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Table 1.

ALMA observation log of G09v1.97.

Band Date Calibrator ttotal ton Condition SPW Science goal νsky Synthesis beam
Bandpass Flux Phase Nant σψ Baseline Size PA



(min) (min) (deg) (mm) (K) (m) (GHz) (″) (°)
2 CO(6–5) 149.207 0.37 × 0.35 64
4 04-Aug-2016 J0750+1231 J0750+1231 J0825+0309 59.9 36.8 39 59 1.25 60 15–1396 0 H2O(211−202) 161.946 0.38 × 0.36 −74
25-Aug-2016 J0750+1231 J0854+2006 J0825+0309 68.7 36.8 38 28 0.65 55 15–1462 1 H2O+ 160.124 0.40 × 0.36 85
0–3 Continuum (a) 154.508 0.32 × 0.28 −82

7 01-Sep-2015 J0739+0137 J0510+1800 J0839+0104 31.4 3.1 34 46 0.29 94 15–1574 Continuum 343.494 0.19 × 0.12 60

Notes. The central observing coordinates (J2000) are RA 08:30:51.156 and Dec +01:32:24.35 for the Band 4 observations and RA 08:30:51.040, Dec +01:32:25.000 for the Band 7 observations. Nant is the number of antennas used during the observations. σψ and is the phase RMS and the mean precipitable water vapor during the observations, respectively. shows the median system temperature. SPW, namely the spectral windows cover the frequencies ranges of 161.100–162.819 GHz (SPW-0), 159.278–160.996 GHz (SPW-1), 148.345–150.064 GHz (SPW-2) and 147.146–148.865 GHz (SPW-3). νsky gives the sky frequencies of the line centers and the continuum. (a)The 2 mm continuum image was made by combining a line-free spectral window SPW-3 and all the line free channels from SPW-0, SPW-1, and SPW-2. The resulted 2 mm continuum data has a representative frequency of 154.508 GHz.

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