Notes. Column (1) lists the identification number as of Table 1, Col. (2) the HD identifier, the equivalent width in Col. (3) of the Ca II K and in Col. (4) of the Ca II H doublet used in Col. (5) for the distance estimate (Megier et al. 2009). Distances obtained from the Gaia parallax are listed in Col. (6) and from the spectral type-luminosity ratio in Col. (7). Appearance of single (S) or multiple (M) velocity components of profiles for the Ca II H and K, the Na I, and the K I lines in Cols. (8–10). The fit parameters of the K I line profile are listed for the position, the column density, and the derived equivalent width in Cols. (11–13). Column (14) lists the classification of cloud environment as cold (c) or warm (w) with or without a CN I detection. Column (15) lists the infrared morphology of the WISE (W4) image. Single-cloud sightlines are highlighted in boldface. ^(LR) low-resolution spectrum has insufficient resolving power for classification as single-cloud sightline, ^(l) saturated line, ^(v) ignored because lines have different velocities, ^(e)WISE image shows artefact. For the complete list, see Table A.3.