J1341+1852: This system is peculiar as it turns out to be a sub-DLA, with column density log N(HI) = 18.18 ± 0.05. The C I and other metal line absorptions are weak, with C Iλ1560 equivalent width ~0.13 Å (well below the mean EW = 0.38,Å in the sample), and W(Mg IIλ2798) = 0.33 Å (for a mean EW = 2.76 Å in the sample). The metallicity is high with [OI/HI] = +0.36, relative to solar. It might be interesting to derive the physical properties of this gas and in particular its ionization state. Indeed, it is surprising to detect C I in such a system. This is, however, out of the scope of the present paper. There are no obvious detections of either Ca II H&K or Na I D. We give EW upper limits for the lines.
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