Figure 5

KNO-scaled multiplicity distribution versus the KNO variable $N_{\rm ch}/\langle N_{\rm ch}\rangle$ in NSD p$-$Pb collisions at $\sqrt{s_{\rm NN}}=5.02$ TeV for various pseudorapidity intervals. Comparison with predictions from HIJING, DPMJET, PYTHIA 8/Angantyr, and the IP-Glasma model are shown. The ratios between models and data are calculated using a linear interpolation between adjacent points.