ALMA resolves the remarkable molecular jet and rotating wind in the extremely radio-quiet galaxy NGC 1377

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Table 1.

Journal of the observations.

Date of	N_ant^(b)	PWV ^(c)	t_on^(d)	B_min/B_max^(e)	Bandpass	Flux	Gain
observations		(mm)	(min)	(m/km)	calibrator	calibrator ( ^(f) Jy)	calibrator
12 Aug 2014 ^(a1)	33	∼0.5	30	31/1.1	J 0423−0120	J 0334−401 (0.46 ± 0.14)	J 0340−2119
12 Nov 2017 ^(a2)	45	∼0.6	50	113/13.9	J 0522−3627	J 0522−3627 (4.81 ± 0.23)	J 0340−2119
21 Nov 2017 ^(a2)	47	0.4–0.6	50	92/8.5	J 0522−3627	J 0522−3627 (4.70 ± 0.19)	J 0340−2119

Notes.

^(a1)

ALMA project number 2012.1.00900.S;

^(a2)

ALMA project number 2017.1.0659.S;

^(b)

number of 12 m-antennas in the array;

^(c)

amount of precipitable water vapour in the atmosphere;

^(d)

on-source time;

^(e)

respectively minimum and maximum projected baseline;

^(f)

flux density at 350 GHz, as retrieved from the ALMA flux monitoring database.

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