tokens: We acknowledge the detailed comments from the anonymous referee. We thank K. Nakanishi, F. Egusa, R. Kawamata, Y. Harikane, M. Ouchi, P. Papadopoulos, and M. Michałowski for fruitful suggestions. This work was supported by NAOJ ALMA Scientific Research Grant Numbers 2018-09B, 2016-01A, and JSPS/MEXT KAKENHI (No. 17H06130, 17H04831, 17KK0098, 17H01110, 18H04333, 17K14252, and 17H01110). E.Z. acknowledges funding from the Swedish National Space Board. T.T.T. is supported by a Sumitomo Foundation Grant for Basic Science Projects (180923). This paper makes use of the following ALMA data: ADS/JAO.ALMA #2016.1.00117, ADS/JAO.ALMA #2013.1.00999.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), MOST, 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. This work is also based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programme 0100.A-0529(A). Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. This work has made use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. IRAF is distributed by the National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation.
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