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Record W2592048703 · doi:10.3847/1538-4357/aa5eb1

Space Telescope and Optical Reverberation Mapping Project. V. Optical Spectroscopic Campaign and Emission-line Analysis for NGC 5548

2017· article· en· W2592048703 on OpenAlex

Why this work is in the frame

A frame that forgets how it found something cannot be audited. These are the routes that admitted this work.

affAt least one author lists a Canadian institution in the pinned OpenAlex snapshot.
fundA Canadian funder is recorded on the work.

Bibliographic record

VenueThe Astrophysical Journal · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAdaptive optics and wavefront sensing
Canadian institutionsYork University
FundersNatural Sciences and Engineering Research Council of CanadaComisión Nacional de Investigación Científica y TecnológicaUniversity of California, Santa BarbaraJet Propulsion LaboratoryNational Research Foundation of KoreaNederlandse Organisatie voor Wetenschappelijk OnderzoekSpace Telescope Science InstituteAmerican Academy in RomeScience and Technology Facilities CouncilNational Research FoundationDanmarks Frie ForskningsfondNational Science FoundationUniversity of WashingtonMinistry of Science, ICT and Future PlanningOhio State UniversityConselho Nacional de Desenvolvimento Científico e TecnológicoGeorgia State UniversityU.S. Department of EnergyCalifornia Institute of TechnologyDanmarks GrundforskningsfondHoward Hughes Medical InstituteNational Aeronautics and Space Administration
KeywordsLight curveLagUltravioletReverberation mappingRADIUSTime lagOptical telescopeLuminosity

Abstract

fetched live from OpenAlex

Abstract We present the results of an optical spectroscopic monitoring program targeting NGC 5548 as part of a larger multiwavelength reverberation mapping campaign. The campaign spanned 6 months and achieved an almost daily cadence with observations from five ground-based telescopes. The H β and He ii λ 4686 broad emission-line light curves lag that of the 5100 Å optical continuum by and , respectively. The H β lag relative to the 1158 Å ultraviolet continuum light curve measured by the Hubble Space Telescope is ∼50% longer than that measured against the optical continuum, and the lag difference is consistent with the observed lag between the optical and ultraviolet continua. This suggests that the characteristic radius of the broad-line region is ∼50% larger than the value inferred from optical data alone. We also measured velocity-resolved emission-line lags for H β and found a complex velocity-lag structure with shorter lags in the line wings, indicative of a broad-line region dominated by Keplerian motion. The responses of both the H β and He ii emission lines to the driving continuum changed significantly halfway through the campaign, a phenomenon also observed for C iv , Ly α , He ii (+O iii ]), and Si iv (+O iv ]) during the same monitoring period. Finally, given the optical luminosity of NGC 5548 during our campaign, the measured H β lag is a factor of five shorter than the expected value implied by the R BLR – L AGN relation based on the past behavior of NGC 5548.

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.

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.000
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.530
Threshold uncertainty score1.000

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0000.000
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0010.000
Scholarly communication0.0010.000
Open science0.0000.000
Research integrity0.0000.000
Insufficient payload (model declined to judge)0.0000.000

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 head0.024
GPT teacher head0.285
Teacher spread0.261 · 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