The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. IV. Unveiling the Embedded Intermediate-Mass Protostar and Disk within OMC2-FIR3/HOPS-370

The authors thank the anonymous referee for a constructive report that improved the quality of the manuscript. The authors wish to acknowledge useful discussions with L. Hartmann and J. Bae about the results. J.J.T. acknowledges support from grant AST-1814762 from the National Science Foundation and past support from the Homer L. Dodge Endowed Chair at the University of Oklahoma. P.D.S is supported by a National Science Foundation Astronomy & Astrophysics Postdoctoral Fellowship under Award No. 2001830. G.A., M.O., and A.K.D.-R. acknowledge financial support from the State Agency for Research of the Spanish MCIU through the AYA2017-84390-C2-1-R grant (co-funded by FEDER) and through the "Center of Excellence Severo Ochoa" award for the Instituto de Astrofisica de Andalucia (SEV-2017-0709). Z.Y.L. is supported in part by NASA 80NSSC18K1095 and NSF AST-1716259. M.K. gratefully acknowledges funding by the University of Tartu ASTRA project 2014-2020.4.01.16-0029 KOMEET "Benefits for Estonian Society from Space Research and Application," financed by the EU European Regional Development Fund. M.L.R.H. acknowledges support from the Michigan Society of Fellows. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.00041.S and ADS/JAO.ALMA#2017.1.00419.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. These results are based on observations obtained with the Apache Point Observatory 3.5m telescope, which is owned and operated by the Astrophysical Research Consortium (ARC). We wish to thank the APO 3.5m telescope operators in their assistance in obtaining these data. Access to the APO 3.5m telescope is funded by the University of Oklahoma and the Homer L. Dodge Endowed Chair. This research made use of APLpy, an open-source plotting package for Python hosted at.http://aplpy.github.com.This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration, 2013) http://www.astropy.org.