Fig. A.15.
J2336−1058: For this system, the Ca II doublet is lost in strong sky absorption features. We detect Na I D. The Na Iλ5891 line is slightly blended with a sky absorption, which is subtracted to derive EW. The C I absorptions are not very strong but we can see two components. The Zn II line is detected and we derive a depletion factor [Fe/Zn] = −1.11 ± 0.10.
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