Fig. 17
Similar to Fig. 16, but for MUSE IDs 942 (z = 2.575) and 7382 (z = 1.094). The extracted spectra clearly show that there are at least two objects lying on the same sight line. A small offset is also seen between the narrowband images of the C iv absorption feature at z = 2.575 and [O ii] at z = 1.094. However, there is no obvious HST object to provide the counterpart for the [O ii] emitter.
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