Mean $p_T$ values of the $\Upsilon(1$S$)$, $\Upsilon(2$S$)$, and $\Upsilon(3$S$)$ states with $p_T\,>\,0\,GeV$ and $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$

Ratio $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $0<p_T<5\,$GeV range

Ratio $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $5<p_T<7\,$GeV range

Ratio $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $7<p_T<9\,$GeV range

Ratio $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $9<p_T<11\,$GeV range

Ratio $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $11<p_T<15\,$GeV range

Ratio $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $15<p_T<20\,$GeV range

Ratio $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $20<p_T<50\,$GeV range

Ratio $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $0<p_T<5\,$GeV range

Ratio $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $5<p_T<7\,$GeV range

Ratio $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $7<p_T<9\,$GeV range

Ratio $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $9<p_T<11\,$GeV range

Ratio $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $11<p_T<15\,$GeV range

Ratio $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $15<p_T<20\,$GeV range

Ratio $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ with $|y|\,<\,1.2$ as a function of track multiplicity $N_{track}$ in $20<p_T<50\,$GeV range

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of "forward" track multiplicity $N_{track}^{\Delta\phi}$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$. Forward tracks are those with momentum direction in $\Delta\phi\,<\,\pi/3$ w.r.t. the $\Upsilon(n$S$)$ momentum direction.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of "transverse" track multiplicity $N_{track}^{\Delta\phi}$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$. Transverse tracks are those with momentum direction in $\pi/3\,<\,\Delta\phi\,<\,2\pi/3$ w.r.t. the $\Upsilon(n$S$)$ momentum direction.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of "backward" track multiplicity $N_{track}^{\Delta\phi}$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$. Backward tracks are those with momentum direction in $\Delta\phi\,>\,2\pi/3$ w.r.t. the $\Upsilon(n$S$)$ momentum direction.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$ and $N^{\Delta R}_{track}\,=\,0$ charged particles produced in $\Delta R\,<\,0.5$ cone around $\Upsilon(n$S$)$ momentum direction.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$ and $N^{\Delta R}_{track}\,=\,1$ charged particles produced in $\Delta R\,<\,0.5$ cone around $\Upsilon(n$S$)$ momentum direction.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$ and $N^{\Delta R}_{track}\,=\,2$ charged particles produced in $\Delta R\,<\,0.5$ cone around $\Upsilon(n$S$)$ momentum direction.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$ and $N^{\Delta R}_{track}\,>\,2$ charged particles produced in $\Delta R\,<\,0.5$ cone around $\Upsilon(n$S$)$ momentum direction.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ in transverse sphericity bin $0.00\,<\,S_T\,<\,0.55$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ in transverse sphericity bin $0.55\,<\,S_T\,<\,0.70$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ in transverse sphericity bin $0.70\,<\,S_T\,<\,0.85$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$.

Ratios $\Upsilon(2$S$)\,/\,\Upsilon(1$S$)$ and $\Upsilon(3$S$)\,/\,\Upsilon(1$S$)$ as functions of track multiplicity $N_{track}$ in transverse sphericity bin $0.85\,<\,S_T\,<\,1.00$ for $\Upsilon(n$S$)$ states with $p_T\,>\,7\,GeV$ and $|y|\,<\,1.2$.

Efficiency-corrected multiplicity bins used in the $\Upsilon(n$S$)$ ratio analysis and the corresponding mean number of charged particle tracks.

Fig. 2. (Color online.) Event-by-event photon multiplicity distributions (solid circles) for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{s_{\mathrm{NN}}}=62.4$ and $200 \mathrm{GeV} .$ The distributions for top $0-5 \%$ central $\mathrm{Au}+$ Au collisions and top $0-10 \%$ central $\mathrm{Cu}+\mathrm{Cu}$ collisions are also shown (open circles). The photon multiplicity distributions for central collisions are observed to be Gaussian (solid line). Only statistical errors are shown. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 2. (Color online.) Event-by-event photon multiplicity distributions (solid circles) for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{s_{\mathrm{NN}}}=62.4$ and $200 \mathrm{GeV} .$ The distributions for top $0-5 \%$ central $\mathrm{Au}+$ Au collisions and top $0-10 \%$ central $\mathrm{Cu}+\mathrm{Cu}$ collisions are also shown (open circles). The photon multiplicity distributions for central collisions are observed to be Gaussian (solid line). Only statistical errors are shown. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 2. (Color online.) Event-by-event photon multiplicity distributions (solid circles) for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{s_{\mathrm{NN}}}=62.4$ and $200 \mathrm{GeV} .$ The distributions for top $0-5 \%$ central $\mathrm{Au}+$ Au collisions and top $0-10 \%$ central $\mathrm{Cu}+\mathrm{Cu}$ collisions are also shown (open circles). The photon multiplicity distributions for central collisions are observed to be Gaussian (solid line). Only statistical errors are shown. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 3. (Color online.) Photon pseudorapidity distributions for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{\mathrm{s}_{\mathrm{NN}}}=62.4$ and $200\mathrm{GeV}$. The results for several centrality classes are shown. The solid curves are results of HIJING simulations for central $(0-5 \%$ for $\mathrm{Au}+\mathrm{Au}$ and $0-10 \%$ for $\mathrm{Cu}+\mathrm{Cu})$ and $30-40 \%$ mid-central collisions. The errors shown are systematic, statistical errors are negligible in comparison. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 3. (Color online.) Photon pseudorapidity distributions for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{\mathrm{s}_{\mathrm{NN}}}=62.4$ and $200\mathrm{GeV}$. The results for several centrality classes are shown. The solid curves are results of HIJING simulations for central $(0-5 \%$ for $\mathrm{Au}+\mathrm{Au}$ and $0-10 \%$ for $\mathrm{Cu}+\mathrm{Cu})$ and $30-40 \%$ mid-central collisions. The errors shown are systematic, statistical errors are negligible in comparison. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 3. (Color online.) Photon pseudorapidity distributions for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{\mathrm{s}_{\mathrm{NN}}}=62.4$ and $200\mathrm{GeV}$. The results for several centrality classes are shown. The solid curves are results of HIJING simulations for central $(0-5 \%$ for $\mathrm{Au}+\mathrm{Au}$ and $0-10 \%$ for $\mathrm{Cu}+\mathrm{Cu})$ and $30-40 \%$ mid-central collisions. The errors shown are systematic, statistical errors are negligible in comparison. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 3. (Color online.) Photon pseudorapidity distributions for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{\mathrm{s}_{\mathrm{NN}}}=62.4$ and $200\mathrm{GeV}$. The results for several classes are shown. The solid curves are results of HIJING simulations for central $(0-5 \%$ for $\mathrm{Au}+\mathrm{Au}$ and $0-10 \%$ for $\mathrm{Cu}+\mathrm{Cu})$ and $30-40 \%$ mid-central collisions. The errors shown are systematic, statistical errors are negligible in comparison. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 4. (Color online.) Top panel: The number of photons divided by $\left\langle N_{\text{part}}\right\rangle / 2$ as a function of average number of participating nucleons for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{\mathrm{s} _{\mathrm{NN}}}=62.4$ and $200 \mathrm{GeV}$ for $-3.7<\eta<-2.3 .$ Errors shown are systematic only and include those for $\left\langle N_{\text {part }}\right\rangle .$ Results from HIJING are shown as lines (solid for $\mathrm{Au}+\mathrm{Au}$ and dashed for $\mathrm{Cu}+\mathrm{Cu}$ ). Bottom panel: Same as above, for both photons and charged particles from PHOBOS [10]. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 4. (Color online.) Top panel: The number of photons divided by $\left\langle N_{\text{part}}\right\rangle / 2$ as a function of average number of participating nucleons for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ at $\sqrt{\mathrm{s} _{\mathrm{NN}}}=62.4$ and $200 \mathrm{GeV}$ for $-3.7<\eta<-2.3 .$ Errors shown are systematic only and include those for $\left\langle N_{\text {part }}\right\rangle .$ Results from HIJING are shown as lines (solid for $\mathrm{Au}+\mathrm{Au}$ and dashed for $\mathrm{Cu}+\mathrm{Cu}$ ). Bottom panel: Same as above, for both photons and charged particles from PHOBOS [10]. NOTE: For points with invisible error bars, the point size was considered as an absolute upper limit for the uncertainty.

Fig. 5. (Color online.) Photon pseudorapidity distributions normalized by the average number of participating nucleon pairs for different collision centralities are plotted as a function of pseudorapidity shifted by the beam rapidity (-5.36 for $200 \mathrm{GeV}$ and -4.19 for $62.4 \mathrm{GeV}$ ) for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ collisions at $\sqrt{s_{\mathrm{NN}}}=62.4$ and $200 \mathrm{GeV}$. Errors are systematic only, statistical errors are negligible in comparison. For clarity of presentation, results for only four centralities are shown. The $\mathrm{Cu}+$ Cu data are shifted by 0.1 unit in $\eta-y_{\text {beam }} .$ The solid line is a second order polynomial fit to the data (see text for details).

Fig. 5. (Color online.) Photon pseudorapidity distributions normalized by the average number of participating nucleon pairs for different collision centralities are plotted as a function of pseudorapidity shifted by the beam rapidity (-5.36 for $200 \mathrm{GeV}$ and -4.19 for $62.4 \mathrm{GeV}$ ) for $\mathrm{Au}+\mathrm{Au}$ and $\mathrm{Cu}+\mathrm{Cu}$ collisions at $\sqrt{s_{\mathrm{NN}}}=62.4$ and $200 \mathrm{GeV}$. Errors are systematic only, statistical errors are negligible in comparison. For clarity of presentation, results for only four centralities are shown. The $\mathrm{Cu}+$ Cu data are shifted by 0.1 unit in $\eta-y_{\text {beam }} .$ The solid line is a second order polynomial fit to the data (see text for details).

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 0-5% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 0-5% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and ZNA estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for CL1 estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for V0A estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for ZNAmult estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for ZNAPb estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions for 5 participant quarks as a function of the number of participants for CL1 estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions for 5 participant quarks as a function of the number of participants for V0A estimator.

Distribution of $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for NSD collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for NSD collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Estimation of $\mathrm{d}N_{\mathrm{ch}}/\mathrm{d}y$ for in the most central Pb-Pb collisions at $\sqrt{s_{_{\mathrm{NN}}}}=5.02\,\mathrm{TeV}$. Also shown is a fit of Gaussian distribution to the data.

Scaling behaviour as a function $\sqrt{s_{_{\mathrm{NN}}}}$ of the width of the charged-particle or -pion rapidity-density distribution with respect to the Landau-Carruthers width (top) and rapidity range (bottom). Charged-pion points from AGS and SPS are adapted from the literature [PRL94.162301], while the PHOBOS (filled crosses) [PRL91,052303] and BRAHMS (open crosses) [PRL88.202301] charged-hadron points are translated from the corresponding $\mathrm{d}N_{\mathrm{ch}}/\mathrm{d}\eta$ results.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 8000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 8000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for INEL collisions.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for NSD collisions.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for INEL>0 collisions.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Mean charged particle multiplicities in 3 pseudorapidity intervals in P P NSD collisions from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -0.5 to 0.5 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -1.0 to 1.0 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -1.5 to 1.5 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 8000 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Centrality dependence of moments of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Centrality dependence of $S\sigma$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV.

Centrality dependence of $S\sigma$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Centrality dependence of $S\sigma$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Centrality dependence of $S\sigma$ for $\Delta N_p$ in Au+Au collisions from Lattice QCD Calculations.

Centrality dependence of $S\sigma$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV from Transport Model Calculations.

Centrality dependence of $S\sigma$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV from Transport Model Calculations.

Centrality dependence of $S\sigma$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations for net-baryon.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations for net-proton (No Decay).

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

Centrality dependence of $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from Transport Model Calculations.

$\sqrt{s_{NN}}$ dependence of $\kappa\sigma^2$ for net proton distributions measured at RHIC. The results are STAR data.

$\sqrt{s_{NN}}$ dependence of $\kappa\sigma^2$ for net proton distributions measured at RHIC. The results are from UrQMD net-proton.

$\sqrt{s_{NN}}$ dependence of $\kappa\sigma^2$ for net proton distributions measured at RHIC. The results are from AMPT default net-proton.

$\sqrt{s_{NN}}$ dependence of $\kappa\sigma^2$ for net proton distributions measured at RHIC. The results are from AMPT String Melting net-proton.

$\sqrt{s_{NN}}$ dependence of $\kappa\sigma^2$ for net proton distributions measured at RHIC. The results are from Therminator net-proton.

$\sqrt{s_{NN}}$ dependence of $\kappa\sigma^2$ for net proton distributions measured at RHIC. The results are from Hijing net-proton.

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$\rm dN_{ch}/dy$ versus y distribution derived from the $\rm dN_{ch}/d\eta$ distribution along with pt distributions and particle ratios measured in ALICE. Errors are systematic.

The ratio of the standard deviation of the rapidity distribution of charged particles to that expected from Landau hydrodynamics versus versus $\sqrt{s}$/nucleon-pair. The standard deviation for data for all charged particles is derived from the $\rm dN_{ch}/d\eta$ distributions measured at various energies and converted to $\rm dN_{ch}/dy$ in a consistent manner. The data from the BRAHMS and PHOBOS experiments derived by the present authors from these experiments $dN/d\eta$ distributions.