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tokens: This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.00773.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Y.-L. W. is grateful to the support from the Heising-Simons Foundation. J.T. would like to acknowledge support from the Homer L. Dodge Endowed Chair. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under grant No. 2012115762. This work was supported by NSF AAG grant 1311910. The results reported herein benefitted from collaborations and/or information exchange within NASA’s Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA’s Science Mission Directorate. The computing for this project was performed at the OU Supercomputing Center for Education and Research (OSCER) at the University of Oklahoma (OU). Software: pdspy (Sheehan 2018 ), CASA (McMullin et al. 2007 ), RADMC-3D (Dullemond 2012 ), emcee (Foreman-Mackey et al. 2013 ), matplotlib (Hunter 2007 ), corner (Foreman-Mackey 2016 ), GALARIO (Tazzari et al. 2018 ).