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Record W4293794695 · doi:10.48550/arxiv.2208.12943

Unveiling the nature of polar-ring galaxies from deep imaging

2022· preprint· en· W4293794695 on OpenAlexfundno aff
А. В. Мосенков, В. П. Решетников, Maria N. Skryabina, Zacory Shakespear

Bibliographic record

VenuearXiv (Cornell University) · 2022
Typepreprint
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 LaboratoryInstituto de Astrofísica de CanariasFermilabMax-Planck-Institut für AstronomieMax-Planck-Institut für AstrophysikCabinet Office, Government of JapanUniversity of Illinois at Urbana-ChampaignRussian Science FoundationUniversidad Nacional Autónoma de MéxicoDeutsche ForschungsgemeinschaftChinese Academy of SciencesAcademia SinicaMinistry of Education, Culture, Sports, Science and TechnologyUniversity of SussexUniversity of OxfordLeibniz-GemeinschaftUniversity of Notre DameNational Aeronautics and Space AdministrationUniversity College LondonCarnegie Mellon UniversityUniversity of WashingtonPrinceton UniversityAlfred P. Sloan FoundationJohns Hopkins UniversityCarnegie Institution of WashingtonUniversity of PortsmouthNew Mexico State UniversityUniversity of UtahVanderbilt UniversityUniversity of ChicagoToray Science FoundationHigh Energy Accelerator Research OrganizationOhio State UniversityYale UniversityU.S. Department of EnergySmithsonian InstitutionFinanciadora de Estudos e ProjetosUniversity of PennsylvaniaCalifornia Institute of TechnologyNational Astronomical Observatory of JapanNational Science Foundation
KeywordsPolarGalaxyAstrophysicsPhysicsSkyPeculiar galaxyAccretion (finance)Surface brightnessAstronomyGalaxy formation and evolutionLenticular galaxy

Abstract

fetched live from OpenAlex

General structural properties and low surface brightness tidal features hold important clues to the formation of galaxies. In this paper, we study a sample of polar-ring galaxies (PRGs) based on optical imaging from the Sloan Digital Sky Survey (SDSS) Stripe82 and other deep surveys. We investigate the deepest images of candidates for PRGs to date. We carry out photometric decomposition on the host galaxies and associated polar structures that allows us to derive the structural properties of both components. We are able to detect very faint tidal structures around most PRGs in our sample. For several galaxies, we can directly observe the formation of the polar ring due to merging, which is manifested in debris of the victim galaxy and an arc-like polar structure made up of its material. In a few cases, we can discern signs of tidal accretion. The results obtained indicate that the gravitational interaction and merging of galaxies are the most plausible mechanisms for the formation of polar-ring 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)0.000
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 score0.002
Threshold uncertainty score0.003

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0000.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0020.001
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 head0.016
GPT teacher head0.168
Teacher spread0.153 · 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

Citations1
Published2022
Admission routes1
Has abstractyes

Explore more

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