The $\Lambda_{\rm {c}}^{+}$/${\rm D}^{0}$ ratio as a function of $p_{\rm {T}}$ measured in pp collisions at $\sqrt{s} = 5.02$ TeV in the rapidity interval $|y|<0.5$.

The $\Lambda_{\rm {c}}^{+}$/${\rm D}^{0}$ ratio as a function of $p_{\rm {T}}$ measured in p-Pb collisions at $\sqrt{s_{\rm {NN}}} = 5.02$ TeV in the rapidity interval $ -0.96\lt y \lt 0.04$.

The $\Lambda_{\rm {c}}^{+}$/${\rm D}^{0}$ ratio measured in p-Pb collisions at $\sqrt{s_{\rm {NN}}} = 5.02$ TeV in the transverse momentum interval $2 \lt p_{\rm T} \lt 12$ GeV/c and in the rapidity interval $-0.96 \lt y \lt 0.04$.

$p_{\rm {T}}$-integrated prompt $\Lambda_{\rm {c}}^{+}$ baryon cross section in pp collisions at $\sqrt{s} = 5.02$ TeV in the rapidity interval $|y|<0.5$, and in p-Pb collisions at $\sqrt{s_{\rm {NN}}} = 5.02$ TeV in the rapidity interval $-0.96 \lt y \lt 0.04$. First column: The $p_{\rm {T}}$-integrated cross section in the visible (measured) $p_{\rm {T}}$ region, which in pp collisions is $1 \lt p_{\rm T} \lt 12$ GeV/c and in p-Pb collisions is $1 \lt p_{\rm T} \lt 24$ GeV/c. The second (sys) error is from the luminosity uncertainty. Second column: The $p_{\rm {T}}$-integrated cross section extrapolated to all $p_{\rm {T}}$. The second (sys) error is from the luminosity uncertainty and the third (sys) error is from the extrapolation to the full $p_{\rm {T}}$ range.

$p_{\rm {T}}$-integrated ($p_{\rm {T}} > 0$) $\Lambda_{\rm {c}}^{+}$/${\rm D}^{0}$ ratio in pp collisions at $\sqrt{s} = 5.02$ TeV in the rapidity interval $|y|<0.5$, and in p-Pb collisions at $\sqrt{s_{\rm {NN}}} = 5.02$ TeV in the rapidity interval $-0.96 \lt y \lt 0.04$. The second (sys) error is from the extrapolation to the full $p_{\rm {T}}$ range.

Distributions of $\Delta\phi_{\mathrm{trk,Z}}$ in 30-50% centrality PbPb collisions at 5.02 TeV.

Distributions of $\Delta\phi_{\mathrm{trk,Z}}$ in 0-30% centrality PbPb collisions at 5.02 TeV.

PbPb - pp difference of $\Delta\phi_{\mathrm{trk,Z}}$ distributions for 70-90% centrality PbPb collisions at 5.02 TeV.

PbPb - pp difference of $\Delta\phi_{\mathrm{trk,Z}}$ distributions for 50-70% centrality PbPb collisions at 5.02 TeV.

PbPb - pp difference of $\Delta\phi_{\mathrm{trk,Z}}$ distributions for 30-50% centrality PbPb collisions at 5.02 TeV.

PbPb - pp difference of $\Delta\phi_{\mathrm{trk,Z}}$ distributions for 0-30% centrality PbPb collisions at 5.02 TeV.

Distributions of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ in pp collisions at 5.02 TeV.

Distributions of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ in 70-90% centrality PbPb collisions at 5.02 TeV.

Distributions of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ in 50-70% centrality PbPb collisions at 5.02 TeV.

Distributions of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ in 30-50% centrality PbPb collisions at 5.02 TeV.

Distributions of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ in 0-30% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ distributions for 70-90% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ distributions for 50-70% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ distributions for 30-50% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of $\xi^{\mathrm{trk,Z}}_{\mathrm{T}}$ distributions for 0-30% centrality PbPb collisions at 5.02 TeV.

Distributions of p$^{\mathrm{trk}}_{\mathrm{T}}$ in pp collisions at 5.02 TeV.

Distributions of p$^{\mathrm{trk}}_{\mathrm{T}}$ in pp collisions at 5.02 TeV.

Distributions of p$^{\mathrm{trk}}_{\mathrm{T}}$ in 70-90% centrality PbPb collisions at 5.02 TeV.

Distributions of p$^{\mathrm{trk}}_{\mathrm{T}}$ in 50-70% centrality PbPb collisions at 5.02 TeV.

Distributions of p$^{\mathrm{trk}}_{\mathrm{T}}$ in 30-50% centrality PbPb collisions at 5.02 TeV.

Distributions of p$^{\mathrm{trk}}_{\mathrm{T}}$ in 0-30% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of p$^{\mathrm{trk}}_{\mathrm{T}}$ distributions for 70-90% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of p$^{\mathrm{trk}}_{\mathrm{T}}$ distributions for 50-70% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of p$^{\mathrm{trk}}_{\mathrm{T}}$ distributions for 30-50% centrality PbPb collisions at 5.02 TeV.

PbPb / pp ratio of p$^{\mathrm{trk}}_{\mathrm{T}}$ distributions for 0-30% centrality PbPb collisions at 5.02 TeV.

RMS of raw subtracted $p_T$ for jets reconstructed in PbPb collisions (in different centrality bins) with the anti-k$_T$ algorythm with a distance parameter $R=0.3$, in $|\eta|<0.2$.

Inclusive jet cross section in pp collisions, for anti-k$_T$ jets with a distance parameter $R=0.2, 0.3, 0.4$, reconstructed in $|\eta|<0.2$. The '3.7%' luminosity uncertainty is a fully correlated uncertainty, and not included in the point-to-point uncertainty.

Inclusive jet spectra in different centrality bins of PbPb collisions, for anti-k$_T$ jets of distance parameter $R=0.2$, reconstructed in $|\eta|<0.2$. The PbPb spectra in each case are scaled by TAA. The uncertainty on the TAA is considered as global uncertainty (common to all points for a given centrality), and it is not included in the point-to-point uncertainties.

Inclusive jet spectra in different centrality bins of PbPb collisions, for anti-k$_T$ jets of distance parameter $R=0.3$, reconstructed in $|\eta|<0.2$. The PbPb spectra in each case are scaled by TAA. The uncertainty on the TAA is considered as global uncertainty (common to all points for a given centrality), and it is not included in the point-to-point uncertainties.

Inclusive jet spectra in different centrality bins of PbPb collisions, for anti-k$_T$ jets of distance parameter $R=0.4$, reconstructed in $|\eta|<0.2$. The PbPb spectra in each case are scaled by TAA. The uncertainty on the TAA is considered as global uncertainty (common to all points for a given centrality), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 0-5\% PbPb centrality. The '5.5%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 5-10\% PbPb centrality. The '5.9%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 10-30\% PbPb centrality. The '6.9%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 30-50\% PbPb centrality. The '10%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 50-70\% PbPb centrality. The '15%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 70-90\% PbPb centrality. The '18%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of average Npart, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, reconstructed in the range $80< p_T < 90$GeV/c and $|\eta|<2$.

Inclusive jet RAA as a function of average Npart, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, reconstructed in the range $130< p_T < 150$GeV/c and $|\eta|<2$.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3$, reconstructed in the range $|\eta|<2$, for 0-10\% PbPb centrality. The '5.7%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

x_J distribution of incluisve dijets in pp collisions

x_J distribution of b-quark dijets in pp collisions

x_J distribution of incluisve dijets in PbPb collisions (0-10%)

x_J distribution of b-quark dijets in PbPb collisions (0-10%)

x_J distribution of incluisve dijets in PbPb collisions (10-30%)

x_J distribution of b-quark dijets in PbPb collisions (10-30%)

x_J distribution of incluisve dijets in PbPb collisions (30-100%)

x_J distribution of b-quark dijets in PbPb collisions (30-100%)

Mean x_J of incluisve dijets in pp and PbPb collisions vs. number of participants

Mean x_J of b-quark dijets in pp and PbPb collisions vs. numberof participants

Mean x_J of inclusive jets and b-quark dijets in PbPb collisions minus mean x_J in pp collisions vs. numberof participants

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the leading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The distribution of charged particle yields within $|\Delta\varphi| < 1.0$ correlated with the subleading jets as a function of $\Delta\eta$ in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$. The PbPb results are shown for different centrality regions.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV. The PbPb results are shown for different centrality regions.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV. The PbPb results are shown for different centrality regions.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV. The PbPb results are shown for different centrality regions.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV. The PbPb results are shown for different centrality regions.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV. The PbPb results are shown for different centrality regions.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV. The PbPb results are shown for different centrality regions.

The leading jet radial momentum profiles in pp and PbPb collisions and a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV. The PbPb results are shown for different centrality regions.

The subleading jet radial momentum profiles in pp and PbPb collisions as a function of $\Delta r$ for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV. The PbPb results are shown for different centrality regions.

The ratio between leading jet radial momentum profiles in PbPb and pp collisions as a function of $\Delta r$.

The ratio between subleading jet radial momentum profiles in PbPb and pp collisions as a function of $\Delta r$.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for leading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for leading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for leading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for leading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for leading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Ratios of leading jet shapes between PbPb and pp collisions. The results from 0-10 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Ratios of leading jet shapes between PbPb and pp collisions. The results from 10-30 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Ratios of leading jet shapes between PbPb and pp collisions. The results from 30-50 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Ratios of leading jet shapes between PbPb and pp collisions. The results from 50-90 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $0.7 < p_{\mathrm{T}}^{\mathrm{ch}} < 1$ GeV.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $1 < p_{\mathrm{T}}^{\mathrm{ch}} < 2$ GeV.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $2 < p_{\mathrm{T}}^{\mathrm{ch}} < 3$ GeV.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $3 < p_{\mathrm{T}}^{\mathrm{ch}} < 4$ GeV.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $4 < p_{\mathrm{T}}^{\mathrm{ch}} < 8$ GeV.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $8 < p_{\mathrm{T}}^{\mathrm{ch}} < 12$ GeV.

Jet shapes for subleading jets in the 0-10 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for subleading jets in the 10-30 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for subleading jets in the 30-50 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for subleading jets in the 50-90 % centrality bin in PbPb collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Jet shapes for subleading jets in pp collisions. The results are shown in different dijet momentum balance bins for the charged particle $p_{\mathrm{T}}$ bin $12 < p_{\mathrm{T}}^{\mathrm{ch}} < 300$ GeV.

Ratios of subleading jet shapes between PbPb and pp collisions. The results from 0-10 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Ratios of subleading jet shapes between PbPb and pp collisions. The results from 10-30 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Ratios of subleading jet shapes between PbPb and pp collisions. The results from 30-50 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Ratios of subleading jet shapes between PbPb and pp collisions. The results from 50-90 % centrality bin in PbPb are compared to pp using several dijet momentum balance selections.

Ratio between unbalanced selection of leading jet shapes to all leading jet shapes in pp and PbPb collisions. The PbPb results are shown for different centrality regions.

Ratio between balanced selection of leading jet shapes to all leading jet shapes in pp and PbPb collisions. The PbPb results are shown for different centrality regions.

Ratio between unbalanced selection of subleading jet shapes to all subleading jet shapes in pp and PbPb collisions. The PbPb results are shown for different centrality regions.

Ratio between balanced selection of subleading jet shapes to all subleading jet shapes in pp and PbPb collisions. The PbPb results are shown for different centrality regions.

Generator-level vs. reconstructed $x_{j}$ values in the analysis $x_{j}$ bins. The plots show the probability to find a generator level $x_{j}$ for a given reconstructed $x_{j}$.

Generator-level vs. reconstructed $x_{j}$ values in the analysis $x_{j}$ bins. The plots show the probability to find a reconstructed $x_{j}$ for a given generator level $x_{j}$.

Invariant charged particle differential yield in the centrality regions 30 TO 50%, 50 TO 70% and 70 TO 90%.

Nuclear modification factor RAA in the centrality regions 0 TO 5%, 5 TO 10% and 10 TO 30%.

Nuclear modification factor RAA in the centrality regions 30 TO 50%, 50 TO 70% and 70 TO 90%.

TAA-scaled ratio of PT spectra in central and peripheral bins, RCP.

95% CL intervals on the double ratio of measured yields, $(N_{\varUpsilon(3S)} / N_{\varUpsilon(1S)})_{\mathrm{PbPb}} / (N_{\varUpsilon(3S)} / N_{\varUpsilon(1S)})_{pp}$, as a function of centrality, for upsilon $|y|<2.4$ and $p_T<30$GeV, and $p_{T}^{\mu}>4$GeV.

68% CL intervals on the double ratio of measured yields, $(N_{\varUpsilon(3S)} / N_{\varUpsilon(1S)})_{\mathrm{PbPb}} / (N_{\varUpsilon(3S)} / N_{\varUpsilon(1S)})_{pp}$, as a function of centrality, for upsilon $|y|<2.4$ and $p_T<30$GeV, and $p_{T}^{\mu}>4$GeV.

Spectra of jets with |eta jet| < 2.0 for R = 0.6, for pp collisions and different centrality classes of PbPb collisions.

Spectra of jets with |eta jet| < 2.0 for R = 0.8, for pp collisions and different centrality classes of PbPb collisions.

Spectra of jets with |eta jet| < 2.0 for R = 1.0, for pp collisions and different centrality classes of PbPb collisions.

The spectra ratio for jets from pp collisions with |eta jet| < 2.0 for R = 0.2–0.8 with respect to R = 1.0.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.2 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.3 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.4 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.6 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.8 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 1.0 and various centrality classes.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 200-250 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 250-300 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 300-400 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 400-500 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 500-1000 GeV.

Detector-level photon $\phi$ distribution

Detector-level dipoton invariant mass distribution

Detector-level diphoton rapidity distribution

Detector-level dipoton p$_{T}$ distribution

Observed exclusion limits at 95% CL in the ALP-photon coupling g$_{a \gamma}$ versus ALP mass $m_{a}$ plane.

The R$_{AA}$ of $B^{0}_{s}$ measured in PbPb collisions at $\sqrt(s_{_{NN}})=5.02$TeV from 7 to 50GeV/c. The global uncertainty comprises the uncertainties in the pp integrated luminosity measurement and $\rm{T_{AA}}$.

The R$_{AA}$ ratio between $B^{0}_{s}$ and $B^{+}$ mesons measured in PbPb collisions at $\sqrt(s_{_{NN}})=5.02$TeV from 7 to 50GeV/c.

No description provided.

No description provided.

No description provided.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ in 10-20% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ in 20-30% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ in 30-40% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ in 40-50% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ in 50-60% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 0-0.2% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 0-5% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 0-10% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 10-20% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 20-30% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 30-40% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 40-50% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ in 50-60% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ for multiplicity class $220 \leq N^{offline}_{trk}<260$ in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ for multiplicity class $185 \leq N^{offline}_{trk}<220$ in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ for multiplicity class $150 \leq N^{offline}_{trk}<185$ in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) elliptic flow, $v^{(\alpha)}_2$, as a function of $p_T$ $120 \leq N^{offline}_{trk}<150$ in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ for multiplicity class $220 \leq N^{offline}_{trk}<260$ in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ for multiplicity class $185 \leq N^{offline}_{trk}<220$ in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ for multiplicity class $150 \leq N^{offline}_{trk}<185$ in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) triangular flow, $v^{(\alpha)}_3$, as a function of $p_T$ for multiplicity class $120 \leq N^{offline}_{trk}<150$ in pPb collisions.

Pearson correlation coefficients $r_2$ and $r_3$ reconstructed using the leading and subleading flows as a function of $p^{a}_{T} - p^{b}_{T}$ in bin $p^{a}_{T}$ for centrality class 0-0.2% in PbPb collisions.

Pearson correlation coefficients $r_2$ and $r_3$ reconstructed using the leading and subleading flows as a function of $p^{a}_{T} - p^{b}_{T}$ in bin $p^{a}_{T}$ for centrality class 0-5% in PbPb collisions.

Pearson correlation coefficients $r_2$ and $r_3$ reconstructed using the leading and subleading flows as a function of $p^{a}_{T} - p^{b}_{T}$ in bin $p^{a}_{T}$ for centrality class 10-20% in PbPb collisions.

Pearson correlation coefficients $r_2$ and $r_3$ reconstructed using the leading and subleading flows as a function of $p^{a}_{T} - p^{b}_{T}$ in bin $p^{a}_{T}$ for centrality class 20-30% in PbPb collisions.

Pearson correlation coefficients $r_2$ and $r_3$ reconstructed using the leading and subleading flows as a function of $p^{a}_{T} - p^{b}_{T}$ in bin $p^{a}_{T}$ for centrality class 30-40% in PbPb collisions.

Pearson correlation coefficients $r_2$ and $r_3$ reconstructed using the leading and subleading flows as a function of $p^{a}_{T} - p^{b}_{T}$ in bin $p^{a}_{T}$ for centrality class 40-50% in PbPb collisions.

Elliptic and triangular ratios of subleading and leading flow as a function of multiplicity for the highest bin 2.5 < $p_T$ < 3.0 GeV in PbPb collisions.

Elliptic and triangular ratios of subleading and leading flow as a function of multiplicity for the highest bin 2.5 < $p_T$ < 3.0 GeV in pPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 0-0.2% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 0-5% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 0-10% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 10-20% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 20-30% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 30-40% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 40-50% centrality PbPb collisions.

Leading ($\alpha$ = 1) and subleading ($\alpha$ = 2) multiplicity modes, $v^{(\alpha)}_0$, as a function of $p_T$ in 50-60% centrality PbPb collisions.

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%.

The standard deviation of the jet charge distributions with different track $p_{T}$ thresholds and $\kappa$ value pf 0.7 for pp collisions and in the various event centrality bins for PbPb collisions compared with the PYTHIA6 prediction.

Fitting results for the extraction of gluon-like jet fractions in pp and PbPb data shown for different track $p_{T}$ threshold values and $p_{T}$-weighting factor $\kappa$ values of 0.5.

Fitting results for the extraction of gluon-like jet fractions in pp and PbPb data shown for $p_{T}$-weighting factor $\kappa$ values of 0.3, 0.5, and 0.7 and minimum track $p_{T}$ of 1 GeV.

Fitting results for the extraction of gluon-like jet fractions in pp and PbPb data shown for $p_{T}$-weighting factor $\kappa$ values of 0.3, 0.5, and 0.7 and minimum track $p_{T}$ of 2 GeV.

Unfolded jet charge measurements for the $p_{T}$-weighting factor $\kappa = 0.5$ and a minimum track $p_{T}$ of 2 GeV for inclusive jets in pp and PbPb data. The PbPb results are shown for different centrality regions.

Unfolded jet charge measurements for the $p_{T}$-weighting factor $\kappa = 0.5$ and a minimum track $p_{T}$ of 4 GeV for inclusive jets in pp and PbPb data. The PbPb results are shown for different centrality regions.

Unfolded jet charge measurements for the $p_{T}$-weighting factor $\kappa = 0.5$ and a minimum track $p_{T}$ of 5 GeV for inclusive jets in pp and PbPb data. The PbPb results are shown for different centrality regions.

Unfolded jet charge measurements for a minimum track $p_{T}$ threshold of 1 GeV and $p_{T}$-weighting factor $\kappa = 0.3$ for inclusive jets in pp and PbPb data. The PbPb results are shown for different centrality regions.

Unfolded jet charge measurements for a minimum track $p_{T}$ threshold of 1 GeV and $p_{T}$-weighting factor $\kappa = 0.7$ for inclusive jets in pp and PbPb data. The PbPb results are shown for different centrality regions.

Unfolded jet charge measurements for a minimum track $p_{T}$ threshold of 2 GeV and $p_{T}$-weighting factor $\kappa = 0.3$ for inclusive jets in pp and PbPb data. The PbPb results are shown for different centrality regions.

Unfolded jet charge measurements for a minimum track $p_{T}$ threshold of 2 GeV and $p_{T}$-weighting factor $\kappa = 0.7$ for inclusive jets in pp and PbPb data. The PbPb results are shown for different centrality regions.

The $ {{{\mathrm {B}}}\to {\mathrm {D^0}}} $ nuclear modification factor $ {R_{\mathrm {AA}}} $ for PbPb collisions at ${\sqrt {\smash [b]{s_{_{\mathrm {NN}}}}}} = $ 5.02 TeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV.

The ratio of theory to data, for the ratio of the pPb to pp $\eta_{\mathrm{dijet}}$ spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV. The total uncertainties on the data points are provided in the column entitled 'DATA UNCERTAINTIES'. The theory points are from the NLO pQCD calculations of DSSZ, EPS09, nCTEQ15, and EPPS16 nPDFs, using CT14 as the baseline PDF.

The ratio of theory to data, for the ratio of the pPb to pp $\eta_{\mathrm{dijet}}$ spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV. The total uncertainties on the data points are provided in the column entitled 'DATA UNCERTAINTIES'. The theory points are from the NLO pQCD calculations of DSSZ, EPS09, nCTEQ15, and EPPS16 nPDFs, using CT14 as the baseline PDF.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the MMHT14 as the baseline PDF.

$v_{2}$ of $\Upsilon(\mathrm{1S})$ as a function of $p_{\mathrm{T}}$ in three centrality ranges, 10-30%, 30-50% and 50-90%.

$v_{2}$ of $\Upsilon(\mathrm{1S})$ as a function of $p_{\mathrm{T}}$ in 5-60% centrality range.

Neutron multiplicity dependence of acoplanarity ($\alpha$) from process $\gamma\gamma$ to $\mu^+\mu^-$ in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV.

Neutron multiplicity dependence of acoplanarity ($\alpha$) from process $\gamma\gamma$ to $\mu^+\mu^-$ in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV.

Neutron multiplicity dependence of acoplanarity ($\alpha$) from process $\gamma\gamma$ to $\mu^+\mu^-$ in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV.

Neutron multiplicity dependence of average core acoplanarity ($<\alpha^{core}>$) distributions from process $\gamma\gamma$ to $\mu^+\mu^-$ in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV.

Neutron multiplicity dependence of average invariant mass ($<m_{\mu\mu}>$) from process $\gamma\gamma$ to $\mu^+\mu^-$ in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV.

Acoplanarity ($\alpha$) distributions from process $\gamma\gamma$ to $\mu^+\mu^-$ for 0n1n class in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV. Dimuon rapidity is in the hemisphere containing larger neutron multiplicity.

Acoplanarity ($\alpha$) distributions from process $\gamma\gamma$ to $\mu^+\mu^-$ for 0nXn class in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV. Dimuon rapidity is in the hemisphere containing larger neutron multiplicity.

Acoplanarity ($\alpha$) distributions from process $\gamma\gamma$ to $\mu^+\mu^-$ for 1nXn class in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV. Dimuon rapidity is in the hemisphere containing larger neutron multiplicity.

Acoplanarity ($\alpha$) distributions from process $\gamma\gamma$ to $\mu^+\mu^-$ for 0n1n class in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV. Dimuon rapidity is in the hemisphere containing smaller neutron multiplicity.

Acoplanarity ($\alpha$) distributions from process $\gamma\gamma$ to $\mu^+\mu^-$ for 0nXn class in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV. Dimuon rapidity is in the hemisphere containing smaller neutron multiplicity.

Acoplanarity ($\alpha$) distributions from process $\gamma\gamma$ to $\mu^+\mu^-$ for 1nXn class in ultraperipheral PbPb at $\sqrt{s_{NN}}=5.02$ TeV. Dimuon rapidity is in the hemisphere containing smaller neutron multiplicity.

The $v_{2}$ result from SP method as a function of $p_{T}$ in 20-30\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from SP method as a function of $p_{T}$ in 30-40\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from SP method as a function of $p_{T}$ in 40-50\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from SP method as a function of $p_{T}$ in 50-60\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{3}$ result from SP method as a function of $p_{T}$ in 0-5\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{3}$ result from SP method as a function of $p_{T}$ in 5-10\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{3}$ result from SP method as a function of $p_{T}$ in 10-20\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{3}$ result from SP method as a function of $p_{T}$ in 20-30\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{3}$ result from SP method as a function of $p_{T}$ in 30-40\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{3}$ result from SP method as a function of $p_{T}$ in 40-50\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{3}$ result from SP method as a function of $p_{T}$ in 50-60\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from 4-, 6- and 8-particle cumulant methods as a function of $p_{T}$ in 5-10\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from 4-, 6- and 8-particle cumulant methods as a function of $p_{T}$ in 10-20\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from 4-, 6- and 8-particle cumulant methods as a function of $p_{T}$ in 20-30\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from 4-, 6- and 8-particle cumulant methods as a function of $p_{T}$ in 30-40\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from 4-, 6- and 8-particle cumulant methods as a function of $p_{T}$ in 40-50\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}$ result from 4-, 6- and 8-particle cumulant methods as a function of $p_{T}$ in 50-60\% centrality bin of PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. Shaded boxes represent systematic uncertainties.

The $v_{2}^{high}$ as a function of $v_{2}^{low}$ results from SP method in PbPb collisions at $sqrt{s_{NN}}$ = 5.02 TeV. Only statistical uncertainties are shown.

The $v_{2}^{high}$ as a function of $v_{2}^{low}$ results from 4-particle cumulant method in PbPb collisions at $sqrt{s_{NN}}$ = 5.02 TeV. Only statistical uncertainties are shown.

95% CL intervals on the double ratio of measured yields, $(N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{\mathrm{PbPb}} / (N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{pp}$, as a function of pT, for the forward rapidity analysis bin.

Double ratio of measured yields, $(N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{\mathrm{PbPb}} / (N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{pp}$, as a function of centrality, for the midrapidity analysis bin.

95% CL intervals on the double ratio of measured yields, $(N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{\mathrm{PbPb}} / (N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{pp}$, as a function of centrality, for the midrapidity analysis bin.

Double ratio of measured yields, $(N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{\mathrm{PbPb}} / (N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{pp}$, as a function of centrality, for the forward rapidity analysis bin.

95% CL intervals on the double ratio of measured yields, $(N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{\mathrm{PbPb}} / (N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{pp}$, as a function of centrality, for the forward rapidity analysis bin.

Double ratio of measured yields, $(N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{\mathrm{PbPb}} / (N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{pp}$, integrated over centrality, for the midrapidity and forward rapidity analysis bins.

95% CL interval on the double ratio of measured yields, $(N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{\mathrm{PbPb}} / (N_{\psi\mathrm{(2S)}} / N_{J/\psi})_{pp}$, integrated over centrality, for the midrapidity and forward rapidity analysis bins.

Nuclear modification factor RAA of psi(2S) integrated over centrality, for the midrapidity and forward rapidity analysis bins.

The b-jet yield as a function of pT is for the 30-50% centrality class of PbPb collisions. The yields are scaled by the equivalent number of minimum bias events sampled and by TAA.

The b-jet yield as a function of pT is for the 50-100% centrality class of PbPb collisions. The yields are scaled by the equivalent number of minimum bias events sampled and by TAA.

The b-jet cross section as a function of pT in pp collisions.

The b-jet nuclear modification factor as a function of the pT for the centrality class 0-100%.

The b-jet nuclear modification factor as a function of centrality for 80 < jet pT < 90 GeV/c.

The b-jet nuclear modification factor as a function centrality for 80 < jet pT < 90 GeV/c.

The b-jet nuclear modification factor as a function of the pT for the centrality class 0-10%.

The b-jet nuclear modification factor as a function of the pT for the centrality class 10-30%.

The b-jet nuclear modification factor as a function of the pT for the centrality class 30-50%.

The b-jet nuclear modification factor as a function of the pT for the centrality class 50-100%.

Differential cross section of J/psi mesons from b hadrons as a function of dimuon pT in pp and PbPb collisions. The PbPb cross sections are normalised by TAA for direct comparison. Global uncertainties arise from the integrated luminosity uncertainty in pp collisions, and the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross section of prompt J/psi mesons as a function of dimuon rapidty in pp and PbPb collisions. The PbPb cross sections are normalised by TAA for direct comparison. Global uncertainties arise from the integrated luminosity uncertainty in pp collisions, and the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross section of J/psi mesons from b hadrons as a function of dimuon rapidty in pp and PbPb collisions. The PbPb cross sections are normalised by TAA for direct comparison. Global uncertainties arise from the integrated luminosity uncertainty in pp collisions, and the number of minimum bias events and TAA uncertainties for PbPb collisions.

Nuclear modification factor of prompt J/psi mesons as a function of dimuon rapidity. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of collision centrality. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of dimuon pT. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of dimuon pT in the mid-rapidity interval. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of dimuon pT in the most forward rapidity interval. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of collision centrality in the mid- and most forward rapidity intervals. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of pT in three centrality bins. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of collision centrality in the most forward rapidity range at moderate and high pT. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of collision centrality in the mid-rapidity range. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of prompt psi(2S) mesons as a function of collision centrality in the mid-rapidity range. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

95% CL intervals on the nuclear modification factor of prompt psi(2S) mesons as a function of collision centrality in the mid-rapidity range. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of prompt J/psi and psi(2S) mesons as a function of dimuon pT in the mid-rapidity range. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of collision centrality in the forward rapidity range. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of prompt psi(2S) mesons as a function of collision centrality in the forward rapidity range. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

95% CL intervals on the nuclear modification factor of prompt psi(2S) mesons as a function of collision centrality in the forward rapidity range. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of prompt J/psi mesons as a function of dimuon pT in the forward rapidity range. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of prompt psi(2S) mesons as a function of dimuon pT in the forward rapidity range. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

95% CL intervals on the nuclear modification factor of prompt psi(2S) mesons as a function of dimuon pT in the forward rapidity range. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of dimuon rapidity. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of collision centrality. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of dimuon pT. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of dimuon pT in the mid-rapidity interval. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of dimuon pT in the most forward rapidity interval. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of collision centrality in the mid- and most forward rapidity intervals. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of pT in three centrality bins. Global uncertainties arise from the integrated luminosity uncertainty of the pp data, and the number of minimum bias events and TAA uncertainties of the PbPb data.

Nuclear modification factor of nonprompt J/psi mesons as a function of collision centrality in the most forward rapidity range at moderate and high pT. Global uncertainties arise from the full pp statistical and systematic uncertainties (including integrated luminosity uncertainty), and the number of minimum bias events uncertainty of the PbPb data.

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

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

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

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

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

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

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

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

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

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

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

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

b-jet Fraction.

b-jet RpA(PYTHIA).

The acceptance- and efficiency-corrected yields for the $\mathrm{B}^{+}$ mesons, scaled by $T_{\mathrm{AA}}$ and $N_{\text{MB}}$ in PbPb collisions at $\sqrt{s_{NN}}=5.02$ TeV. The results are shown as a function of the event $\langle N_{part} \rangle$.

The acceptance- and efficiency-corrected $\mathrm{B}^{0}_{\mathrm{s}}/\mathrm{B}^{+}$ yields in PbPb collisions at $\sqrt{s_{NN}}=5.02$. TeV. The results are shown as a function of the meson $p_T$.

The acceptance- and efficiency-corrected $\mathrm{B}^{0}_{\mathrm{s}}/\mathrm{B}^{+}$ yields in PbPb collisions at $\sqrt{s_{NN}}=5.02$. The results are shown as a function of the event $\langle N_{part} \rangle$.

Charged particle yield distributions $Y(\Delta r)$ of b jets with $1 < p_{\text{T}}^{\text{trk}} < 12$ GeV are presented as functions of $\Delta r$.b jets with $p_T > 120$ GeV and charged particles with $1 < p^{\text{trk}}_{\text{T}} < 12$ GeV are used to construct the distributions as functions of $\Delta r$ differential $p_{\text{T}}^{\text{trk}}$ bins.

Charged particle yield differences of b to inclusive jets for $1 < p_{\text{T}}^{\text{trk}} < 12$ GeV are presented as functions of $\Delta r$.b jets with $p_T > 120$ GeV and charged particles with $1 < p^{\text{trk}}_{\text{T}} < 12$ GeV are used to construct the distributions as functions of $\Delta r$ differential $p_{\text{T}}^{\text{trk}}$ bins.

The jet shapes $\rho(\Delta r)$ of inclusive jets with $p_{\text{T}} > 120$ GeV and $p^{trk}_T > 1$ GeV are presented as functions of $\Delta r$ for differential $p_{\text{T}}^{\text{trk}}$ bin.

The jet shape distributions $\rho(\Delta r)$ of b jets with $p_{\text{T}} > 120$ GeV and $1< p^{\text{trk}}_{\text{T}} < 12$ GeV are presented as functions of $\Delta r$ for differential $p_{\text{T}}^{\text{trk}}$ bin.

The jet shapes $\rho (\Delta r)$ of inclusive jets with $p_{\text{T}} > 120$ GeV and $p^{\text{trk}}_{\text{T}} > 1$ GeV are presented as functions of $\Delta r.

The jet shapes $\rho (\Delta r)$ of b jets with $p_{\text{T}} > 120$ GeV and $p^{\text{trk}}_{\text{T}} > 1$ GeV are presented as functions of $\Delta r.

The b-to-inclusive jet shape ratios for $p_{\text{T}} > 120$ GeV and $p^{\text{trk}}_{\text{T}} > 1$ GeV are presented as functions of $\Delta r.

The nuclear modification factor R$_{\rm AA}$, as a function of $z$ in the 0-20 and 20-30 collisions centrality ranges.

The $\langle x_{\mathrm{j}\gamma} \rangle$ and $R_{\mathrm{j}\gamma}$, the number of associated jets per photon, in 0-30% and 30-100% centrality PbPb collisions. The smeared pp data are added for comparison. A value of 999 in the bin range indicates that there is no upper limit.

The $I_{\mathrm{AA}}^{\mathrm{jet}}$ vs. $p_{\mathrm{T}}^{\mathrm{jet}}$ for 0-30% and 30-100% centrality PbPb collisions. Bins for which there are no data points are denoted as 'empty'.

The centrality dependence of $x_{\mathrm{j}\gamma}$ of photon+jet pairs normalized by the number of photons for PbPb and smeared pp data. Empty bins are denoted as 'empty' in the table.

The $\langle x_{\mathrm{j}\gamma} \rangle$ and $R_{\mathrm{j}\gamma}$ as a function of $\langle N_{\mathrm{part}} \rangle$ for $p_{\mathrm{T}}^{\gamma} > 60$ and 80 GeV. The PbPb results are compared to pp results smeared by the relative jet energy resolution corresponding to each centrality interval.

The measured Z boson production cross section in pp collisions as a function of the Z boson rapidity for the dielectron decay channel.

The measured Z boson production cross section in pp collisions as a function of the Z boson rapidity for the combined leptonic decay channel.

The measured Z boson production cross section in pp collisions as a function of the Z boson pT for the combined leptonic decay channel in |y|<1.44.

Charged-hadron pseudorapidity density in XeXe collisions at $\sqrt{s_{NN}} = 5.44$ TeV at midrapidity, normalised by $2A$, where $A$ is the atomic number of the nuclei, as a function of event centrality. The total uncertainty is dominated by the systematic uncertainty, and statistical uncertainties are negligible.

Average charged-hadron pseudorapidity density at midrapidity normalised by $\langle N_{part} \rangle$, shown as a function of $\langle N_{part} \rangle$. The total uncertainty is dominated by the systematic uncertainty, and statistical uncertainties are negligible.

Average charged-hadron pseudorapidity density at midrapidity normalised by $\langle N_{part} \rangle$, shown as a function of $\langle N_{part} \rangle/2A$, where $A$ is the atomic number of the nuclei. The total uncertainty is dominated by the systematic uncertainty, and statistical uncertainties are negligible.

Average charged-hadron pseudorapidity density at midrapidity normalised by $2A$, shown as a function of $\langle N_{part} \rangle/2A$, where $A$ is the atomic number of the nuclei. The total uncertainty is dominated by the systematic uncertainty, and statistical uncertainties are negligible.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.0<p^{trig}_{T}<1.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $1.5<p^{trig}_{T}<2.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.0<p^{trig}_{T}<2.5$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ for $2.5<p^{trig}_{T}<3.0$ GeV/c for centrality 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $220<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $150<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{3}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $120<=N^{offline}_{trk}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $100<=N^{offline}_{trk}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.0<p^{trig}_{T}<1.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $1.5<p^{trig}_{T}<2.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.0<p^{trig}_{T}<2.5$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $p_{T}$-dependent factorization ratio, $r_{2}$, as a function of $p^{a}_{T} - p^{b}_{T}$ with $2.5<p^{trig}_{T}<3.0$ GeV/c and multiplicity bin $185<=N^{offline}_{trk}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Factorization ratio, $r_{2}$, as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

Factorization ratio, $r_{3}$, as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

Factorization ratio, $r_{2}$, as a function of event multiplicity in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Factorization ratio, $r_{3}$, as a function of event multiplicity in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{2}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-5% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 5-10% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 10-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-30% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 30-40% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 40-50% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{3}$, as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 50-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 3.0<$\eta_b$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 3.0<$\eta_b$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 3.0<$\eta_b$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 4.4<$\eta_b$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-0.2% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 4.4<$\eta_b$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 0-20% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The $\eta$-dependent factorization ratio, $r_{4}$, as a function of $\eta^{a}$ for 4.4<$\eta_b$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for centrality class 20-60% in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $120<=N_{trk}^{offline}<150$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $150<=N_{trk}^{offline}<185$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $185<=N_{trk}^{offline}<220$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^{a}, \eta^{b}){\cdot(-\eta^{a}, -\eta^{b})}}$ a function of $\eta^{a}$ for 3.0<$\eta^{b}$<4.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for multiplicity bin $220<=N_{trk}^{offline}<260$ in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The square root of the product of factorization ratios $\sqrt{r_2(\eta^a, \eta^b)\cdot{r_2(-\eta^{a}, -\eta^{b})}}$ as a function of $\eta^{a}$ for 4.4<$\eta^{b}$<5.0 averaged over 0.3<$p^{a}_{T}$<3 GeV for a given multiplicity class in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

$F^{\eta}_2$ as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

$F^{\eta}_3$ as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

$F^{\eta}_4$ as a function of event multiplicity in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV.

$F^{\eta}_2$ as a function of event multiplicity in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Summary of the systematic uncertainties on the ratio RMN.

Summary of the systematic uncertainties on the ratio Rincl_veto.

Summary of the systematic uncertainties on the ratio RMN_veto.

Differential cross section dσincl/d∆y for inclusive dijet production together with predictions of different MC models.

Differential cross section dσMN/d∆y for Mueller-Navelet dijet production together with predictions of different MC models.

Ratio Rincl of the cross sections for inclusive to ”exclusive” dijet production together with predictions of different MC models.

Ratio Rincl_veto of the cross sections for inclusive to ”exclusive” with veto dijet production together with predictions of different MC models.

Ratio RMN of the cross sections for Mueller-Navelet to ”exclusive” dijet production together with predicgtion of different MC models.

Ratio RMN_veto of the cross sections for Mueller-Navelet to ”exclusive” with veto dijet production together with predictions of different MC models.

Summary of the systematic uncertainties on the cross section dσincl/d∆y.

Summary of the systematic uncertainties on the cross section dσMN/d∆y.

Summary of the systematic uncertainties on the ratio Rincl.

Summary of the systematic uncertainties on the ratio RMN.

Summary of the systematic uncertainties on the ratio Rincl_veto.

Summary of the systematic uncertainties on the ratio RMN_veto.

Differential cross section dσincl/d∆y for inclusive dijet production together with predictions of different MC models.

Differential cross section dσMN/d∆y for Mueller-Navelet dijet production together with predictions of different MC models.

Ratio Rincl of the cross sections for inclusive to ”exclusive” dijet production together with predictions of different MC models.

Ratio Rincl_veto of the cross sections for inclusive to ”exclusive” with veto dijet production together with predictions of different MC models.

Ratio RMN of the cross sections for Mueller-Navelet to ”exclusive” dijet production together with predicgtion of different MC models.

Ratio RMN_veto of the cross sections for Mueller-Navelet to ”exclusive” with veto dijet production together with predictions of different MC models.

The difference between the PbPb and pp measurements from Table 3.

The distribution of jet-correlated charged-particle tracks as a function of $\Delta\mathrm{r}$ in pp and PbPb collisions. The PbPb results are shown for different centrality regions.

The difference between the PbPb and pp measurements from Table 5.

The distribution of jet-correlated charged-particle tracks with $\Delta\mathrm{r} <1$ as a function of ${p_{\mathrm{T}}^{\text{trk}}}$ in PbPb and pp collisions. The PbPb results are shown for different centrality regions.

The corresponding results for the difference between the PbPb and pp measurements from Table 7.

The radial jet momentum distribution $\mathrm{P}(\Delta\mathrm{r})$ of jets in pp and PbPb collisions. The PbPb results are shown for different centrality regions.

The ratio between PbPb and pp measurements from Table 9 for the indicated intervals of ${p_{\mathrm{T}}^{\text{trk}}}$.

The jet shape $\rho(\Delta\mathrm{r})$ in pp and PbPb collisions. The PbPb results are shown for different centrality regions.

The ratio between the PbPb and pp measurements from Table 11 for the inclusive range $0.7< {p_{\mathrm{T}}^{\text{trk}}} <300GeV$.

Differential cross section (multiplied by the dimuon branching fraction) of prompt $\psi$(2S) mesons in pPb collisions at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, as a function of $p_{\textrm{T}}$, for three forward $y_{\mathrm{CM}}$ regions. The fully correlated luminosity uncertainty of 3.5% is not included in the point-by-point uncertainty. NOTE- The cross section unit is nb (nano barn); the y-axes of the figures in the publication show pb (pico barn) by mistake.

Differential cross section (multiplied by the dimuon branching fraction) of prompt $\psi$(2S) mesons in pp collisions at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, as a function of $p_{\textrm{T}}$, for four $y_{\mathrm{CM}}$ regions. The fully correlated luminosity uncertainty of 2.3% is not inlcuded in the point-by-point uncertainty.

Differential cross section (multiplied by the dimuon branching fraction) of prompt $\psi$(2S) mesons in pp collisions at $\sqrt(s)=5.02 $ TeV, as a function of $p_{\textrm{T}}$, for four $y_{\mathrm{CM}}$ regions. The fully correlated luminosity uncertainty of 2.3% is not included in the point-by-point uncertainty. NOTE- The cross section unit is nb (nano barn); the y-axes of the figures in the publication show pb (pico barn) by mistake.

Rapidity dependence of $R_{\mathrm{pPb}}$ for prompt $\psi$(2S) mesons at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, in three $p_{\mathrm{T}}$ ranges. The fully correlated global uncertainty of 4.2% is not inlcuded in the point-by-point uncertainty.

Rapidity dependence of $R_{\mathrm{pPb}}$ for prompt $\psi$(2S) mesons at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, in three $p_{\mathrm{T}}$ ranges. The fully correlated global uncertainty of 4.2% is not included in the point-by-point uncertainty.

Transverse momentum dependence of $R_{\mathrm{pPb}}$ for prompt $\psi$(2S) mesons at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, in seven $y_{\mathrm{CM}}$ ranges. The fully correlated global uncertainty of 4.2% is not inlcuded in the point-by-point uncertainty.

Transverse momentum dependence of $R_{\mathrm{pPb}}$ for prompt $\psi$(2S) mesons at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, in seven $y_{\mathrm{CM}}$ ranges. The fully correlated global uncertainty of 4.2% is not incuded in the point-by-point uncertainty.

The inclusive charged particle invariant differential cross section, as a function of XT and scaled by sqrt(s)*4.9, at 7 TeV for |eta|<1.

The interpolated invariant charged particle differential cross section at 2.76 GeV for |eta|<1.

Ratio rho_PbPb(dR)/rho_pp(dR) of leading jet shape for peripheral PbPb data (centrality 50-100%) to leading jet shape for pp data.

Ratio rho_PbPb(dR)/rho_pp(dR) of leading jet shape for central PbPb data (centrality 0-30%) to leading jet shape for pp data.

Subleading jet shape rho(dR) versus dR for pp data, normalized to unity over the range dR < 0.3.

Subleading jet shape rho(dR) versus dR for peripheral PbPb data (centrality 50-100%), normalized to unity over the range dR < 0.3.

Subleading jet shape rho(dR) versus dR for central PbPb data (centrality 0-30%), normalized to unity over the range dR < 0.3.

Ratio rho_PbPb(dR)/rho_pp(dR) of subleading jet shape for peripheral PbPb data (centrality 50-100%) to subleading jet shape for pp data.

Ratio rho_PbPb(dR)/rho_pp(dR) of subleading jet shape for central PbPb data (centrality 0-30%) to subleading jet shape for pp data.

Difference of the total track transverse momentum distributions between subleading and leading hemispheres in pp data (denoted d, projected into relative azimuth, for balanced dijets with Aj < 0.22.

Difference of the total track transverse momentum distributions (P = 1/N dSum(pT)/dPhi) between subleading and leading hemispheres in peripheral PbPb data (centrality 50-100%), projected into relative azimuth, for balanced dijets with Aj < 0.22. Hemisphere subleading-to-leading difference is denoted dP.

Difference of the total track transverse momentum distributions (P = 1/N dSum(pT)/dPhi) between subleading and leading hemispheres in central PbPb data (centrality 0-30%), projected into relative azimuth, for balanced dijets with Aj < 0.22. Hemisphere subleading-to-leading difference is denoted dP.

Double difference of transverse momentum distributions, subleading minus leading, peripheral PbPb minus pp (dP_PbPb - dP_p), projected into relative azimuth, for balanced dijets with Aj < 0.22.

Double difference of transverse momentum distributions, subleading minus leading, central PbPb minus pp (dP_PbPb - dP_p), projected into relative azimuth, for balanced dijets with Aj < 0.22.

Difference of the total track transverse momentum distributions (P = 1/N dSum(pT)/dPhi) between subleading and leading hemispheres in pp data, projected into relative azimuth, for unbalanced dijets with Aj > 0.22. Hemisphere subleading-to-leading difference is denoted dP.

Difference of the total track transverse momentum distributions (P = 1/N dSum(pT)/dPhi) between subleading and leading hemispheres in peripheral PbPb data (centrality 50-100%), projected into relative azimuth, for unbalanced dijets with Aj > 0.22. Hemisphere subleading-to-leading difference is denoted dP.

Difference of the total track transverse momentum distributions (P = 1/N dSum(pT)/dPhi) between subleading and leading hemispheres in central PbPb data (centrality 0-30%), projected into relative azimuth, for unbalanced dijets with Aj > 0.22. Hemisphere subleading-to-leading difference is denoted dP.

Double difference of transverse momentum distributions, subleading minus leading, peripheral PbPb minus pp (dP_PbPb - dP_p), projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Double difference of transverse momentum distributions, subleading minus leading, central PbPb minus pp (dP_PbPb - dP_p), projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Jet peak (long-range subtracted) distribution of transverse momentum (P = 1/N dSum(pT)/dPhi) for leading jets in pp data, projected into relative azimuth and plotted in the negative direction, for balanced dijets with Aj < 0.22.

Jet peak (long-range subtracted) distribution of transverse momentum (P = 1/N dSum(pT)/dPhi) for subleading jets in pp data, projected into relative azimuth, for balanced dijets with Aj < 0.22.

Jet peak (long-range subtracted) distribution of transverse momentum (P = 1/N dSum(pT)/dPhi) for leading jets in peripheral PbPb data, projected into relative azimuth and plotted in the negative direction, for balanced dijets with Aj < 0.22.