Top panel : comparison of the Raa as a function of <Npart>, integrated in rapidity, measured at $\sqrt{s_{NN}}$= 5.02 TeV for several $p_T$ ranges with theory. Bottom panel : comparison of the Raa ratios as a function of <Npart>, integrated in rapidity, measured at $\sqrt{s_{NN}}$= 5.02 TeV and $\sqrt{s_{NN}}$= 2.76 TeV for several $p_T$ ranges with theory. The error bars represent the statistical uncertainties, the boxes around the data points the uncorrelated systematic uncertainties, while the correlated global uncertainties are shown as filled boxes around 1. The brackets shown in the three most peripheral centrality intervals in the range $0.3<p_T<2$ represent the range of variation of the hadronic J/psi Raa under extreme hypothesis on the photo-production contamination on the inclusive Raa.
Top panel : comparison of the Raa as a function of <Npart>, integrated in rapidity, measured at $\sqrt{s_{NN}}$= 5.02 TeV for several $p_T$ ranges with theory. Bottom panel : comparison of the Raa ratios as a function of <Npart>, integrated in rapidity, measured at $\sqrt{s_{NN}}$= 5.02 TeV and $\sqrt{s_{NN}}$= 2.76 TeV for several $p_T$ ranges with theory. The error bars represent the statistical uncertainties, the boxes around the data points the uncorrelated systematic uncertainties, while the correlated global uncertainties are shown as filled boxes around 1. The brackets shown in the three most peripheral centrality intervals in the range $0.3<p_T<2$ represent the range of variation of the hadronic J/psi Raa under extreme hypothesis on the photo-production contamination on the inclusive Raa.