Differential cross section (multiplied by the dimuon branching fraction) of prompt J/$\psi$ mesons in pPb collisions at backward $y_{\mathrm{CM}}$.

Rapidity dependence of the cross section (multiplied by the dimuon branching fraction) for prompt J/$\psi$ mesons in the $p_{\mathrm{T}}$ intervals 6.5<$p_{\mathrm{T}}$<10 GeV and 10<$p_{\mathrm{T}}$<30 GeV in pp collisions.

Rapidity dependence of the cross section (multiplied by the dimuon branching fraction) for prompt J/$\psi$ mesons in the $p_{\mathrm{T}}$ intervals 6.5<$p_{\mathrm{T}}$<10 GeV and 10<$p_{\mathrm{T}}$<30 GeV in pPb collisions.

Transverse momentum dependence of $R_{\mathrm{pPb}}$ for prompt J/$\psi$ mesons in seven $y_{\mathrm{CM}}$ ranges.

Rapidity dependence of $R_{\mathrm{pPb}}$ for prompt J/$\psi$ mesons in $p_{\mathrm{T}}$ range 6.5<$p_{\mathrm{T}}$<10 GeV.

Rapidity dependence of $R_{\mathrm{pPb}}$ for prompt J/$\psi$ mesons in $p_{\mathrm{T}}$ range 10<$p_{\mathrm{T}}$<30 GeV.

Transverse momentum dependence of $R_{\mathrm{FB}}$ for prompt J/$\psi$ mesons in the 0<$y_{\mathrm{CM}}$<0.9 range.

Transverse momentum dependence of $R_{\mathrm{FB}}$ for prompt J/$\psi$ mesons in the 0.9<$y_{\mathrm{CM}}$<1.5 range.

Transverse momentum dependence of $R_{\mathrm{FB}}$ for prompt J/$\psi$ mesons in the 1.5<$y_{\mathrm{CM}}$<1.93 range.

Dependence of $R_{\mathrm{FB}}$ for prompt J/$\psi$ mesons on the hadronic activity in the event, given by the transverse energy deposited in the CMS detector at large pseudorapidities $E_{\mathrm{T}}^{\mathrm{HF}|\eta|>4}$.

Differential cross section (multiplied by the dimuon branching fraction) of nonprompt J/$\psi$ mesons in pp collisions at forward $y_{\mathrm{CM}}$.

Differential cross section (multiplied by the dimuon branching fraction) of nonprompt J/$\psi$ mesons in pp collisions at backward $y_{\mathrm{CM}}$.

Differential cross section (multiplied by the dimuon branching fraction) of nonprompt J/$\psi$ mesons in pPb collisions at forward $y_{\mathrm{CM}}$.

Differential cross section (multiplied by the dimuon branching fraction) of nonprompt J/$\psi$ mesons in pPb collisions at backward $y_{\mathrm{CM}}$.

Rapidity dependence of the cross section (multiplied by the dimuon branching fraction) for nonprompt J/$\psi$ mesons in the $p_{\mathrm{T}}$ intervals 6.5<$p_{\mathrm{T}}$<10 GeV and 10<$p_{\mathrm{T}}$<30 GeV in pp collisions.

Rapidity dependence of the cross section (multiplied by the dimuon branching fraction) for nonprompt J/$\psi$ mesons in the $p_{\mathrm{T}}$ intervals 6.5<$p_{\mathrm{T}}$<10 GeV and 10<$p_{\mathrm{T}}$<30 GeV in pPb collisions.

Transverse momentum dependence of $R_{\mathrm{pPb}}$ for nonprompt J/$\psi$ mesons in seven $y_{\mathrm{CM}}$ ranges.

Rapidity dependence of $R_{\mathrm{pPb}}$ for nonprompt J/$\psi$ mesons in $p_{\mathrm{T}}$ range 6.5<$p_{\mathrm{T}}$<10 GeV.

Rapidity dependence of $R_{\mathrm{pPb}}$ for nonprompt J/$\psi$ mesons in $p_{\mathrm{T}}$ range 10<$p_{\mathrm{T}}$<30 GeV.

Transverse momentum dependence of $R_{\mathrm{FB}}$ for nonprompt J/$\psi$ mesons in the 0<$y_{\mathrm{CM}}$<0.9 range.

Transverse momentum dependence of $R_{\mathrm{FB}}$ for nonprompt J/$\psi$ mesons in the 0.9<$y_{\mathrm{CM}}$<1.5 range.

Transverse momentum dependence of $R_{\mathrm{FB}}$ for nonprompt J/$\psi$ mesons in the 1.5<$y_{\mathrm{CM}}$<1.93 range.

Dependence of $R_{\mathrm{FB}}$ for nonprompt J/$\psi$ mesons on the hadronic activity in the event, given by the transverse energy deposited in the CMS detector at large pseudorapidities $E_{\mathrm{T}}^{\mathrm{HF}|\eta|>4}$.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 1.5 at a centre-of-mass energy of 900 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.0 at a centre-of-mass energy of 900 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.4 at a centre-of-mass energy of 900 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 0.5 at a centre-of-mass energy of 2360 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 1.0 at a centre-of-mass energy of 2360 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 1.5 at a centre-of-mass energy of 2360 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.0 at a centre-of-mass energy of 2360 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.4 at a centre-of-mass energy of 2360 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 0.5 at a centre-of-mass energy of 7000 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 1.0 at a centre-of-mass energy of 7000 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 1.5 at a centre-of-mass energy of 7000 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.0 at a centre-of-mass energy of 7000 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.4 at a centre-of-mass energy of 7000 GeV.

Normalised moments C_Q at a centre-of-mass energy of 0.9 TeV.

Normalised moments C_Q at a centre-of-mass energy of 2.36 TeV.

Normalised moments C_Q at a centre-of-mass energy of 7.0 TeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.4 and PT > 500 MeV at a centre-of-mass energy of 900 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.4 and PT > 500 MeV at a centre-of-mass energy of 2360 GeV.

Fully corrected charged hadron multiplicity spectrum for |pseudorapidity| < 2.4 and PT > 500 MeV at a centre-of-mass energy of 7000 GeV.

Mean transverse momentum for |pseudorapidity| < 2.4 at a centre-of-mass energy of 900 GeV.

Mean transverse momentum for |pseudorapidity| < 2.4 at a centre-of-mass energy of 2360 GeV.

Mean transverse momentum for |pseudorapidity| < 2.4 at a centre-of-mass energy of 7000 GeV.

The charged hadron multiplicity distributions in KNO form for |pseudorapidity| < 0.5 at a centre-of-mass energy of 900 GeV.

The charged hadron multiplicity distributions in KNO form for |pseudorapidity| < 2.4 at a centre-of-mass energy of 900 GeV.

The charged hadron multiplicity distributions in KNO form for |pseudorapidity| < 0.5 at a centre-of-mass energy of 7000 GeV.

The charged hadron multiplicity distributions in KNO form for |pseudorapidity| < 2.4 at a centre-of-mass energy of 7000 GeV.

Unfolded groomed jet radius distribution in PbPb normalized to the number of jets that pass the $x_J$>0.4 selection. All systematic uncertainties are bin-to-bin fully correlated (allowing for sign-changes bin-to-bin).The covaraince matrices are provided for the statistical uncertainties from data and MC in this HepData record.The negative (-0.05,0) bin accounts for jets that failed the soft-drop grooming condition.

Covariance matrix of the statistical uncertainty in data for the unfolded groomed jet radius distribution in PbPb for jets that pass the $x_J$>0.4 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Covariance matrix of the statistical uncertainty in MC for the unfolded groomed jet radius distribution in PbPb for jets that pass the $x_J$>0.4 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Unfolded jet girth distribution in PbPb normalized to the number of jets that pass the $x_J$>0.8 selection. All systematic uncertainties are bin-to-bin fully correlated (allowing for sign-changes bin-to-bin).The covaraince matrices are provided for the statistical uncertainties from data and MC in this HepData record.

Covariance matrix of the statistical uncertainty in data for the unfolded jet girth distribution in PbPb for jets that pass the $x_J$>0.4 selection.The bin indices correspond to the bins used in the jet girth distribution.

Covariance matrix of the statistical uncertainty in MC for the unfolded jet girth distribution in PbPb for jets that pass the $x_J$>0.8 selection.The bin indices correspond to the bins used in the jet girth distribution.

Unfolded groomed jet radius distribution in PbPb normalized to the number of jets that pass the $x_J$>0.8 selection. All systematic uncertainties are bin-to-bin fully correlated (allowing for sign-changes bin-to-bin).The covaraince matrices are provided for the statistical uncertainties from data and MC in this HepData record.The negative (-0.05,0) bin accounts for jets that failed the soft-drop grooming condition.

Covariance matrix of the statistical uncertainty in data for the unfolded groomed jet radius distribution in PbPb for jets that pass the $x_J$>0.8 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Covariance matrix of the statistical uncertainty in MC for the unfolded groomed jet radius distribution in PbPb for jets that pass the $x_J$>0.8 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Unfolded jet girth distribution in pp normalized to the number of jets that pass the $x_J$>0.4 selection. All systematic uncertainties are bin-to-bin fully correlated (allowing for sign-changes bin-to-bin).The covaraince matrices are provided for the statistical uncertainties from data and MC in this HepData record.

Covariance matrix of the statistical uncertainty in data for the unfolded jet girth distribution in pp for jets that pass the $x_J$>0.4 selection.The bin indices correspond to the bins used in the jet girth distribution.

Covariance matrix of the statistical uncertainty in MC for the unfolded jet girth distribution in pp for jets that pass the $x_J$>0.4 selection.The bin indices correspond to the bins used in the jet girth distribution.

Unfolded groomed jet radius distribution in pp normalized to the number of jets that pass the $x_J$>0.4 selection. All systematic uncertainties are bin-to-bin fully correlated (allowing for sign-changes bin-to-bin).The covaraince matrices are provided for the statistical uncertainties from data and MC in this HepData record.The negative (-0.05,0) bin accounts for jets that failed the soft-drop grooming condition.

Covariance matrix of the statistical uncertainty in data for the unfolded groomed jet radius distribution in pp for jets that pass the $x_J$>0.4 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Covariance matrix of the statistical uncertainty in MC for the unfolded groomed jet radius distribution in pp for jets that pass the $x_J$>0.4 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Unfolded jet girth distribution in pp normalized to the number of jets that pass the $x_J$>0.8 selection. All systematic uncertainties are bin-to-bin fully correlated (allowing for sign-changes bin-to-bin).The covaraince matrices are provided for the statistical uncertainties from data and MC in this HepData record.

Covariance matrix of the statistical uncertainty in data for the unfolded jet girth distribution in pp for jets that pass the $x_J$>0.8 selection.The bin indices correspond to the bins used in the jet girth distribution.

Covariance matrix of the statistical uncertainty in MC for the unfolded jet girth distribution in pp for jets that pass the $x_J$>0.8 selection.The bin indices correspond to the bins used in the jet girth distribution.

Unfolded groomed jet radius distribution in pp normalized to the number of jets that pass the $x_J$>0.8 selection. All systematic uncertainties are bin-to-bin fully correlated (allowing for sign-changes bin-to-bin).The covaraince matrices are provided for the statistical uncertainties from data and MC in this HepData record.The negative (-0.05,0) bin accounts for jets that failed the soft-drop grooming condition.

Covariance matrix of the statistical uncertainty in data for the unfolded groomed jet radius distribution in pp for jets that pass the $x_J$>0.8 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Covariance matrix of the statistical uncertainty in MC for the unfolded groomed jet radius distribution in pp for jets that pass the $x_J$>0.8 selection.The bin indices correspond to the bins used in the groomed jet radius distribution.

Ratio of yields in PbPb to pp for the unfolded jet girth distribution normalized to the number of jets that pass the $x_J$>0.4 selection. Each uncertainty is symmetrized and added in quadrature.All systematic uncertainties have been obtained assuming the PbPb and pp uncertainties are uncorrelated.

Ratio of yields in PbPb to pp for the unfolded groomed jet radius distribution normalized to the number of jets that pass the $x_J$>0.4 selection. Each uncertainty is symmetrized and added in quadrature.All systematic uncertainties have been obtained assuming the PbPb and pp uncertainties are uncorrelated.The negative (-0.05,0) bin accounts for jets that failed the soft-drop grooming condition.

Ratio of yields in PbPb to pp for the unfolded jet girth distribution normalized to the number of jets that pass the $x_J$>0.8 selection. Each uncertainty is symmetrized and added in quadrature.All systematic uncertainties have been obtained assuming the PbPb and pp uncertainties are uncorrelated.

Ratio of yields in PbPb to pp for the unfolded groomed jet radius distribution normalized to the number of jets that pass the $x_J$>0.8 selection. Each uncertainty is symmetrized and added in quadrature.All systematic uncertainties have been obtained assuming the PbPb and pp uncertainties are uncorrelated.The negative (-0.05,0) bin accounts for jets that failed the soft-drop grooming condition.

RMS of raw subtracted $p_T$ for jets reconstructed in PbPb collisions (in different centrality bins) with the anti-k$_T$ algorythm with a distance parameter $R=0.3$, in $|\eta|<0.2$.

Inclusive jet cross section in pp collisions, for anti-k$_T$ jets with a distance parameter $R=0.2, 0.3, 0.4$, reconstructed in $|\eta|<0.2$. The '3.7%' luminosity uncertainty is a fully correlated uncertainty, and not included in the point-to-point uncertainty.

Inclusive jet spectra in different centrality bins of PbPb collisions, for anti-k$_T$ jets of distance parameter $R=0.2$, reconstructed in $|\eta|<0.2$. The PbPb spectra in each case are scaled by TAA. The uncertainty on the TAA is considered as global uncertainty (common to all points for a given centrality), and it is not included in the point-to-point uncertainties.

Inclusive jet spectra in different centrality bins of PbPb collisions, for anti-k$_T$ jets of distance parameter $R=0.3$, reconstructed in $|\eta|<0.2$. The PbPb spectra in each case are scaled by TAA. The uncertainty on the TAA is considered as global uncertainty (common to all points for a given centrality), and it is not included in the point-to-point uncertainties.

Inclusive jet spectra in different centrality bins of PbPb collisions, for anti-k$_T$ jets of distance parameter $R=0.4$, reconstructed in $|\eta|<0.2$. The PbPb spectra in each case are scaled by TAA. The uncertainty on the TAA is considered as global uncertainty (common to all points for a given centrality), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 0-5\% PbPb centrality. The '5.5%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 5-10\% PbPb centrality. The '5.9%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 10-30\% PbPb centrality. The '6.9%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 30-50\% PbPb centrality. The '10%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 50-70\% PbPb centrality. The '15%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, with $|\eta|<2$, for 70-90\% PbPb centrality. The '18%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

Inclusive jet RAA as a function of average Npart, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, reconstructed in the range $80< p_T < 90$GeV/c and $|\eta|<2$.

Inclusive jet RAA as a function of average Npart, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3, 0.4$, reconstructed in the range $130< p_T < 150$GeV/c and $|\eta|<2$.

Inclusive jet RAA as a function of jet $p_T$, for anti-k$_T$ jets with distance parameter $R=0.2, 0.3$, reconstructed in the range $|\eta|<2$, for 0-10\% PbPb centrality. The '5.7%' combined uncertainty on the pp luminosity and PbPb TAA is considered as global uncertainty (common to all points), and it is not included in the point-to-point uncertainties.

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

Spectra of jets with |eta jet| < 2.0 for R = 0.6, for pp collisions and different centrality classes of PbPb collisions.

Spectra of jets with |eta jet| < 2.0 for R = 0.8, for pp collisions and different centrality classes of PbPb collisions.

Spectra of jets with |eta jet| < 2.0 for R = 1.0, for pp collisions and different centrality classes of PbPb collisions.

The spectra ratio for jets from pp collisions with |eta jet| < 2.0 for R = 0.2–0.8 with respect to R = 1.0.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.2 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.3 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.4 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.6 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 0.8 and various centrality classes.

The RAA for jets with |eta jet| < 2.0 as a function of jet PT for R = 1.0 and various centrality classes.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 200-250 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 250-300 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 300-400 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 400-500 GeV.

The RAA-ratio for jets with |eta jet| < 2.0 as a function of R for R = 0.3–1.0 with respect to R = 0.2, in various event centrality classes and jet PT = 500-1000 GeV.

Invariant charged particle differential yield in the centrality regions 30 TO 50%, 50 TO 70% and 70 TO 90%.

Nuclear modification factor RAA in the centrality regions 0 TO 5%, 5 TO 10% and 10 TO 30%.

Nuclear modification factor RAA in the centrality regions 30 TO 50%, 50 TO 70% and 70 TO 90%.

TAA-scaled ratio of PT spectra in central and peripheral bins, RCP.