These are four example H i spectra taken at the coordinates of WiFeS fields in the SMC. The H i data are from Staveley-Smith et al. (1995, 1997) and Stanimirović et al. (1999, 2004). The spectra are drawn from a data cube with a 98 arcsec beam, so around three times bigger on a side than the WiFeS field. The zero of radial velocity for the SMC has been set as 157 km s|$^{-1}$| based on the distribution of our WiFeS fields. The dashed line in each plot is the radial velocity of the H |$\alpha$| line for the corresponding WiFeS field. The green line is the Gaussian fit to H i emission line linked to the H |$\alpha$| line. The spectra are organized by increasing Right Ascension. Top left has coordinates R.A. = 11|$_{.}^{\circ }$|658 Dec. = |$-73_{.}^{\circ }$|377, top right R.A. = 12|$_{.}^{\circ }$|702 Dec. = |$-73_{.}^{\circ }$|348, bottom left R.A. = 15|$_{.}^{\circ }$|842 Dec. = |$-72_{.}^{\circ }$|060, and bottom right R.A. = 18|$_{.}^{\circ }$|961 Dec. = |$-73_{.}^{\circ }$|182.