The double ratio R_double at 7000 GeV in different bins of charged particle multiplicity and kT.

The double ratio R_double at 7000 GeV in different bins of charged particle multiplicity.

Parameters of the fit to the double ratio R_double at 900 GeV.

Parameters of the fit to the double ratio R_double at 7000 GeV.

Inclusive relative fluctuation $\sqrt{C}/M(p_{\rm T})$ as a function of $\sqrt{s}$ in pp collisions.

Relative fluctuation $\sqrt{C_m}/M(p_{\rm T})_m$ as a function of $\langle {\rm d}N_{\rm ch}/{\rm d}\eta \rangle$ in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV.

Relative fluctuation $\sqrt{C_m}/M(p_{\rm T})_m$ as a function of $\langle N_{\rm part} \rangle$ in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV.

Relative fluctuation $\sqrt{C_m}/M(p_{\rm T})_m$ normalized to $\langle {\rm d}N_{\rm ch}/{\rm d}\eta \rangle^{-0.5}$ as a function of $\langle {\rm d}N_{\rm ch}/{\rm d}\eta \rangle$ in pp collisions at $\sqrt{s}$ = 2.76 TeV.

Relative fluctuation $\sqrt{C_m}/M(p_{\rm T})_m$ normalized to $\langle {\rm d}N_{\rm ch}/{\rm d}\eta \rangle^{-0.5}$ as a function of $\langle {\rm d}N_{\rm ch}/{\rm d}\eta \rangle$ in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV.

C2 versus qinv for mixed-charge pions in six kT intervals. 45-50% centrality.

Fit parameters from two-pion correlations. 0-5% and 45-50% centrality. EW = Edgeworth, Gauss=Gaussian.

C3 versus Q3 for same-charge pions in six centrality intervals. Low KT3.

Cummulant c3 versus Q3 for same-charge pions in six centrality intervals. Low KT3.

C3 versus Q3 for same-charge pions in six centrality intervals. High KT3.

Cummulant c3 versus Q3 for same-charge pions in six centrality intervals. High KT3.

C3 versus Q3 for mixed-charge pions in six centrality intervals. Low KT3.

Cummulant c3 versus Q3 for mixed-charge pions in six centrality intervals. Low KT3.

C3 versus Q3 for mixed-charge pions in six centrality intervals. High KT3.

Cummulant c3 versus Q3 for mixed-charge pions in six centrality intervals. High KT3.

r3 for 0-5% centrality.

r3 for 5-10% centrality.

r3 for 10-20% centrality.

r3 for 20-30% centrality.

r3 for 30-40% centrality.

r3 for 40-50% centrality.

The centrality dependence of the correlator three-particle charge-dependent MEAN(COS(PHI(A)+COS(PHI(B)-2*PHI(RP)) measured from correlations with the reaction plane (RP) estimated using the ZDC detector.

The centrality dependence of the two-particle charge-dependentcorrelator MEAN(COS(PHI(A)-COS(PHI(B)) measured with the cumulant method.

The decomposition of the correlators into the COS*COS terms.

The decomposition of the correlators into the SIN*SIN terms.

The dependence of the three-particle charge-dependent correlator MEAN(COS(PHI(A)+COS(PHI(B)-2*PHI(RP)) on the PT difference between the two particles A and B for the centrality range 30-40%.

The dependence of the three-particle charge-dependent correlator MEAN(COS(PHI(A)+COS(PHI(B)-2*PHI(RP)) on the average PT of the two particles A and B for the centrality range 30-40%.

The dependence of the three-particle charge-dependent correlator MEAN(COS(PHI(A)+COS(PHI(B)-2*PHI(RP)) on the difference in pseudorapidity of the two particles A and B for the centrality range 30-40%.

Correlation between y and x components of the Q-vector of projectile (Qpy) and target (Qtx) spectators, MEAN(QpyQtx).

Odd directed flow component (v1odd) relative to the spectator plane as a function of pseudorapidity.

Even directed flow component (v1even) relative to the spectator plane as a function of pseudorapidity.

Odd and even components of the relative momentum shift (pXodd and pXeven) wrt. to the spectator plane as a function of pseudorapidity.

Odd directed flow component (v1odd) relative to the spectator plane as a function of pseudorapidity.

Odd and even directed flow components (v1odd) relative to the spectator plane as a function of collision centrality.

Odd and even components of the relative momentum shift (pXodd and pXeven) wrt. to the spectator plane as a function of collision centrality.

Odd and even directed flow components (v1odd) relative to the spectator plane as a function of transverse momentum.

Odd directed flow component (v1odd) relative to the spectator plane as a function of transverse momentum.

$\lambda_{{\rm \overline{p}}{\rm \overline{p}}}+\lambda_{{\rm \overline{p}} \overline{\Lambda}}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$\lambda_{{\rm \overline{p}}{\rm \overline{p}}}+\lambda_{{\rm \overline{p}} \overline{\Lambda}}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$\lambda_{{\rm \overline{p}}{\rm \overline{p}}}+\lambda_{{\rm \overline{p}} \overline{\Lambda}}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$\lambda_{{\rm p}{\rm {p}}}+\lambda_{{\rm {p}}\Lambda}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm {p}}{\rm {p}}$.

$\lambda_{{\rm p}{\rm {p}}}+\lambda_{{\rm {p}}\Lambda}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm {p}}{\rm {p}}$.

$\lambda_{{\rm p}{\rm {p}}}+\lambda_{{\rm {p}}\Lambda}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm {p}}{\rm {p}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $0-10\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $10-30\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$\lambda$ parameter vs. $m_{\rm T}$ for $30-50\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm \overline{p}}{\rm \overline{p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm {p}}{\rm {p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm {p}}{\rm {p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm {p}}{\rm {p}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{ 0}_S}{\rm K^{ 0}_S}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for ${\rm K^{\pm}}{\rm K^{\pm}}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $0-10\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $10-30\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

$R_{\rm inv}$ vs. $m_{\rm T}$ for $30-50\%$ centrality for $\pi^{\pm}\pi^{\pm}$.

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.

Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Pion HBT radii for the 5% most central collisions.

Pion HBT radii for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.;.

Pion HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

Product of the three HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

The decoupling time extracted from R_long(KT) as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

C(k*)/(linear baseline fit) for K0s K+ and all kT bin

C(k*)/(linear baseline fit) for K0s K+ and kT < 0.675 GeV/c bin

C(k*)/(linear baseline fit) for K0s K+ and kT > 0.675 GeV/c bin

C(k*)/(linear baseline fit) for K0s K- and all kT bin

C(k*)/(linear baseline fit) for K0s K- and kT < 0.675 GeV/c bin

C(k*)/(linear baseline fit) for K0s K- and kT > 0.675 GeV/c bin

R vs. kT for K0s K- with Achasov1 parameters

lambda vs. kT for K0s K- with Achasov1 parameters

R vs. kT for K0s K+- with Achasov1 parameters and linear fit

lambda vs. kT for K0s K+- with Achasov1 parameters and linear fit

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for PbPb collisions at $\sqrt{ s_{NN} }$=2.76 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T} < $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for p+Pb collisions at $ \sqrt{ s_{NN} } $= 5.02 TeV.

$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T}< $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for Pb+Pb collisions at $ \sqrt{ s_{NN} } $= 2.76 TeV.