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Record W4386217506 · doi:10.3847/1538-4365/acdd79

Magellan/M2FS and MMT/Hectochelle Spectroscopy of Dwarf Galaxies and Faint Star Clusters within the Galactic Halo*

2023· article· en· W4386217506 on OpenAlexfundno aff
Matthew G. Walker, Nelson Caldwell, Mario Mateo, Edward W. Olszewski, Andrew B. Pace, John I. Bailey, S. E. Koposov, Ian U. Roederer

Bibliographic record

VenueThe Astrophysical Journal Supplement Series · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryLos Alamos National LaboratoryLawrence Berkeley National LaboratoryArgonne National LaboratoryCentro de Investigaciones Energéticas, Medioambientales y TecnológicasLeibniz-GemeinschaftScience Mission DirectorateUniversity of Illinois at Urbana-ChampaignMax-Planck-Institut für AstrophysikUniversity of SussexSpace Telescope Science InstituteInstitut de Física d'Altes EnergiesEötvös Loránd TudományegyetemYale UniversityU.S. Department of EnergyFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroConselho Nacional de Desenvolvimento Científico e TecnológicoScience and Technology Facilities CouncilYork UniversityMinistério da Ciência, Tecnologia e InovaçãoIntegrated Electronics Engineering Center, Binghamton UniversityUniversity of EdinburghQueen's UniversityDeutsche ForschungsgemeinschaftUniversity of Colorado BoulderOffice of ScienceFermilabMax-Planck-Institut für AstronomieUniversity of NottinghamUniversity of OxfordInstituto de Astrofísica de CanariasUniversity of CambridgeDurham UniversityUniversidad Nacional Autónoma de MéxicoNational Central UniversityUniversity of Notre DameJoint Institute for Nuclear Astrophysics - Center for the Evolution of the ElementsNational Science FoundationUniversity of MichiganCarnegie Mellon UniversityUniversity of WashingtonSmithsonian Astrophysical ObservatoryEuropean Space AgencyAlfred P. Sloan FoundationJohns Hopkins UniversityPlanetary Science DivisionCarnegie Institution of WashingtonUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahVanderbilt UniversityUniversity of ChicagoOhio State UniversitySmithsonian InstitutionFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaUniversity College LondonNational Aeronautics and Space AdministrationQueen's University BelfastGordon and Betty Moore Foundation
KeywordsPhysicsAstrophysicsSurface gravityMilky WayAstronomyGalaxyStarsDwarf galaxyHaloDwarf spheroidal galaxySurface brightnessRadial velocity

Abstract

fetched live from OpenAlex

Abstract We present spectroscopic data for 16,369 stellar targets within and/or toward 38 dwarf spheroidal galaxies and faint star clusters within the Milky Way halo environment. All spectra come from observations with the multiobject, fiber-fed echelle spectrographs M2FS at the Magellan/Clay telescope or Hectochelle at the MMT, reaching a typical limiting magnitude G ≲ 21. Data products include processed spectra from all observations and catalogs listing estimates—derived from template model fitting—of line-of-sight velocity (median uncertainty 1.4 km s−1) effective temperature (255 K), (base-10 logarithm of) surface gravity (0.59 dex in cgs units), [Fe/H] (0.4 dex) and [Mg/Fe] (0.27 dex) abundance ratios. The sample contains multiepoch measurements for 3720 sources, with up to 15 epochs per source, enabling studies of intrinsic spectroscopic variability. The sample contains 6087 likely red giant stars (based on surface gravity), and 4492 likely members (based on line-of-sight velocity and Gaia-measured proper motion) of the target systems. The number of member stars per individual target system ranges from a few, for the faintest systems, to ∼850 for the most luminous. For most systems, our new samples extend over wider fields than have previously been observed; of the likely members in our samples, 820 lie beyond 2 times the projected half-light radius of their host system, and 42 lie beyond 5 R half.

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 score0.009
Threshold uncertainty score0.018

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0030.002
Science and technology studies0.0000.000
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 head0.010
GPT teacher head0.232
Teacher spread0.222 · 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

Citations15
Published2023
Admission routes1
Has abstractyes

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