Open Access

Fig. A.3.


J0854+0317: The Ca II K line is detected in this system, when the Ca II H line is lost in the noise. The spectrum around the expected position of Na I D is relatively good but no absorption is seen down to 0.23 Å. There is a slight shift of ~−25 km s−1 between the strongest component of Fe II and Si II and the strongest C Iλ1656 component. The C Iλ1560 line is blended with other lines at ~−125 km s−1 and 400 km s−1. Weak lines of Zn II and Mn II are detected.

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