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VENGA is a large-scale extragalactic IFU survey, which maps the bulges, barsand large parts of the outer disks of 32 nearby normal spiral galaxies. Thetargets are chosen to span a wide range in Hubble types, star formationactivities, morphologies, and inclinations, at the same time of having vastavailable multi-wavelength coverage from the far-UV to the mid-IR, andavailable CO and 21cm mapping. The VENGA dataset will provide 2D maps of theSFR, stellar and gas kinematics, chemical abundances, ISM density andionization states, dust extinction and stellar populations for these 32galaxies. The uniqueness of the VIRUS-P large field of view permits theselarge-scale mappings to be performed. VENGA will allow us to correlate allthese important quantities throughout the different environments present ingalactic disks, allowing the conduction of a large number of studies in starformation, structure assembly, galactic feedback and ISM in galaxies.

The VIRUS-P Exploration of Nearby Galaxies (VENGA): Survey Design and First Results