Table 3: Small Magellanic Cloud atomic column densities for Na I, Ca II and Ti II derived via the construction of apparent column density velocity profiles and subsequent line profile integration (v  80-200 km s^-1). The error in log N is 0.02 dex for Ti II and Ca II K, and 0.03-0.04 dex for the more saturation sensitive Na I D line. Line transition wavelengths and oscillator strengths are adopted from Morton (2003). For both Na I and Ca II the individual doublet line column densities are given, as well as the "optical depth - velocity'' corrected column densities (see text for details).

	Column density log N (cm-2)
	Na I				Ca II				Ti II
	D1	D2	corr		K	H	corr
AzV 456	12.41	12.17	12.98		12.34	12.51	12.73		12.39
AzV 18	12.63	12.48	12.72		12.94	12.92	12.94		12.95
AzV 214	12.73	12.55	12.95		12.81	12.90	12.97		12.86
AzV 398	12.88	12.69	13.17		13.17	13.14	13.17		13.16
AzV 65	12.37	12.27	12.48		13.06	13.16	13.25		13.24
Sk 191	12.28	11.98	12.3		12.19	12.23	12.24		12.17
AzV 242	12.09	12.01	12.17		12.72	12.74	12.74		12.64

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