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Record W4389049117 · doi:10.3847/1538-4357/acfdac

AGN STORM 2. IV. Swift X-Ray and Ultraviolet/Optical Monitoring of Mrk 817

2023· article· en· W4389049117 on OpenAlexaff
Edward M. Cackett, J. M. Gelbord, Aaron J. Barth, Gisella De Rosa, Rick Edelson, M. R. Goad, Y. Homayouni, K. Horne, Erin Kara, G. A. Kriss, K. T. Korista, Hermine Landt, Rachel Plesha, Nahum Arav, Misty C. Bentz, Benjamin D. Boizelle, E. Dalla Bontà, Maryam Dehghanian, Fergus R. Donnan, Pu Du, G. J. Ferland, C. Fian, A. V. Filippenko, D. González–Buitrago, C. J. Grier, Patrick B. Hall, Hu Chen, D. Ilić, J. S. Kaastra, S. Kaspi, C. S. Kochanek, Andjelka B. Kovačević, Daniel Kynoch, Yanrong Li, Jacob N. McLane, M. Mehdipour, Jake Miller, John Montano, H. Netzer, Christos Panagiotou, Ethan R. Partington, Luka Č. Popović, Daniel Proga, Daniele Rogantini, David Sanmartim, M. R. Siebert, Thaisa Storchi‐Bergmann, M. Vestergaard, Jian‐Min Wang, T.P. Waters, Fatima Zaidouni

Bibliographic record

VenueThe Astrophysical Journal · 2023
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsYork University
FundersScience and Technology Facilities CouncilYouth Innovation Promotion Association of the Chinese Academy of SciencesUniversity of California, IrvineChinese Academy of SciencesNational Natural Science Foundation of ChinaUniversity of LeicesterAlexander von Humboldt-StiftungNational Aeronautics and Space AdministrationNuclear Safety and Security CommissionYouth Innovation Promotion AssociationSpace Telescope Science InstituteNational Science Foundation
KeywordsPhysicsLight curveAstrophysicsUltravioletFlareEmission spectrumWavelengthAmplitudeActive galactic nucleusTorusGalaxyAccretion discQuasarAstronomySpectral lineOpticsGeometry

Abstract

fetched live from OpenAlex

Abstract The AGN STORM 2 campaign is a large, multiwavelength reverberation mapping project designed to trace out the structure of Mrk 817 from the inner accretion disk to the broad emission line region and out to the dusty torus. As part of this campaign, Swift performed daily monitoring of Mrk 817 for approximately 15 months, obtaining observations in X-rays and six UV/optical filters. The X-ray monitoring shows that Mrk 817 was in a significantly fainter state than in previous observations, with only a brief flare where it reached prior flux levels. The X-ray spectrum is heavily obscured. The UV/optical light curves show significant variability throughout the campaign and are well correlated with one another, but uncorrelated with the X-rays. Combining the Swift UV/optical light curves with Hubble Space Telescope UV continuum light curves, we measure interband continuum lags, τ ( λ ), that increase with increasing wavelength roughly following τ ( λ ) ∝ λ 4/3 , the dependence expected for a geometrically thin, optically thick, centrally illuminated disk. Modeling of the light curves reveals a period at the beginning of the campaign where the response of the continuum is suppressed compared to later in the light curve—the light curves are not simple shifted and scaled versions of each other. The interval of suppressed response corresponds to a period of high UV line and X-ray absorption, and reduced emission line variability amplitudes. We suggest that this indicates a significant contribution to the continuum from the broad-line region gas that sees an absorbed ionizing continuum.

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 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 categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.878
Threshold uncertainty score0.528

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 studies0.0000.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
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 head0.017
GPT teacher head0.248
Teacher spread0.232 · 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 teacher head, 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

Citations33
Published2023
Admission routes1
Has abstractyes

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