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Record W2608320463 · doi:10.3847/1538-4357/aa832b

Space Telescope and Optical Reverberation Mapping Project. VII. Understanding the Ultraviolet Anomaly in NGC 5548 with X-Ray Spectroscopy

2017· article· en· W2608320463 on OpenAlexaff
S. Mathur, Anjali Gupta, K. L. Page, Richard W. Pogge, Y. Krongold, M. R. Goad, S. M. Adams, Matthew Anderson, P. Arévalo, Aaron J. Barth, C. Bazhaw, Thomas G. Beatty, Misty C. Bentz, A. Bigley, S. Bisogni, G. A. Borman, Todd A. Boroson, M. C. Bottorff, W. N. Brandt, A. A. Breeveld, J.E.C. Brown, J. S. Brown, Edward M. Cackett, Gabriela Canalizo, M. T. Carini, K. I. Clubb, Julia M. Comerford, Carl T. Coker, E. M. Corsini, D. M. Crenshaw, S. Croft, K. V. Croxall, E. Dalla Bontà, Alis J. Deason, K. D. Denney, A. de Lorenzo-Cáceres, Gisella De Rosa, M. Dietrich, Rick Edelson, Justin Ely, Michael Eracleous, P. A. Evans, Michael Fausnaugh, G. J. Ferland, A. V. Filippenko, K. Flatland, Ori D. Fox, E. L. Gates, N. Gehrels, S. Geier, J. M. Gelbord, Varoujan Gorjian, Jenny E. Greene, C. J. Grier, D. Grupe, Patrick B. Hall, Calen B. Henderson, S. Hicks, Erika M. Holmbeck, T. W. S. Holoien, D. Horenstein, K. Horne, Taylor A. Hutchison, Myungshin Im, J. J. Jensen, C. A. Johnson, M. D. Joner, Jeremy Jones, J. S. Kaastra, S. Kaspi, Brandon C. Kelly, Patrick L. Kelly, J. A. Kennea, Minjin Kim, Sohye Kim, S. C. Kim, A. L. King, S. A. Klimanov, C. S. Kochanek, K. T. Korista, G. A. Kriss, Marie Wingyee Lau, J. C. Lee, Douglas C. Leonard, M. Li, P. Lira, Zhiyuan Ma, F. MacInnis, E. R. Manne-Nicholas, Matthew A. Malkan, Jon C. Mauerhan, Rosalie McGurk, I. M. McHardy, C. Montouri, L. Morelli, A. M. Mosquera, D. Mudd, Francisco Müller-Sánchez, R. Musso, S. V. Nazarov, H. Netzer, M. L. Nguyen, R. P. Norris, J. A. Nousek, P. Ochner, D. N. Okhmat, B. Ou-Yang, Anna Pancoast, I. E. Papadakis, J. R. Parks, L. Pei, B. M. Peterson, A. Pizzella, R. Poleski, Jörg‐Uwe Pott, S. E. Rafter, Hans‐Walter Rix, Jessie C. Runnoe, D. A. Saylor, J. S. Schimoia, K. Schnülle, С. Г. Сергеев, B. J. Shappee, I. Shivvers, M. H. Siegel, G. Simonian, A. Siviero, A. Skielboe, Garrett Somers, M. Spencer, D. Starkey, Daniel J. Stevens, Hyun-Il Sung, Jamie Tayar, Nicolás Tejos, C. S. Turner, P. Uttley, Jennifer L. van Saders, M. Vestergaard, Laura Vican, Steven Villanueva, C. Villforth, Y. Weiss, Jong-Hak Woo, Haojing Yan, S. Young, Heechan Yuk, WeiKang Zheng, Wei Zhu, Ying Zu

Bibliographic record

VenueThe Astrophysical Journal · 2017
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysical Phenomena and Observations
Canadian institutionsYork University
FundersScience and Technology Facilities CouncilSmithsonian Astrophysical ObservatoryUniversity of LeicesterNational Aeronautics and Space AdministrationSpace Telescope Science InstituteSmithsonian InstitutionConsejo Nacional de Ciencia y TecnologíaNational Science Foundation
KeywordsPhysicsAstrophysicsSpectral lineAnomaly (physics)Emission spectrumSpectroscopyUltravioletLine (geometry)South Atlantic AnomalyAstronomyMagnetospherePlasmaOptics

Abstract

fetched live from OpenAlex

Abstract During the Space Telescope and Optical Reverberation Mapping Project observations of NGC 5548, the continuum and emission-line variability became decorrelated during the second half of the six-month-long observing campaign. Here we present Swift and Chandra X-ray spectra of NGC 5548 obtained as part of the campaign. The Swift spectra show that excess flux (relative to a power-law continuum) in the soft X-ray band appears before the start of the anomalous emission-line behavior, peaks during the period of the anomaly, and then declines. This is a model-independent result suggesting that the soft excess is related to the anomaly. We divide the Swift data into on- and off-anomaly spectra to characterize the soft excess via spectral fitting. The cause of the spectral differences is likely due to a change in the intrinsic spectrum rather than to variable obscuration or partial covering. The Chandra spectra have lower signal-to-noise ratios, but are consistent with the Swift data. Our preferred model of the soft excess is emission from an optically thick, warm Comptonizing corona, the effective optical depth of which increases during the anomaly. This model simultaneously explains all three observations: the UV emission-line flux decrease, the soft-excess increase, and the emission-line anomaly.

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 categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.780
Threshold uncertainty score0.999

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 studies0.0020.000
Scholarly communication0.0010.001
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 head0.027
GPT teacher head0.257
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 teacher head, not a consensus.

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

Citations41
Published2017
Admission routes1
Has abstractyes

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