$A_{UT}$ as a function of $<M_{inv}>$ for pT bin $<p_{T}>$ = 5 GeV/c for $\eta > 0$ and $\eta < 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned.

$A_{UT}$ as a function of $<M_{inv}>$ for pT bin $<p_{T}>$ = 6 GeV/c for $\eta > 0$ and $\eta < 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned.

$A_{UT}$ as a function of $<M_{inv}>$ for pT bin $<p_{T}>$ = 8 GeV/c for $\eta > 0$ and $\eta < 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned.

$A_{UT}$ as a function of $<M_{inv}>$ for pT bin $<p_{T}>$ = 13 GeV/c for $\eta > 0$ and $\eta < 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned.

Same-charge, momentum ordered asymmetry $A_{UT}$ as a function of $<M_{inv}>$ for pT bin $<p_{T}>$ = 4 GeV/c for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned.

Same-charge, momentum ordered asymmetry $A_{UT}$ as a function of $<M_{inv}>$ for pT bin $<p_{T}>$ = 6 GeV/c for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned.

Same-charge, momentum ordered asymmetry $A_{UT}$ as a function of $<M_{inv}>$ for pT bin $<p_{T}>$ = 13 GeV/c for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned.

$A_{UT}$ as a function of $<p_{T}>$ for $<M_{inv}>$ = 0.4 GeV/$c^{2}$ for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned. The systematic uncertainty numbers marked with (*) are based on marker size, and may not reflect actual experimental uncertainties.

$A_{UT}$ as a function of $<p_{T}>$ for $<M_{inv}>$ = 0.5 GeV/$c^{2}$ for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned. The systematic uncertainty numbers marked with (*) are based on marker size, and may not reflect actual experimental uncertainties.

$A_{UT}$ as a function of $<p_{T}>$ for $<M_{inv}>$ = 0.6 GeV/$c^{2}$ for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned. The systematic uncertainty numbers marked with (*) are based on marker size, and may not reflect actual experimental uncertainties.

$A_{UT}$ as a function of $<p_{T}>$ for $<M_{inv}>$ = 0.7 GeV/$c^{2}$ for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned. The systematic uncertainty numbers marked with (*) are based on marker size, and may not reflect actual experimental uncertainties.

$A_{UT}$ as a function of $<p_{T}>$ for $<M_{inv}>$ = 1.0 GeV/$c^{2}$ for $\eta > 0$. In addition to statistical uncertainties, systematic uncertainties originating from PID and trigger bias systematic uncertainties are also mentioned. The systematic uncertainty numbers marked with (*) are based on marker size, and may not reflect actual experimental uncertainties.

A summary of worldwide $^3_{\Lambda}$H R_3 experimental measurements and theoretical calculations. The marker represents the present analysis. This Fig. summarizes previous measurements of this decay branching ratio in the literature. The present results close to the combined measurement from helium bubble chamber experiments and is consistent with the average value of 0.35 ± 0.04 based on early measurements in helium bubble chambers.

Invariant differential yields of tritons and antitritons in inelastic pp collisions at $\sqrt{s}$ = 7 TeV. The uncertainties of $_{-2.0}^{+5.0}$% due to the extrapolation to inelastic pp collisions are not included in the systematic uncertainties.

Invariant differential yields of $^{3}$He and $^{3}\overline{\text{He}}$ nuclei in inelastic pp collisions at $\sqrt{s}$ = 7 TeV. The uncertainties of $_{-2.0}^{+5.0}$% due to the extrapolation to inelastic pp collisions are not included in the systematic uncertainties.

Coalescence parameter ($B_{2}$) of deuterons and antideuterons in inelastic pp collisions at $\sqrt{s}$ = 0.9 TeV.

Coalescence parameter ($B_{2}$) of deuterons and antideuterons in inelastic pp collisions at $\sqrt{s}$ = 2.76 TeV.

Coalescence parameter ($B_{2}$) of deuterons and antideuterons in inelastic pp collisions at $\sqrt{s}$ = 7 TeV.

Coalescence parameter ($B_{3}$) of tritons and antitritons in inelastic pp collisions at $\sqrt{s}$ = 7 TeV.

Coalescence parameter ($B_{3}$) of $^{3}$He and $^{3}\overline{\text{He}}$ nuclei in inelastic pp collisions at $\sqrt{s}$ = 7 TeV.

Integrated deuteron-to-proton (d/p) and antideuteron-to-antiproton ($\overline{\text{d}}/\overline{\text{p}}$) ratios in inelastic pp collisions as a function of the average charged particle multiplicity for different center-of-mass energies.

$v_2^{J/\psi}${2,sub} in bins of $p_T^{J/\psi}$ for p-Pb collisions in Pb-going direction at $\sqrt{s_{NN}}$ = 8.16 TeV. The quoted global systematic uncertainties correspond to the combined statistical and systematic uncertainties of the measured $v_2^{tracklet}$ coefficient. The results are obtained by subtracting associated per-trigger yields in low-multiplicity (40-100% V0M) collisions from the yields in high-multiplicity (0-20% V0M) collisions.

Transverse momentum dependence of inclusive J/$\psi$ $v_2$ at $\sqrt{s_{\rm NN}}=5.02$ TeV for the 40-60% centrality class (forward rapidity). The first uncertainty (stat) is statistical, the second (sys,uncorrel) is the uncorrelated systematic, while the third one (sys,correl) is a $p_{\rm T}$-correlated systematic uncertainty.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (20-30% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (30-40% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (40-50% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (50-60% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (60-70% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (70-80% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (80-90% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$v_2\{EP\}$ with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (90-100% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for unbiased events in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (0-10% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (10-20% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (20-30% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (30-40% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (40-50% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (50-60% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (60-70% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (70-80% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (80-90% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (90-100% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for unbiased events in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (0-10% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (10-20% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (20-30% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (30-40% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (40-50% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (50-60% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (60-70% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (70-80% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (80-90% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (same charge pairs) with $|\Delta\eta| > 2.0$ as a function of centrality for shape selected events (90-100% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for unbiased events in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (0-10% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (10-20% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (20-30% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (30-40% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (40-50% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (50-60% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (60-70% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (70-80% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (80-90% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (opposite charge pairs) as a function of centrality for shape selected events (90-100% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for unbiased events in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (0-10% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (10-20% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (20-30% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (30-40% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (40-50% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (50-60% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (60-70% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (70-80% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (80-90% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} - \varphi_{\beta}) \rangle$ (same charge pairs) as a function of centrality for shape selected events (90-100% $q_2$) in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of $v_2\{EP\}$ for centrality class 0-5% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of $v_2\{EP\}$ for centrality class 5-10% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of $v_2\{EP\}$ for centrality class 10-20% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of $v_2\{EP\}$ for centrality class 20-30% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of $v_2\{EP\}$ for centrality class 30-40% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of $v_2\{EP\}$ for centrality class 40-50% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of $v_2\{EP\}$ for centrality class 50-60% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ multiplied by the charged-particle density, $dN/d\eta$, as a function of $v_2\{EP\}$ for centrality class 0-5% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ multiplied by the charged-particle density, $dN/d\eta$, as a function of $v_2\{EP\}$ for centrality class 5-10% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ multiplied by the charged-particle density, $dN/d\eta$, as a function of $v_2\{EP\}$ for centrality class 10-20% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ multiplied by the charged-particle density, $dN/d\eta$, as a function of $v_2\{EP\}$ for centrality class 20-30% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ multiplied by the charged-particle density, $dN/d\eta$, as a function of $v_2\{EP\}$ for centrality class 30-40% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ multiplied by the charged-particle density, $dN/d\eta$, as a function of $v_2\{EP\}$ for centrality class 40-50% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ multiplied by the charged-particle density, $dN/d\eta$, as a function of $v_2\{EP\}$ for centrality class 50-60% in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$p_1$ parameter from a linear fit to $\langle \cos(\varphi_{\alpha} + \varphi_{\beta} - 2\Psi_{2}) \rangle$ (opposite - same) with $|\Delta\eta| > 2.0$ as a function of centrality in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

CME fraction extracted from the slope parameter of fits to data and MC—Glauber model as a function of centrality in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

CME fraction extracted from the slope parameter of fits to data and MC—KLN CGC model as a function of centrality in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

CME fraction extracted from the slope parameter of fits to data and EKRT model as a function of centrality in Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

Most probable charge deposit signal normalised to that of minimum ionising particles as a function of $\beta\gamma$ for cosmic-ray muons (dE/dx). Statistical uncertainties as vertical error bars. Uncertainties in momentum and thus $\beta \gamma$ determination are drawn as horizontal error bars.

Most probable charge deposit signal normalised to that of minimum ionising particles as a function of $\beta\gamma$ for cosmic-ray muons (dE/dx + TR). Statistical uncertainties as vertical error bars. Uncertainties in momentum and thus $\beta \gamma$ determination are drawn as horizontal error bars.

Out projection of raw 3D LCMS KS KS correlation function for 1.0 < kT < 1.5 GeV/c bin

Side projection of raw 3D LCMS KS KS correlation function for 1.0 < kT < 1.5 GeV/c bin

Long projection of raw 3D LCMS KS KS correlation function for 1.0 < kT < 1.5 GeV/c bin

Rout vs. mT for PI+- PI+- for centrality 0-10%

Rside vs. mT for PI+- PI+- for centrality 0-10%

Rlong vs. mT for PI+- PI+- for centrality 0-10%

Rout vs. mT for PI+- PI+- for centrality 10-30%

Rside vs. mT for PI+- PI+- for centrality 10-30%

Rlong vs. mT for PI+- PI+- for centrality 10-30%

Rout vs. mT for PI+- PI+- for centrality 30-50%

Rside vs. mT for PI+- PI+- for centrality 30-50%

Rlong vs. mT for PI+- PI+- for centrality 30-50%

Rout vs. mT for PI+- PI+- for centrality 0-5%

Rside vs. mT for PI+- PI+- for centrality 0-5%

Rlong vs. mT for PI+- PI+- for centrality 0-5%

Ratio Rout/Rside vs. mT for PI+- PI+- for centrality 0-5%

Ratio Rout/Rside vs. mT for PI+- PI+- for centrality 0-10%

Ratio Rout/Rside vs. mT for PI+- PI+- for centrality 10-30%

Ratio Rout/Rside vs. mT for PI+- PI+- for centrality 30-50%

Rlong^2 vs. mT for PI+- PI+- for centrality 0-5%

Centrality dependence of observables SC(5,3) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables SC(4,3) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables SC(4,3) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(5,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(5,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(5,3) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(5,3) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,3) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,3) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(3,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables SC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(3,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables NSC(4,2) in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_2$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_3$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Transeverse momemtum dependence of observables $v_4$ in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables $v_5$ in Pb-Pb collisions at 2.76 TeV.

Centrality dependence of observables $v_5$ in Pb-Pb collisions at 2.76 TeV.

Raw $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 27 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 39 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 200 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collisions energy dependence of $M/\sigma^2$ for $\Delta N_k$ multiplicity distributions from 0–5% most central and 70–80% peripheral collisions in Au+Au collisions at \sqrt{s_{NN}} = 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collisions energy dependence of $S\sigma$ for $\Delta N_k$ multiplicity distributions from 0–5% most central and 70–80% peripheral collisions in Au+Au collisions at \sqrt{s_{NN}} = 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collisions energy dependence of $\kappa\sigma^2$ for $\Delta N_k$ multiplicity distributions from 0–5% most central and 70–80% peripheral collisions in Au+Au collisions at \sqrt{s_{NN}} = 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.