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Record W4417386364 · doi:10.3847/1538-4357/ae1f18

The SDSS-V Black Hole Mapper Reverberation Mapping Project: Light Echoes of the Coronal-line Region in a Luminous Quasar

2025· article· en· W4417386364 on OpenAlexaff
Theodore B. Smith, Logan B. Fries, Jonathan R. Trump, C. J. Grier, Yue Shen, Scott F. Anderson, W. N. Brandt, Megan C. Davis, T. Dwelly, Patrick B. Hall, K. Horne, Y. Homayouni, Jeffrey D. McKaig, Sean Morrison, Hugh W. Sharp, Roberto J. Assef, F. E. Bauer, Anton M. Koekemoer, Donald P. Schneider, Benny Trakhtenbrot, Héctor J. Ibarra-Medel, C. A. Negrete

Bibliographic record

VenueThe Astrophysical Journal · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicGalaxies: Formation, Evolution, Phenomena
Canadian institutionsYork University
Fundersnot available
KeywordsReverberation mappingRADIUSLine (geometry)Active galactic nucleusLuminosityEmission spectrumContext (archaeology)Spectral line

Abstract

fetched live from OpenAlex

Abstract We present a reverberation mapping (RM) analysis of the coronal line [Ne v ] λ 3427-emitting region of the quasar COS168 (SDSS J095910.30+020732.2). [Ne v ] λ 3427 is known as one of the “coronal lines,” which are a species of emission lines present in active galactic nuclei (AGN) spectra with high ionization potentials (≥ 100 eV) that can serve as tracers for AGN activity. The spatial extent of the coronal line region has been studied with only spatial resolving techniques that are not sensitive to the innermost regions of AGN. Through our RM analysis of [Ne v ] λ 3427, we measure a nominal “optimal emission radius” for [Ne v ] λ 3427 of 381 . 1 − 22 + 16 lt-day (observed frame). We place the coronal line region in context with other AGN regions by comparing it with the characteristic radius of H α , the dust-sublimation radius, and the dusty torus. The coronal line region is located at a larger radius from the black hole than the characteristic radius of the dusty torus, measured using a torus–radius luminosity relationship. The virial product ( v 2 R / G ) of both H α and [Ne v ] λ 3427 is consistent within the uncertainties, implying that the coronal line region, as probed by the [Ne v ] λ 3427 line, may be in a virialized orbit that is dominated by the gravitational potential of the black hole. This plausibly suggests that coronal lines could be an effective method for estimating black hole masses.

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 score0.003
Threshold uncertainty score0.007

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0010.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0010.000
Science and technology studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
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 head0.010
GPT teacher head0.227
Teacher spread0.217 · 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

Citations0
Published2025
Admission routes1
Has abstractyes

Explore more

Same venueThe Astrophysical Journal→Same topicGalaxies: Formation, Evolution, Phenomena→French-language works237,207→