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The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300deg^2 of the celestial sphere in twelve optical bands using a dedicated 0.8 mrobotic telescope, the T80-South, at the Cerro Tololo Inter-AmericanObservatory, Chile. The telescope is equipped with a 9.2k by 9.2k e2v detectorwith 10 um pixels, resulting in a field-of-view of 2 deg^2 with a plate scaleof 0.55"/pixel. The survey consists of four main subfields, which include twonon-contiguous fields at high Galactic latitudes (8000 deg^2 at |b| > 30 deg)and two areas of the Galactic plane and bulge (for an additional 1300 deg^2).S-PLUS uses the Javalambre 12-band magnitude system, which includes the 5 u, g,r, i, z broad-band filters and 7 narrow-band filters centered on prominentstellar spectral features: the Balmer jump/[OII], Ca H+K, H-delta, G-band, Mg btriplet, H-alpha, and the Ca triplet. S-PLUS delivers accurate photometricredshifts (delta_z/(1+z) = 0.02 or better) for galaxies with r < 20 AB mag andredshift < 0.5, thus producing a 3D map of the local Universe over a volume ofmore than 1 (Gpc/h)^3. The final S-PLUS catalogue will also enable the study ofstar formation and stellar populations in and around the Milky Way and nearbygalaxies, as well as searches for quasars, variable sources, andlow-metallicity stars. In this paper we introduce the main characteristics ofthe survey, illustrated with science verification data highlighting the uniquecapabilities of S-PLUS. We also present the first public data release of ~336deg^2 of the Stripe-82 area, which is available athttp://datalab.noao.edu/splus.

The Southern Photometric Local Universe Survey (S-PLUS): improved SEDs, morphologies and redshifts with 12 optical filters