$\Delta\phi$ projection of balance function in low $p_{T}$ in 0-10% centrality

$\Delta\phi$ projection of balance function in low $p_{T}$ in 30-40% centrality

1D $\Delta\eta$ projection of balance function in low $p_{T}$ in 70-80% centrality

$\Delta\eta$ projection of balance function in low $p_{T}$ in 0-40 $N_{trk}$

$\Delta\eta$ projection of balance function in low $p_{T}$ in 120-150 $N_{trk}$

$\Delta\eta$ projection of balance function in low $p_{T}$ in 270-300 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 0-40 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 120-150 $N_{trk}$

$\Delta\phi$ projection of balance function in low $p_{T}$ in 270-300 $N_{trk}$

The width of balance function in $<|\Delta\eta|>$ in low $p_{T}$ for PbPb collisions

Balance function width in low $p_{T}$ PbPb relative $<|\Delta\eta|>/<|\Delta\eta|>_{N_{ch}<65}$

The width of balance function in $<|\Delta\eta|>$ in low $p_{T}$ for pPb collisions

Balance function width in low $p_{T}$ in pPb relative $<|\Delta\eta|>/<|\Delta\eta|>_{N_{ch}<24}$

The width of the balance function in $<|\Delta\phi|>$ in low $p_{T}$ for PbPb collisions

Balance function width in low $p_{T}$ in PbPb for relative $<|\Delta\phi|>/<|\Delta\phi|>_{N_{ch}<65}$

The width of the balance function in $<|\Delta\phi|>$ in low $p_{T}$ for pPb collisions

Balance function width in low $p_{T}$ in pPb for relative $|\Delta\phi|/<|\Delta\phi|>_{N_{ch}<24}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 0-40 $N_{trk}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 120-150 $N_{trk}$

Balance function projection as a function of $\Delta\eta$ in intermediate $p_{T}$ in pPb for 270-300 $N_{trk}$

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\phi$ in intermediate $p_{T}$ in pPb for $N_{trk}$ 270-300

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 0-10% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 30-40% centrality

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for 70-80% centrality

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\eta$ in high $p_{T}$ in pPb for $N_{trk}$ 270-300

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 0-40

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 120-150

Balance function projection as a function of $\Delta\phi$ in high $p_{T}$ in PbPb for $N_{trk}$ 270-300

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \phi$ with $p_{T}$ for low $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \eta$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for low $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for intermediate $p_{T}$

Average width of the balance function in $\Delta \phi$ with $N_{ch}$ for high $p_{T}$

Differential cross section times dimuon branching fraction of Y(1S) as a function of $y^{Y}_{CM}$ in pPb collisions. The global uncertainty arises from the integrated luminosity uncertainty in pPb collisions.

Differential cross section times dimuon branching fraction of Y(2S) as a function of $y^{Y}_{CM}$ in pPb collisions. The global uncertainty arises from the integrated luminosity uncertainty in pPb collisions.

Differential cross section times dimuon branching fraction of Y(3S) as a function of $y^{Y}_{CM}$ in pPb collisions. The global uncertainty arises from the integrated luminosity uncertainty in pPb collisions.

Differential cross section times dimuon branching fraction of Y(1S) as a function of pT in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(2S) as a function of pT in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(3S) as a function of pT in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(1S) as a function of $|y^{Y}_{CM}|$ in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(2S) as a function of $|y^{Y}_{CM}|$ in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross section times dimuon branching fraction of Y(3S) as a function of $|y^{Y}_{CM}|$ in pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Nuclear modification factor of Y(1S) as a function of pT. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) as a function of pT. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) as a function of pT. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(1S) as a function of $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) as a function of $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) as a function of $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(1S) at forward and backward $y^{Y}_{CM}$ for pT < 6 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) at forward and backward $y^{Y}_{CM}$ for pT < 6 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) at forward and backward $y^{Y}_{CM}$ for pT < 6 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(1S) at forward and backward $y^{Y}_{CM}$ for 6 < pT < 30 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(2S) at forward and backward $y^{Y}_{CM}$ for 6 < pT < 30 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Nuclear modification factor of Y(3S) at forward and backward $y^{Y}_{CM}$ for 6 < pT < 30 GeV/c. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

RFB of Y(1S) versus $N^{|\eta_{lab}|<2.4}_{tracks}$.

RFB of Y(2S) versus $N^{|\eta_{lab}|<2.4}_{tracks}$.

RFB of Y(3S) versus $N^{|\eta_{lab}|<2.4}_{tracks}$.

RFB of Y(1S) versus $E^{|\eta_{lab}|>4}_{T}$.

RFB of Y(2S) versus $E^{|\eta_{lab}|>4}_{T}$.

RFB of Y(3S) versus $E^{|\eta_{lab}|>4}_{T}$.

Nuclear modification factor of Y(1S), Y(2S), and Y(3S) integrated over pT and $y^{Y}_{CM}$. The global uncertainty arises from the integrated luminosity uncertainties in pPb and pp collisions.

Corrected inclusive charged-particle jet distributions in Au+Au collisions at 200 GeV for R=0.2, 0.3, and 0.4 in peripheral (60-80%) Au+Au collisions for pTlead,min = 7 GeV/c. The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric).

pTlead,min (7/5 GeV/c) ratios of inclusive charged-particle jet distributions in Au+Au collisions at 200 GeV for R=0.2, 0.3, and 0.4 in peripheral Au+Au collisions. The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric).

pTlead,min (7/5 GeV/c) ratios of inclusive charged-particle jet distributions in Au+Au collisions at 200 GeV for R=0.2, 0.3, and 0.4 in central Au+Au collisions. The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric).

R_CP (0-10%/60-80%) ratios of inclusive charged-particle jet distributions in Au+Au collisions at 200 GeV for R = 0.2, 0.3, and 0.4 for pTlead,min = 5 GeV/c. The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric). In addition, the systematic uncertainty for the T_AA normalization (30%) has to be added.

R_CP (0-10%/60-80%) ratios of inclusive charged-particle jet distributions in Au+Au collisions at 200 GeV for R = 0.2 and 0.3 for pTlead,min = 5 GeV/c. The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric). In the paper are shown all these three uncertainty sources (statistical, shape, correlated) summed in quadrature. The systematic uncertainty for the T_AA normalization (30%) has not been included (as for the other measurements compared with the STAR data).

R_AA for peripheral (60-80%) Au+Au collisions at 200 GeV for R = 0.2, 0.3, and 0.4 for pTlead,min = 5 GeV/c. The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric). In addition, the systematic uncertainty for the T_AA normalization (29%) and PYTHIA reference (22%, 20%, 18% for R = 0.2, 0.3 and 0.4) have to be added.

R_AA for central (0-10%) Au+Au collisions at 200 GeV for R = 0.2, 0.3, and 0.4 for pTlead,min = 5 GeV/c. The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric). In addition, the systematic uncertainty for the T_AA normalization (7%) and PYTHIA reference (22%, 20%, 18% for R = 0.2, 0.3 and 0.4) have to be added. The unbiased data points are the 4 highest for R=0.2 and 3 highest for R=0.3 and 0.4, resp.

Ratio of inclusive charged-particle jet yields for R=0.2/R=0.4 for peripheral (60-80%) Au+Au collisions at 200 GeV for pTlead,min = 5 GeV/c (only unbiased region). The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric). Please note that in the paper, the uncertainties shown are the quadrature sums of the uncertainties listed in the table.

Ratio of inclusive charged-particle jet yields for R=0.2/R=0.4 for central (0-10%) Au+Au collisions at 200 GeV for pTlead,min = 5 GeV/c (only unbiased region). The first uncertainty is statistical (symmetric), followed by shape uncertainty (asymmetric) and correlated uncertainty (asymmetric). Please note that in the paper, the uncertainties shown are the quadrature sums of the uncertainties listed in the table.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential fiducial cross section (without the acceptance correction) for the DY process measured in the muon channel, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Integrated fiducial cross section for the DY process measured in the muon channel. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of dimuon invariant mass. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of rapidity in the centre-of-mass frame for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of rapidity in the centre-of-mass frame for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Differential cross section for the DY process measured in the muon channel, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Integrated cross section for the DY process measured in the muon channel. The quoted error is the quadratic sum of the statistical and systematic uncertainties. The global normalisation uncertainty of 3.5% is listed separately.

Forward-backward ratios for $15<m_{\mu\mu}<60$ GeV. Quoted uncertainties are the quadratic sum of the statistical and systematic uncertainties.

Forward-backward ratios for $60<m_{\mu\mu}<120$ GeV. Quoted uncertainties are the quadratic sum of the statistical and systematic uncertainties.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of dimuon invariant mass.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$ for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$ for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$ for $15<m_{\mu\mu}<60$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$ for $60<m_{\mu\mu}<120$ GeV.

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of rapidity in the centre-of-mass frame, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in rapidity in the centre-of-mass frame. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $p_{\textrm{T}}$, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in $p_{\textrm{T}}$. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

Correlation matrix for the systematic uncertainties, excluding integrated luminosity, as a function of $\phi^*$, putting together low and high masses. Each bin is labeled lm_i or hm_i, where lm stands for $15<m_{\mu\mu}<60$ GeV, hm stands for $60<m_{\mu\mu}<120$ GeV, and i is the corresponding bin number in $\phi^*$. The global normalisation uncertainty of 3.5% is not included. Data from Figure [3, 4, 4].

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

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

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.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $N_{ch}(p_T < 0.4 GeV)$ (EvSel_$N_{ch}$) for PbPb collisions at $\sqrt{ s_{NN} }$=2.76 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_2\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_2\{4\}/v_2\{2, | \Delta \eta > 2 \}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{6\}/v_2\{4\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_2\{8\}/v_2\{6\}$ ratio for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_3\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_3\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$c_4\{2, | \Delta \eta > 2\}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$c_4\{2, | \Delta \eta > 2 \}$ cumulants for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_3\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_3\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.3 $< p_T <$ 3.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pp collisions at $\sqrt{s}$= 13 TeV.

$v_4\{2, | \Delta \eta > 2\}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for pPb collisions at $\sqrt{ s_{NN} }$= 5.02 TeV.

$v_4\{2, | \Delta \eta > 2 \}$ harmonics for reference particles with 0.5 $< p_T <$ 5.0 GeV selected according to $M_{ref}$ (EvSel_$M_{ref}$) for PbPb collisions at $\sqrt{ s_{NN} }$= 2.76 TeV.

$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T} < $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for p+Pb collisions at $ \sqrt{ s_{NN} } $= 5.02 TeV.

$ v_2\{4\} $ harmonics for reference particles with 0.2 $ < p_{T}< $ 3.0 GeV as a function of $ < N_{ch}(|\eta|<1) > $ for Pb+Pb collisions at $ \sqrt{ s_{NN} } $= 2.76 TeV.

D(pt) distributions for pp and Pb+Pb collisions, jet rapidity 1.2 < |y| < 2.1.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 2.1.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 0.3.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity 0.3 < |y| < 0.8.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity 1.2 < |y| < 2.1.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

The difference between the total yield of particles with 1 < pt^trk < 4 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total yield of particles with 4 < pt^trk < 25 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total yield of particles with 25 < pt^trk < 100 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total transverse momentum of particles with 1 < pt^trk < 4 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total transverse momentum of particles with 4 < pt^trk < 25 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total transverse momentum of particles with 25 < pt^trk < 100 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The ratio of R_D(z) distributions in three rapidity selections for 0-10 PCT Pb+Pb collisions.

The ratio of R_D(z) distributions in three rapidity selections for 10-20 PCT Pb+Pb collisions.

The ratio of R_D(z) distributions in three rapidity selections for 20-30 PCT Pb+Pb collisions.