The normalized correction factors, $\epsilon$, for each reconstruction method for $\pi^{0}$ (left) and $\eta$ mesons (right) plotted versus \pT bins used in the analysis The factors contain the detector acceptances and the respective reconstruction efficiencies, where acceptances are further normalized by the rapidity windows accessible with each method, $\Delta y$, and full azimuth coverage of $2\pi$, in order to enable a direct comparison between the different methods. | ![](https://alice-publications.web.cern.ch/sites/default/files/papers/3716/Pi0_AcceptanceTimesEff_incPHOS-88518.png ) ![](https://alice-publications.web.cern.ch/sites/default/files/papers/3716/Eta_AcceptanceTimesEff-88522.png ) |