The Study of Nebular Emission on Nearby Spiral Galaxies in the IFU Era
Figure 1
(a) Examples of the PINGS IFS mosaics, each panel shows a -band Digital Sky Survey image of the galaxy with the PPAK mosaic pointings as overlaid hexagons indicating the FoV of the central fibre bundle. (b) Examples of the face-on spirals drawn from the Mármol-Queraltó et al. [21] sample of IFS galaxies, each panel shows a colour-composite SDSS image of the galaxy with the PPAK FoV footprint overlaid.
