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Table A.3

Column densities of H i, Ca ii, Ti ii, and Mn ii for DLAs and sub-DLAs from the sample of Guber & Richter (2016).

QSO-sightline zabs log N(H i) log N(Ca ii) log N(Ti ii) log N(Mn ii)

J095456+174331 0.23782 21.32a 12.21±0.03 12.57±0.05 12.89±0.05
J113007144927 0.31271 21.71b 12.59±0.02 12.76±0.04 13.16±0.02
J123200022404 0.39498 20.6c 12.40±0.02 12.36±0.05 13.29±0.02
J045608215909 0.47439 19.5d 12.23±0.02 11.83±0.05 12.53±0.02

Additional Ca ii systems with upper limits for N(Mn ii)

J124646254749 0.49282 12.77±0.08 <11.93 <12.33
J220743534633 0.43720 12.00±0.07 <11.50 <11.95
J051707441055 0.42913 10.48±0.06 <10.20 <10.54
J232820+002238 0.41277 11.52±0.08 <11.14 <11.64
J224752123719 0.40968 12.27±0.04 <11.34 <12.00
J050112015914 0.40310 12.35±0.05 <12.08 <12.47
J110325264515 0.35896 11.25±0.04 <10.55 <12.17
J142253000149 0.34468 12.35±0.05 <11.88 <12.02
J231359370446 0.33980 12.54±0.03 <12.19 <12.31
J102837010027 0.32427 12.50±0.03 <11.68 <12.11

Notes.

(*)

This absorption line system is the multicomponent DLA toward PKS 1127144 at zabs = 0.31271 studied in this paper. The given column densities for this absorber (for Ca ii, Ti ii, and Mn ii), each, are summed over the six components as given in the last row of Table 1.

Reference.

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