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.

No description provided.

No description provided.

No description provided.

$\rm dN_{ch}/dy$ 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.

Extrapolation to the total number of charged particles as a function of the number of participating nucleons [PRC88.044909]. Data on the 0 to 30 PCT most central events are available in previous publication [PLB726.610].

The measured differential jet shape $\rho(r)$ for jets with 40 GeV $< p_{\mathrm{T}} <$ 50 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 50 GeV $< p_{\mathrm{T}} <$ 60 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 60 GeV $< p_{\mathrm{T}} <$ 70 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 70 GeV $< p_{\mathrm{T}} <$ 80 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 80 GeV $< p_{\mathrm{T}} <$ 90 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 90 GeV $< p_{\mathrm{T}} <$ 100 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 100 GeV $< p_{\mathrm{T}} <$ 110 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 110 GeV $< p_{\mathrm{T}} <$ 125 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 125 GeV $< p_{\mathrm{T}} <$ 140 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 140 GeV $< p_{\mathrm{T}} <$ 160 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 160 GeV $< p_{\mathrm{T}} <$ 180 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 180 GeV $< p_{\mathrm{T}} <$ 200 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 200 GeV $< p_{\mathrm{T}} <$ 225 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 225 GeV $< p_{\mathrm{T}} <$ 250 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 250 GeV $< p_{\mathrm{T}} <$ 300 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 300 GeV $< p_{\mathrm{T}} <$ 400 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 400 GeV $< p_{\mathrm{T}} <$ 500 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 500 GeV $< p_{\mathrm{T}} <$ 600 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 600 GeV $< p_{\mathrm{T}} <$ 1000 GeV and 0 <|y|< 0.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 20 GeV $< p_{\mathrm{T}} <$ 25 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 25 GeV $< p_{\mathrm{T}} <$ 30 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 30 GeV $< p_{\mathrm{T}} <$ 40 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 40 GeV $< p_{\mathrm{T}} <$ 50 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 50 GeV $< p_{\mathrm{T}} <$ 60 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 60 GeV $< p_{\mathrm{T}} <$ 70 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 70 GeV $< p_{\mathrm{T}} <$ 80 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 80 GeV $< p_{\mathrm{T}} <$ 90 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 90 GeV $< p_{\mathrm{T}} <$ 100 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 100 GeV $< p_{\mathrm{T}} <$ 110 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 110 GeV $< p_{\mathrm{T}} <$ 125 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 125 GeV $< p_{\mathrm{T}} <$ 140 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 140 GeV $< p_{\mathrm{T}} <$ 160 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 160 GeV $< p_{\mathrm{T}} <$ 180 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 180 GeV $< p_{\mathrm{T}} <$ 200 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 200 GeV $< p_{\mathrm{T}} <$ 225 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 225 GeV $< p_{\mathrm{T}} <$ 250 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 250 GeV $< p_{\mathrm{T}} <$ 300 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 300 GeV $< p_{\mathrm{T}} <$ 400 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 400 GeV $< p_{\mathrm{T}} <$ 500 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 500 GeV $< p_{\mathrm{T}} <$ 600 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 600 GeV $< p_{\mathrm{T}} <$ 1000 GeV and 0.5 <|y|< 1.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 20 GeV $< p_{\mathrm{T}} <$ 25 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 25 GeV $< p_{\mathrm{T}} <$ 30 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 30 GeV $< p_{\mathrm{T}} <$ 40 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 40 GeV $< p_{\mathrm{T}} <$ 50 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 50 GeV $< p_{\mathrm{T}} <$ 60 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 60 GeV $< p_{\mathrm{T}} <$ 70 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 70 GeV $< p_{\mathrm{T}} <$ 80 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 80 GeV $< p_{\mathrm{T}} <$ 90 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 90 GeV $< p_{\mathrm{T}} <$ 100 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 100 GeV $< p_{\mathrm{T}} <$ 110 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 110 GeV $< p_{\mathrm{T}} <$ 125 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 125 GeV $< p_{\mathrm{T}} <$ 140 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 140 GeV $< p_{\mathrm{T}} <$ 160 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 160 GeV $< p_{\mathrm{T}} <$ 180 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 180 GeV $< p_{\mathrm{T}} <$ 200 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 200 GeV $< p_{\mathrm{T}} <$ 225 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 225 GeV $< p_{\mathrm{T}} <$ 250 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 250 GeV $< p_{\mathrm{T}} <$ 300 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 300 GeV $< p_{\mathrm{T}} <$ 400 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 400 GeV $< p_{\mathrm{T}} <$ 500 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 500 GeV $< p_{\mathrm{T}} <$ 600 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 600 GeV $< p_{\mathrm{T}} <$ 1000 GeV and 1.0 <|y|< 1.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 20 GeV $< p_{\mathrm{T}} <$ 25 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 25 GeV $< p_{\mathrm{T}} <$ 30 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 30 GeV $< p_{\mathrm{T}} <$ 40 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 40 GeV $< p_{\mathrm{T}} <$ 50 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 50 GeV $< p_{\mathrm{T}} <$ 60 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 60 GeV $< p_{\mathrm{T}} <$ 70 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 70 GeV $< p_{\mathrm{T}} <$ 80 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 80 GeV $< p_{\mathrm{T}} <$ 90 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 90 GeV $< p_{\mathrm{T}} <$ 100 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 100 GeV $< p_{\mathrm{T}} <$ 110 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 110 GeV $< p_{\mathrm{T}} <$ 125 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 125 GeV $< p_{\mathrm{T}} <$ 140 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 140 GeV $< p_{\mathrm{T}} <$ 160 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 160 GeV $< p_{\mathrm{T}} <$ 180 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 180 GeV $< p_{\mathrm{T}} <$ 200 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 200 GeV $< p_{\mathrm{T}} <$ 225 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 225 GeV $< p_{\mathrm{T}} <$ 250 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 250 GeV $< p_{\mathrm{T}} <$ 300 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 300 GeV $< p_{\mathrm{T}} <$ 400 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 400 GeV $< p_{\mathrm{T}} <$ 500 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 500 GeV $< p_{\mathrm{T}} <$ 600 GeV and 1.5 <|y|< 2.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 20 GeV $< p_{\mathrm{T}} <$ 25 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 25 GeV $< p_{\mathrm{T}} <$ 30 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 30 GeV $< p_{\mathrm{T}} <$ 40 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 40 GeV $< p_{\mathrm{T}} <$ 50 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 50 GeV $< p_{\mathrm{T}} <$ 60 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 60 GeV $< p_{\mathrm{T}} <$ 70 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 70 GeV $< p_{\mathrm{T}} <$ 80 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 80 GeV $< p_{\mathrm{T}} <$ 90 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 90 GeV $< p_{\mathrm{T}} <$ 100 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 100 GeV $< p_{\mathrm{T}} <$ 110 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 110 GeV $< p_{\mathrm{T}} <$ 125 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 125 GeV $< p_{\mathrm{T}} <$ 140 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 140 GeV $< p_{\mathrm{T}} <$ 160 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 160 GeV $< p_{\mathrm{T}} <$ 180 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 180 GeV $< p_{\mathrm{T}} <$ 200 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 200 GeV $< p_{\mathrm{T}} <$ 225 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 225 GeV $< p_{\mathrm{T}} <$ 250 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 250 GeV $< p_{\mathrm{T}} <$ 300 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 300 GeV $< p_{\mathrm{T}} <$ 400 GeV and 2.0 <|y|< 2.5. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 20 GeV $< p_{\mathrm{T}} <$ 25 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 25 GeV $< p_{\mathrm{T}} <$ 30 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 30 GeV $< p_{\mathrm{T}} <$ 40 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 40 GeV $< p_{\mathrm{T}} <$ 50 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 50 GeV $< p_{\mathrm{T}} <$ 60 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 60 GeV $< p_{\mathrm{T}} <$ 70 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 70 GeV $< p_{\mathrm{T}} <$ 80 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 80 GeV $< p_{\mathrm{T}} <$ 90 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 90 GeV $< p_{\mathrm{T}} <$ 100 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 100 GeV $< p_{\mathrm{T}} <$ 110 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 110 GeV $< p_{\mathrm{T}} <$ 125 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 125 GeV $< p_{\mathrm{T}} <$ 140 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 140 GeV $< p_{\mathrm{T}} <$ 160 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 160 GeV $< p_{\mathrm{T}} <$ 180 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 180 GeV $< p_{\mathrm{T}} <$ 200 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 200 GeV $< p_{\mathrm{T}} <$ 225 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 225 GeV $< p_{\mathrm{T}} <$ 250 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 250 GeV $< p_{\mathrm{T}} <$ 300 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The measured differential jet shape $\rho(r)$ for jets with 300 GeV $< p_{\mathrm{T}} <$ 400 GeV and 2.5 <|y|< 3.0. The CF in the table refers to unfolding correction factor from {\sc pythia6} Tune Z2. The systematic uncertainties from different sources, jet energy scale (JES), unfolding, and single particle response (SPR), are also presented.

The dependence of $\langle N_\mathrm{ch} \rangle$ on the transverse momentum of jets in two different rapidity regions, $|y| < 1$ and $1 < |y| < 2$.

The dependence of $\langle \delta R^2 \rangle$ on the transverse momentum of jets in two different rapidity regions, $|y| < 1$ and $ 1 < |y| < 2 $.

The dependence of $\langle\delta \eta^2\rangle/\langle\delta \phi^2\rangle$ on the transverse momentum for jets with $|y| < 1$.

Energy dependence of average photon multiplicity in INEL proton-proton collisions.

Energy dependence of average photon multiplicity in NSD proton-proton collisions.

Photon pseudorapidity distribution in INEL proton-proton collisions at sqrt(s)=0.9 TeV.

Photon pseudorapidity distribution in INEL proton-proton collisions at sqrt(s)=2.76 TeV.

Photon pseudorapidity distribution in INEL proton-proton collisions at sqrt(s)=7 TeV.

Fully corrected average charged particle scalar Sum(pT) per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransMAX region.

Fully corrected average charged particle multiplicity per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransMIN region.

Fully corrected average charged particle scalar Sum(pT) per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransMIN region.

Fully corrected average charged particle multiplicity per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransDIF region.

Fully corrected average charged particle scalar Sum(pT) per unit of pseudorapidity and per radian as a function of the leading track-jet transverse momentum for proton-proton collisions at a centre-of-mass energy of 2.76 TeV in the TransDIF region.

Same as above with bigger centrality classes.

Same as above with bigger centrality classes.

Same as above with bigger centrality classes.

Integrated elliptic flow at sqrt(sNN) = 2.76 TeV for centrality 20-30%.

Uncorrected multiplicity distribution of charged particles in the Time Projection Chamber (|eta| < 0.8).

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Differential cross section for XI- production.

Differential cross section for XI(1530)0 production.

Differential cross section for XI(1530)0 production.

Differential cross section for LAMBDA production.

Differential cross section for LAMBDA production.

Differential cross section for XI- production.

Mean number per hadronic event in the restricted PT and ETARAP phase space.

Mean number per hadronic event extrapolated to the full phase space.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 172.3 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 182.8 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 188.6 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 194.4 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 200.2 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 130.1 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 136.1 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 161.3 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 172.3 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 182.8 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 188.6 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 194.4 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 200.2 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Jet fractions using the Cambridge algorithm as a function of the jet resolution parameter YCUT at c.m. energy 202.2 GeV.

Jet fractions using the Cambridge algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for the C-Parameter.

Differential distributions for the C-Parameter.

Differential distributions for the C-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the THRUST at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the RHO(C=HEAVY) at c.m. energy 91.2 GeV forlight quark (udsc) and b quark events.

Differential distributions for the BT at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the BW at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the C-PARAM at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the D-PARAM at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Mean values (first moment) and dispersion (second moment) of the THRUST distribution as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the scaled heavy jet mass (RHO(C=HEAVY)) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the total jet broadening (BT) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the wide jet broadening (BW) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the C-PARAM as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the D-PARAM as a function of c.m. energy.

Charged particle multiplicities at c.m. energy 91.2 GeV for all flavour, light quark (udsc) and bottom (b) flavour events.

Charged particle multiplicity.

Charged particle multiplicity.

Charged particle multiplicity.

First and second moment of the charged particle multiplicity distribution at c.m. energy 91.2 GeV for all flavours and for udsc an b flavours.

First and second moment of the charged particle multiplicity distribution at c.m. energy.

Distribution of LN(1/X) at c.m. energy 91.2 GeV.

Distribution of LN(1/X) at higher c.m. energies.

Distribution of LN(1/X) at higher c.m. energies.

Distribution of LN(1/X) at higher c.m. energies.

Jet flavor tagging is used. (C=DUSCB), (C=DUSC), (C=UDS) mean quark-jet flavors. CONST(C=GLUON/JET) is the ratio gluon/jet for all charged particles. 'Y' events, mirror symmetric events, the angle between the most energetic jet and other two jets is 150 +- 15 deg.

Jet flavor tagging is used. (C=DUSCB), (C=DUSC), (C=UDS) mean quark-jet flavors. CONST(C=GLUON/JET) is the ratio gluon/jet for all charged particles. 'Mercedes' events, three-fold symmetric events, the angle between three jets is 120 +- 15 deg.

Jet flavor tagging is used. (C=DUSCB), (C=DUSC), (C=UDS) mean quark-jet flavors. CONST(C=GLUON/JET) is the ratio gluon/jet for all charged particles. 'Mercedes' events, three-fold symmetric events, the angle between three jets is 120 +- 15 deg.

Jet flavor tagging is used. (C=DUSCB), (C=DUSC), (C=UDS) mean quark-jet flavors. CONST(C=GLUON/JET) is the ratio gluon/jet for all charged particles. 'Mercedes' events, three-fold symmetric events, the angle between three jets is 120 +- 15 deg.

Jet flavor tagging is used. (C=DUSCB), (C=DUSC), (C=UDS) mean quark-jet flavors. CONST(C=GLUON/JET) is the ratio gluon/jet for all charged particles. 'Mercedes' events, three-fold symmetric events, the angle between three jets is 120 +- 15 deg.

Jet flavor tagging is used. 'Y' events, mirror symmetric events, the angle between the most energetic jet and other two jets is 150 +- 15 deg.. CONST(NAME=XISTAR) is maximum of log(P(C=CHARGED)/P(C=JET)) distribution.

Jet flavor tagging is used. 'Mercedes' events, three-fold symmetric events, the angle between three jets is 120 +- 15 deg.. CONST(NAME=XISTAR) is maximum of log(P(C=CHARGED)/P(C=JET)) distribution.

No description provided.

Moments of the charged particle multiplicity distribution without KOS and LAMBDA decay for light quark events.

Moments of the charged particle multiplicity distribution with KOS and LAMBDA decay for b-quark events.

Moments of the charged particle multiplicity distribution without KOS and LAMBDA decay for b-quark events.

The standard deviation (DISPERSION) of the subject multiplicity for gluon jets and quark jets for different values of the subject resolution parameter Y0.

The ratio of the multiplicities and their standard deviations for the subject in quark and gluon jets as a function of the subject resolution parameter Y0.

The measured fragmentation function for charged particles within quark and gluon jets.

Inclusive charged particle distribution as a function of PT out of the event plane.

Mean charged particle multiplicity.

Inclusive charged particle distribution as a function of -LN(XP).

Distribution of Thrust.

Distribution of -LN(Y3).

Normalised PI+- production rates in Z0-->Q-QBAR events.

Normalised K+- production rates in Z0-->Q-QBAR events.

Normalised P PBAR production rates in Z0-->Q-QBAR events.

Normalised Heavy Particle (P and K) production rates in Z0-->Q-QBAR events.

Normalised PI+- production rates in Z0-->B-BBAR events.

Normalised K+- production rates in Z0-->B-BBAR events.

Normalised P PBAR production rates in Z0-->B-BBAR events.

Normalised Heavy Particle (P and K) production rates in Z0-->B-BBAR events.

Normalised PI+- production rates in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Normalised K+- production rates in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Normalised P PBAR production rates in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Normalised Heavy Particle (K and P) production rates in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Differential cross section for charged particles in Z0 -->Q-QBAR events.

Differential cross section for charged particles in Z0 -->Q-QBAR events.

Differential cross section for PI+- in Z0-->Q-QBAR events.

Differential cross section for PI+- in Z0-->Q-QBAR events.

Differential cross section for K+- in Z0-->Q-QBAR events.

Differential cross section for K+- in Z0-->Q-QBAR events.

Differential cross section for P PBAR in Z0-->Q-QBAR events.

Differential cross section for P PBAR in Z0-->Q-QBAR events.

Differential cross section for charged particles in Z0 -->B-BBAR events.

Differential cross section for charged particles in Z0 -->B-BBAR events.

Differential cross section for PI+- in Z0-->B-BBAR events.

Differential cross section for PI+- in Z0-->B-BBAR events.

Differential cross section for K+- in Z0-->B-BBAR events.

Differential cross section for K+- in Z0-->B-BBAR events.

Differential cross section for P PBAR in Z0-->B-BBAR events.

Differential cross section for P PBAR in Z0-->B-BBAR events.

Differential cross section for charged particles in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Differential cross section for charged particles in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Differential cross section for PI+- in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Differential cross section for PI+- in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Differential cross section for K+- in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Differential cross section for K+- in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

Differential cross section for P PBAR in Z0-->(U-UBAR,D-DBAR,S-SBAR) events.

No description provided.

Scaled energy distribution of charged hadrons produced in Gluon jets in 'Mercedes' topology 3-JET events.

Subjet multiplicity-1 as a function of the jet resolution parameter ycut for Quark jets in 'Y' topology events.

Subjet multiplicity-1 as a function of the jet resolution parameter ycut for Gluon jets in 'Y' topology events.

Ratio of the sub-jet multiplicity-1 for gluon jets to the sub-jet multiplicity-1 for quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Total 1-jet rate for Quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Total 1-jet rate for Gluon jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Differential 1-jet rate for Quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Differential 1-jet rate for Gluon jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Splitting Function for Quark jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Splitting Function for Gluon jets as a function of the jet resolution parameter ycut in 'Y' topology events.

Ratio of Splitting Functions for Gluon jets and Quark jets as a function ofthe jet resolution parameter ycut in 'Y' topology events.

ALPHAS from the fits to the event shape variables.

Second systematic error (DSYS) is from the theory.

ALPHAS from the fits to the event shape variables.

Second systematic error (DSYS) is from the theory.

The measured ALPHAS values evolved to the MZ scale. The quoted errors are experimental only.

(Transverse + longitudinal) components of the differential cross section.

No description provided.

Ratio of the longitudinal to the transverse component of the fragmentation function.

Transverse and longitudinal components of the differential cross section.

Transverse and longitudinal componentS of the differential cross section.

No description provided.

Tmajor distribution.

Tminor distribution.

Oblateness distribution.

Sphericity distribution.

Aplanarity distribution.

C-parameter distribution.

Heavy Jet Mass distribution.

Total Jet Broadening distribution.

Wide Jet Broadening distribution.

The mean of the event shape distributions.

The width of the event shape distributions.

The skewness of the event shape distributions.

Jet rates using the JADE E0 scheme as a function of ycut (the cut-off parameter).

Jet rates using the Durham Scheme as a function of ycut (the cut-off parameter).

Jet rates using the Cone algorithm as a function of the cone size R. Minimum jet energy is fixed at 7 GeV.

Jet rates using the Cone algorithm as a function of the minimum jet energy. The cone size is fixed at 0.7 radians.

Differential two jet rate using the Durham jet finding algorithm.

PTIN distribution.

PTOUT distribution.

Rapidity distribution of charged particles.

Fragmentation function.

The ln(1/xe) distribution.

Multiplicity distribution of charged particles.