the Stripe 82 equatorial field, observed with the T80S, a 0.8m robotic telescope with a wide of $\sim 1.8$ deg$^{\text{2}}$, located in Cerro Tololo, Chile. The DR1 data are already reduced and are publicly available in the NSF’s National Optical-Infrared Astronomy Research Laboratory archive[^1]. Details about the survey strategy and data reduction process are described by @2019MNRAS.489..241M while the photometric calibration is described in Sampedro et al. (in prep.).

The main survey strategy is aimed at obtaining large coverage of the Southern sky ($\sim 9000$ deg$^{\text{2}}$) for astronomical and cosmological studies in the local universe. The S-PLUS uses the same photometric system of the J-PLUS survey [@2012SPIE.8450E..3SM], which consists of twelve optical bands, including 5 broad-bands similar to those used by the $ugriz$ system, and a set of seven narrow-band ($\Delta\lambda= 100-200$) filters placed at various rest-frame optical features, including \[OII\] ($\lambda_{\text{eff}}=3771$ ), Ca H+K ($\lambda_{\text{eff}}=3941$ ), H$\delta$ ($\lambda_{\text{eff}}=4094$ ), G-band ($\lambda_{\text{eff}}=4292$ ), Mg $b$ triplet ($\lambda_{\text{eff}}=5133$ ), H$\alpha$ ($\lambda_{\text{eff}}=6614$ ) and the Ca triplet ($\lambda_{\text{eff}}=8611$ ). Considering a threshold of 3, the survey is complete in the broad bands to magnitudes of $u=21.07$, $g=21.79$, $r=21.6$, $i=21.22$ and $z=20.64$, whereas it is complete to magnitudes of $\sim20.4$ in all narrow 