Fig. 1
Vacuum rest-frame 1D spectrum of the MUSE HDFS galaxy ID#13 covering the Fe ii and Mg ii transitions. The spectrum is in black with the 1σ error in magenta. Resonant transitions detected in absorption are labeled in blue. Non-resonant Fe ii* transitions detected in emission are labeled in red. The C ii] nebular emission, which is a blend of five transitions, is labeled in green.
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