Fig. 4
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A comparison of the PV arrays from X-shooter (left) and MUSE (right) for the Hα line. The X-shooter spectra have been degraded to match the resolution of MUSE. The contours are on a log scale corresponding to log Fλ = [−17.4, −17.2, −16.9, −16.6, −16.4, −16.0, −15.7] for the X-shooter data and log Fλ = [−18.8, −18.6, −18.3, −18.0, −17.7, −17.4, −17.0] for the MUSE data.
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