tokens: We thank the anonymous referee for the insightful comments. EC and RS acknowledges partial support from the Russian Science Foundation grant 19-12-00369. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00760.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. Basic research in radio astronomy at the US Naval Research Laboratory is funded by 6.1 Base funding, supporting T. Clarke. The scientific results reported in this article are obtained using the following softwares: AstroPy , a community-developed core Python package for Astronomy ( Astropy Collaboration et al. 2018 ); dynesty ( Speagle 2019 ); galario ( Tazzari et al. 2018 ).
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