The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the $N_{offline}^{trk}$ < 35 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K_{S}^{0}$ as a function of $p_{T}$ from the correlation in the 35 $\leq N_{offline}^{trk}$ < 60 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K_{S}^{0}$ as a function of $p_{T}$ from the correlation in the 60 $\leq N_{offline}^{trk}$ < 120 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the $N_{offline}^{trk}$ < 35 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 35 $\leq N_{offline}^{trk}$ < 60 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 60 $\leq N_{offline}^{trk}$ < 120 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the $N_{offline}^{trk}$ < 35 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 35 $\leq N_{offline}^{trk}$ < 60 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 60 $\leq N_{offline}^{trk}$ < 120 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K_{S}^{0}$ as a function of $p_{T}$ from the correlation in the $N_{offline}^{trk}$ < 35 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K_{S}^{0}$ as a function of $p_{T}$ from the correlation in the 35 $\leq N_{offline}^{trk}$ < 60 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K_{S}^{0}$ as a function of $p_{T}$ from the correlation in the 60 $\leq N_{offline}^{trk}$ < 120 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the $N_{offline}^{trk}$ < 35 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 35 $\leq N_{offline}^{trk}$ < 60 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 60 $\leq N_{offline}^{trk}$ < 120 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in pPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in pPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in PbPb.

The elliptic flow v2(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 120 $\leq N_{offline}^{trk}$ < 150 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 150 $\leq N_{offline}^{trk}$ < 185 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 220 multiplicity class in PbPb.

The elliptic flow per constituent quark v2(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 220 $\leq N_{offline}^{trk}$ < 260 multiplicity class in PbPb.

The triangular flow v3(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in PbPb.

The triangular flow v3(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in PbPb.

The triangular flow v3(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in PbPb.

The triangular flow per constituent quark v3(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in PbPb.

The triangular flow per constituent quark v3(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in PbPb.

The triangular flow v3(2, $|\Delta\eta| > 2$) extracted for all charged particles as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in pPb.

The triangular flow v3(2, $|\Delta\eta| > 2$) extracted for $K^{0}_{S}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in pPb.

The triangular flow v3(2, $|\Delta\eta| > 2$) extracted for $\Lambda/\bar{\Lambda}$ as a function of $p_{T}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in pPb.

The triangular flow per constituent quark v3(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in pPb.

The triangular flow per constituent quark v3(2, $|\Delta\eta| > 2$)/$n_{q}$ extracted for $\Lambda/\bar{\Lambda}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ from the correlation in the 185 $\leq N_{offline}^{trk}$ < 350 multiplicity class in pPb.

Selection efficiencies in % for the signal in the top squark search, estimated from the simulation.

The final $S_{\text{T}}$ distribution for the leptoquark search with the $\text{e}\tau_{\text{h}}$ and $\mu\tau_{\text{h}}$ channels combined. The last bin contains the overflow events.

The final $S_{\text{T}}$ distribution for the top squark search with the $\text{e}\tau_{\text{h}}$ and $\mu\tau_{\text{h}}$ channels combined. The last bin contains the overflow events.

The expected and observed combined upper limits on the third-generation LQ pair production cross section $\sigma$ times the square of the branching fraction, $\mathcal{B}^2$, at 95% CL, as a function of the LQ mass. These limits also apply to top squarks decaying directly via the coupling $\lambda^{\prime}_{333}$.

The expected and observed combined upper limits on the top squark pair production cross section $\sigma$ times the square of the branching fraction, $\mathcal{B}^2$, at 95% CL, as a function of the top squark mass. These limits apply to top squarks with a chargino-mediated decay through the coupling $\lambda^{\prime}_{3jk}$.

The expected and observed 95% CL upper limits on the branching fraction for the leptoquark decay to a tau lepton and a bottom quark, as a function of the leptoquark mass. A search for top squark pair production [EPJC 73(2013)2677] has the same kinematic signature as the leptoquark decay to a tau neutrino and a top quark. This search is reinterpreted to provide the expected and observed 95% CL upper limits for low values of $\mathcal{B}$, assuming the leptoquark only decays to third-generation fermions.

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.

Correlation matrix for the asymmetries as a function of $p_\text{T}^\mathrm{t\bar{t}}$ in the fiducial phase space. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using three bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using three bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using six bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the fiducial phase space, using six bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $|y_\mathrm{t\bar{t}}|$ in the full phase space. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $|y_\mathrm{t\bar{t}}|$ in the full phase space. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $p_\text{T}^\mathrm{t\bar{t}}$ in the full phase space. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $p_\text{T}^\mathrm{t\bar{t}}$ in the full phase space. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using three bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using three bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Corrected asymmetry as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using six bins in $m_\mathrm{t\bar{t}}$. The value 9999 is used as a placeholder for infinity. The correlation matrix for these values can be found in a separate table.

Correlation matrix for the asymmetries as a function of $m_\mathrm{t\bar{t}}$ in the full phase space, using six bins in $m_\mathrm{t\bar{t}}$. Both statistical and systematic effects are considered.

Measured dijet angular distributions in bin of dijet invariant mass. P=3 and P=4 refers to the two jets in the final state.

Measured dijet angular distributions in bin of dijet invariant mass. P=3 and P=4 refers to the two jets in the final state.

Transverse thrust for $320 < p_{T,1} < 390$ GeV.

Transverse thrust for $p_{T,1} > 390$ GeV.

Jet broadening for $110 < p_{T,1} < 170$ GeV.

Jet broadening for $170 < p_{T,1} < 250$ GeV.

Jet broadening for $250 < p_{T,1} < 320$ GeV.

Jet broadening for $320 < p_{T,1} < 390$ GeV.

Jet broadening for $p_{T,1} > 390$ GeV.

Total jet mass for $110 < p_{T,1} < 170$ GeV.

Total jet mass for $170 < p_{T,1} < 250$ GeV.

Total jet mass for $250 < p_{T,1} < 320$ GeV.

Total jet mass for $320 < p_{T,1} < 390$ GeV.

Total jet mass for $p_{T,1} > 390$ GeV.

Total transverse jet mass for $110 < p_{T,1} < 170$ GeV.

Total transverse jet mass for $170 < p_{T,1} < 250$ GeV.

Total transverse jet mass for $250 < p_{T,1} < 320$ GeV.

Total transverse jet mass for $320 < p_{T,1} < 390$ GeV.

Total transverse jet mass for $p_{T,1} > 390$ GeV.

Third-jet resolution parameter for $110 < p_{T,1} < 170$ GeV.

Third-jet resolution parameter for $170 < p_{T,1} < 250$ GeV.

Third-jet resolution parameter for $250 < p_{T,1} < 320$ GeV.

Third-jet resolution parameter for $320 < p_{T,1} < 390$ GeV.

Third-jet resolution parameter for $p_{T,1} > 390$ GeV.

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.

Normalized differential tt cross section (from l+jets channel) as a function of the pseudo-rapidity eta(b-jet) of the b-jet. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum pt(bb) of the system consisting of the two selected b-jets. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from l+jets channel) as a function of the invariant mass m(bb) of the system consisting of the two selected b-jets. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the transverse momentum pt of the lepton. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the pseudo-rapidity eta of the lepton. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the transverse momentum pt of the dilepton system. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the mass (m) of the dilepton system. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the transverse momentum pt(b-jet) of the b-jet. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the pseudo-rapidity eta(b-jet) of the b-jet. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the transverse momentum pt(bb) of the system consisting of the two selected b-jets. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the invariant mass m(bb) of the system consisting of the two selected b-jets. The results are presented at particle level in the fiducial phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum pt(top) of the top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum pt(top) of the top quark or antiquark.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum pt(top) of the top quark or antiquark.

Normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum pt*(top) of the top quark or antiquark in the ttbar rest frame. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum pt(top) of the top quark or antiquark in the ttbar rest frame.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum pt(top) of the top quark or antiquark in the ttbar rest frame.

Normalized differential tt cross section (from l+jets channel) as a function of the rapidity y of the top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section (from l+jets channel) as a function of the rapidity y of the top quark or antiquark.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section (from l+jets channel) as a function of the rapidity y of the top quark or antiquark.

Normalized differential tt cross section (from l+jets channel) as a function of the azimuthal opening angle between the top quark and antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section (from l+jets channel) as a function of the azimuthal opening angle between the top quark and antiquark.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section (from l+jets channel) as a function of the azimuthal opening angle between the top quark and antiquark.

Normalized differential tt cross section in the l+jets channels as a function of the transverse momentum of the leading (pt1) top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section in the l+jets channels as a function of the transverse momentum of the leading (pt1) top quark or antiquark.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section in the l+jets channels as a function of the transverse momentum of the leading (pt1) top quark or antiquark.

Normalized differential tt cross section in the l+jets channels as a function of the transverse momentum of the trailing (pt2) top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section in the l+jets channels as a function of the transverse momentum of the trailing (pt2) top quark or antiquark.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section in the l+jets channels as a function of the transverse momentum of the trailing (pt2) top quark or antiquark.

Normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum ptt of the top quark pair. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum ptt of the top quark pair.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section (from l+jets channel) as a function of the transverse momentum ptt of the top quark pair.

Normalized differential tt cross section (from l+jets channel) as a function of the rapidity y_tt of the top quark pair. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section (from l+jets channel) as a function of the rapidity y_tt of the top quark pair.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section (from l+jets channel) as a function of the rapidity y_tt of the top quark pair.

Normalized differential tt cross section (from l+jets channel) as a function of the invariant mass m_tt of the top quark pair. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Statistical covariance matrix for the normalized differential tt cross section (from l+jets channel) as a function of the invariant mass m_tt of the top quark pair.

Breakdown of systematic uncertainties per bin for the normalized differential tt cross section (from l+jets channel) as a function of the invariant mass m_tt of the top quark pair.

Normalized differential tt cross section (from dilepton channel) as a function of the transverse momentum pt(top) of the top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the transverse momentum pt*(top) of the top quark or antiquark in the ttbar rest frame. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the rapidity y of the top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the azimuthal opening angle between the top quark and antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section in the dilepton channels as a function of the transverse momentum of the leading (pt1) top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section in the dilepton channels as a function of the transverse momentum of the trailing (pt2) top quark or antiquark. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the transverse momentum ptt of the top quark pair. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the rapidity y_tt of the top quark pair. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalized differential tt cross section (from dilepton channel) as a function of the invariant mass m_tt of the top quark pair. The horizontally-corrected bin centres according to the MADGRAPH+PYTHIA6 prediction are also provided. The results are presented at parton level in the full phase space. The statistical and systematic uncertainties are added in quadrature to yield the total uncertainty.

Normalised differential TOP TOPBAR production cross section as a function of the number of additional jets with PT(JET) > 30 GeV in the lepton+jets channel. The total uncertainties are shown and include the statistical and systematic uncertainties.

Measured gap fraction in the dilepton channel as a function of the additional jet transverse momentum, GAPFRAC(PT) = N(PT)/N(TOTAL) where N(PT) is the number of events that do not contain additional jets above the given PT threshold.

Measured gap fraction in the dilepton channel as a function of the scalar sum of the transverse momentum of the additional jets, HT = SUM(PT(ADD. JETS)), GAPFRAC(HT) = N(HT)/N(TOTAL) where N(HT) is the number of events in which HT (with PT > 30 GeV) is less than the given threshold.

Observed and expected numbers of events with exactly three leptons with the scalar sum of jet transverse momentum values HT < 200 GeV. "On-Z" refers to events with at least one E+ E- or MU+ MU- (OSSF) pair with dilepton mass between 75 and 105 GeV, while "Off-Z" refers to events with one or two OSSF pairs, none of which fall in this mass range. The OSSFN designation refers to the number of E+ E- and MU+ MU- pairs in the event. Search channels binned in ET have been combined into coarse ET bins for the purposes of presentation.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z GRAVITINO) = 0.5 for strong plus electroweak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0 for strong plus electroweak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0 for strong plus electroweak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z0 GRAVITINO) = 0.5. The chargino-Higgsino mass is fixed at 150 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z0 GRAVITINO) = 0.5. The chargino-Higgsino mass is fixed at 350 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 150 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 350 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 150 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 350 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 150 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 250 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0 and strong plus weak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 350 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0 and strong plus weak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the slepton co-NLSP model in the gluino-chargino (wino-like chargino) mass plane.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the stau-NLSP and stau-NNLSP scenario in the degenerate smuon- and selectron- stau mass plane.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the T1tttt model in the gluino-neutralino mass plane.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the T6ttWW model in the sbottom-chargino mass plane.

Observed 95% C.L. exclusion contour for the T1tttt scenario.

Observed - 1sig(theoretical) 95% C.L. exclusion contour for the T1tttt scenario.

Observed + 1sig(theoretical) 95% C.L. exclusion contour for the T1tttt scenario.

Expected 95% C.L. exclusion contour for the T1tttt scenario.

Expected - 1sig 95% C.L. exclusion contour for the T1tttt scenario.

Expected + 1sig 95% C.L. exclusion contour for the T1tttt scenario.

Observed 95% C.L. exclusion contour for the T6ttWW scenario.

Observed - 1sig(theoretical) 95% C.L. exclusion contour for the T6ttWW scenario.

Observed + 1sig(theoretical) 95% C.L. exclusion contour for the T6ttWW scenario.

Expected 95% C.L. exclusion contour for the T6ttWW scenario.

Expected - 1sig 95% C.L. exclusion contour for the T6ttWW scenario.

Expected + 1sig 95% C.L. exclusion contour for the T6ttWW scenario.

Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z GRAVITINO) = 0.5 for strong plus electroweak production.

Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0 for strong plus electroweak production. Successive instances of SIG(OBS) = SIG(EXP) =0 have been rebinned over M(STOP) to reduce the size of the table.

Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> Z0 GLUINO) = 1.0 for strong plus electroweak production.

Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 150 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 250 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 350 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

Observed and expected 95% C.L. limits for the slepton co-NLSP model in the gluino-chargino (wino-like chargino) mass plane are shown.

Observed and expected 95% C.L. limits for the stau-NLSP and stau-NNLSP scenario in the degenerate smuon- and selectron- stau mass plane are shown. Successive instances of SIG(OBS) = SIG(EXP) =0 have been rebinned over M(SELECTRON) to reduce the size of the table.

Observed and expected 95% C.L. limits for the T1tttt model in the gluino-neutralino mass plane are shown.

Observed and expected 95% C.L. limits for the T6ttWW model in the sbottom-chargino mass plane are given.

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

Event centrality dependence of the $\mbox{Z}\rightarrow\mu^{+}\mu^{-}$ yields per MB event in PbPb collisions, divided by the expected average nuclear overlap function, $T_{\rm AA}$. On the horizontal axis, event centrality is depicted as the average number of participating nucleons, $N_{\rm part}$.

Event centrality dependence of the $\mbox{Z}\rightarrow e^{+}e^{-}$ yields per MB event in PbPb collisions, divided by the expected average nuclear overlap function, $T_{\rm AA}$. On the horizontal axis, event centrality is depicted as the average number of participating nucleons, $N_{\rm part}$.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson $p_{\rm T}$ for the dimuon decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson $p_{\rm T}$ for the dielectron decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson rapidity for the dimuon decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson rapidity for the dielectron decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson rapidity for the combined leptonic decay channel.

The measured Z boson yields per MB event in PbPb collisions as a function of the Z boson $p_{\rm T}$ for the combined leptonic decay channel.

Event centrality dependence of the $\mbox{Z}\rightarrow l^{+}l^{-}$ yields per MB event in PbPb collisions, divided by the expected average nuclear overlap function, $T_{\rm AA}$. On the horizontal axis, event centrality is depicted as the average number of participating nucleons, $N_{\rm part}$.

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.

Covariance matrix (statistical and systematic uncertainties combined) with the muon $p_{T}>35$ GeV. The units are in $10^{-4}$.

Inclusive Jet cross section with R = 0.5 in the rapidity bin 1.5 < |y| < 2. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.5 in the rapidity bin 2 < |y| < 2.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.5 in the rapidity bin 2.5 < |y| < 3. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 0 < |y| < 0.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 0.5 < |y| < 1. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 1 < |y| < 1.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 1.5 < |y| < 2. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 2 < |y| < 2.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Inclusive Jet cross section with R = 0.7 in the rapidity bin 2.5 < |y| < 3. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources, especially the luminosity uncertainty of 2.2%. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 0 < |y| < 0.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 0.5 < |y| < 1. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 1 < |y| < 1.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 1.5 < |y| < 2. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 2 < |y| < 2.5. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Jet radius ratio R(0.5, 0.7) in the rapidity bin 2.5 < |y| < 3. The total uncorrelated uncertainty includes statistical one and systematic uncorrelated. The total systematic uncertainty includes all other sources. The total error can be obtained as a quadratic sum of uncorrelated and correlated one. The NP correction can be used to scale theory prediction to compare to data at particle level.

Toward $\sum p_\perp$ density vs $p_\perp^{\mu\mu}$.

Transverse $\sum p_\perp$ density vs $p_\perp^{\mu\mu}$.

Away $\sum p_\perp$ density vs $p_\perp^{\mu\mu}$.

Toward $\langle p_\perp \rangle$ vs $p_\perp^{\mu\mu}$.

Transverse $\langle p_\perp \rangle$ vs $p_\perp^{\mu\mu}$.

Away $\langle p_\perp \rangle$ vs $p_\perp^{\mu\mu}$.

Towards $+$ transverse $N_\text{chg}$ density vs $m_{\mu\mu}$, $p_\perp^{\mu\mu} < 5$ GeV.

Towards $+$ transverse $\sum p_\perp$ density vs $m_{\mu\mu}$, $p_\perp^{\mu\mu} < 5$ GeV.

Towards $+$ transverse $\langle p_\perp \rangle$ vs $m_{\mu\mu}$, $p_\perp^{\mu\mu} < 5$ GeV.

Toward $N_\text{chg}$.

Transverse $N_\text{chg}$.

Away $N_\text{chg}$.

Toward $p_\perp$.

Transverse $p_\perp$.

Away $p_\perp$.

Transverse $N_\text{chg}$, $p_\perp(\mu\mu) < 5$ GeV.

Transverse $p_\perp$, $p_\perp(\mu\mu) < 5$ GeV.