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

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

The differential jet shape, $\rho(r)$, for jets associated with an isolated photon in 10-30% centrality PbPb collisions.

The differential jet shape, $\rho(r)$, for jets associated with an isolated photon in 0-10% centrality PbPb collisions.

PbPb / pp ratio of $\rho(r)$ for 50-100% centrality PbPb collisions.

PbPb / pp ratio of $\rho(r)$ for 30-50% centrality PbPb collisions.

PbPb / pp ratio of $\rho(r)$ for 10-30% centrality PbPb collisions.

PbPb / pp ratio of $\rho(r)$ for 0-10% centrality PbPb collisions.

The nuclear modification factor of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The nuclear modification factor of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points. Bins where no data point has been reported are denoted as 'empty'.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The average N_part, N_coll, and TAA for various centrality classes of XeXe collisions at 5.44 TeV.

Differential cross sections of the Y(2S) meson as a function of pT for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of pT for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of pT for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Differential cross sections of the Y(1S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(1S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(2S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(2S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Nuclear modification factor of the Y(1S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(1S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(3S) meson as a function of pT.

Nuclear modification factor of the Y(3S) meson as a function of pT.

Nuclear modification factor of the Y(1S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(1S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(3S) meson as a function of rapidity.

Nuclear modification factor of the Y(3S) meson as a function of rapidity.

Nuclear modification factor of the Y(1S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(1S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(1S) state.

Nuclear modification factor of the Y(1S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(1S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(1S) state.

Nuclear modification factor of the Y(2S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(2S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(2S) state.

Nuclear modification factor of the Y(2S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(2S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(2S) state.

Confidence intervals on the nuclear modification factors of the Y(3S) mesons as a function of collision centrality.

Confidence intervals on the nuclear modification factors of the Y(3S) mesons as a function of collision centrality.

Confidence intervals on the nuclear modification factors of the Y(2S) mesons as a function of collision centrality.

Confidence intervals on the nuclear modification factors of the Y(2S) mesons as a function of collision centrality.

Nuclear modification factors of the Y(1S) and Y(2S) mesons in the integrated pT, rapidity and centrality.

Nuclear modification factors of the Y(1S) and Y(2S) mesons in the integrated pT, rapidity and centrality.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

The 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.

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

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

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

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

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

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

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

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

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

x_J distribution of incluisve dijets in pp collisions

x_J distribution of b-quark dijets in pp collisions

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

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

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

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

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

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

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

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

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

$\xi^\mathrm{jet}$ distributions for jets associated with an isolated photon in pp and 0-10% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 50-100% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 30-50% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 10-30% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\mathrm{jet}$ distributions for 0-10% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 50-100% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 30-50% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 10-30% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

$\xi^\gamma_{\mathrm{T}}$ distributions for jets associated with an isolated photon in pp and 0-10% centrality PbPb collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 50-100% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 30-50% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 10-30% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.

PbPb / pp ratio of $\xi^\gamma_{\mathrm{T}}$ distributions for 0-10% centrality collisions. The resolutions of the measured jet energy and azimuthal angle in pp are smeared to match those in the PbPb sample.