Distributions of the b-tagging efficiency as a function of the mistag rate of charm jets for pp collisions in a PYTHIA simulation.

Distributions of the b-tagging efficiency as a function of the mistag rate of light jets for pPb collisions in a PYTHIA+HIJING simulation.

Distributions of the b-tagging efficiency as a function of the mistag rate of charm jets for pPb collisions in a PYTHIA+HIJING simulation.

Distributions of the Secondary Vertex Mass after applying the SSV tagger selection.

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from -2.5 < eta_CM < -1.5.

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from -1.5 < eta_CM < -0.5 (x 10^2).

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from -0.5 < eta_CM < 0.5 (x10^4).

b-jet cross-sections in pPb, scaled by the Glauber nuclear overlap function, as well as a b-jet cross-section from a PYTHIA simulation from 0.5 < eta_CM < 1.5 (x10^6).

b-jet RpA (PYTHIA) from 0.5 < eta_CM < 1.5.

b-jet RpA (PYTHIA) from -0.5 < eta_CM < 0.5.

b-jet RpA (PYTHIA) from -1.5 < eta_CM < -0.5.

b-jet RpA (PYTHIA) from -2.5 < eta_CM < -1.5.

b-jet Fraction.

b-jet RpA(PYTHIA).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}<$ 35 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 80 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 35 $<N_{offline}^{trk}<$ 90 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 80 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and 90 $<N_{offline}^{trk}<$ 105 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 0.1 $<p_{T}<$ 1.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 1.0 $<p_{T}<$ 2.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 2.0 $<p_{T}<$ 3.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}>$ 105 bins for pp data at $\sqrt =$ 13 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Correlated yield obtained with the ZYAM procedure as a function of $|\Delta\Phi|$, averaged over 2 $<|\Delta\eta|<$ 4 in for 3.0 $<p_{T}<$ 4.0 $GeV/c$ and $N_{offline}^{trk}>$ 110 bins for pp data at $\sqrt =$ 7 $TeV$. The $p_{T}$ selection applies to both particles in the pair. Only statistical uncertainties are given. The subtracted ZYAM constant is given ($C_{ZYAM}$).

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 and integrated over the region $|\Delta\Phi| < \Delta\Phi_{ZYAM}$ for pp data at $\sqrt{s} =$ 13 $TeV$. The associated yield as a function of $p_{T}$ for events with $N^{offline}_{trk} \geq$ 105. The $p_{T}$ value for each $p_{T}$ bin is the average $p_{T}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 for pp data at $\sqrt{s} =$ 7 $TeV$. The associated yield as a function of $p_{T}$ for events with $N^{offline}_{trk} \geq$ 110. The $p_{T}$ value for each $p_{T}$ bin is the average $p_{T}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 and integrated over the region $|\Delta\Phi| < \Delta\Phi_{ZYAM}$ for pp data at $\sqrt{s} =$ 13 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 for pp data at $\sqrt{s} =$ 7 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 pPb data at $\sqrt{s} =$ 5.02 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.

Associated yield for the near side of the correlation function averaged over 2 $<|\Delta\eta|<$ 4 PbPb data at $\sqrt{s} =$ 2.76 $TeV$. The associated yield as a function of $N_{trk}^{offline}$ for events with 1.0 $< p_{T} <$ 2.0 GeV/c. The $N_{trk}^{offline}$ value for each $N_{trk}^{offline}$ bin is the average $N_{trk}^{offline}$ value.

Raw number of J/$\psi$ (N$_{\rm AA}^{\rm J/\psi}$), expected raw number of hadronic J/$\psi$ (N$_{\rm AA}^{\rm{h J}/\psi}$) and measured excess in the number of J/$\psi$ (N$_{\rm AA}^{\rm{exess J}/\psi}$), all three numbers in the $p_{\rm T}$ range (0-0.3) GeV/$c$, and J/$\psi$ coherent photoproduction cross section, as a function of centrality, with their statistical and systematic uncertainties. An additional correlated systematic uncertainty also applies to the cross section. In the most central classes, an upper limit (95% CL) on the J/$\psi$ yield excess and on the cross section is given.

Nuclear modification factor $R_{\rm AA}$ of D$_s^+$ mesons in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$=2.76 TeV in the centrality class 20-50% in |y| < 0.5 as a function of $p_{\rm T}$.

Ratio of D$_s^+$ to D$^0$ meson yield in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$=2.76 TeV in the centrality class 0-10% in |y| < 0.5 as a function of $p_{\rm T}$. Branching ratio of D$_s^+$->$\phi\pi^+$->$K^+K^-\pi^+$ : 0.0224. Branching ratio of D$^0$->K$^-\pi^+$ : 0.0388.

Ratio of D$_s^+$ to D$^+$ meson yield in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$=2.76 TeV in the centrality class 0-10% in |y| < 0.5 as a function of $p_{\rm T}$. Branching ratio of D$_s^+$->$\phi\pi^+$->$K^+K^-\pi^+$ : 0.0224. Branching ratio of D$^+$->K$^-\pi^+\pi^+$ : 0.0913.

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].

Balance function in $\Delta\eta$ 0_5%.

Balance function in $\Delta\eta$ 30_40%.

Balance function in $\Delta\eta$ 70_80%.

Balance function in $\Delta\varphi$ 0_5%.

Balance function in $\Delta\varphi$ 30_40%.

Balance function in $\Delta\varphi$ 70_80%.

Balance function in $\Delta\eta$ 0-10%.

Balance function in $\Delta\eta$ 30-40%.

Balance function in $\Delta\eta$ 70-80%.

Balance function in $\Delta\eta$ 0-10%.

Balance function in $\Delta\eta$ 30-40%.

Balance function in $\Delta\eta$ 70-80%.

Balance function in $\Delta\varphi$ 0-10%.

Balance function in $\Delta\varphi$ 30-40%.

Balance function in $\Delta\varphi$ 70-80%.

Balance function in $\Delta\eta$ 0To10%.

Balance function in $\Delta\eta$ 30To40%.

Balance function in $\Delta\eta$ 70To80%.

Balance function in $\Delta\eta$ 0To10%.

Balance function in $\Delta\eta$ 30To40%.

Balance function in $\Delta\eta$ 70To80%.

Balance function in $\Delta\varphi$ 0To10%.

Balance function in $\Delta\varphi$ 30To40%.

Balance function in $\Delta\varphi$ 70To80%.

$\sigma_{\Delta\eta}$ as a function of the multiplicity class.

Relative decrease of $\sigma_{\Delta\eta}$ as a function of the multiplicity class.

$\sigma_{\Delta\eta}$ as a function of the multiplicity class.

Relative decrease of $\sigma_{\Delta\eta}$ as a function of the multiplicity class.

$\sigma_{\Delta\eta}$ as a function of the multiplicity class.

Relative decrease of $\sigma_{\Delta\eta}$ as a function of the multiplicity class.

$\sigma_{\Delta\varphi}$ as a function of the multiplicity class.

Relative decrease of $\sigma_{\Delta\varphi}$ as a function of the multiplicity class.

$\sigma_{\Delta\varphi}$ as a function of the multiplicity class.

Relative decrease of $\sigma_{\Delta\varphi}$ as a function of the multiplicity class.

$\sigma_{\Delta\varphi}$ as a function of the multiplicity class.

Relative decrease of $\sigma_{\Delta\varphi}$ as a function of the multiplicity class.

Balance function in $\Delta\eta$ 0_5%.

Balance function in $\Delta\eta$ 30_40%.

Balance function in $\Delta\eta$ 60_80%.

Balance function in $\Delta\varphi$ 0_5%.

Balance function in $\Delta\varphi$ 30_40%.

Balance function in $\Delta\varphi$ 60_80%.

Balance function in $\Delta\eta$ 0-10%.

Balance function in $\Delta\eta$ 30-40%.

Balance function in $\Delta\eta$ 70-80%.

Balance function in $\Delta\varphi$ 0-10%.

Balance function in $\Delta\varphi$ 30-40%.

Balance function in $\Delta\varphi$ 70-80%.

Balance function in $\Delta\eta$ 0To10%.

Balance function in $\Delta\eta$ 30To40%.

Balance function in $\Delta\eta$ 70To80%.

Balance function in $\Delta\varphi$ 0To10%.

Balance function in $\Delta\varphi$ 30To40%.

Balance function in $\Delta\varphi$ 70To80%.

Balance function in $\Delta\eta$ 0_5%.

Balance function in $\Delta\eta$ 30_40%.

Balance function in $\Delta\eta$ 50_60%.

Balance function in $\Delta\varphi$ 0_5%.

Balance function in $\Delta\varphi$ 30_40%.

Balance function in $\Delta\varphi$ 50_60%.

Balance function in $\Delta\eta$ 0-10%.

Balance function in $\Delta\eta$ 30-40%.

Balance function in $\Delta\eta$ 70-80%.

Balance function in $\Delta\varphi$ 0-10%.

Balance function in $\Delta\varphi$ 30-40%.

Balance function in $\Delta\varphi$ 70-80%.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

Sigma as function of the multiplicity class for $p_{\rm{T}}$ low, intermediate, and high.

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.