Fig. 1 Left, data for jet radius R=0.4. Unfolded pp full jet cross-section at $\sqrt{s}$ = 5.02 TeV for R = 0.1 − 0.6. No leading track requirement is imposed.

Fig. 1 Left, data for jet radius R=0.5. Unfolded pp full jet cross-section at $\sqrt{s}$ = 5.02 TeV for R = 0.1 − 0.6. No leading track requirement is imposed.

Fig. 1 Left, data for jet radius R=0.6. Unfolded pp full jet cross-section at $\sqrt{s}$ = 5.02 TeV for R = 0.1 − 0.6. No leading track requirement is imposed.

Fig. 2, values for jet radius R=0.1. Non-perturbative correction factor applied to parton-level NLO+NLL predictions, obtained from PYTHIA 8 tune A14 as the ratio of the inclusive jet spectrum at hadron-level with MPI compared to parton-level without MPI.

Fig. 2, values for jet radius R=0.2. Non-perturbative correction factor applied to parton-level NLO+NLL predictions, obtained from PYTHIA 8 tune A14 as the ratio of the inclusive jet spectrum at hadron-level with MPI compared to parton-level without MPI.

Fig. 2, values for jet radius R=0.3. Non-perturbative correction factor applied to parton-level NLO+NLL predictions, obtained from PYTHIA 8 tune A14 as the ratio of the inclusive jet spectrum at hadron-level with MPI compared to parton-level without MPI.

Fig. 2, values for jet radius R=0.4. Non-perturbative correction factor applied to parton-level NLO+NLL predictions, obtained from PYTHIA 8 tune A14 as the ratio of the inclusive jet spectrum at hadron-level with MPI compared to parton-level without MPI.

Fig. 2, values for jet radius R=0.5. Non-perturbative correction factor applied to parton-level NLO+NLL predictions, obtained from PYTHIA 8 tune A14 as the ratio of the inclusive jet spectrum at hadron-level with MPI compared to parton-level without MPI.

Fig. 2, values for jet radius R=0.6. Non-perturbative correction factor applied to parton-level NLO+NLL predictions, obtained from PYTHIA 8 tune A14 as the ratio of the inclusive jet spectrum at hadron-level with MPI compared to parton-level without MPI.

Fig. 3 Bottom, data for jet radius ratio R=0.1/R=0.2. Unfolded pp jet cross-section ratios for various R. With R = 0.1 in the numerator.

Fig. 3 Bottom, data for jet radius ratio R=0.1/R=0.3. Unfolded pp jet cross-section ratios for various R. With R = 0.1 in the numerator.

Fig. 3 Bottom, data for jet radius ratio R=0.1/R=0.4. Unfolded pp jet cross-section ratios for various R. With R = 0.1 in the numerator.

Fig. 3 Bottom, data for jet radius ratio R=0.1/R=0.5. Unfolded pp jet cross-section ratios for various R. With R = 0.1 in the numerator.

Fig. 3 Bottom, data for jet radius ratio R=0.1/R=0.6. Unfolded pp jet cross-section ratios for various R. With R = 0.1 in the numerator.

Fig. 3 Top, data for jet radius ratio R=0.2/R=0.3. Unfolded pp jet cross-section ratios for various R. With R = 0.2 in the numerator.

Fig. 3 Top, data for jet radius ratio R=0.2/R=0.4. Unfolded pp jet cross-section ratios for various R. With R = 0.2 in the numerator.

Fig. 3 Top, data for jet radius ratio R=0.2/R=0.5. Unfolded pp jet cross-section ratios for various R. With R = 0.2 in the numerator.

Fig. 3 Top, data for jet radius ratio R=0.2/R=0.6. Unfolded pp jet cross-section ratios for various R. With R = 0.2 in the numerator.

Fig. 4 Left, data for pp. Unfolded pp and Pb-Pb full jet spectra at $\sqrt{s}=5.02$ TeV for $R=0.2$, with 5 GeV leading track requirement. The pp data points correspond to $\frac{\mathrm{d}^{2}\sigma}{\mathrm{d}p_{\mathrm{T,jet}} \mathrm{d}\eta_{\mathrm{jet}}}$.

Fig. 4 Left, data for PbPb. Unfolded pp and Pb-Pb full jet spectra at $\sqrt{s}=5.02$ TeV for $R=0.2$, with 5 GeV leading track requirement. The pp data points correspond to $\frac{\mathrm{d}^{2}\sigma}{\mathrm{d}p_{\mathrm{T,jet}} \mathrm{d}\eta_{\mathrm{jet}}}$.

Fig. 4 Right, data for pp. Unfolded pp and Pb-Pb full jet spectra at $\sqrt{s}=5.02$ TeV for $R=0.4$, with 7 GeV leading track requirement.

Fig. 4 Right, data for PbPb. Unfolded pp and Pb-Pb full jet spectra at $\sqrt{s}=5.02$ TeV for $R=0.4$, with 7 GeV leading track requirement.

Fig. 5 Left, data for pp jet cross section with leading track bias ratio 5/0. Ratio of the pp jet cross-section with various leading charged particle requirements

Fig. 5 Left, data for pp jet cross section with leading track bias ratio 7/0. Ratio of the pp jet cross-section with various leading charged particle requirements

Fig. 5 Left, data for pp jet cross section with leading track bias ratio 7/5. Ratio of the pp jet cross-section with various leading charged particle requirements

Fig. 5 Right. Ratio of the R = 0.2 Pb–Pb jet cross-section with a 7 GeV/c leading charged particle requirement compared to a 5 GeV/c leading charged particle requirement.

Fig. 6 Top Left. Jet $R_{\mathrm{AA}}$ at $\sqrt{s}=5.02$ TeV for $R=0.2$. Same leading track requirement of 5 GeV is imposed on the numerator as well as denominator.

Fig. 6 Top Right. Jet $R_{\mathrm{AA}}$ at $\sqrt{s}=5.02$ TeV for $R=0.4$. Same leading track requirement of 7 GeV is imposed on the numerator as well as denominator.

Fig. 6 Bottom Left. Jet $R_{\mathrm{AA}}$ at $\sqrt{s}=5.02$ TeV for $R=0.2$. PbPb with leading track requirement of 5 GeV. pp reference without a leading track requirement.

Fig. 6 Bottom Right. Jet $R_{\mathrm{AA}}$ at $\sqrt{s}=5.02$ TeV for $R=0.4$. PbPb with leading track requirement of 7 GeV. pp reference without a leading track requirement.

Rapidity dependence (in 0-90% centrality class) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a rapidity-correlated systematic uncertainty.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 4. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

Rapidity dependence (in 0-90% centrality class) of the ratio of the inclusive J/$\psi$ $R_{\rm AA}$ at $\sqrt{s_{NN}}$= 5.02 and 2.76 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a rapidity-correlated systematic uncertainty.

Transverse momentum dependence (in 0-20% centrality class) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a $p_{\rm T}$-correlated systematic uncertainty.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 7. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

Transverse momentum dependence (in 0-20% centrality class) of the ratio of the inclusive J/$\psi$ $R_{\rm AA}$ at $\sqrt{s_{NN}}$= 5.02 and 2.76 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a $p_{\rm T}$-correlated systematic uncertainty.

Transverse momentum dependence (in 20-40% centrality class) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a $p_{\rm T}$-correlated systematic uncertainty.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 10. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

Transverse momentum dependence (in 20-40% centrality class) of the ratio of the inclusive J/$\psi$ $R_{\rm AA}$ at $\sqrt{s_{NN}}$= 5.02 and 2.76 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a $p_{\rm T}$-correlated systematic uncertainty.

Transverse momentum dependence (in 40-90% centrality class) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a $p_{\rm T}$-correlated systematic uncertainty.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 13. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

Transverse momentum dependence (in 40-90% centrality class) of the ratio of the inclusive J/$\psi$ $R_{\rm AA}$ at $\sqrt{s_{NN}}$= 5.02 and 2.76 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a $p_{\rm T}$-correlated systematic uncertainty.

Rapidity dependence (in 0-20% centrality class) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a rapidity-correlated systematic uncertainty.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 16. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

Rapidity dependence (in 20-40% centrality class) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a rapidity-correlated systematic uncertainty.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 18. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

Rapidity dependence (in 40-90% centrality class) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a rapidity-correlated systematic uncertainty.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 20. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 0.3 < $p_{\rm T}$ < 2 $GeV/c$) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 22. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 0.3 < $p_{\rm T}$ < 2 $GeV/c$) of the ratio of the inclusive J/$\psi$ $R_{\rm AA}$ at $\sqrt{s_{NN}}$= 5.02 and 2.76 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

$\langle N_{part} \rangle$-dependence (for 2 < $p_{\rm T}$ < 5 $GeV/c$) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 25. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 2 < $p_{\rm T}$ < 5 $GeV/c$) of the ratio of the inclusive J/$\psi$ $R_{\rm AA}$ at $\sqrt{s_{NN}}$= 5.02 and 2.76 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

$\langle N_{part} \rangle$-dependence (for 5 < $p_{\rm T}$ < 8 $GeV/c$) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 28. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 5 < $p_{\rm T}$ < 8 $GeV/c$) of the ratio of the inclusive J/$\psi$ $R_{\rm AA}$ at $\sqrt{s_{NN}}$= 5.02 and 2.76 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

$\langle N_{part} \rangle$-dependence (for 8 < $p_{\rm T}$ < 12 $GeV/c$) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 31. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 0.3 < $p_{\rm T}$ < 8 $GeV/c$) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, 60–70%, 70–80% and 80–90%. The values, already published in https://doi.org/10.1016/j.physletb.2016.12.064 (Figure.4), were updated with the improved $\langle T_{AA} \rangle$ calculations reported in https://cds.cern.ch/record/2636623.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 33. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 2.5 < $y$ < 3) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 35. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 3 < $y$ < 3.5) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 37. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$\langle N_{part} \rangle$-dependence (for 3.5 < $y$ < 4) of the inclusive J/$\psi$ $R_{\rm AA}$. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The minimum and maximum variations for the $R_{\rm AA}$ of prompt J/$\psi$ with respect to the $R_{\rm AA}$ values of inclusive J/$\psi$ reported in Table 39. The variations correspond to two extreme hypotheses on the unknown contribution of non-prompt J/$\psi$.

$p_{\rm T}$-differential yields of the inclusive J/$\psi$ in various centrality classes. The first uncertainty is statistical, while the second is the uncorrelated systematic.

$\langle N_{part} \rangle$-dependence of the inclusive J/$\psi$ average $p_{\rm T}$. The first uncertainty is statistical, while the second is the uncorrelated systematic. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

$\langle N_{part} \rangle$-dependence of the inclusive J/$\psi$ $r_{\rm AA}$. The first uncertainty is the quadratic sum of the statistical and uncorrelated systematic ones, while the second is a centrality-correlated systematic uncertainty. The $\langle N_{part} \rangle$ values correspond descendingly to the centrality classes 0–10%, 10–20%, 20–30%, 30–40%, 40–50%, 50–60%, and 60–90%.

The $\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\bar\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

The $\bar\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

The $\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\bar\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

The $\bar\Lambda$ global polarization as function of centrality for Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

The average $(\Lambda+\bar\Lambda) \times (2.76+5.02)$ global polarization in Pb-Pb collisions for centrality 15-50%.

The $\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 5-15% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 15-50% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\bar\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 5-15% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\bar\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 15-50% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=2.76$~TeV.

The $\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 5-15% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

The $\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 15-50% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

The $\bar\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 5-15% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

The $\bar\Lambda$ global polarization as function of transverse momentum ($p_{\mathrm{T}}$) for 15-50% centrality in Pb-Pb collisions at $\sqrt{s_{\mathrm{NN}}}=5.02$~TeV.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - V0M multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets08 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Lambda+\bar{\Lambda}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$\Omega^{-}+\bar{\Omega^{+}}$ transverse momentum spectrum ratios to INEL>0 - SPDtracklets0815 multiplicity classes. Total systematic uncertainties include both correlated and uncorrelated uncertainties across multiplicity. Uncorrelated systematic originating from the multiplicity dependence of the efficiency (2%) is not included.

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ average transverse momentum vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ average transverse momentum vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ self-normalized yields vs self-normalized multiplicity - SPDTracklets0815 multiplicity classes

$K^{0}_{S}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$\Lambda+\bar{\Lambda}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$\Xi^{-}+\bar{\Xi^{+}}$ transverse momentum spectra ratios SPDTracklets-to-V0M

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$, $K^{0}_{S}$ integrated yields vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets08 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets0815 multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$ integrated yields (no extr.) vs multiplicity - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - SPDtracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}$ integrated yields (no extr.) vs multiplicity - V0M multiplicity classes

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$, $\Omega^{-}+\bar{\Omega^{+}}$ integrated yields - INEL>0. V0M multiplicity dependent yields are already listed in Table 8c.

$K^{0}_{S}$, $\Lambda+\bar{\Lambda}$, $\Xi^{-}+\bar{\Xi^{+}}$, $\Omega^{-}+\bar{\Omega^{+}}$ integrated yields - INEL>0. V0M multiplicity dependent yields at 7 TeV are listed in the corresponding repository ("https://www.hepdata.net/record/77284").

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - Tracklets08 multiplicity classes

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - Tracklets0815 multiplicity classes

$\Lambda+\bar{\Lambda}/K^{0}_{S}$, $\Xi^{-}+\bar{\Xi^{+}}/K^{0}_{S}$ - V0M multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - Tracklets08 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - Tracklets0815 multiplicity classes

$\Omega^{-}+\bar{\Omega^{+}}/K^{0}_{S}$ - V0M multiplicity classes

The $\Upsilon$(1S) $v_2$ coefficient in three centrality intervals integrated over the transverse momentum range 2~$<$~$p_{\rm T}$~$<$~15 GeV/$c$ in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

$p_{\rm{T}}$ differential cross section of prompt D0 mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$. For $0<p_{\rm{T}}<1$ GeV/$c$ the cross section is obtained from the analysis without vertexing recostruction and for $p_{\rm{T}}>1$ GeV/c the analysis with vertexing reconstruction is used.

$p_{\rm{T}}$ differential cross section of prompt D0 mesons in pp collisions at $\mathbf{\sqrt{\textit s}~=~5.02~TeV}$ multiplied by A=208. For $0<p_{\rm{T}}<1$ GeV/$c$ the cross section is obtained from the analysis without vertexing recostruction and for $p_{\rm{T}}>1$ GeV/c the analysis with vertexing reconstruction is used.

$p_{\rm{T}}$ differential cross section of prompt D* mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$p_{\rm{T}}$ differential cross section of prompt D* mesons in pp collisions at $\mathbf{\sqrt{{\textit s}}~=~5.02~TeV}$ multiplied by A=208.

$p_{\rm{T}}$ differential cross section of prompt D+ mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$p_{\rm{T}}$ differential cross section of prompt D+ mesons in pp collisions at $\mathbf{\sqrt{{\textit s}}~=~5.02~TeV}$ multiplied by A=208.

$p_{\rm{T}}$ differential cross section of prompt Ds mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$p_{\rm{T}}$ differential cross section of prompt Ds mesons in pp collisions at $\mathbf{\sqrt{{\textit s}}~=~5.02~TeV}$ multiplied by A=208.

$R_{\rm{pPb}}$ of prompt D0 mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$R_{\rm{pPb}}$ of prompt D* mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$R_{\rm{pPb}}$ of prompt D+ mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$R_{\rm{pPb}}$ of prompt Ds mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$R_{\rm{pPb}}$ of prompt non-strange D mesons in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

$Q_{\rm pPb}$ of prompt D mesons in different centrality classes in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$

$Q_{\rm CP}$ of prompt D mesons in different centrality classes in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$

Ratio of prompt D+ over D0 production cross section as a function of transverse momentum in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$

Ratio of prompt D*+ over D0 production cross section as a function of transverse momentum in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$

Ratio of prompt Ds+ over D0 production cross section as a function of transverse momentum in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$

Ratio of prompt Ds+ over D+ production cross section as a function of transverse momentum in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$

Ratio of prompt Ds+ over D+ production cross section as a function of the charged particle pseudorapidity density in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

Ratio of prompt Ds+ over D+ production cross section as a function of the charged particle pseudorapidity density in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

Ratio of prompt Ds+ over D+ production cross section as a function of the charged particle pseudorapidity density in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

Ratio of prompt Ds+ over D+ production cross section as a function of the charged particle pseudorapidity density in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

Ratio of prompt Ds+ over D+ production cross section as a function of the charged particle pseudorapidity density in p-Pb collisions at $\mathbf{\sqrt{{\textit s}_{\rm NN}}~=~5.02~TeV}$.

Transverse momentum distributions of deuterons in the 40-60% V0A multiplicity class

Transverse momentum distributions of deuterons in the 60-100% V0A multiplicity class

Transverse momentum distributions of anti-deuterons in the 0-10% V0A multiplicity class

Transverse momentum distributions of anti-deuterons in the 10-20% V0A multiplicity class

Transverse momentum distributions of anti-deuterons in the 20-40% V0A multiplicity class

Transverse momentum distributions of anti-deuterons in the 40-60% V0A multiplicity class

Transverse momentum distributions of anti-deuterons in the 60-100% V0A multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in the 0-10% V0A multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in the 10-20% V0A multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in the 20-40% V0A multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in the 40-60% V0A multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in the 60-100% V0A multiplicity class

Transverse momentum distribution of $^{3}\overline{\mathrm{He}}$ for all non single diffractive (NSD) p-Pb collisions.

Transverse momentum distribution of $^{3}\mathrm{He}$ for all non single diffractive (NSD) p-Pb collisions.

Integrated yield of nuclei produced in NSD p-Pb collisions normalised by the spin degeneracy factor as a function of the mass number

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the 0-10% V0A multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the 10-20% V0A multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the 20-40% V0A multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the 40-60% V0A multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the 60-100% V0A multiplicity class

Mean transverse momentum of deuteron produced in p-Pb collisions as a function of the charged particle multiplicity density ad mid-rapidity

Deuteron over proton ratio in p-Pb collisions as a function of the charged particle multiplicity density ad mid-rapidity

$\overline{\mathrm{K}}$-p correlation function in p-p collisions at $\sqrt{s}=5$ TeV.

$\overline{\mathrm{K}}$-p correlation function in p-p collisions at $\sqrt{s}=7$ TeV.

$\overline{\mathrm{K}}$-p correlation function in p-p collisions at $\sqrt{s}=13$ TeV.

Combination of $\overline{\mathrm{K}}$-p correlation function in p-p collisions.

Exclusion plot for the $\Lambda$-$\Lambda$ scattering parameters (1$\sigma$ contour).

Exclusion plot for the $\Lambda$-$\Lambda$ scattering parameters (2$\sigma$ contour).

Exclusion plot for the $\Lambda$-$\Lambda$ scattering parameters (3$\sigma$ contour).

Exclusion plot for the $\Lambda$-$\Lambda$ binding energy (statistical uncertainty).

Exclusion plot for the $\Lambda$-$\Lambda$ binding energy (total uncertainty).

Transverse momentum spectra as a function of the event multiplicity for pp collisions at 5.02 TeV. Event multiplicity is estimated with the signal in the VZERO detector. Uncorrelated systematic uncertainties are the multiplicity dependent systematic uncertainties.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 0-100% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 0-10% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 10-20% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 20-30% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 30-40% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 40-50% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 50-60% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 60-70% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 70-80% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 80-90% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 90-100% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Spherocity intervals used in this analysis.

Average transverse momentum as a function of event multiplicity in pp collisions at 13 TeV. Results for the 90-100% spherocity class are presented. Spherocty-dependent uncertainties are indicated as uncorrelated.

Spherocity intervals used in this analysis.

Mean $p_{\rm T}$ of the inclusive J/$\psi$ spectrum at 5.02 TeV.

$p_{\rm T}$-differential production cross section of muons from heavy-flavour hadron decays in $3.7 < y < 4$.

$p_{\rm T}$-differential production cross section of muons from heavy-flavour hadron decays in $3.4 < y < 3.7$.

$p_{\rm T}$-differential production cross section of muons from heavy-flavour hadron decays in $3.1 < y < 3.4$.

$p_{\rm T}$-differential production cross section of muons from heavy-flavour hadron decays in $2.8 < y < 3.1$.

$p_{\rm T}$-differential production cross section of muons from heavy-flavour hadron decays in $2.5 < y < 2.8$.

Ratio of the $p_{\rm T}$-differential production cross section of muons from heavy-flavour hadron decays at forward rapidity in pp collisions at $\sqrt{s} = 7$ TeV to that at $\sqrt{s} = 5.02$ TeV.

Ratio of the $p_{\rm T}$-differential production cross section of muons from heavy-flavour hadron decays in $3.7 < y < 4$ to that in $2.5 < y < 2.8$ in pp collisions at $\sqrt{s}=5.02$ TeV.

Charged jet differential cross sections without UE subtraction in pp collisions at $\sqrt{s}$ = 5.02 TeV with the leading track bias. All jets must contain at least one track with $p_{T}$ > 5 GeV/$c$. Statistical uncertainties are displayed as vertical error bars. The total systematic uncertainties are shown as shaded bands around the data points. Data are scaled to enhance visibility

$z_{||}^{\rm ch}$-differential cross section of D$^0$-meson tagged track-based jets in pp collisions at $\sqrt{s}$ = 7 TeV, with $p_{\rm T,D}$ > 6 GeV/$c$ and 15 < $p_{\rm T,jet}^{\rm ch}$ < 30 GeV/$c$.

Rate of D$^0$-meson tagged track-based jets as a function of the jet momentum fraction carried by the D$^0$ mesons in the direction of the jet axisin pp collisions at $\sqrt{s}$ = 7 TeV, with $p_{\rm T,D}$ > 2 GeV/$c$ and 5 < $p_{\rm T,jet}^{\rm ch}$ < 15 GeV/$c$.

Rate of D$^0$-meson tagged track-based jets as a function of the jet momentum fraction carried by the D$^0$ mesons in the direction of the jet axisin pp collisions at $\sqrt{s}$ = 7 TeV, with $p_{\rm T,D}$ > 6 GeV/$c$ and 15 < $p_{\rm T,jet}^{\rm ch}$ < 30 GeV/$c$.

Correlation function as a function of pair relative momentum for 20-40% multiplicity class and pair transverse momentum range (0.5-1.0) GeV/c.

Correlation function as a function of pair relative momentum for 40-90% multiplicity class and pair transverse momentum range (0.2-0.5) GeV/c.

Correlation function as a function of pair relative momentum for 40-90% multiplicity class and pair transverse momentum range (0.5-1.0) GeV/c.

Femtoscopic radii as a function of the pair transverse momentum.

Correlation strengths as a function of the pair transverse momentum.

$v_2\{4\}$ with 3-subevent method in pp collisions at $\sqrt{s} = 13$ TeV.

$v_2\{6\}$ in pp collisions at $\sqrt{s} = 13$ TeV.

SC$(4,2)$ with 3-subevent method in pp collisions at $\sqrt{s} = 13$ TeV.

SC$(3,2)$ with 3-subevent method in pp collisions at $\sqrt{s} = 13$ TeV.

SC$(4,2)$ with 3-subevent method divided with $\langle v_4\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in pp collisions at $\sqrt{s} = 13$ TeV.

SC$(3,2)$ with 3-subevent method divided with $\langle v_3\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in pp collisions at $\sqrt{s} = 13$ TeV.

$v_2\{2\}$ with $|\Delta \eta| > 1.4$ in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_3\{2\}$ with $|\Delta \eta| > 1.0$ in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_4\{2\}$ with $|\Delta \eta| > 1.0$ in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{4\}$ in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{4\}$ with 3-subevent method in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{6\}$ in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(4,2)$ with 3-subevent method in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(3,2)$ with 3-subevent method in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(4,2)$ with 3-subevent method divided with $\langle v_4\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(3,2)$ with 3-subevent method divided with $\langle v_3\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in p-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{2\}$ with $|\Delta \eta| > 1.4$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

$v_3\{2\}$ with $|\Delta \eta| > 1.0$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

$v_4\{2\}$ with $|\Delta \eta| > 1.0$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

$v_2\{4\}$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

$v_2\{4\}$ with 3-subevent method in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

$v_2\{6\}$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

$v_2\{8\}$ in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

SC$(4,2)$ with 3-subevent method in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

SC$(3,2)$ with 3-subevent method in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

SC$(4,2)$ with 3-subevent method divided with $\langle v_4\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

SC$(3,2)$ with 3-subevent method divided with $\langle v_3\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in Xe-Xe collisions at $\sqrt{s_{NN}} = 5.44$ TeV.

$v_2\{2\}$ with $|\Delta \eta| > 1.4$ in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_3\{2\}$ with $|\Delta \eta| > 1.0$ in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_4\{2\}$ with $|\Delta \eta| > 1.0$ in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{4\}$ in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{4\}$ with 3-subevent method in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{6\}$ in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{6\}$ with 2-subevent method in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{8\}$ in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

$v_2\{8\}$ with 2-subevent method in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(4,2)$ with 3-subevent method in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(3,2)$ with 3-subevent method in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(4,2)$ with 3-subevent method divided with $\langle v_4\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

SC$(3,2)$ with 3-subevent method divided with $\langle v_3\{2\}^2\rangle\langle v_2\{2\}^2\rangle$ with $|\Delta \eta| > 1.0$ and 1.4 in Pb-Pb collisions at $\sqrt{s_{NN}} = 5.02$ TeV.

Transverse-momentum spectra of deuterons and anti-deuterons measured at mid-rapidity in V0M multiplicity class VI+VII

Transverse-momentum spectra of deuterons and anti-deuterons measured at mid-rapidity in V0M multiplicity class VIII+IX+X

Coalescence parameter $B_2$ of (anti-)deuterons vs. the transverse momentum per nucleon in V0M multiplicity class I+II

Coalescence parameter $B_2$ of (anti-)deuterons vs. the transverse momentum per nucleon in V0M multiplicity class III

Coalescence parameter $B_2$ of (anti-)deuterons vs. the transverse momentum per nucleon in V0M multiplicity class IV+V

Coalescence parameter $B_2$ of (anti-)deuterons vs. the transverse momentum per nucleon in V0M multiplicity class VI+VII

Coalescence parameter $B_2$ of (anti-)deuterons vs. the transverse momentum per nucleon in V0M multiplicity class VIII+IX+X

Mean transverse momentum ($\langle p_T \rangle$) of (anti-)deuterons as a function of charged-particle multiplicity at mid-rapidity ($\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$)

Ratio between the $p_T$-integrated yield of deuterons and protons (d/p) as a function of charged-particle multiplicity at mid-rapidity ($\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$)

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Opposite-sign pion pair correlation functions in PYTHIA simulations for sphericity S_{T} > 0.7 (spherical events).

Same-sign pion pair correlation functions in data for sphericity S_{T} < 0.3 (jet-like events).

Same-sign pion pair correlation functions for simulated events with sphericity S_{T} < 0.3 (jet-like events).

Same-sign pion pair correlation functions in data for sphericity S_{T} > 0.7 (spherical events).

Same-sign pion pair correlation functions for simulated events with sphericity S_{T} > 0.7 (spherical events).

Comparison of exponential and Gaussian fit results for $C^{QS}(q)$ functions in events with sphericity S_{T} < 0.3 (jet-like events).

Comparison of exponential and Gaussian fit results for $C^{QS}(q)$ functions in events with sphericity S_{T} > 0.7 (spherical events).

Measured 1D source radii as a function of pair k_{T} for spherical events with $<dN_{\textrm{ch}}/d\eta> = 5.3 \pm 2.2$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Measured 1D source radii as a function of pair k_{T} for spherical events with $<dN_{\textrm{ch}}/d\eta> = 10.5 \pm 2.10$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Measured 1D source radii as a function of pair k_{T} for spherical events with $<dN_{\textrm{ch}}/d\eta> = 14.9 \pm 2.3$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Measured 1D source radii as a function of pair k_{T} for spherical events with $<dN_{\textrm{ch}}/d\eta> = 20.4 \pm 3.2$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Measured 1D source radii as a function of pair k_{T} for jet-like events with $<dN_{\textrm{ch}}/d\eta> = 4.3 \pm 2.0$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Measured 1D source radii as a function of pair k_{T} for jet-like events with $<dN_{\textrm{ch}}/d\eta> = 9.6 \pm 2.0$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Measured 1D source radii as a function of pair k_{T} for jet-like events with $<dN_{\textrm{ch}}/d\eta> = 13.9 \pm 2.2$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Measured 1D source radii as a function of pair k_{T} for jet-like events with $<dN_{\textrm{ch}}/d\eta> = 18.7 \pm 3.2$ in pp collisions at $\sqrt{{\textit s}}=7$ TeV.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and CL1 estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 0-5% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and V0A estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 0-5% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 5-10% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 10-20% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 20-40% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 40-60% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 60-80% centrality class and ZNA estimator.

Pseudorapidity density of charged particles in p–Pb NSD collisions at 8.16 TeV for 80-100% centrality class and ZNA estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for CL1 estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for V0A estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for ZNAmult estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions as a function of the number of participants for ZNAPb estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions for 5 participant quarks as a function of the number of participants for CL1 estimator.

Average pseudorapidity density of charged particles in p–Pb NSD collisions for 5 participant quarks as a function of the number of participants for V0A estimator.

The J/$\psi$ $v_3$ coefficient as a function of $p_{\rm T}$ in 0-10% centrality interval in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

The J/$\psi$ $v_3$ coefficient as a function of $p_{\rm T}$ in 10-30% centrality interval in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

The J/$\psi$ $v_3$ coefficient as a function of $p_{\rm T}$ in 30-50% centrality interval in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

The J/$\psi$ $v_3$ coefficient as a function of $p_{\rm T}$ in 0-50% centrality interval in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

The J/$\psi$ $v_3/v_2$ ratio as a function of $p_{\rm T}$ in 5-40% centrality interval in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

The J/$\psi$ $v_3/v_2$ ratio as a function of $p_{\rm T}$ in 10-50% centrality interval in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

The J/$\psi$ $v_2$ as a function of $p_{\rm T}$ for unbiased events (no event-shape selection) in the 5-40% centrality interval in Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV.

The J/$\psi$ $v_2$ as a function of $p_{\rm T}$ for lowest $q_2^{\rm V0A}$ event-shape class in the 5-40% centrality interval in Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV. The systematic uncertainties are the same as the ones given in Table 10 for the unbiased event sample.

The J/$\psi$ $v_2$ as a function of $p_{\rm T}$ for highest $q_2^{\rm V0A}$ event-shape class in the 5-40% centrality interval in Pb--Pb collisions at $\sqrt{s_{\rm NN}}$ = 5.02 TeV. The systematic uncertainties are the same as the ones given in Table 10 for the unbiased event sample.