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  3. 1 CONTRIBUTI IN RIVISTE (Journal articles)
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  5. Space Telescope and Optical Reverberation Mapping Project. V. Optical Spectroscopic Campaign and Emission-line Analysis for NGC 5548
 

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

Journal
THE ASTROPHYSICAL JOURNAL  
Date Issued
2017
Author(s)
Pei, L.
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Fausnaugh, M. M.
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Barth, A. J.
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Peterson, B. M.
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Bentz, M. C.
•
De Rosa, G.  
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Denney, K. D.
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Goad, M. R.
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Kochanek, C. S.
•
Korista, K. T.
•
Kriss, G. A.
•
Pogge, R. W.
•
Bennert, V. N.
•
Brotherton, M.
•
Clubb, K. I.
•
Dalla Bontà, E.
•
Filippenko, A. V.
•
Greene, J. E.
•
Grier, C. J.
•
Vestergaard, M.
•
Zheng, W.
•
Adams, Scott M.
•
Beatty, Thomas G.
•
Bigley, A.
•
Brown, Jacob E.
•
Brown, Jonathan S.
•
Canalizo, G.
•
Comerford, J. M.
•
Coker, Carl T.
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Corsini, E. M.
•
Croft, S.
•
Croxall, K. V.
•
Deason, A. J.
•
Eracleous, Michael
•
Fox, O. D.
•
Gates, E. L.
•
Henderson, C. B.
•
Holmbeck, E.
•
Holoien, T. W. -S.
•
Jensen, J. J.
•
Johnson, C. A.
•
Kelly, P. L.
•
Kim, S.
•
King, A.
•
Lau, M. W.
•
Li, Miao
•
Lochhaas, Cassandra
•
Ma, Zhiyuan
•
Manne-Nicholas, E. R.
•
Mauerhan, J. C.
•
Malkan, M. A.
•
McGurk, R.
•
Morelli, L.
•
Mosquera, Ana
•
Mudd, Dale
•
Muller Sanchez, F.
•
Nguyen, M. L.
•
Ochner, P.
•
Ou-Yang, B.
•
Pancoast, A.
•
Penny, Matthew T.
•
Pizzella, A.
•
Poleski, Radosław
•
Runnoe, Jessie
•
Scott, B.
•
Schimoia, Jaderson S.
•
Shappee, B. J.
•
Shivvers, I.
•
Simonian, Gregory V.
•
Siviero, A.
•
Somers, Garrett
•
Stevens, Daniel J.
•
Strauss, M. A.
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Tayar, Jamie
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Tejos, N.
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Treu, T.
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Van Saders, J.
•
Vican, L.
•
Villanueva, S., Jr.
•
Yuk, H.
•
Zakamska, N. L.
•
Zhu, W.
•
Anderson, M. D.
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Arévalo, P.
•
Bazhaw, C.
•
Bisogni, Susanna  
•
Borman, G. A.
•
Bottorff, M. C.
•
Brandt, W. N.
•
Breeveld, A. A.
•
Cackett, E. M.
•
Carini, M. T.
•
Crenshaw, D. M.
•
De Lorenzo-Cáceres, A.
•
Dietrich, M.
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Edelson, R.
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Efimova, N. V.
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Ely, J.
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Evans, P. A.
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Ferland, G. J.
•
Flatland, K.
•
Gehrels, N.
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Geier, S.
•
Gelbord, J. M.
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Grupe, D.
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Gupta, A.
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Hall, P. B.
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Hicks, S.
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Horenstein, D.
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Horne, Keith
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Hutchison, T.
•
Im, M.
•
Joner, M. D.
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Jones, J.
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Kaastra, J.
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Kaspi, S.
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Kelly, B. C.
•
Kennea, J. A.
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Kim, M.
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Kim, S. C.
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Klimanov, S. A.
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Lee, J. C.
•
Leonard, D. C.
•
Lira, P.
•
MacInnis, F.
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Mathur, S.
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McHardy, I. M.
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Montouri, C.
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Musso, R.
•
Nazarov, S. V.
•
Netzer, H.
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Norris, R. P.
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Nousek, J. A.
•
Okhmat, D. N.
•
Papadakis, I.
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Parks, J. R.
•
Pott, J. -U.
•
Rafter, S. E.
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Rix, H. -W.
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Saylor, D. A.
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Schnülle, K.
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Sergeev, S. G.
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Siegel, M.
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Skielboe, A.
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Spencer, M.
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Starkey, D.
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Sung, H. -I.
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Teems, K. G.
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Turner, C. S.
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Uttley, P.
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Villforth, C.
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Weiss, Y.
•
Woo, J. -H.
•
Yan, H.
•
Young, S.
•
Zu, Y.
DOI
10.3847/1538-4357/aa5eb1
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 Hβ and He II λ4686 broad emission-line light curves lag that of the 5100 Å optical continuum by {4.17}-0.36+0.36 {days} and {0.79}-0.34+0.35 {days}, respectively. The Hβ 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 Hβ 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 Hβ and He II emission lines to the driving continuum changed significantly halfway through the campaign, a phenomenon also observed for C IV, Lyα, 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 Hβ 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.
Volume
837
Issue
2
Start page
131
Uri
http://hdl.handle.net/20.500.12386/26963
Url
https://iopscience.iop.org/article/10.3847/1538-4357/aa5eb1
Issn Identifier
0004-637X
Ads BibCode
2017ApJ...837..131P
Rights
open.access
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