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Here we describe the \emph{Siding Spring Southern Seyfert SpectroscopicSnapshot Survey} (S7) and present results on 64 galaxies drawn from the firstdata release. The S7 uses the Wide Field Spectrograph (WiFeS) mounted on theANU 2.3m telescope located at the Siding Spring Observatory to deliver anintegral field of $38\times25$~ arcsec at a spectral resolution of $R=7000$ inthe red ($530-710$nm), and $R=3000$ in the blue ($340-560$nm). {From these datacubes we have extracted the Narrow Line Region (NLR) spectra from a 4 arc secaperture centred on the nucleus. We also determine the H$\beta$ and[OIII]~$\lambda$5007 fluxes in the narrow lines, the nuclear reddening, thereddening-corrected relative intensities of the observed emission lines, andthe H$\beta$ and \lOIII\ luminosities {determined from spectra for which thestellar continuum has been removed.} We present a set of images of the galaxiesin [OIII]~$\lambda$5007, [NII]~$\lambda$6584 and H$\alpha$ which serve todelineate the spatial extent of the extended narrow line region (ENLR) and {\bfalso to} reveal the structure and morphology of the surrounding \HII\ regions.Finally, we provide a preliminary discussion of those Seyfert~1 and Seyfert~2galaxies which display coronal emission lines in order to explore the origin ofthese lines.

Probing the Physics of Narrow Line Regions in Active Galaxies II: The Siding Spring Southern Seyfert Spectroscopic Snapshot Survey (S7)