%AVillafaña, Lizvette%AWilliams, Peter%ATreu, Tommaso%ABrewer, Brendon%ABarth, Aaron%AU, Vivian%ABennert, Vardha%AAlexander Vogler, H.%AGuo, Hengxiao%ABentz, Misty%ACanalizo, Gabriela%AFilippenko, Alexei%AGates, Elinor%AHamann, Frederick%AJoner, Michael%AMalkan, Matthew%AWoo, Jong-Hak%AAbolfathi, Bela%AAbramson, L.%AArmen, Stephen%ABae, Hyun-Jin%ABohn, Thomas%ABoizelle, Benjamin%ABostroem, K.%ABrandel, Andrew%ABrink, Thomas%AChanna, Sanyum%ACooper, M.%ACosens, Maren%ADonohue, Edward%AFillingham, Sean%AGonzález-Buitrago, Diego%AHalevi, Goni%AHalle, Andrew%AHood, Carol%AHorne, Keith%AChuck Horst, J.%Ade Kouchkovsky, Maxime%AKuhn, Benjamin%AKumar, Sahana%ALeonard, Douglas%ALoveland, Donald%AManzano-King, Christina%AMcHardy, Ian%AMichel, Raúl%AKae B. Olaes, Melanie%APark, Daeseong%APark, Songyoun%APei, Liuyi%ARoss, Timothy%ARunco, Jordan%ASánchez, Javier%AScott, Bryan%ASexton, Remington%AShin, Jaejin%AShivvers, Isaac%ASpencer, Chance%AStahl, Benjamin%AStegman, Samantha%AStomberg, Isak%AValenti, Stefano%AWalsh, Jonelle%AYuk, Heechan%AZheng, WeiKang%BJournal Name: The Astrophysical Journal; Journal Volume: 930; Journal Issue: 1 %D2022%I %JJournal Name: The Astrophysical Journal; Journal Volume: 930; Journal Issue: 1 %K %MOSTI ID: 10327880 %PMedium: X %TThe Lick AGN Monitoring Project 2016: Dynamical Modeling of Velocity-resolved Hβ Lags in Luminous Seyfert Galaxies %XAbstract We have modeled the velocity-resolved reverberation response of the H β broad emission line in nine Seyfert 1 galaxies from the Lick Active Galactic Nucleus (AGN) Monitoring Project 2016 sample, drawing inferences on the geometry and structure of the low-ionization broad-line region (BLR) and the mass of the central supermassive black hole. Overall, we find that the H β BLR is generally a thick disk viewed at low to moderate inclination angles. We combine our sample with prior studies and investigate line-profile shape dependence, such as log 10 ( FWHM / σ ) , on BLR structure and kinematics and search for any BLR luminosity-dependent trends. We find marginal evidence for an anticorrelation between the profile shape of the broad H β emission line and the Eddington ratio, when using the rms spectrum. However, we do not find any luminosity-dependent trends, and conclude that AGNs have diverse BLR structure and kinematics, consistent with the hypothesis of transient AGN/BLR conditions rather than systematic trends. %0Journal Article