Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/39616
Title: Space Telescope and Optical Reverberation Mapping Project. V. Optical Spectroscopic Campaign and Emission-Line Analysis for NGC 5548
Authors: Pei, L.
Fauanaugh, M. M.
Barth, A. J.
Peterson, B. M.
Bentz, M. C.
De Rosa, G.
Denney, K. D.
Goad, M. R.
Kochanek, C. S.
Korista, K. T.
Kriss, G. A.
Norris, R. P.
Nousek, J. A.
Okhmat, D. N.
Papadakis, I.
Parks, J. R.
Pott, J.-U.
Rafter, S. E.
Rix, H.-W.
Saylor, D. A.
Clubb, K. I.
Li, Miao
Schnülle, K.
Sergeev, S. G.
Siegel, M.
Skielboe, A.
Spencer, M.
Starkey, D.
Sung, H.-I.
Teems, K. G.
Turner, C. S.
Uttley, P.
Lochhaas, Cassandra
Dalla Bontà, E.
Villforth, C.
Weiss, Y.
Woo, J.-H.
Yan22, H.
Young58, S.
Filippenko, A. V.
Greene, J. E.
Grier, C. J.
Vestergaard, M.
Ma, Zhiyuan
Zheng, W.
Adams, Scott M.
Beatty, Thomas G.
Bigley, A.
Brown, Jacob E.
Brown, Jonathan S.
Canalizo, G.
Comerford, J. M.
Coker, Carl T.
Corsini, E. M.
Manne-Nicholas, E. R.
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.
Mauerhan, J. C.
Johnson, C. A.
Kelly, P. L.
Kim, S.
King, A.
Lau, M. W.
Malkan, M. A.
McGurk, R
Morelli, L.
Mosquera, Ana
Mudd, Dale
Flatland, K.
Sanchez, F. Muller
Nguyen, M. L.
Ochner, P.
Ou-Yang, B.
Pancoast, A.
Penny, Matthew T.
Pizzella, A.
Poleski, Radosław
Runnoe, Jessie
Scott, B.
Gehrels, N.
Schimoia, Jaderson S.
Shappee, B. J.
Shivvers, I.
Simonian, Gregory V.
Siviero, A.
Somers, Garrett
Stevens, Daniel J.
Strauss, M. A.
Tayar, Jamie
Tejos, N.
Geier, S.
Treu, T.
Van Saders, J.
Vican, L.
Villanueva Jr., S.
Yuk, H.
Zakamska, N. L.
Zhu, W.
Anderson, M. D.
Arévalo, P.
Bazhaw, C.
Gelbord, J. M.
Bisogni, S.
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.
Grupe, D.
Edelson, R.
Efimova, N. V.
Ely, J.
Evans, P. A.
Ferland, G. J.
Gupta, A.
Hall, P. B.
Hicks, S.
Horenstein, D.
Horne, Keith
Pogge, R. W.
Hutchison, T.
Im, M.
Joner, M. D.
Jones, J.
Kaastra, J.
Kaspi, S.
Kelly, B. C.
Kennea, J. A.
Kim, M.
Kim, S. C.
Bennert, V. N.
Klimanov, S. A.
Lee, J. C.
Leonard, D. C.
Lira, P.
MacInnis, F.
Mathur, S.
McHardy, I. M.
Montouri, C.
Musso, R.
Nazarov, S. V.
Brotherton, M.
Netzer, H.
Zu, Y.
First Published: 10-Mar-2017
Publisher: American Astronomical Society, IOP Publishing
Citation: Astrophysical Journal, 2017, 837(2)
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 ${4.17}_{-0.36}^{+0.36}\,\mathrm{days}$ and ${0.79}_{-0.34}^{+0.35}\,\mathrm{days}$, 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.
DOI Link: 10.3847/1538-4357/aa5eb1
ISSN: 0004-637X
eISSN: 1538-4357
Links: http://iopscience.iop.org/article/10.3847/1538-4357/aa5eb1
http://hdl.handle.net/2381/39616
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © 2017, American Astronomical Society, IOP Publishing. Deposited with reference to the publisher’s open access archiving policy.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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