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Table 2

ALMA observations.

Source Band Obs. date Config. Baselines Nant tint (min) vCASA Project ID
(1) (2) (3) (4) (5) (6) (7) (8) (9)
Survey Tau (a) 7 24/11/2016 C40-4 15 m–0.7 km 43 1.1 4.7 2016.1.00460.S
18/08/2017 C40-7 21 m–3.6 km 43 3.7 5.1 2016.1.00460.S
4 27/09/2017 C40-8/9 41 m–14.9 km 43 6.7 5.1 2016.1.00460.S
Survey Cha(b) 7 15/11/2016 C40-4/6 15 m–0.9 km 42 1.1 4.7 2016.1.00460.S
HH 30 7 14, 15, 21/10/2016 C40-6 19 m–2.5 km 42–46 174 4.7 2016.1.01505.S
6 19, 21/07/2015 C34-6/7 13 m–1.6 km 42 78 4.3 2013.1.01175.S
4 23/10/2016 C40-6 19 m–1.8 km 48 12 4.7 2016.1.01505.S
12/09/2017 C40-8/9 41 m–9.5 km 44 31 4.7 2016.1.01505.S
Tau 042021 6 05/12/2016 C40-3 15 m–0.7 km 41 7.5 4.7 2016.1.00771.S
21/10/2016 C40-6 18 m–1.8 km 44 25 4.7 2016.1.00771.S
Oph 163131 6 25/04/2017 C40-3 15 m–0.5 km 41 8.5 4.7 2016.1.00771.S
07/07/2017 C40-5 17 m–2.6 km 44 27 4.7 2016.1.00771.S

Notes. Column 1: Target name, Col. 2: Observing band, Col. 3: Observing date, Col. 4: ALMA array configuration, Col. 5: Minimum and maximum baseline range, Col. 6: Number of antennas, Col. 7: On source integrating time, Col. 8: Calibrating CASA version. (a) The Taurus sources included in the survey are Tau 042021, IRAS 04302, HK Tau B, HV Tau C, IRAS 04200, Haro 6-5B, and IRAS 04158. (b) The Chamaeleon I sources included in the survey are ESO-Hα 569, ESO-Hα 574, and HH 48 NE.

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