{"paper":{"title":"The Lick AGN Monitoring Project 2016: Dynamical Modeling of Velocity-Resolved H\\b{eta} Lags in Luminous Seyfert Galaxies","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.GA","authors_text":"Aaron J. Barth, Alexei V. Filippenko, Andrew Brandel, Andrew Halle, Azalee Bostroem, Bela Abolfathi, Benjamin D. Boizelle, Benjamin E. Stahl, Benjamin Kuhn, Brendon J. Brewer, Bryan Scott, Carol E. Hood, Chance L. Spencer, Christina Manzano-King, Daeseong Park, Diego Gonzalez-Buitrago, Donald Loveland, Douglas C. Leonard, Edward Donohue, Elinor Gates, Frederick Hamann, Gabriela Canalizo, Goni Halevi, H. Alexander Vogler, Heechan Yuk, Hengxiao Guo, Hyun-Jin Bae, Ian McHardy, Isaac Shivvers, Isak Stomberg, Jaejin Shin, Javier Sanchez, J. Chuck Horst, Jenna Samuel, Jonelle L. Walsh, Jong-Hak Woo, Jordan N. Runco, Keith Horne, L. E. Abramson, Liuyi Pei, Lizvette Villafa\\~na, Maren Cosens, Matthew A. Malkan, Maxime de Kouchkovsky, M. C. Cooper, Melanie Kae B. Olaes, Michael D. Joner, Misty C. Bentz, Peter R. Williams, Raul Michel, Remington O. Sexton, Sahana Kumar, Samantha Stegman, Sanyum Channa, Sean P. Fillingham, Songyoun Park, Stefano Valenti, Stephen F. Armen, Thomas Bohn, Thomas G. Brink, Timothy W. Ross, Tommaso Treu, Vardha N. Bennert, Vivian U, Weikang Zheng","submitted_at":"2022-03-28T18:07:04Z","abstract_excerpt":"We have modeled the velocity-resolved reverberation response of the H\\b{eta} broad emission line in nine Seyfert 1 galaxies from the Lick Active Galactic Nucleus (AGN) Monitioring 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\\b{eta} 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 log10(FWHM/{\\sigma}), on BLR structure and k"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.15000","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2203.15000/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}