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Record W2017305484 · doi:10.1088/0004-6256/135/6/1998

THE NATURE AND ORIGIN OF SUBSTRUCTURE IN THE OUTSKIRTS OF M31. I. SURVEYING THE STELLAR CONTENT WITH THE<i>HUBBLE SPACE TELESCOPE</i>ADVANCED CAMERA FOR SURVEYS

2008· article· en· W2017305484 on OpenAlexaff
Jenna Richardson, A. M. N. Ferguson, R. A. Johnson, M. J. Irwin, N. R. Tanvir, Daniel Faria, Rodrigo Ibata, Kathryn V. Johnston, Geraint F. Lewis, Alan W. McConnachie, S. C. Chapman

Bibliographic record

VenueThe Astronomical Journal · 2008
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of Victoria
FundersScience and Technology Facilities Council
KeywordsPhysicsAstrophysicsRed clumpAdvanced Camera for SurveysHorizontal branchAstronomyRed-giant branchHaloLuminosityStarsGalaxyStar formationGlobular clusterMilky Way

Abstract

fetched live from OpenAlex

We present the largest and most detailed survey to date of the stellar populations in the outskirts of M31 based on the homogeneous analysis of 14 deep Hubble Space Telescope Advanced Camera for Surveys ( HST /ACS) pointings spanning the range 11.5 kpc ≲ R proj ≲ 45 kpc. Many of these pointings sample coherent substructure discovered in the course of the Isaac Newton Telescope Wide Field Camera (INT/WFC) imaging survey of M31 while others sample more diffuse structure in the extended disk. We conduct a quantitative comparison of the resolved stellar populations in these fields and identify several striking trends. The color–magnitude diagrams (CMDs), which reach ≳3 mag below the red clump with high completeness, can be classified into two main categories based on their morphologies. "Stream-like" fields, so named for their similarity to the CMD of the giant stellar stream, are characterized by a red clump that slants blueward at fainter magnitudes and an extended horizontal branch. They show no evidence for young populations. On the other hand, "disk-like" fields exhibit rounder red clumps with significant luminosity width, lack an obvious horizontal branch, and show evidence for recent star formation (∼0.25–2 Gyr ago). We compare the spatial and line-of-sight distribution of stream-like fields with a recent simulation of the giant stream progenitor orbit and find an excellent agreement. These fields are found across much of the inner halo of M31, and attest to the high degree of pollution caused by this event. Disk-like material resides in the extended disk structure of M31 and is detected here up to R proj ∼ 44 kpc; the uniform populations in these fields, including the ubiquitous presence of young populations, and the strong rotation reported elsewhere are most consistent with a scenario in which this structure has formed through heating and disruption of the existing thin disk, perhaps due to the impact of the giant stream progenitor. Our comparative analysis sheds new light on the likely composition of two of the ultra-deep pointings formerly presented as pure outer disk and pure halo in the literature.

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)0.000
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 score0.007
Threshold uncertainty score0.013

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.000
Scholarly communication0.0000.000
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 head0.019
GPT teacher head0.234
Teacher spread0.215 · 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

Citations95
Published2008
Admission routes1
Has abstractyes

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