Fig. 7
UDF Galaxy ID 13 at z = 0.9973. Same panels as Fig. 6. For this redshift, the Fe ii UV2 and UV3 multiplets are not fully covered in the MUSE spectral range. Like the galaxy ID 8 (Fig. 6), this galaxy appears to be face on but disturbed, and the spectrum shows Fe ii, Mg ii, and Mg i absorption features, with Fe ii* emission.
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