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Table 1.

The sample and some of its properties.

ID r25 PA cz d vc
zc1 Disc structure
H I data This paper
(″) (°) (km s−1) (Mpc) (km s−1) (km s−1) (″)
ESO 157-49 52.1 30.4 1656 17.3 99 107 6.1 Well defined thin and thick disc
ESO 443-21 36.9 160.8 2819 52.2 164 196 No distinct thin and thick disc
ESO 469-15 55.9 149.2 1636 28.3 104 83 4.8 Well defined thin and thick disc
ESO 544-27 46.5 153.3 2454 45.9 125 129 4.0 Well defined thin and thick disc
IC 217 59.9 35.7 1890 21.1 104 115 5.4 Well defined thin and thick disc
IC 1553 40.5 15.0 2905 36.5 128 142 5.0 Well defined thin and thick disc
PGC 28308 59.9 125.2 2719 43.1 180 130 Well defined thin and thick disc; the
thin disc dominates at all heights
PGC 30591 45.4 169.2 2028 35.5 122 97 No distinct thin and thick disc

Notes. Position angle (PA) values from Salo et al. (2015). Heliocentric recession velocities (cz) from the NED except for ESO 157-49 and IC 1553 where we estimated cz by making the amplitude of the stellar rotation curve in the midplane roughly similar for the approaching and the receding sides. Distance estimates (d) from Tully et al. (2008, 2016). H I circular velocity values (vc) from Mathewson & Ford (1996), Theureau et al. (2006), and Courtois et al. (2009). The vc values as estimated in this paper come from fitting Eq. (2) to the midplane line emission curves extracted from the maps in Figs. A.1A.8 (see also Fig. 2). The heights above which the thick disc dominates in S4G images (zc1) are from Comerón et al. (2018) and so are the disc structure descriptions.

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