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Table A.4

Data relating the absorption structure complexity and the absorber galaxy connection.

QSO sightline zabs Comp. nr. ΔvCaII λ3934 Imp. par. d Ref.
[km s−1] [kpc]
Sample A/Class 1

J095456+174331 0.23782 4 105 <4.8 a
J235731112539 0.24763 3 53
J113007144927 0.31273 8 230 18.5 b
J123200022404 0.39498 5 111 6.6 c
J045608215909 0.47439 4 102
Q0118-272 0.558 10.7 d
Sample B

J121509+330955 0.00396 3 149 9.7 e
J133007205616 0.01831 9 378
J215501+092224 0.08091 1 38 36.5 f
J012517001828 0.23864 1 22
J000344232355 0.27051 2 42
J142249272756 0.27563 1 29
J042707130253 0.28929 2 122
J102837010027 0.32427 2 143
J110325264515 0.35896 1 31
J121140+103002 0.39293 1 30
J050112015914 0.40310 3 103
J224752123719 0.40968 2 101
J220743534633 0.43720 1 26
J044117431343 0.44075 3 60
J144653+011356 0.44402 1 42
Other systems

J044117431343 0.10114 7 130 7.9 g
J231359370446 0.33980 3 41
J094253110426 0.39098 2 31

Notes. Redshifts, component number and velocity widths of the Ca ii λ3934 are from Richter et al. (2011). The last column includes the references for impact parameters (calculated from angles using λCDM cosmology and the cosmological parameters from Planck Collaboration XVI (2014) listed in Sect. 2.2.

Reference. (a) Rao et al. (2003); (b) Lane et al. (1998); (c) Le Brun et al. (1996); Vladilo et al. (1997); (e) Miller et al. (1999); (f) Jenkins et al. (2003); (g) Chen et al. (2004).

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