The role of molecular gas in the nuclear regions of IRAS 00183-7111 - ALMA and X-ray investigations of an ultraluminous infrared galaxy

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Volume 616 (August 2018)

A&A, 616 (2018) A127

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Table 1.

Summary of the properties of the ALMA Cycle 0 observations.

Band	Observation date	Sky frequency coverage (GHz)	Time on target^a (min)	Flux calibrator	PWV^b (mm)	Tsys^c (K)	Number of antennas (12 m)
B3	18/12/2012	86–88/96–98	45.9	Neptune	3.4	70	25
B3	18–19/12/2012		16.1	Callisto	3.6	70	25
B3	31/12/2012		16.1	Neptune	1.9	60	24
B6	29/12/2011	257–259/272–274	31.4	Neptune	1.15	100	14
B6	13/01/2012		31.4	Neptune	1.6	110	17
B6	23/01/2012		27.22	Neptune	2	110	17
B6	23/01/2012		27.22	Neptune	2.2	130	17
B6	26/11/2011	253–255/266–268	24.7	Callisto	1.5	100	18
B6	28/11/2011		23.8	Neptune	2	110	14
B6	10/01/2012		24.7	Neptune	4.2	170	17
B6	13/01/2012		24.7	Neptune	3.3	150	17

Notes. The upper panel shows the properties of Band 3 (B3) observations are unpublished, Band 6 (B6) data were previously analysed by Imanishi & Nakanishi (2014).

^(a)

Total integration time on the science target.

^(b)

Median Amount of Precipitable Water Vapour (PWV) quantified during the observation time.

^(c)

System Temperature (T_sys) median value recorded in each run.

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