Normalized $\sigma_{\psi(2S)}/\sigma_{J/\psi}$ in $6.5<p_T<30.0\,GeV$ and $ 1 < y_{CM} < 1.935$ as functions of normalized $\text{N}^{{\text{corr.}}}_{\text{track}}$

Normalized $\sigma_{\psi(2S)}/\sigma_{J/\psi}$ in $6.5<p_T<30.0\,GeV$ and $ -2.865 < y_{CM} < 1.935$ as functions of normalized $\text{N}^{{\text{corr.}}}_{\text{track}}$

Normalized $\sigma_{\psi(2S)}/\sigma_{J/\psi}$ in $3.0<p_T<6.5\,GeV$ and $ -2.865 < y_{CM} < -2 $ as functions of normalized $\text{N}^{{\text{corr.}}}_{\text{track}}$

Normalized $\sigma_{\psi(2S)}/\sigma_{J/\psi}$ in $3.0<p_T<6.5\,GeV$ and $ 1 < y_{CM} < 1.935 $ as functions of normalized $\text{N}^{{\text{corr.}}}_{\text{track}}$

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.

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 $\varepsilon$ 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 $\Delta R_{g}$ 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 $\tau_{21}$ 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 $\tau_{43}$ 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 $C_{1}^{(0.2)}$ 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 $C_{1}^{(1.0)}$ 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 $C_{2}^{(0.0)}$ 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 $C_{2}^{(0.5)}$ 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 $C_{2}^{(2.0)}$ 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 $C_{3}^{(0.2)}$ 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 $C_{3}^{(1.0)}$ 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 $M_{2}^{(1)}$ 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 $N_{3}^{(1)}$ 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 $N_{2}^{(2)}$ 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 $\lambda_{0}^{0}$ (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 $\lambda_{0.5}^{1}$ (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 $\lambda_{2}^{1}$ (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 $z_{g}$ 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 $n_{SD}$ 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 $\tau_{32}$ 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 $C_{1}^{(0.0)}$ 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 $C_{1}^{(0.5)}$ 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 $C_{1}^{(2.0)}$ 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 $C_{2}^{(0.2)}$ 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 $C_{2}^{(1.0)}$ 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 $C_{3}^{(0.0)}$ 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 $C_{3}^{(0.5)}$ 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 $C_{3}^{(2.0)}$ 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 $N_{2}^{(1)}$ 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 $M_{2}^{(2)}$ 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 $N_{3}^{(2)}$ 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 $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ 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 $\lambda_{1}^{1}$ (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 $\varepsilon$ 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 $\Delta R_{g}$ 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 $\tau_{21}$ 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 $\tau_{43}$ 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 $C_{1}^{(0.2)}$ 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 $C_{1}^{(1.0)}$ 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 $C_{2}^{(0.0)}$ 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 $C_{2}^{(0.5)}$ 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 $C_{2}^{(2.0)}$ 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 $C_{3}^{(0.2)}$ 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 $C_{3}^{(1.0)}$ 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 $M_{2}^{(1)}$ 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 $N_{3}^{(1)}$ 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 $N_{2}^{(2)}$ 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 $\lambda_{0}^{0}$ (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 $\lambda_{0.5}^{1}$ (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 $\lambda_{2}^{1}$ (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 $z_{g}$ 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 $n_{SD}$ 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 $\tau_{32}$ 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 $C_{1}^{(0.0)}$ 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 $C_{1}^{(0.5)}$ 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 $C_{1}^{(2.0)}$ 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 $C_{2}^{(0.2)}$ 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 $C_{2}^{(1.0)}$ 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 $C_{3}^{(0.0)}$ 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 $C_{3}^{(0.5)}$ 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 $C_{3}^{(2.0)}$ 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 $N_{2}^{(1)}$ 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 $M_{2}^{(2)}$ 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 $N_{3}^{(2)}$ 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.

Measured pseudorapidity dependence of DN/DETARAP for NSD collisions at a centre-of-mass energy of 2360 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 normalized to the bin width in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.0 to 1.0 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.3 to 1.3 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

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

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.0 to 1.0 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.3 to 1.3 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 2360 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.0 to 1.0 for NSD collisions at a centre-of-mass energy of 2360 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.3 to 1.3 for NSD collisions at a centre-of-mass energy of 2360 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 2360 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.0 to 1.0 for INEL collisions at a centre-of-mass energy of 2360 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Multiplicity distribution normalized to the bin width in the pseudorapidity region -1.3 to 1.3 for INEL collisions at a centre-of-mass energy of 2360 GeV. Note that the statistical as well as the systematic uncertainties are strongly correlated between neighbouring points. See text of paper for details.

Mean charged particle multiplicities in 3 pseudorapidity intervals in P P NSD collisions at 900 and 2360 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 900 and 2360 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 900 and 2360 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -1.3 to 1.3 in P P NSD collisions at centre-of-mass energies 900 and 2360 GeV.

Pseusdorapidity densities for the INEL>0 class of data as a function of pseudorapidity for centre-of mass energy 0.9 TeV. Note that this data is not in the paper but has been approved by the collaboration.

Pseusdorapidity densities for the INEL>0 class of data as a function of pseudorapidity for centre-of mass energy 2.36 TeV. Note that this data is not in the paper but has been approved by the collaboration.

Pseusdorapidity densities for the INEL>0 class of data as a function of pseudorapidity for centre-of mass energy 7 TeV. Note that this data is not in the paper but has been approved by the collaboration.

No description provided.

x spectra using JETSET as model in efficiency corrections.

x spectra using HERWIG as model in efficiency corrections.

LN(1/X) distribution using average of JETSET and HERWIG in efficiency corrections.

x spectra using JETSET as model in efficiency corrections.

x spectra using HERWIG as model in efficiency corrections.

LN(1/X) distribution using average of JETSET and HERWIG in efficiency corrections.