Photo-z performance of the J-PLUS filter system. Left: the figure shows an example of the SED-fitting for an early-type cluster galaxy. Inner-panel shows the PDF computed by the BPZ code. Right: the figure shows the obtained accuracy as a function of the cumulative r magnitude. Gray vertical bars represent the fraction of the galaxies per magnitude bin. Globally, this sample yields an accuracy of δ_z/(1 + z) ~ 1.0% with an averaged magnitude ⟨r⟩ = 16.6. A precision of δ_z/(1 + z) = 0.005 is obtained for the 177 galaxies brighter than magnitude r < 17, showing the enormous potential of this technique to study the nearby galaxies.