Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of centrality with individual track pT between 0.3 to 3.0 GeV/c, where the average multiplicity value is plotted on figure in order to compare with pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side, p-going side in pPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of multiplicity with individual track pT between 0.3 to 3.0 GeV/c.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions as a function of centrality with individual track pT between 0.3 to 3.0 GeV/c, where the average multiplicity value is plotted on figure in order to compare with pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going and p-going direction in pPb collisions and in PbPb collisions as a function DeltaEta for multiplicity [185,220) with individual track pT between 0.3 to 3.0 GeV/c. Data points are plotted at the bin center.

Prompt J/$\psi$ $v_{2}$ as a function of rapidity.

Prompt J/$\psi$ $v_{2}$ as a function of $p_{T}$.

Prompt J/$\psi$ $v_{2}$ as a function of $p_{T}$.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of rapidity.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of rapidity.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of $p_{\rm T}$.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of $p_{\rm T}$.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of centrality at high $p_{\rm T}$, 6.5$<p_{\rm T}<$30 GeV/c, in three different $|y|$ regions.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of centrality at high $p_{\rm T}$, 6.5$<p_{\rm T}<$30 GeV/c, in three different $|y|$ regions.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of centrality, at forward rapidity, 1.6$<|y|<$2.4, for two different $p_{\rm T}$ regions.

Prompt J/$\psi$ $R_{\rm AA}$ as a function of centrality, at forward rapidity, 1.6$<|y|<$2.4, for two different $p_{\rm T}$ regions.

Nonprompt J/$\psi$ $v_{2}$ as a function of $p_{\rm T}$.

Nonprompt J/$\psi$ $v_{2}$ as a function of $p_{\rm T}$.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of rapidity.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of rapidity.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of $p_{\rm T}$.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of $p_{\rm T}$.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Nonprompt J/$\psi$ $R_{\rm AA}$ as a function of centrality. The average ${N}_{\rm part}$ values correspond to events flatly distributed across centrality.

Charged-particle per-event yields measured in 5-10% PbPb centrality class.

Charged-particle per-event yields measured in 10-30% PbPb centrality class.

Charged-particle per-event yields measured in 10-30% PbPb centrality class.

Charged-particle per-event yields measured in 30-50% PbPb centrality class.

Charged-particle per-event yields measured in 30-50% PbPb centrality class.

Charged-particle per-event yields measured in 50-70% PbPb centrality class.

Charged-particle per-event yields measured in 50-70% PbPb centrality class.

Charged-particle per-event yields measured in 70-90% PbPb centrality class.

Charged-particle per-event yields measured in 70-90% PbPb centrality class.

Charged-particle per-event yields measured in pp collisions. A factor of 70 mb is used to scale the pp spectrum from a differential cross section to a per-event yield for direct comparison to the PbPb spectra. The lumi uncertainty is a 2.3% fully correlated uncertainty.

Charged-particle per-event yields measured in pp collisions. A factor of 70 mb is used to scale the pp spectrum from a differential cross section to a per-event yield for direct comparison to the PbPb spectra. The lumi uncertainty is a 2.3% fully correlated uncertainty.

PbPb nuclear modification factor measured in 0-5% PbPb centrality class.

PbPb nuclear modification factor measured in 0-5% PbPb centrality class.

PbPb nuclear modification factor measured in 5-10% PbPb centrality class.

PbPb nuclear modification factor measured in 5-10% PbPb centrality class.

PbPb nuclear modification factor measured in 10-30% PbPb centrality class.

PbPb nuclear modification factor measured in 10-30% PbPb centrality class.

PbPb nuclear modification factor measured in 30-50% PbPb centrality class.

PbPb nuclear modification factor measured in 30-50% PbPb centrality class.

PbPb nuclear modification factor measured in 50-70% PbPb centrality class.

PbPb nuclear modification factor measured in 50-70% PbPb centrality class.

PbPb nuclear modification factor measured in 70-90% PbPb centrality class.

PbPb nuclear modification factor measured in 70-90% PbPb centrality class.

PbPb nuclear modification factor measured in 0-10% PbPb centrality class.

PbPb nuclear modification factor measured in 0-10% PbPb centrality class.

PbPb nuclear modification factor measured in 0-100% PbPb centrality class.

PbPb nuclear modification factor measured in 0-100% PbPb centrality class.

pPb nuclear modification factor.

pPb nuclear modification factor.

Differential cross section for Y(2S) states as a function of their transverse momentum and per unit of rapidity in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(3S) states as a function of their transverse momentum and per unit of rapidity in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(3S) states as a function of their transverse momentum and per unit of rapidity in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(1S) states as a function of their transverse momentum and per unit of rapidity in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Differential cross section for Y(1S) states as a function of their transverse momentum and per unit of rapidity in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Differential cross section for Y(2S) states as a function of their transverse momentum and per unit of rapidity in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Differential cross section for Y(2S) states as a function of their transverse momentum and per unit of rapidity in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Differential cross section for Y(1S) states as a function of their rapidity and integrated over transverse momentum in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(1S) states as a function of their rapidity and integrated over transverse momentum in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(2S) states as a function of their rapidity and integrated over transverse momentum in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(2S) states as a function of their rapidity and integrated over transverse momentum in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(3S) states as a function of their rapidity and integrated over transverse momentum in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(3S) states as a function of their rapidity and integrated over transverse momentum in pp collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 3.7% are not displayed.

Differential cross section for Y(1S) states as a function of their rapidity and integrated over transverse momentum in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Differential cross section for Y(1S) states as a function of their rapidity and integrated over transverse momentum in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Differential cross section for Y(2S) states as a function of their rapidity and integrated over transverse momentum in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Differential cross section for Y(2S) states as a function of their rapidity and integrated over transverse momentum in PbPb collisions. Statistical (systematic) uncertainties are displayed as error bars (boxes). Global relative uncertainties of 6.5% are not displayed.

Nuclear modification factor for Υ(1S) states in PbPb collisions as a function of pT. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factor for Υ(1S) states in PbPb collisions as a function of pT. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factor for Υ(2S) states in PbPb collisions as a function of pT. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factor for Υ(2S) states in PbPb collisions as a function of pT. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factor for Υ(1S) states in PbPb collisions as a function of |y|. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factor for Υ(1S) states in PbPb collisions as a function of |y|. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factor for Υ(2S) states in PbPb collisions as a function of |y|. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factor for Υ(2S) states in PbPb collisions as a function of |y|. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainty (7.5%) is displayed as a grey box at unity.

Nuclear modification factors for Υ(1S) meson production in PbPb collisions, as a function of centrality, displayed as the average number of participating nucleons. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainties from the PbPb data (3.2%) or from the pp reference (6.3%) are displayed at unity as empty and filled red black boxes, respectively.

Nuclear modification factors for Υ(1S) meson production in PbPb collisions, as a function of centrality, displayed as the average number of participating nucleons. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainties from the PbPb data (3.2%) or from the pp reference (6.3%) are displayed at unity as empty and filled red black boxes, respectively.

Nuclear modification factors for Υ(2S) meson production in PbPb collisions, as a function of centrality, displayed as the average number of participating nucleons. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainties from the PbPb data (3.2%) or from the pp reference (6.9%) are displayed at unity as empty and filled black black boxes, respectively.

Nuclear modification factors for Υ(2S) meson production in PbPb collisions, as a function of centrality, displayed as the average number of participating nucleons. Statistical (systematic) uncertainties are displayed as error bars (boxes), while the global (fully correlated) uncertainties from the PbPb data (3.2%) or from the pp reference (6.9%) are displayed at unity as empty and filled black black boxes, respectively.

Nuclear modification factors for Υ(1S), Υ(2S) and Υ(3S) meson production in PbPb collisions, integrated over centrality. For the Υ(3S), the upper limit derived on the nuclear modification factor is given.

Nuclear modification factors for Υ(1S), Υ(2S) and Υ(3S) meson production in PbPb collisions, integrated over centrality. For the Υ(3S), the upper limit derived on the nuclear modification factor is given.

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.

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.

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

Difference, peripheral PbPb minus pp data in subleading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth, for balanced dijets with Aj < 0.22.

Difference, central PbPb minus pp data in subleading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth, for balanced dijets with Aj < 0.22.

Difference, peripheral PbPb minus pp data in leading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth and plotted in the negative direction, for balanced dijets with Aj < 0.22.

Difference, central PbPb minus pp data in leading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth and plotted in the negative direction, for balanced dijets with Aj < 0.22.

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

Double difference, central PbPb minus pp, subleading minus leading (dP_PbPb - dP_pp), in jet peak transverse momentum distributions, 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 pp data, projected into relative azimuth and plotted in the negative direction, for unbalanced 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, forunbalanced dijets with Aj > 0.22.

Jet peak (long-range subtracted) distribution of transverse momentum for leading jets in peripheral PbPb data, projected into relative azimuth and plotted in the negative direction, for unbalanced dijets with Aj > 0.22.

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

Jet peak (long-range subtracted) distribution of transverse momentum for subleading jets in central PbPb data, projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Difference, peripheral PbPb minus pp data in subleading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Difference, central PbPb minus pp data in subleading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Difference, peripheral PbPb minus pp data in leading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth and plotted in the negative direction, for unbalanced dijets with Aj > 0.22.

Difference, central PbPb minus pp data in leading jet peak transverse momentum distributions (P_PbPb - P_pp), projected into relative azimuth and plotted in the negative direction, for unbalanced dijets with Aj > 0.22.

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

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

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

Difference of the long range track transverse momentum distributions between subleading and leading hemispheres (dP) in peripheral PbPb data (centrality 50-100%), projected into relative azimuth, for balanced dijets with Aj < 0.22.

Difference of the long range track transverse momentum distributions between subleading and leading hemispheres (dP) in central PbPb data (centrality 0-30%), projected into relative azimuth, for balanced dijets with Aj < 0.22.

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

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

Difference of the long range track transverse momentum distributions between subleading and leading hemispheres (dP) in pp data, projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Difference of the long range track transverse momentum distributions between subleading and leading hemispheres (dP) in peripheral PbPb data (centrality 50-100%), projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Difference of the long range track transverse momentum distributions between subleading and leading hemispheres (dP) in central PbPb data (centrality 0-30%), projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

Double difference of the long range transverse momentum distributions, subleading minus leading, peripheral PbPb minus pp, projected into relative azimuth, for unbalanced dijets with Aj > 0.22.

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

Integrated transverse momentum in the long-range correlated distribution, as a function of track-pT, for balanced dijets with Aj < 0.22.

Integrated transverse momentum in the long-range correlated distribution, as a function of track-pT, for unbalanced dijets with Aj > 0.22.

Integrated transverse momentum difference central PbPb minus pp of the jet peak distributions (subleading minus leading), as a function of track-pT, for balanced dijets with Aj < 0.22.

Integrated transverse momentum difference central PbPb minus pp of the jet peak distributions (subleading minus leading), as a function of track-pT, for unbalanced dijets with Aj > 0.22.

Integrated transverse momentum difference central PbPb minus pp of the total transverse momentum distributions (subleading minus leading), as a function of track-pT, for balanced dijets with Aj < 0.22.

Integrated transverse momentum difference central PbPb minus pp of the total transverse momentum distributions (subleading minus leading), as a function of track-pT, for unbalanced dijets with Aj > 0.22.

Integrated transverse momentum difference peripheral PbPb minus pp of the jet peak distributions (subleading minus leading), as a function of track-pT, for balanced dijets with Aj < 0.22.

Integrated transverse momentum difference peripheral PbPb minus pp of the jet peak distributions (subleading minus leading), as a function of track-pT, for unbalanced dijets with Aj > 0.22.

Integrated transverse momentum difference peripheral PbPb minus pp of the total transverse momentum distributions (subleading minus leading), as a function of track-pT, for balanced dijets with Aj < 0.22.

Integrated transverse momentum difference peripheral PbPb minus pp of the total transverse momentum distributions (subleading minus leading), as a function of track-pT, for unbalanced dijets with Aj > 0.22.

The cumulant $c_2\{8\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The elliptic flow $v_2\{6\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in PbPb collisions.

The elliptic flow $v_2\{8\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in PbPb collisions.

The elliptic flow $v_2\{\text{LYZ}\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in PbPb collisions.

The elliptic flow $v_2\{6\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The elliptic flow $v_2\{8\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The elliptic flow $v_2\{\text{LYZ}\}$ extracted for all charged particles with $0.3 < p_T < 3.0$ GeV/c as a function of $N_{trk}^{offline}$ in pPb collisions.

The cumulant ratio $c_2\{6\}/v_2\{4\}$ as a function of $c_2\{4\}/v_2\{2\}$ in pPb collisions.

The cumulant ratio $c_2\{8\}/v_2\{6\}$ as a function of $c_2\{4\}/v_2\{2\}$ in pPb collisions.

The cumulant ratio $c_2\{6\}/v_2\{4\}$ as a function of $c_2\{4\}/v_2\{2\}$ in PbPb collisions.

The cumulant ratio $c_2\{8\}/v_2\{6\}$ as a function of $c_2\{4\}/v_2\{2\}$ in PbPb collisions.

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.

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%.