Open Access

Fig. A.11.

image

J1314+0543: There is a clear detection of Na I D in this system. The spectrum is affected by a spike near Na Iλ5897, thus we fit the Na Iλ5891 line and show the corresponding Na Iλ5897 line. The EW values in Table 2 are from the VPFIT fit. There is not apparent detection of Ca II and we give upper limits on EW. There are two strong components at υ = 0, 160 km s−1 in the Fe II, Si II, C I, and Mg I absorption profiles. The spike in the spectrum could be due at least partly to Na Iλ5891 in the second component, the corresponding Na Iλ5897 being affected by a residual from sky subtraction. We detect Zn II, Mn II and Ni II, with depletion factor [Fe/Zn] = −0.95 ± 0.05.

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