Accretion luminosity as a function of stellar luminosity for the Taurus sample studied in this work. The position of heavily spotted sources, with Teff and L_* based on the 2 Teff fit, is shown as red points, and the positions obtained assuming a single Teff are shown as blue points. The position of sources without evidence of spots is shown as black points. Differences between the two methods are within the averaged errors in L_* and do not affect the L_acc − L_* distribution.