Fig. 5
Top panel: comparison between g-band images extracted from CALIFA datacubes of the galaxy NGC 5406 (ID=684) created using the V2.2 (DR3) and V1.5 (DR2) pipelines, together with the corresponding SDSS image convolved with a Gaussian function to match the spatial resolution of the CALIFA datacubes. Bottom panel: similar comparison between Hα images extracted from the same datacubes using the Pipe3D pipeline, and a resolution-matched Hα image taken with the 4.2 m William Herschel Telescope (Roque de los Muchachos Observatory, La Palma, Spain), using the AUXCAM detector (Sánchez-Menguiano et al., in prep.). The FoV has been reduced to match that of CALIFA.
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