Open Access

Table 1.

ALMA observation & imaging pipeline data product details.

Property Observation 1 Observation 2 Observation 3 Observation 4
Project Code 2018.1.01852.S 2019.1.01615.S 2019.1.01615.S 2019.1.01615.S
Observation Dates 2019 Mar. 13, Apr. 1, 3 2020 Jan. 13 2020 Jan. 14, 16, 25 2020 Feb. 28
Max baseline length 360–500 m 178 m 167–180 m 784 m
No. of antennasa 45–48 38–41 40–42 38
Bandpass Calibrator J1058+0133 J1058+0133 J1058+0133 J1058+0133
Bandpass Cal Flux ∼4.6 Jy ∼2.6 Jy ∼2.6 Jy ∼2.9 Jy
Phase Calibrator J0948+022 J1008+0029 J1008+0029 J1008+0621
Phase Cal Flux ∼90–210 mJy ∼61 mJy ∼61 mJy ∼140 mJy
SFR UV + IR $ _\mathrm{{UV}+\rm{IR}} $ Target Selection > 1 M yr−1 ∼0.4 M yr−1 ∼0.6 M yr−1 Replacementc
COSMOS targets 0969208, 1189669, 1399657, 1440745 1008875, 1009969, 1429536, 1430950
1197519, 1200839, 1197786, 1440643
1204323, 1411106
No. of Executions 3 3 7 1
Time on source 20 min 75 min 60 min 50 min
Cube beam size 2.1″ × 1.6″ 1.7″ × 1.5″ 1.7″ × 1.5″ 1.8″ × 1.1″
Cube RMS noiseb 1.1 mJy beam−1 0.65 mJy beam−1 0.81 mJy beam−1 0.69 mJy beam−1
Cube RMS noise (5″)b 1.5 mJy beam−1 1.0 mJy beam−1 1.2 mJy beam−1 2.2 mJy beam−1

Notes. aNumber of antennas after flagging. bNoise per channel in the final products from the ALMA Interferometric Pipeline (see Section 2.1). The value does not account for noise correlation between channels. cReplacement observations for bad LO tuning.

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