$p_{\rm T}$-differential cross section of prompt $\rm{D_{s}}$ mesons in pp collisions at $\sqrt{\rm{s_{NN}}}$=5.02 TeV in the rapidity interval $|y|$<0.5. Branching ratio of $\rm{D_{s}}\rightarrow\phi\pi\rightarrow K K \pi$ : 0.0227.

$p_{\rm T}$-differential cross section of inclusive $\rm{D}^{0}$ mesons (including also $\rm{D}^{0}$ mesons from beauty-hadron decays) in pp collisions at $\sqrt{\rm{s_{NN}}}$=5.02 TeV in the rapidity interval $|y|$<0.5. Branching ratio of $\rm{D}^{0}\rightarrow K\pi$ : 0.0389.

Ratio of $\rm {D}^{+}$ to $\rm{D}^{0}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=5.02 TeV in |y|<0.5 as a function of $p_{\rm T}$. Branching ratio of $\rm{D^{+}}\rightarrow K\pi\pi$ : 0.0898. Branching ratio of $\rm{D^{0}}\rightarrow K\pi$ : 0.0389.

Ratio of $\rm {D}^{*+}$ to $\rm{D}^{0}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=5.02 TeV in |y|<0.5 as a function of $p_{\rm T}$. Branching ratio of $\rm D^{+-}\rightarrow K{\rm{\pi}}{\rm{\pi}}$: 0.0389*0.677. Branching ratio of $\rm{D^{0}}\rightarrow K\pi$ : 0.0389.

Ratio of $\rm {D}_{s}$ to $\rm{D}^{0}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=5.02 TeV in |y|<0.5 as a function of $p_{\rm T}$. Branching ratio of $\rm{D_s}\rightarrow \phi \pi \rightarrow KK\pi$ : 0.0227. Branching ratio of $\rm{D^{0}}\rightarrow K\pi$ : 0.0389.

Ratio of $\rm {D}_{s}$ to $\rm {D}^{+}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=5.02 TeV in |y|<0.5 as a function of $p_{\rm T}$. Branching ratio of $\rm{D_s}\rightarrow \phi \pi \rightarrow KK\pi$ : 0.0227. Branching ratio of $\rm{D^{+}}\rightarrow K\pi\pi$ : 0.0898.

Ratio of $\rm {D}^{+}$ to $\rm{D}^{0}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV in |y|<0.5 as a function of $p_{\rm T}$. The cross section for $\rm {D}^{0}$ and $\rm {D}^{+}$ mesons in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV were updated with respect to Eur.Phys.J. C77 no.8 (2017)550 to account for the change of the world-average BR of $\rm{D^{0}}\rightarrow K\pi$ and $\rm{D^{+}}\rightarrow K\pi\pi$ from ($3.93\% \pm 0.04$) to ($3.89\% \pm 0.04$), and from ($9.46\% \pm 0.24$) to ($8.98\% \pm 0.28$), respectively. Branching ratio of $\rm{D^{+}}\rightarrow K\pi\pi$ : 0.0898. Branching ratio of $\rm{D^{0}}\rightarrow K\pi$ : 0.0389.

Ratio of $\rm {D}^{*+}$ to $\rm{D}^{0}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV in |y|<0.5 as a function of $p_{\rm T}$. The cross section for $\rm {D}^{0}$ in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV was updated with respect to Eur.Phys.J. C77 no.8 (2017)550 to account for the change of the world-average BR of $\rm{D^{0}}\rightarrow K\pi$ from ($3.93\% \pm 0.04$) to ($3.89\% \pm 0.04$). Branching ratio of $\rm D^{+-}\rightarrow K{\rm{\pi}}{\rm{\pi}}$: 0.0389*0.677. Branching ratio of $\rm{D^{0}}\rightarrow K\pi$ : 0.0389.

Ratio of $\rm {D}_{s}$ to $\rm{D}^{0}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV in |y|<0.5 as a function of $p_{\rm T}$. The cross section for $\rm {D}^{0}$ mesons in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV was updated with respect to Eur.Phys.J. C77 no.8 (2017)550 to account for the change of the world-average BR of $\rm{D^{0}}\rightarrow K\pi$ from ($3.93\% \pm 0.04$) to ($3.89\% \pm 0.04$). Branching ratio of $\rm{D_s}\rightarrow \phi \pi \rightarrow KK\pi$ : 0.0227. Branching ratio of $\rm{D^{0}}\rightarrow K\pi$ : 0.0389.

Ratio of $\rm {D}_{s}$ to $\rm {D}^{+}$ meson yield in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV in |y|<0.5 as a function of $p_{\rm T}$. The cross section for $\rm {D}^{+}$ mesons in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV was updated with respect to Eur.Phys.J. C77 no.8 (2017)550 to account for the change of the world-average BR of $\rm{D^{+}}\rightarrow K\pi\pi$ from ($9.46\% \pm 0.24$) to ($8.98\% \pm 0.28$). Branching ratio of $\rm{D_s}\rightarrow \phi \pi \rightarrow KK\pi$ : 0.0227. Branching ratio of $\rm{D^{+}}\rightarrow K\pi\pi$ : 0.0898.

Ratios of $\rm {D}^{0}$-mesons production cross sections in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV and $\sqrt{\rm{s_{NN}}}$=5.02 TeV as a function of $p_{\rm T}$. The cross section for $\rm {D}^{0}$ mesons in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV was updated with respect to Eur.Phys.J. C77 no.8 (2017)550 to account for the change of the world-average BR of $\rm{D}^{0}\rightarrow K\pi$ from ($3.93\% \pm 0.04$) to ($3.89\% \pm 0.04$). Branching ratio of $\rm{D}^{0}\rightarrow K\pi$ : 0.0389.

Ratios of $\rm {D}^{+}$-mesons production cross sections in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV and $\sqrt{\rm{s_{NN}}}$=5.02 TeV as a function of $p_{\rm T}$. The cross section for $\rm {D}^{+}$ mesons in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV was updated with respect to Eur.Phys.J. C77 no.8 (2017)550 to account for the change of the world-average BR of $\rm D^{+-}\rightarrow K{\rm{\pi}}{\rm{\pi}}$ from ($9.46\% \pm 0.24$) to ($8.98\% \pm 0.28$). Branching ratio of $\rm D^{+-}\rightarrow K{\rm{\pi}}{\rm{\pi}}$ : 0.0898.

Ratios of $\rm {D}^{*+}$-mesons production cross sections in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV and $\sqrt{\rm{s_{NN}}}$=5.02 TeV as a function of $p_{\rm T}$. Branching ratio of $\rm{D}^{*+}\rightarrow \rm{D}^{0}\pi\rightarrow K\pi\pi$: 0.02633.

Ratios of $\rm{D_{s}}$-mesons production cross sections in pp collisions at $\sqrt{\rm{s_{NN}}}$=7 TeV and $\sqrt{\rm{s_{NN}}}$=5.02 TeV as a function of $p_{\rm T}$ Branching ratio of $\rm{D_{s}}\rightarrow\phi\pi\rightarrow K K \pi$ : 0.0227.

First Column: Production cross sections for prompt D mesons (D0, D+, D*+ and D_s) at mid-rapidity in |y|<0.5 and full pT range, in pp collisions at 5.02 TeV. The second (sys) error is from the luminosity uncertainty, the third (sys) error is from the branching-ratio uncertainty. For D+, D*+ and Ds, the fourth (sys) error is due to the extrapolation to pt=0. Second column: value of <pT> of prompt D0 mesons in |y|<0.5. The first uncertainty is statistical, the second is the systematic uncertainty.

trigger particle momentum dependence of observables RMS for wide component in p-p collisions at 7 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables RMS for wide component in p-p collisions at 7 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables RMS for wide component in p-p collisions at 7 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables RMS for narrow component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables RMS for narrow component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables RMS for narrow component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables RMS for wide component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables RMS for wide component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables RMS for wide component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-p collisions at 7 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-p collisions at 7 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-p collisions at 7 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-p collisions at 7 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-p collisions at 7 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-p collisions at 7 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for narrow component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-Pb collisions at 5.02 TeV with 0.2<xlong<0.4.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-Pb collisions at 5.02 TeV with 0.4<xlong<0.6.

trigger particle momentum dependence of observables per-trigger yield for wide component in p-Pb collisions at 5.02 TeV with 0.6<xlong<1.0.

Fully corrected $p_{\rm T} D$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $p_{\rm T} D$ distributions pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 Tune 4C simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Ratio of fully corrected $p_{\rm T} D$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Fully corrected $LeSub$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$.

Ratio of fully corrected $LeSub$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 Tune 4C simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

Ratio of fully corrected $LeSub$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

Fully corrected $g$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $g$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 Tune 4C simulations. The systematic uncertainty of $g$ is propagated to the ratio.

Ratio of fully corrected $g$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $g$ is propagated to the ratio.

Fully corrected $p_{\rm T} D$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $p_{\rm T} D$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Ratio of fully corrected $p_{\rm T} D$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Fully corrected $LeSub$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $LeSub$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

Ratio of fully corrected $LeSub$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

The elliptic flow, $v_{2}$, for $\Omega^{-}$ as a function of $p_{T}$ in pPb collision at 8.16 TeV.

The elliptic flow, $v_{2}$, for $D^{0}$ mesons as a function of $p_{T}$ in pPb collision at 8.16 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $K^{0}_{S}$ as a function of $p_{T}$ in pPb collision at 8.16 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $\Lambda$ as a function of $p_{T}$ in pPb collision at 8.16 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $\Xi^{-}$ as a function of $p_{T}$ in pPb collision at 8.16 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $\Omega^{-}$ as a function of $p_{T}$ in pPb collision at 8.16 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $D^{0}$ mesons as a function of $p_{T}$ in pPb collision at 8.16 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in pPb collision at 8.16 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $\Lambda$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in pPb collision at 8.16 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $\Xi^{-}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in pPb collision at 8.16 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $\Omega^{-}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in pPb collision at 8.16 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $D^{0}$ meson as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in pPb collision at 8.16 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $K^{0}_{S}$ as a function of $p_{T}$ in PbPb collision at 5.02 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $\Lambda$ as a function of $p_{T}$ in PbPb collision at 5.02 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $\Xi^{-}$ as a function of $p_{T}$ in PbPb collision at 5.02 TeV.

The elliptic flow after correcting back-to-back jet contribution, $v_{2}^{sub}$, for $\Omega^{-}$ as a function of $p_{T}$ in PbPb collision at 5.02 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $K^{0}_{S}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in PbPb collision at 5.02 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $\Lambda$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in PbPb collision at 5.02 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $\Xi^{-}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in PbPb collision at 5.02 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $\Omega^{-}$ as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in PbPb collision at 5.02 TeV.

The elliptic flow per constituent quark after correcting back-to-back jet contribution, $v_{2}^{sub}/n_{q}$, for $D^{0}$ meson as a function of transverse kinetic energy per constituent quark $KE_{T}/n_{q}$ in PbPb collision at 5.02 TeV.

Invariant differential cross section of inclusive GAMMA produced in inelastic pp collisions at center-of-mass energy 8 TeV, the uncertainty of $\sigma_{MB}$ of 2.6% is not included in the systematic error. Values are given in the center of the PT bin.

Invariant differential cross section of direct GAMMA produced in inelastic pp collisions at center-of-mass energy 2.76 TeV, the uncertainty of $\sigma_{MB}$ of 2.5% is not included in the systematic error. Values are given in the center of the PT bin.

Invariant differential cross section of direct GAMMA produced in inelastic pp collisions at center-of-mass energy 8 TeV, the uncertainty of $\sigma_{MB}$ of 2.6% is not included in the systematic error. Values are given in the center of the PT bin.

Invariant differential yield of inclusive GAMMA produced in inelastic pp collisions at center-of-mass energy 2.76 TeV. Values are given in the center of the PT bin.

Invariant differential yield of inclusive GAMMA produced in inelastic pp collisions at center-of-mass energy 8 TeV. Values are given in the center of the PT bin.

Invariant differential yield of direct GAMMA produced in inelastic pp collisions at center-of-mass energy 2.76 TeV. Values are given in the center of the PT bin.

Invariant differential yield of direct GAMMA produced in inelastic pp collisions at center-of-mass energy 8 TeV. Values are given in the center of the PT bin.

The Symmetric cumulant $SC(n,m)$ results as a function of multiplicity ($N_{trk}^{offline}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

The Symmetric cumulant $SC(n,m)$ results as a function of multiplicity ($N_{trk}^{offline}$) in pPb collisions at $\sqrt{s_{NN}}$ = 8.16 TeV.

The Symmetric cumulant $SC(n,m)$ results as a function of multiplicity ($N_{trk}^{offline}$) in pp collisions at $\sqrt{s}$ = 13.0 TeV.

The Normalized Symmetric cumulant $NSC(n,m)$ results as a function of multiplicity ($N_{trk}^{offline}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV. The results are normalized by $\left<(v_2^{\text{sub}})^{2}\right> \, \left<(v_3^{\text{sub}})^{2}\right>$ and $\left<(v_2^{\text{sub}})^{2}\right> \, \left<(v_4^{\text{sub}})^{2}\right>$ from two-particle correlations.

The Normalized Symmetric cumulant $NSC(n,m)$ results as a function of multiplicity ($N_{trk}^{offline}$) in pPb collisions at $\sqrt{s_{NN}}$ = 8.16 TeV. The results are normalized by $\left<(v_2^{\text{sub}})^{2}\right> \, \left<(v_3^{\text{sub}})^{2}\right>$ and $\left<(v_2^{\text{sub}})^{2}\right> \, \left<(v_4^{\text{sub}})^{2}\right>$ from two-particle correlations.

The Normalized Symmetric cumulant $NSC(n,m)$ results as a function of multiplicity ($N_{trk}^{offline}$) in pp collisions at $\sqrt{s}$ = 13.0 TeV. The results are normalized by $\left<(v_2^{\text{sub}})^{2}\right> \, \left<(v_3^{\text{sub}})^{2}\right>$ and $\left<(v_2^{\text{sub}})^{2}\right> \, \left<(v_4^{\text{sub}})^{2}\right>$ from two-particle correlations.

Three-particle correlation with respect to the 3rd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Two-particle correlation in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane from Pb-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane from p-going side in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane in Pb-going direction in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in p-going direction in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane in Pb-going direction in pPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Three-particle correlation with respect to the 3rd order event plane in PbPb collisions.

Two-particle correlation in pPb collisions.

Two-particle correlation in PbPb collisions.

Two-particle correlation in PbPb collisions.

Three-particle to two-particle correlation ratio from Pb-going side in pPb collisions.

Three-particle to two-particle correlation ratio in PbPb collisions.

Three-particle to two-particle correlation ratio in PbPb collisions.

Three-particle to two-particle correlation ratio in pPb (Pb- and p-going direction) collisions.

Three-particle to two-particle correlation ratio in pPb (Pb- and p-going direction) collisions.

Three-particle to two-particle correlation ratio in pPb (Pb- and p-going direction) collisions.

Three-particle to two-particle correlation ratio in PbPb collisions.

Three-particle to two-particle correlation ratio in PbPb collisions.

Three-particle to two-particle correlation ratio in PbPb collisions.

Three-particle correlation with respect to the 2nd order event plane from Pb-going side as a function of v2 in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane from p-going side as a function of v2 in pPb collisions.

Three-particle correlation with respect to the 2nd order event plane as a function of v2 in PbPb collisions.

Three-particle correlation (OS-SS) with respect to the 2nd order event plane as a function of v2 in pPb collisions.

Three-particle correlation (OS-SS) with respect to the 2nd order event plane as a function of v2 in PbPb collisions.

Three-particle correlation (OS-SS) with respect to the 2nd order event plane as a function of v2 in PbPb collisions.

Two-particle correlation (OS-SS) as a function of v2 in pPb collisions.

Two-particle correlation (OS-SS) as a function of v2 in PbPb collisions.

Ratio of three-particle and two-particle correlation (OS-SS) as a function of v2 in pPb collisions.

Ratio of three-particle and two-particle correlation (OS-SS) as a function of v2 in PbPb collisions.

Extracted intercept parameter b_norm in PbPb collisions.

Extracted intercept parameter b_norm in pPb collisions.

Upper limit on v2-independent gamma_112 correlator component in PbPb collisions.

Upper limit on v2-independent gamma_112 correlator component in pPb collisions.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 0.9\ TeV$ events with the unlike-charge reference sample for various multiplicity intervals $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV$ events with the unlike-charge reference sample for various multiplicity intervals $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. The statistical uncertainties at $7\ TeV$ were corrected on the $\sqrt{\chi^{2}/ndf}$ and they more smaller than systematic uncertainties. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV\ HM$ events with the unlike-charge reference sample for various multiplicity intervals $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 0.9\ TeV$ ($n_{ch} \ge 2$) events with the unlike-charge reference sample for various $k_{T}$ intervals for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV$ ($n_{ch} \ge 2$) events with the unlike-charge reference sample for various $k_{T}$ intervals for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$ , this represents the statistical uncertainty only. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$. The statistical uncertainties at $7\ TeV$ more smaller than systematic uncertainties.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV\ HM$ ($n_{ch} \ge 150$) events with the unlike-charge reference sample for various $k_{T}$ intervals for the exponential parametrization $\Omega^{(E)}$. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$.Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The results of fits of the two-particle double-ratio correlation function $R_{2} (Q)$ for $\sqrt{s} = 7\ TeV$ events with the unlike-charge reference sample for various $k_{T}$ intervals of different multiplicity regions $n_{ch}$ for the exponential parametrization $\Omega^{(E)}$. The statistical uncertainties were corrected on the $\sqrt{\chi^{2}/ndf}$ when $\chi^{2}/ndf > 1$. The statistical uncertainties smaller than systematic uncertainties. The uncertainties for parameters $\lambda$ and $R$ are square root from the quadratic sum of statistical and systematic errors. Where only one error is shown for parameters $C_{0}$ and $\epsilon$, this represents the statistical uncertainty only.

The $Q$ distribution measured at $0.9\ TeV$ for unlike-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $Q$ distribution measured at $0.9\ TeV$ for like-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $Q$ distribution measured at $7\ TeV$ for unlike-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $Q$ distribution measured at $7\ TeV$ for like-sign pairs for $p_{T} > 100\ MeV$ and $|\eta|<2.5$, renormalized to the total number of charged-particle pairs. The error bars represents the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $0.9\ TeV$ using unlike-charge particle reference sample for different $n_{ch}$ intervals $p_{T} > 100\ MeV$ and $|\eta|<2.5$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $0.9\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals with multiplicity $n_{ch} \ge 2$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different multiplicity intervals $n_{ch}$ with $p_{T} > 100\ MeV$ and $|\eta| < 2.5$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals with multiplicity $n_{ch} \ge 2$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV\ HM$ using unlike-charge particle reference sample for different $n_{ch}$ intervals $p_{T} > 100\ MeV$ and $|\eta|<2.5$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured with $7\ TeV\ HM$ data using unlike-charge particle reference sample for different $k_{T}$ intervals with multiplicity $n_{ch} \ge 150$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 2-9$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 10-24$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 25-80$. The error bars represents only the statistical uncertainties.

The $R_{2}(Q)$ correlation function measured at $7\ TeV$ using unlike-charge particle reference sample for different $k_{T}$ intervals within multiplicity interval $n_{ch} = 81-125$. The error bars represents only the statistical uncertainties.

The measured inclusive jet double-differential cross section in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured inclusive jet double-differential cross section in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.4 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.6 as a function of the jet XT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.4 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin |y| < 0.3 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.3 <= |y| < 0.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 0.8 <= |y| < 1.2 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 1.2 <= |y| < 2.1 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.1 <= |y| < 2.8 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 2.8 <= |y| < 3.6 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.

The measured ratio of inclusive jet cross sections at sqrt(s)=2.76 TeV to the one at sqrt(s)=7 TeV in the rapidity bin 3.6 <= |y| < 4.4 for anti-kt jets with R = 0.6 as a function of the jet PT. The first (sys) error is the combined correlated systematic error and the second the combined uncorrelated systematic error, excluding the luminosity uncertainty. Also shown are the multiplicative non-perturbative corrections, NPcorr.