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Fig. 6


Similar to Fig. 5, but for a quality B (confidence 3) object (MUSE-Wide ID 107021114, strongest line in S/N is O ii). Only one emission line is detected above the detection threshold, but other lines are clearly visible in the LSDCat generated S/N cube and in the flux datacube. In this object the [O iii] λ5007 line falls on a sky emission line (as can bee seen by the increased noise level in the bottom right panel), so its S/N is lower compared to the intrinsically weaker [O iii] λ4959 line.

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