The inhomogeneous ISM toward PKS 1830–211 SW: A detailed view of molecular gas at a look-back time of 7.5 Gyr

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Volume 574 (February 2015)

A&A, 574 (2015) A108

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Table 3

CS J = 1←0 one component Gaussian fit parameters.

Epoch	^∫(T_L/T_c)dV	V _LSR	ΔV
	(km s^-1)

Dec. 15, 2001	–4.43 ± 0.07	10.6 ± 0.2	23.5 ± 0.5
Dec. 22, 2001	–4.42 ± 0.11	09.8 ± 0.3	24.9 ± 0.8
Dec. 30, 2001	–4.38 ± 0.05	11.3 ± 0.1	22.1 ± 0.3
Mar. 11, 2002	–4.76 ± 0.05	09.6 ± 0.1	26.4 ± 0.3
Sep. 27, 2002	–4.42 ± 0.06	11.0 ± 0.1	23.4 ± 0.4
Jan. 05, 2003	–3.57 ± 0.04	11.5 ± 0.1	19.1 ± 0.2
Mar. 18, 2006	–3.13 ± 0.04	10.9 ± 0.1	15.5 ± 0.2
Apr. 01. 2011	–3.32 ± 0.04	09.9 ± 0.1	18.3 ± 0.3
Dec. 08, 2011	–4.28 ± 0.03	10.3 ± 0.1	19.4 ± 0.1
Apr. 08, 2012	–4.60 ± 0.02	10.1 ± 0.1	20.0 ± 0.1

Notes. Adopted redshifted frequency: ν = 25.978596 GHz. The absorption peak is slightly (typically 1.0–2.5 km s^-1) blueshifted with respect to the velocities given in Col. 3, caused by the asymmetry in the overall lines (Fig. 3). For integrated optical depths, see Fig. 4.

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