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Table 1.

Observations presented in this work.

Target name RA Dec zspec Programme ID Sensitivity (a) Beam Ancillary ID Sens. (b) Ang. res. (d)
[deg] [deg] [mJy/beam] [arcsec] [mJy/beam] [arcsec]
(NOEMA)
HPC1001 150.4656 2.6359 3.613 M21AA 0.13 4.7 × 3.7 2013.1.00034.S 0.06 0.4
COS-SBCX3 150.3113 2.4511 3.031 M21AA 0.15 5.4 × 4.5 2016.1.00463.S 0.26 0.8
COS-SBCX4 150.7509 2.4132 2.646 M21AA 0.13 4.2 × 1.8 2016.1.00463.S 0.27 0.8
COS-SBCX7 149.9898 1.7978 2.415 M21AA 0.14 4.7 × 3.8 2015.1.00137.S 0.12 1.0

(ALMA)
COS-SBC3 150.7196 2.6995 2.365 2021.1.00815.S 0.13 0.84 × 0.55 2021.1.00246.S 0.02 1.6
COS-SBC6 149.7057 2.2160 2.323 2021.1.00815.S 0.13 0.87 × 0.53 2016.1.00463.S 0.27 0.8
COS-SBC4 150.0364 2.2177 1.65 (c) 2021.1.00815.S 0.13 0.72 × 0.57 2016.1.00463.S 0.27 0.8

(NOEMA + ALMA)
COS-SBCX1 150.3492 2.7619 2.422 M21AA 0.14 4.8 × 3.8 2016.1.00463.S 0.26 0.8
2021.1.00815.S 0.23 0.83 × 0.66

Notes.

(a)

Line sensitivity over 500 km s−1.

(b)

The redshift is measured from Subaru/FMOS observations (Kashino et al. 2019).

(c)

Continuum sensitivity of the ancillary ALMA data.

(d)

Angular resolution of the ancillary ALMA data.

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