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Table 1.
Overview of new observations presented in this paper.
| ID( * ) | RA, Dec | 3mm | Beam3mm | 1mm | 870 μm | line scan |
|---|---|---|---|---|---|---|
| 3117 | 150.58858, 2.31908 | S18DI | 3.4″ × 2.3″ | – | 2016.1.00463.S | NOEMA |
| 5340 | 150.34488, 2.01271 | S18DI,W20DM | 5.1″ × 3.9″ | – | 2016.1.00463.S | NOEMA |
| 6309 | 150.08060, 1.68511 | S18DI,W20DM | 5.7″ × 4.3″ | 2016.1.00279.S | 2016.1.00463.S | NOEMA |
| 7549 | 149.54492, 2.10318 | S18DI | 4.0″ × 1.9″ | 2016.1.00279.S | 2016.1.00463.S | NOEMA |
| 9316 | 149.99498, 2.58278 | 2018.1.00874.S | 0.41″ × 0.36″ | 2013.1.00118.S | 2016.1.00478.S | ALMA |
| 12646( * ) | 189.11469, 62.20501 | W17EK,W19DQ | 1.6″ × 1.1″ | W18EY | – | NOEMA |
Notes. ( * )ID12646 is from the Liu et al. (2018) catalog, while the remaining IDs are originally from the radio catalog of Smolčić et al. (2017) and are also used in the COSMOS super-deblended catalog (IDJin = IDSmolcic+2E7).
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