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.