MétaCan
Menu
Back to cohort
Record W4404940497 · doi:10.3847/2041-8213/ad927c

Three Quenched, Faint Dwarf Galaxies in the Direction of NGC 300: New Probes of Reionization and Internal Feedback

2024· article· en· W4404940497 on OpenAlexfundno aff
David J. Sand, Burçı̇n Mutlu-Pakdı̇l, Michael G. Jones, Ananthan Karunakaran, Jennifer E. Andrews, Paul Bennet, Denija Crnojević, Giuseppe Donatiello, A. Drlica-Wagner, Catherine E. Fielder, David Martínez‐Delgado, C. E. Martínez-Vázquez, Kristine Spekkens, Amandine Doliva-Dolinsky, Laura E. Hunter, Jeffrey L. Carlin, W. Cerny, T. N. Hai, Kristen B. W. McQuinn, Andrew B. Pace, Adam Smercina

Bibliographic record

VenueThe Astrophysical Journal Letters · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersNatural Sciences and Engineering Research Council of CanadaAspen Center for PhysicsAgencia Nacional de Investigación y DesarrolloNational Aeronautics and Space AdministrationMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesNational Science FoundationKorea Astronomy and Space Science InstituteSpace Telescope Science Institute
KeywordsReionizationDwarf galaxyPhysicsAstrophysicsGalaxyGlobular clusterAstronomyDwarf galaxy problemInteracting galaxyRedshift

Abstract

fetched live from OpenAlex

Abstract We report the discovery of three faint and ultrafaint dwarf galaxies—Sculptor A, Sculptor B, and Sculptor C—in the direction of NGC 300 ( D = 2.0 Mpc), a Large Magellanic Cloud–mass galaxy. Deep ground-based imaging with Gemini/GMOS resolves all three dwarf galaxies into stars, each displaying a red giant branch indicative of an old, metal-poor stellar population. No young stars or H i gas are apparent, and the lack of a GALEX UV detection suggests that all three systems are quenched. Sculptor C ( D = 2.04 − 0.13 + 0.10 Mpc; M V = −9.1 ± 0.1 mag or L V = (3.7 − 0.3 + 0.4 ) × 10 5 L ⊙ ) is consistent with being a satellite of NGC 300. Sculptor A ( D = 1.35 − 0.08 + 0.22 Mpc; M V = −6.9 ± 0.3 mag or L V = (5 − 1 + 1 ) × 10 4 L ⊙ ) is likely in the foreground of NGC 300 and at the extreme edge of the Local Group, analogous to the recently discovered ultrafaint Tucana B in terms of its physical properties and environment. Sculptor B ( D = 2.48 − 0.24 + 0.21 Mpc; M V = −8.1 ± 0.3 mag or L V = (1.5 − 0.4 + 0.5 ) × 10 5 L ⊙ ) is likely in the background, but future distance measurements are necessary to solidify this statement. It is also of interest due to its quiescent state and low stellar mass. Both Sculptor A and B are ≳2–4 r vir from NGC 300 itself. The discovery of three dwarf galaxies in isolated or low-density environments offers an opportunity to study the varying effects of ram-pressure stripping, reionization, and internal feedback in influencing the star formation history of the faintest stellar systems.

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 score0.005
Threshold uncertainty score0.009

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
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 head0.009
GPT teacher head0.217
Teacher spread0.208 · 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

Citations12
Published2024
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical Journal LettersSame topicStellar, planetary, and galactic studiesFrench-language works237,207