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%.

No description provided.

No description provided.

No description provided.

Measured fiducial cross section in all $\ell^+\ell^-\ell'^+\ell'^-$ channels combined, where $\ell, \ell' = e, \mu$. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

Cross section extrapolated to total phase space and all Z boson decays. The first systematic uncertainty is the combined systematic uncertainty excluding luminosity uncertainty, the second is the luminosity uncertainty.

Optimised angular observables evaluated by the unbinned maximum likelihood fit. The first uncertainties are statistical and the second systematic.

CP-averaged angular observables evaluated using the method of moments. The first uncertainties are statistical and the second systematic.

CP-asymmetries evaluated using the method of moments. The first uncertainties are statistical and the second systematic.

Optimised observables evaluated using the method of moments. The first uncertainties are statistical and the second systematic.

Zero-crossing points determined with an amplitude fit.

Likelihood correlation matrix $0.1 < q^2 < 0.98~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $1.1 < q^2 < 2.5~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $2.5 < q^2 < 4.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $4.0 <q^2< 6.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $6.0 < q^2 < 8.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $11.0 <q^2< 12.5 ~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $15.0 < q^2 < 17.0 ~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $17.0 <q^2< 19.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $1.1 <q^2< 6.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $15.0 <q^2< 19.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $0.1 < q^2 < 0.98~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $1.1 < q^2 < 2.5~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $2.5 < q^2 < 4.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $4.0 <q^2< 6.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $6.0 < q^2 < 8.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $11.0 <q^2< 12.5 ~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $15.0 <q^2< 17.0 ~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $17.0 <q^2< 19.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $1.1 <q^2< 6.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $15.0 <q^2< 19.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $0.1 < q^2 < 0.98~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $1.1 < q^2 < 2.5~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $2.5 < q^2 < 4.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $4.0 <q^2< 6.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $6.0 < q^2 < 8.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $11.0 <q^2< 12.5 ~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $15.0 <q^2< 17.0 ~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $17.0 <q^2< 19.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $1.1 <q^2< 6.0~{\rm GeV}^2/c^4$.

Likelihood correlation matrix $15.0 <q^2< 19.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $0.10 < q^2 < 0.98~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $1.1 < q^2 < 2.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $2.0 < q^2 < 3.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $3.0 < q^2 < 4.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $4.0 < q^2 < 5.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $5.0 < q^2 < 6.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $6.0 < q^2 < 7.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $7.0 < q^2 < 8.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $11.00 <q^2 < 11.75~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $11.75 <q^2 < 12.50~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $15.0 <q^2 < 16.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $16.0 <q^2 < 17.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $17.0 <q^2 < 18.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $18.0 <q^2 < 19.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $15.0 <q^2 < 19.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $0.10 < q^2 < 0.98~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $1.1 < q^2 < 2.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $2.0 < q^2 < 3.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $3.0 < q^2 < 4.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $4.0 < q^2 < 5.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $5.0 < q^2 < 6.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $6.0 < q^2 < 7.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $7.0 < q^2 < 8.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $11.00 <q^2 < 11.75~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $11.75 <q^2 < 12.50~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $15.0 <q^2 < 16.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $16.0 <q^2 < 17.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $17.0 <q^2 < 18.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $18.0 <q^2 < 19.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $15.0 <q^2 < 19.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $0.1 <q^2 < 0.98~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $1.1 <q^2 < 2.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $2.0 <q^2 < 3.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $3.0 <q^2 < 4.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $4.0 <q^2 < 5.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $5.0 <q^2 < 6.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $6.0 <q^2 < 7.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $7.0 <q^2 < 8.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $11.0 <q^2 < 11.75~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $11.75 <q^2 < 12.5~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $15.0 <q^2 < 16.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $16.0 <q^2 < 17.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $17.0 < q^2 < 18.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $18.0 < q^2 < 19.0~{\rm GeV}^2/c^4$.

Bootstrap correlation matrix $15.0 < q^2 < 19.0~{\rm GeV}^2/c^4$.

Summary of results for cross-section of non-prompt $J/\psi$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of prompt $\psi(2S)$ decaying to a muon pair for 7 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of prompt $\psi(2S)$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of non-prompt $\psi(2S)$ decaying to a muon pair for 7 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for cross-section of non-prompt $\psi(2S)$ decaying to a muon pair for 8 TeV data in nb/GeV. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $J/\psi$ decaying to a muon pair as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $J/\psi$ decaying to a muon pair as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $\psi(2S)$ decaying to a muon pair as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt fraction of $\psi(2S)$ decaying to a muon pair as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 7 TeV data. Uncertainties are statistical and systematic, respectively.

Summary of results for non-prompt $\psi(2S)$ over $J/\psi$ ratio as a percentage for 8 TeV data. Uncertainties are statistical and systematic, respectively.

Mean weight correction factor for $J/\psi$ under the "longitudinal" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse zero" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse positive" spin-alignment transverse positive hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "transverse negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "longitudinal" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse zero" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "transverse negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 7 TeV.

Mean weight correction factor for $J/\psi$ under the "longitudinal" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse zero" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "transverse negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $J/\psi$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "longitudinal" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse zero" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "transverse negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane positive" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

Mean weight correction factor for $\psi(2S)$ under the "off-($\lambda_{\theta}$--$\lambda_{\phi}$)-plane negative" spin-alignment hypothesis for 8 TeV. Those intervals not measured in the analysis at low $p_{T}$, high rapidity are also excluded here.

The measured differential cross sections $\rm{d}\sigma/\rm{d}|\eta|$ of $D^{*\pm}$ and $D^\pm$ production with $20<p_T<100\,$GeV. The first and second errors are the statistical and systematic uncertainties, respectively. The systematic uncertainty fractions corresponding to the tracking ($\delta_2$) uncertainties (Table 2 of the paper) are strongly correlated. The fully correlated uncertainties linked with the luminosity measurement ($3.5\%$) and branching fractions ($1.5\%$ and $2.1\%$ for $D^{*\pm}$ and $D^\pm$, respectively) are not shown.

1$\sigma$ C.L. contour in $\sin^{2}\bar{\theta}_{23}$-$\Delta\bar{m}^{2}_{32}$ plane (inverted hierarchy).

90% C.L. contour in $\sin^{2}\bar{\theta}_{23}$-$\Delta\bar{m}^{2}_{32}$ plane (inverted hierarchy).

Best-fit point in $\sin^{2}\bar{\theta}_{23}$-$\Delta\bar{m}^{2}_{32}$ plane (inverted hierarchy).