Top: from left to right, SDSS image of NGC 5056 with the PPAK aperture superimposed on scale; two-dimensional maps of the extinction-corrected Hα flux and the velocity measured from the Hα-line shift. Bottom: from left to right, two-dimensional maps of the contribution of the young stars (<100 Myr) to the total luminosity, the light-weighted average stellar age, and the extinction (A_V). In all 2D maps with IFS data, × determines the galaxy center and + the SN position. The contour levels overplotted on the maps are derived from the Hα flux map. The x − y coordinates are in arcsec with respect to the center of the FoV. The orientation of the images is north up, east left.