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Table 1

Intersections of clouds towards targets.

Target Na I Ca II K I
HD 36982 S M S
HD 37367 dS
HD 37903 Ma M
HD 38087 M
HD 75309 dS dS dS
HD 79186 S dS S
HD 91824 dS M dS
HD 91983 M
HD 93205 M M M
HD 94493 dS M dS
HD 103779 Ma M M
HD 104705 M M M
HD 112272 M M M
HD 122879 M
HD 129557 S S
HD 147888 S S
HD 147889 S
HD 148379 M M
HD 149404 M M
HD 151804 M M M
HD 152235 M dS M
HD 152249 dS M dS
HD 152408 M M
HD 152424 dS
HD 154368 dS dS M
HD 164740 S
HD 169454 M dS
HD 170740 S dS S
HD 203532 S S S
HD 210121 S dS S
HD 303308 M
CPD 63 2495 M M

Notes. We distinguish Na I, Ca II and K I lines into single (“S”), dominated by a single (“dS”), and multiple component (“M”) profiles. Stars observed through sight-lines with a single dust cloud are highlighted with boldface fonts. (a)Low signal-noise spectra.

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