Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

No description provided.

Systematic covariance matrix for the 12 bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\varphi$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\varphi$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\varphi$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$.

Values of the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$.

Statistical covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$.

Systematic covariance matrix for the 6 bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$.

Values of $A_{\Delta\phi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{\cos\varphi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{c1c2}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{c1c2}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{c1c2}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{P}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{P}^{\rm{CPV}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $M_\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $M_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $M_\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $M_\mathrm{t\bar{t}}$.

Values of $A_{\Delta\phi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{\cos\varphi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{c1c2}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{c1c2}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{c1c2}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{P}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{P}^{\rm{CPV}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $p_\mathrm{T}^\mathrm{t\bar{t}}$.

Values of $A_{\Delta\phi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{\Delta\phi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $12\times3$ bins of the normalized differential cross section as a function of $\left|\Delta \phi_{\ell^+\ell^-}\right|$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{\cos\varphi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{\cos\varphi}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\varphi$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{c1c2}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{c1c2}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{c1c2}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell^+} \cos\theta^{\star}_{\ell^-}$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{P}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{P}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_\ell$ and $|y_\mathrm{t\bar{t}}|$.

Values of $A_{P}^{\rm{CPV}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$, and inclusively (bottom row). The value 9999 is used as a placeholder for infinity.

Statistical correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Systematic correlation matrix for $A_{P}^{\rm{CPV}}$ in the 3 bins of $|y_\mathrm{t\bar{t}}|$.

Fraction of events in each of the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $|y_\mathrm{t\bar{t}}|$. The value 9999 is used as a placeholder for infinity.

Statistical covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $|y_\mathrm{t\bar{t}}|$.

Systematic covariance matrix for the $6\times3$ bins of the normalized differential cross section as a function of $\cos\theta^{\star}_{\ell,\mathrm{CPV}}$ and $|y_\mathrm{t\bar{t}}|$.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Difference PbPb - pp of symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Difference PbPb - pp of symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Difference PbPb - pp of symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Difference PbPb - pp of symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to inclusive jets with pT > 120 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to leading jets with pT > 120 GeV and subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to leading jets with pT > 120 GeV and subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to leading jets with pT > 120 GeV and subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Difference PbPb - pp of symmetrized dEta distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to leading jets with pT > 120 GeV and subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp leading jets with pT > 120 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 30-50% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to PbPb and pp subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 0-10% central events.

Difference PbPb - pp of symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to leading jets with pT > 120 GeV and subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 50-100% central events.

Difference PbPb - pp of symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to leading jets with pT > 120 GeV and subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV in 10-30% central events.

Difference PbPb - pp of symmetrized dPhi distributions (projected over |dPhi|<1) of background-subtracted particle yields correlated to leading jets with pT > 120 GeV and subleading jets with pT > 50 GeV for tracks with 1 < pT < GeV 0-10% central events.

Total excess correlated yield observed in the PbPb data with respect to the reference measured in pp collisions, shown as a function of track pT in in centrality interval 50-100% for both leading jets with pT >120GeV and subleading jets with pT > 50 GeV.

Total excess correlated yield observed in the PbPb data with respect to the reference measured in pp collisions, shown as a function of track pT in in centrality interval 30-50% for both leading jets with pT >120GeV and subleading jets with pT > 50 GeV.

Total excess correlated yield observed in the PbPb data with respect to the reference measured in pp collisions, shown as a function of track pT in in centrality interval 10-30% for both leading jets with pT >120GeV and subleading jets with pT > 50 GeV.

Total excess correlated yield observed in the PbPb data with respect to the reference measured in pp collisions, shown as a function of track pT in in centrality interval 0-10% for both leading jets with pT >120GeV and subleading jets with pT > 50 GeV.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 50-100%.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 30-50%.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 10-30%.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 0-10%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 50-100%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 30-50%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 10-30%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 0-10%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 50-100%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 30-50%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 10-30%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 0-10%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 50-100%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 30-50%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 10-30%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to leading jets with pT > 120GeV, as a function of track pT for centrality interval 0-10%.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 50-100%.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 30-50%.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 10-30%.

Comparison of the widths in PbPb and pp of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 0-10%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 50-100%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 30-50%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 10-30%.

Difference of the widths in PbPb and pp data of the dEta charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 0-10%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 50-100%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 30-50%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 10-30%.

Comparison of the widths in PbPb and pp of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 0-10%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 50-100%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 30-50%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 30-50%.

Difference of the widths in PbPb and pp data of the dPhi charged-particle distributions correlated to subleading jets with pT > 50GeV, as a function of track pT for centrality interval 0-10%.

Mixed charge (- - - +) C4QS, a4QS, c4QS at high KT4 in pPb collisions projected against Q4.

Mixed charge (- - - +) C4QS, a4QS, c4QS at low KT4 in PbPb collisions projected against Q4. 0-5% Centrality. The varied c4QS represents an alternate calculation of the cumulant correlation function. By default, the three N2QS(+-)N1(+)N1(+) terms are subtracted. The varied c4QS leaves these terms unsubtracted. In the absence of pion coherence and perfect FSI correction, these terms should not contribute to the cumulant correlation function.

Mixed charge (- - - +) C4QS, a4QS, c4QS at high KT4 in PbPb collisions projected against Q4. 0-5% Centrality. The varied c4QS represents an alternate calculation of the cumulant correlation function. By default, the three N2QS(+-)N1(+)N1(+) terms are subtracted. The varied c4QS leaves these terms unsubtracted. In the absence of pion coherence and perfect FSI correction, these terms should not contribute to the cumulant correlation function.

Mixed charge (- - + +) C4QS, a4QS, c4QS at low KT4 in pp collisions projected against Q4.

Mixed charge (- - + +) C4QS, a4QS, c4QS at high KT4 in pp collisions projected against Q4.

Mixed charge (- - + +) C4QS, a4QS, c4QS at low KT4 in pPb collisions projected against Q4.

Mixed charge (- - + +) C4QS, a4QS, c4QS at high KT4 in pPb collisions projected against Q4.

Mixed charge (- - + +) C4QS, a4QS, c4QS at low KT4 in PbPb collisions projected against Q4. 0-5% Centrality. The varied c4QS represents an alternate calculation of the cumulant correlation function. By default, the four N2QS(+-)N1(+)N1(-) terms are subtracted. The varied c4QS leaves these terms unsubtracted. In the absence of pion coherence and perfect FSI correction, these terms should not contribute to the cumulant correlation function.

Mixed charge (- - + +) C4QS, a4QS, c4QS at high KT4 in PbPb collisions projected against Q4. 0-5% Centrality. The varied c4QS represents an alternate calculation of the cumulant correlation function. By default, the four N2QS(+-)N1(+)N1(-) terms are subtracted. The varied c4QS leaves these terms unsubtracted. In the absence of pion coherence and perfect FSI correction, these terms should not contribute to the cumulant correlation function.

Same charge C3QS, and c3QS at low KT3 in pp collisions projected against Q3. 0-5% Centrality. Edgeworth parameters for the C3QS fit are: s=1.217, R=2.351, kappa_3=0.592, kappa_4=0.240, kappa_5=-0.217, kappa_6=2.512. Edgeworth parameters for the c3QS fit are: s=1.089, R=1.894, kappa_3=-0.042, kappa_4=1.243, kappa_5=-2.189, kappa_6=2.780.

Same charge C3QS, and c3QS at low KT3 in pPb collisions projected against Q3. 0-5% Centrality. Edgeworth parameters for the C3QS fit are: s=1.058, R=2.680, kappa_3=0.287, kappa_4=0.960, kappa_5=-1.486, kappa_6=3.415. Edgeworth parameters for the c3QS fit are: s=1.300, R=3.613, kappa_3=0.276, kappa_4=1.293, kappa_5=-2.423, kappa_6=5.069.

Same charge C3QS, and c3QS at low KT3 in PbPb collisions projected against Q3. 0-5% Centrality. Edgeworth parameters for the C3QS fit are: s=1.061, R=11.326, kappa_3=0.152, kappa_4=0.847, kappa_5=-1.380, kappa_6=2.374. Edgeworth parameters for the c3QS fit are: s=1.278, R=14.173, kappa_3=-0.055, kappa_4=1.864, kappa_5=-3.460, kappa_6=4.624.

Same charge C4QS, a4QS, b4QS, c4QS, and ratios in pp collisions projected against Q4.

Same charge 4-pion expected correlations in pp collisions projected against Q4.

Same charge C4QS, a4QS, b4QS, c4QS, and ratios in pPb collisions projected against Q4.

Same charge 4-pion expected correlations in pPb collisions projected against Q4.

Same charge C4QS, a4QS, b4QS, c4QS, and ratios in PbPb collisions projected against Q4. 0-5% Centrality.

Same charge 4-pion expected correlations in PbPb collisions projected against Q4. 0-5% Centrality.

Same charge 3-pion measured and expected correlations at low KT3 in PbPb collisions projected against Q3. 0-5% Centrality.

Same charge 3-pion measured and expected correlations at high KT3 in PbPb collisions projected against Q3. 0-5% Centrality.

Same charge 4-pion measured correlations and ratio at low KT4 in PbPb collisions projected against Q4. 0-5% Centrality.

Same charge 4-pion expected correlations at low KT4 in PbPb collisions projected against Q4. 0-5% Centrality.

Same charge 4-pion measured correlations and ratio at high KT4 in PbPb collisions projected against Q4. 0-5% Centrality.

Same charge 4-pion expected correlations at high KT4 in PbPb collisions projected against Q4. 0-5% Centrality.

Same charge 4-pion expected correlations and ratio at low KT4 in PbPb collisions projected against Q4. 0-5% Centrality.

Same charge 3-pion expected correlations and ratio at low KT3 in PbPb collisions projected against Q3. 0-5% Centrality.

Coherent fractions (G) extracted from 4-pion correlations versus centrality for low and high KT4 in PbPb collisions.

Three-pion mixed-charge cumulant correlation functions for low and high KT3 in PbPb collisions.

Xi pt spectrum in 20-40% multiplicity class.

Xi pt spectrum in 40-60% multiplicity class.

Xi pt spectrum in 60-80% multiplicity class.

Xi pt spectrum in 80-100% multiplicity class.

Omega pt spectrum in 0-5% multiplicity class.

Omega pt spectrum in 5-10% multiplicity class.

Omega pt spectrum in 10-20% multiplicity class.

Omega pt spectrum in 20-40% multiplicity class.

Omega pt spectrum in 40-60% multiplicity class.

Omega pt spectrum in 60-80% multiplicity class.

Omega pt spectrum in 80-100% multiplicity class.

Mean pT of XI- in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV for each V0A multiplicity event class.

Mean pT of XIBAR+ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV for each V0A multiplicity event class.

Mean pT of OMEGA- in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV for each V0A multiplicity event class.

Mean pT of OMEGABAR+ in p-Pb collisions with centre-of-mass energy/nucleon=5.02 TeV for each V0A multiplicity event class.

XiMinus yield as a function of charged particle multiplicity per unit pseudorapidity.

XiPlus yield as a function of charged particle multiplicity per unit pseudorapidity.

OmegaMinus yield as a function of charged particle multiplicity per unit pseudorapidity.

OmegaPlus yield as a function of charged particle multiplicity per unit pseudorapidity.

Xi/pi ratio as a function of charged particle multiplicity per unit pseudorapidity.

Omega/pi ratio as a function of charged particle multiplicity per unit pseudorapidity.

No description provided.

No description provided.

No description provided.

three particle correlator, 3rd harmonic, difference neg-pos, as a function of centrality.

three particle correlator, 4th harmonic, as a function of centrality.

three particle correlator, 4th harmonic, difference neg-pos, as a function of centrality.

three particle correlator, 2nd harmonic, inferred slope parameter, as a function of centrality.

charge correlation, as a function of Delta eta.

three particle correlator, 2nd harmonic, as a function of Delta eta.

three particle correlator, 3rd harmonic, as a function of Delta eta.

three particle correlator, 4th harmonic, as a function of Delta eta.