Erratum: Signature of Energy Losses on the Cosmic Ray Electron Spectrum [Phys. Rev. Lett. 125, 051101 (2020)]

Figure 1

Left: energy loss timescale for CREs as a function of energy during their propagation in the Galaxy. The timescales are multiplied by $E$ to give prominence to the deviations from the standard $b\propto E^2$ regime (reproduced from [5]). Right: electron flux from SNRs is shown with a red dashed line, and the total flux of electrons (including pulsars and secondary products of CR interactions) with a red solid line. The total flux obtained neglecting the KN effect (dash-dotted green line) is also shown (reproduced from [5]).