J. T. A. de Jong

Bibliographic record

VenueThe Astronomical Journal · 2007
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of Victoria
Fundersnot available
KeywordsPhysicsAstrophysicsStarsStellar populationMilky WayPopulationStar countGalaxyGalactic planeLine (geometry)MetallicityAstronomyStar formationGeometryT Tauri star

Abstract

fetched live from OpenAlex

We present the first results from a large-area (∼80° × 20°), sparsely sampled, two-filter ( B and R ) imaging survey toward the Canis Major stellar overdensity, which is claimed to be a disrupting Milky Way satellite galaxy. Using stellar color-magnitude diagrams reaching to B ∼ 22 mag, we provide a first delineation of its surface density distribution using main-sequence stars. It is located below the Galactic midplane, and can be discerned to at least b = -15°. Its projected shape is highly elongated, nearly parallel to the Galactic plane, with an axis ratio of at least 5 : 1, substantially more so than what Martin and coworkers originally found. We also provide a first map of a prominent overdensity of blue, presumably younger main-sequence stars, which extends in latitude to b ∼ -10°. We estimate an upper limit on the line-of-sight depth σ los of the old population based on the main-sequence width, obtaining σ los < 1.8 ± 0.3 kpc at an adopted D ⊙ = 7.5 ± 1 kpc. For the young stellar population, we find σ los < 1.5 kpc. The overall picture presented is one of a young stellar population that is less extended, both in terms of its line-of-sight depth and angular size, than the older population. While the data provide no firm arguments against an out-of-plane spiral arm interpretation, the data provide clear implications for others: (1) We infer from the strong elongation of the overdensity in longitude, and simulations in the literature, that the CMa overdensity is unlikely to be a gravitationally bound system at the present epoch, but may well be just a recently disrupted satellite remnant. The possible "flattening" of the young main-sequence population may, however, be a complexity for the satellite origin. (2) Based on modeling, the line-of-sight depth of the main-sequence overdensity in old stars is clearly inconsistent with published locally axisymmetric descriptions of the warped Galactic disk, such as those considered by Momany and coworkers. Without detailed modeling, the data set itself does not allow a distinction between interpretations as substructure in the warped outer Galactic disk or a disrupted satellite.

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 score0.129
Threshold uncertainty score0.256

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0060.004
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0010.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0030.002

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 head0.022
GPT teacher head0.239
Teacher spread0.216 · 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

Citations25
Published2007
Admission routes1
Has abstractyes

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