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Fig. 2.
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[OIII] flux maps for NGC 1796, using rebinned (degraded) data. The first three panels from the left show: bin size = 120 pc, 100 pc, 60 pc. The last panel shows the same [OIII] flux using the unbinned data. Each panel shows the 1′ × 1′ field of view of MUSE.
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