Fig. 6

image

UDF Galaxy ID 8 at z = 1.0948. Top row: sections of the MUSE spectrum with the UV2 and UV3 Fe ii multiplets (Fe iiλ2344, Fe ii*λ2365, Fe iiλλ2374,2382 and Fe ii*λ2396), the UV1 Fe ii multiplet (Fe iiλλ2586,2600 and Fe ii*λ2612,2626), and Mg iiλλ2796,2803 with Mg iλ2852. The blue (purple) dashed lines indicate the resonant Fe ii (Mg ii) transitions, and the red dashed lines show the non-resonant Fe ii* emission. Bottom row: HST F775W image and the MUSE [O ii] λ3729 flux map with an asinh scale, along with the corresponding MUSE S/N map with a threshold of S/N> 10. This galaxy is large and face-on. The spectrum shows Fe ii, Mg ii, and Mg i absorption features, with Fe ii* emission.

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