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Record W4390628939 · doi:10.1051/0004-6361/202348494

The occurrence rate of galaxies with polar structures may be significantly underestimated

2024· article· en· W4390628939 on OpenAlexfundno aff
А. В. Мосенков, S. K. H. Bahr, В. П. Решетников, Zacory Shakespear, D. V. Smirnov

Bibliographic record

VenueAstronomy and Astrophysics · 2024
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersSLAC National Accelerator LaboratoryArgonne National LaboratoryHigh Energy PhysicsDivision of Astronomical SciencesJapan Science and Technology AgencyIntegrated Electronics Engineering Center, Binghamton UniversityJapan Society for the Promotion of ScienceSmithsonian Astrophysical ObservatoryYork UniversityMinistério da Ciência, Tecnologia e InovaçãoScience and Technology Facilities CouncilOffice of ScienceUniversity of Colorado BoulderLawrence Berkeley National LaboratoryJet Propulsion LaboratoryCabinet Office, Government of JapanUniversity of Illinois at Urbana-ChampaignInstituto de Astrofísica de CanariasFermilabMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikUniversidad Nacional Autónoma de MéxicoDeutsche ForschungsgemeinschaftChinese Academy of SciencesAcademia SinicaMinistry of Education, Culture, Sports, Science and TechnologyUniversity of SussexUniversity of NottinghamUniversity of OxfordUniversity of ChicagoNational Energy Research Scientific Computing CenterLeibniz-GemeinschaftNational Science FoundationUniversity of MichiganUniversity of Notre DameNational Aeronautics and Space AdministrationUniversity College LondonCarnegie Mellon UniversityUniversity of WashingtonPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityVanderbilt UniversityToray Science FoundationHigh Energy Accelerator Research OrganizationOhio State UniversityCarnegie Institution of WashingtonYale UniversityU.S. Department of EnergySmithsonian InstitutionFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaCalifornia Institute of TechnologyNational Astronomical Observatory of JapanNew Mexico State UniversityUniversity of Portsmouth
KeywordsPhysicsAstrophysicsSkyPolarGalaxyDiscAstronomyPeculiar galaxyGalaxy formation and evolution

Abstract

fetched live from OpenAlex

Polar-ring galaxies are photometrically and kinematically decoupled systems that are highly inclined to the major axis of the host. These galaxies have been explored since the 1970s, but the rarity of these systems has made such systematic studies difficult. However, over 250 good candidates have been identified. In this work, we examine a sample of over 18 000 galaxies from the Sloan Digital Sky Survey (SDSS) Stripe 82 for the presence of galaxies with polar structures. Using deep SDSS Stripe 82, DESI Legacy Imaging Surveys, and Hyper Suprime-Cam Subaru Strategic Program, we selected 53 good candidate galaxies with photometrically decoupled polar rings, 9 galaxies with polar halos, 6 galaxies with polar bulges, and 34 possibly forming polar-ring galaxies, versus 13 polar-ring candidates previously selected in Stripe 82. Our results suggest that the occurrence rate of galaxies with polar structures may be significantly underestimated, as revealed by the deep observations, and may amount to 1–3% of non-dwarf galaxies.

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)0.003
metaresearch head score (Gemma)0.006
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 score0.014

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.006
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
Science and technology studies0.0000.001
Scholarly communication0.0010.001
Open science0.0000.001
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0020.001

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 head0.008
GPT teacher head0.214
Teacher spread0.206 · 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

Citations13
Published2024
Admission routes1
Has abstractyes

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