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Beyond diagnostic-diagrams: A critical exploration of the classification of ionization processes

2025· article· en· W7116393014 on OpenAlexfundno aff
S. F. Sánchez, C. Muñoz–Tuñón, J. Sánchez Almeida, O. González-Martín, E. Pérez

Bibliographic record

VenueSpringer Link (Chiba Institute of Technology) · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsnot available
FundersLawrence Berkeley National LaboratoryBrookhaven National LaboratoryDirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de MéxicoAgencia Estatal de InvestigaciónCollege of Engineering, Michigan State UniversityUniversidade do PortoJohns Hopkins UniversityYale UniversityVanderbilt UniversityNew Mexico State UniversityUniversity of PortsmouthUniversity of WashingtonOhio State UniversityPrinceton UniversityMinisterio de Ciencia e InnovaciónYork UniversityNational Aeronautics and Space Administration
KeywordsGalaxyClassification schemeActive galactic nucleusIonizationSkySample (material)Fraction (chemistry)

Abstract

fetched live from OpenAlex

Context. Diagnostic diagrams based on optical emission lines, especially classical BPT diagrams, have long been used to distinguish the dominant ionisation mechanisms in galaxies. However, these methods suffer from degeneracies and limitations, particularly when applied to complex systems such as galaxies, where multiple ionisation sources coexist. Aims. We aim to critically assess the effectiveness of commonly used diagnostic diagrams in identifying star-forming galaxies, retired galaxies (RGs), and active galactic nuclei (AGNs). We also explore alternative diagnostics and propose a revised classification scheme to reduce misclassifications and better reflect the physical mechanisms ionizing gas in galaxies. Methods. Using a comprehensive sample of nearby galaxies from the NASA-Sloan Atlas (NSA) cross-matched with Sloan Digital Sky Survey (SDSS) spectroscopic data, we defined archetypal subsamples of late-type and star-forming galaxies, early-type and retired galaxies, and multiwavelength-selected AGNs. We evaluated their distribution across classical and more recent diagnostic diagrams, including the WHaN, WHaD, and a newly proposed WHaO diagram, which combine Hα equivalent width with additional indicators (N II/Hα, σHα and O III/O II, respectively). We carried out a quantitative comparison of the resulting classification across multiple schemes. Results. Classical BPT diagrams systematically overestimate the number of star-forming galaxies (∼10%) and misclassify a significant fraction of AGNs (up to 45%) and RGs (up to 100%). Diagrams incorporating the equivalent width of Hα, such as WHaN, WHaD, or WHaO, yield more reliable separations (with ∼20% of AGNs and ∼15% of RGs erroneously classified). A new classification scheme based on EW(Hα) thresholds and concordant WHaD/WHaO results achieves an improved level of purity for all classes (with ∼8–25% sources erroneously classified) and a better alignment with known physical properties. Conclusions. The widely used BPT-based classifications fail to accurately distinguish between ionisation mechanisms, especially in galaxies hosting low-luminosity AGNs or retired stellar populations. Updated schemes incorporating EW(Hα) and complementary diagnostics, despite their respective limitations, provide a more accurate view of galaxy ionisation and should be adopted in future studies of galaxy populations and evolution.

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)0.007
metaresearch head score (Gemma)0.038
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.007
Threshold uncertainty score0.037

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0070.038
Meta-epidemiology (narrow)0.0010.000
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0070.004
Science and technology studies0.0010.002
Scholarly communication0.0040.005
Open science0.0020.003
Research integrity0.0010.002
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 head0.012
GPT teacher head0.241
Teacher spread0.229 · 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 designTheoretical or conceptual
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".

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Citations0
Published2025
Admission routes1
Has abstractyes

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