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Record W4297434854 · doi:10.3847/1538-4357/acdd78

Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey

2023· article· en· W4297434854 on OpenAlexaff
W. Cerny, C. E. Martínez-Vázquez, A. Drlica-Wagner, Andrew B. Pace, Burçı̇n Mutlu-Pakdı̇l, Ting S. Li, A. H. Riley, Denija Crnojević, Clécio R. Bom, J. A. Carballo-Bello, Jeffrey L. Carlin, Anirudh Chiti, Yumi Choi, Michelle Collins, Elise Darragh-Ford, P. S. Ferguson, Marla Geha, David Martínez‐Delgado, Pol Massana, S. Mau, G. E. Medina, Ricardo R. Muñoz, Ethan O. Nadler, Noelia E. D. Noël, Knut Olsen, A. Pieres, J. D. Sakowska, Joshua D. Simon, Guy S. Stringfellow, Erik Tollerud, A. K. Vivas, A. R. Walker, Risa H. Wechsler

Bibliographic record

VenueThe Astrophysical Journal · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicStellar, planetary, and galactic studies
Canadian institutionsUniversity of Toronto
FundersSLAC National Accelerator LaboratoryArgonne National LaboratoryIntegrated Electronics Engineering Center, Binghamton UniversityScience and Technology Facilities CouncilUniversity of Illinois at Urbana-ChampaignAgencia Nacional de Investigación y DesarrolloFundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de JaneiroMinistério da Ciência, Tecnologia, Inovações e ComunicaçõesKorea Astronomy and Space Science InstituteCentro de Investigaciones Energéticas, Medioambientales y TecnológicasConselho Nacional de Desenvolvimento Científico e TecnológicoChinese Academy of SciencesHigh Energy PhysicsDeutsche ForschungsgemeinschaftOffice of ScienceUniversity of EdinburghCenter for Cosmology and Astroparticle Physics, Ohio State UniversityUniversity of SussexUniversity of NottinghamUniversity of CambridgeKavli Institute for Cosmological Physics, University of ChicagoNational Energy Research Scientific Computing CenterNational Aeronautics and Space AdministrationUniversity College LondonInstitut de Física d'Altes EnergiesEidgenössische Technische Hochschule ZürichNational Centre for Supercomputing ApplicationsUniversity of MichiganJet Propulsion LaboratoryUniversity of California, Santa CruzOhio State UniversityLawrence Berkeley National LaboratoryDivision of Astronomical SciencesFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaUniversity of ChicagoUniversity of CaliforniaCalifornia Institute of TechnologyU.S. Department of EnergyW. M. Keck FoundationEuropean Space AgencyFermilabLaboratory Directed Research and DevelopmentNational Science FoundationUniversity of PortsmouthYale University
KeywordsPhysicsMilky WayLocal GroupAstrophysicsAstronomyDwarf galaxyGalaxyProper motionStars

Abstract

fetched live from OpenAlex

Abstract We report the discovery of six ultra-faint Milky Way satellites identified through matched-filter searches conducted using Dark Energy Camera (DECam) data processed as part of the second data release of the DECam Local Volume Exploration (DELVE) survey. Leveraging deep Gemini/GMOS-N imaging (for four candidates) as well as follow-up DECam imaging (for two candidates), we characterize the morphologies and stellar populations of these systems. We find that these candidates all share faint absolute magnitudes (M V ≥ −3.2 mag) and old, metal-poor stellar populations (τ > 10 Gyr, [Fe/H] < −1.4 dex). Three of these systems are more extended (r 1/2 > 15 pc), while the other three are compact (r 1/2 < 10 pc). From these properties, we infer that the former three systems (Boötes V, Leo Minor I, and Virgo II) are consistent with ultra-faint dwarf galaxy classifications, whereas the latter three (DELVE 3, DELVE 4, and DELVE 5) are likely ultra-faint star clusters. Using data from the Gaia satellite, we confidently measure the proper motion of Boötes V, Leo Minor I, and DELVE 4, and tentatively detect a proper-motion signal from DELVE 3 and DELVE 5; no signal is detected for Virgo II. We use these measurements to explore possible associations between the newly discovered systems and the Sagittarius dwarf spheroidal, the Magellanic Clouds, and the Vast Polar Structure, finding several plausible associations. Our results offer a preview of the numerous ultra-faint stellar systems that will soon be discovered by the Vera C. Rubin Observatory and highlight the challenges of classifying 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)0.001
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 score0.003
Threshold uncertainty score0.006

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
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 head0.029
GPT teacher head0.258
Teacher spread0.230 · 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

Citations59
Published2023
Admission routes1
Has abstractyes

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