$p_T$-distributions of kaons ($K^{+}+K^{-}$) measured in pp collisions at $\sqrt{s}$ = 5.02 TeV.

$p_T$-distributions of protons ($p+pbar$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

$p_T$-distributions of protons ($p+pbar$) measured in pp collisions at $\sqrt{s}$ = 5.02 TeV.

$p_T$-distributions of kaons ($K^{+}+K^{-}$)/pions (${\pi }^{+}+{\pi }^{-}$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

$p_T$-distributions of kaons ($K^{+}+K^{-}$)/pions (${\pi }^{+}+{\pi }^{-}$) measured in pp collisions at $\sqrt{s}$ = 5.02 TeV.

$p_T$-distributions of protons ($p+pbar$)/pions (${\pi }^{+}+{\pi }^{-}$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

$p_T$-distributions of protons ($p+pbar$)/pions (${\pi }^{+}+{\pi }^{-}$) measured in pp collisions at $\sqrt{s}$ = 5.02 TeV.

Integrated yield ratios of kaons ($K^{+}+K^{-}$) to pions (${\pi }^{+}+{\pi }^{-}$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Integrated yield ratios of kaons ($K^{+}+K^{-}$) to pions (${\pi }^{+}+{\pi }^{-}$) measured in pp collisions at $\sqrt{s}$ = 5.02 TeV.

Integrated yield ratios of protons ($p+pbar$) to pions (${\pi }^{+}+{\pi }^{-}$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

Integrated yield ratios of protons ($p+pbar$) to pions (${\pi }^{+}+{\pi }^{-}$) measured in pp collisions at $\sqrt{s}$ = 5.02 TeV.

$p_T$-dependent nuclear modification factor of pions (${\pi }^{+}+{\pi }^{-}$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

$p_T$-dependent nuclear modification factor of kaons ($K^{+}+K^{-}$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

$p_T$-dependent nuclear modification factor of protons ($p+pbar$) measured in Pb-Pb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV.

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.

The spectral shape is characterized by the exponent of the power-law function which fits the high-pTpart (pT>6 GeV/c) of the invariant yields. The power-law exponent is presented for different V0M multiplicity classes.

The spectral shape is characterized by the exponent of the power-law function which fits the high-pTpart (pT>6 GeV/c) of the invariant yields. The power-law exponent is presented for different event classes based on the number of SPD tracklets.

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.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Ratio of transverse momentum spectra in Xe-Xe and Pb-Pb.

Raa vs $⟨dNch/d\eta ⟩$.

Raa vs $⟨dNch/d\eta ⟩$.

Raa vs $⟨dNch/d\eta ⟩$.

Average transverse momentum vs centrality percentage for PbPb and XeXe. And the ratio between collision systems.

Transverse momentum spectra of charged particles in pp collisions.

Ratio Data/MC

Additional systematic error for pp data: +3.0 pct -3.0 pct Additional systematic error for PBPB 0-5 pct data: +0.08 pct -0.08 pct Additional systematic error for PBPB 5-10 pct data: +0.24 pct -0.24 pct Additional systematic error for PBPB 10-20 pct data: +0.46 pct -0.46 pct Additional systematic error for PBPB 20-30 pct data: +0.81 pct -0.81 pct Additional systematic error for PBPB 30-40 pct data: +1.26 pct -1.26 pct Additional systematic error for PBPB 40-50 pct data: +1.86 pct -1.86 pct Additional systematic error for PBPB 50-60 pct data: +2.64 pct -2.64 pct Additional systematic error for PBPB 60-70 pct data: +3.67 pct -3.67 pct Additional systematic error for PBPB 70-80 pct data: +5.01 pct -5.01 pct.

Additional systematic error for PBPB 0-5 pct data: +2.2 pct -2.2 pct Additional systematic error for PBPB 5-10 pct data: +2.2 pct -2.2 pct Additional systematic error for PBPB 10-20 pct data: +2.4 pct -2.4 pct Additional systematic error for PBPB 20-30 pct data: +2.7 pct -2.7 pct Additional systematic error for PBPB 30-40 pct data: +3.4 pct -3.4 pct Additional systematic error for PBPB 40-50 pct data: +3.7 pct -3.7 pct Additional systematic error for PBPB 50-60 pct data: +4.9 pct -4.9 pct Additional systematic error for PBPB 60-70 pct data: +6.7 pct -6.7 pct Additional systematic error for PBPB 70-80 pct data: +7.1 pct -7.1 pct.

Additional systematic error for PBPB 0-5 pct data: +2.7 pct -2.7 pct Additional systematic error for PBPB 5-10 pct data: +3.5 pct -3.5 pct Additional systematic error for PBPB 10-20 pct data: +3.5 pct -3.5 pct Additional systematic error for PBPB 20-30 pct data: +4.1 pct -4.1 pct Additional systematic error for PBPB 30-40 pct data: +3.7 pct -3.7 pct Additional systematic error for PBPB 40-50 pct data: +3.9 pct -3.9 pct Additional systematic error for PBPB 50-60 pct data: +3.6 pct -3.6 pct Additional systematic error for PBPB 60-70 pct data: +4.6 pct -4.6 pct Additional systematic error for PBPB 70-80 pct data: +5.9 pct -5.9 pct.

Additional systematic error for P-PB NSD data: +4.6 pct -4.6 pct.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for NSD collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for NSD collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for NSD collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for NSD collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL>0 collisions at a centre-of-mass energy of 900 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Multiplicity distribution in the pseudorapidity region -2.0 to 2.0 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -2.4 to 2.4 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.0 to 3.0 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 3.4 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Multiplicity distribution in the pseudorapidity region -3.4 to 5.0 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in NSD collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in NSD collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in NSD collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL>0 collisions at center-of-mass energy 900 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL>0 collisions at center-of-mass energy 7000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.0 to 2.0 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -2.4 to 2.4 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.0 to 3.0 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 3.4 in INEL>0 collisions at center-of-mass energy 8000 GeV.

Set of fit parameters for the multiplicity distribution in pseudorapidity range -3.4 to 5.0 in INEL>0 collisions at center-of-mass energy 8000 GeV.

$K_S^0$ transverse momentum spectrum: V0M Class IV (pp at $\sqrt{s}=7$ TeV).

$K_S^0$ transverse momentum spectrum: V0M Class V (pp at $\sqrt{s}=7$ TeV).

$K_S^0$ transverse momentum spectrum: V0M Class VI (pp at $\sqrt{s}=7$ TeV).

$K_S^0$ transverse momentum spectrum: V0M Class VII (pp at $\sqrt{s}=7$ TeV).

$K_S^0$ transverse momentum spectrum: V0M Class VIII (pp at $\sqrt{s}=7$ TeV).

$K_S^0$ transverse momentum spectrum: V0M Class IX (pp at $\sqrt{s}=7$ TeV).

$K_S^0$ transverse momentum spectrum: V0M Class X (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class I (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class II (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class III (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class IV (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class V (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class VI (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class VII (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class VIII (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class IX (pp at $\sqrt{s}=7$ TeV).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ transverse momentum spectrum: V0M Class X (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class I (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class II (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class III (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class IV (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class V (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class VI (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class VII (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class VIII (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class IX (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ transverse momentum spectrum: V0M Class X (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+}$ transverse momentum spectrum: V0M Class I+II (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+}$ transverse momentum spectrum: V0M Class III+IV (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+}$ transverse momentum spectrum: V0M Class V+VI (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+}$ transverse momentum spectrum: V0M Class VII+VIII (pp at $\sqrt{s}=7$ TeV).

${\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+}$ transverse momentum spectrum: V0M Class IX+X (pp at $\sqrt{s}=7$ TeV).

$2K_S^0/({\pi }^{+}+{\pi }^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

$(\mathrm{\Lambda }+\overline{\mathrm{\Lambda }})/({\pi }^{+}+{\pi }^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

$({\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+})/({\pi }^{+}+{\pi }^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

$({\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+})/({\pi }^{+}+{\pi }^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of the average charged particle multiplicity density at midrapidity.

${\pi }^{+}+{\pi }^{-}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$p+\overline{p}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$K_S^0$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$\mathrm{\Lambda }+\overline{\mathrm{\Lambda }}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

${\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

${\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+}$ integrated yields, pp at $\sqrt{s}=7$ TeV (V0M Multiplicity Classes).

$(\mathrm{\Lambda }+\overline{\mathrm{\Lambda }})/2K_S^0$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of charged particle multiplicity density at midrapidity.

$(p+\overline{p})/({\pi }^{+}+{\pi }^{-})$ ratio for pp collisions at $\sqrt{s}=7$ TeV as a function of charged particle multiplicity density at midrapidity.

$(2K_S^0)/({\pi }^{+}+{\pi }^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

$(\mathrm{\Lambda }+\overline{\mathrm{\Lambda }})/({\pi }^{+}+{\pi }^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

$({\mathrm{\Xi }}^{-}+{\overline{\mathrm{\Xi }}}^{+})/({\pi }^{+}+{\pi }^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

$({\mathrm{\Omega }}^{-}+{\overline{\mathrm{\Omega }}}^{+})/({\pi }^{+}+{\pi }^{-})$ double-ratio vs multiplicity for pp collisions at $\sqrt{s}=7$ TeV.

Event multiplicity classes, their corresponding fraction of the INEL>0 cross-section and their corresponding average charged particle density at midrapidity ($|\eta |<0.5$). The value of in the inclusive (INEL>0) class is 5.96 $\pm$ 0.23. The uncertainties are the quadratic sum of statistical and systematic contributions.

Ratios of transverse-momentum distributions of charged particles in three intervals of multiplicities to the respective one for inclusive (INEL>0) collisions. The spectra were normalised by the integral prior to division.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 2760 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 7000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL collisions at a centre-of-mass energy of 8000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for NSD collisions at a centre-of-mass energy of 8000 GeV.

Measured pseudorapidity dependence of $dN/d\eta$ for INEL>0 collisions at a centre-of-mass energy of 8000 GeV.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for INEL collisions.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for NSD collisions.

Charged particle pseudorapidiy densities in the pseudorapidity region -0.5 to 0.5 for INEL>0 collisions.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for INEL collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -0.5 to 0.5 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1.5 to 1.5 for NSD collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 900 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 2760 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 7000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Multiplicity distribution in the pseudorapidity region -1 to 1 for INEL>0 collisions at a centre-of-mass energy of 8000 GeV. Note that the uncertainties are strongly correlated between neighbouring points. See the paper text for details.

Mean charged particle multiplicities in 3 pseudorapidity intervals in P P NSD collisions from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -0.5 to 0.5 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -1.0 to 1.0 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Mean CQ moments of the multiplicity distributions for the pseudorapidity range -1.5 to 1.5 in P P NSD collisions at centre-of-mass energies from 900 to 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 900 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 2760 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 7000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-0.5 to 0.5 in P P NSD collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P NSD collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1 to 1 in P P INEL>0 collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P INEL collisions at center-of-mass energy 8000 GeV.

Individual sets of fit parameters for the multiplicity distribution in pseudorapidity range-1.5 to 1.5 in P P NSD collisions at center-of-mass energy 8000 GeV.

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-$\phi$ windows of the width $\delta \eta =0.2$, $\delta \phi =\pi /4$, measured in $p_{\mathrm{T}}$ range $0.3-1.5$ (GeV/c).

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-$\phi$ windows of the width $\delta \eta =0.2$, $\delta \phi =\pi /4$, measured in $p_{\mathrm{T}}$ range $0.3-1.5$ (GeV/c).

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-windows of the width $\delta \eta =0.2$, measured in several $p_{\mathrm{T}}$ ranges.

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-windows of the width $\delta \eta =0.2$, measured in $p_{\mathrm{T}}$ range $0.30-0.40$ (GeV/c).

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-windows of the width $\delta \eta =0.2$, measured in $p_{\mathrm{T}}$ range $0.40-0.52$ (GeV/c).

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-windows of the width $\delta \eta =0.2$, measured in $p_{\mathrm{T}}$ range $0.52-0.70$ (GeV/c).

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-windows of the width $\delta \eta =0.2$, measured in $p_{\mathrm{T}}$ range $0.70-1.03$ (GeV/c).

Correlation strength $b_{\mathrm{c}\mathrm{o}\mathrm{r}\mathrm{r}}$ for $\eta$-windows of the width $\delta \eta =0.2$, measured in $p_{\mathrm{T}}$ range $1.03-6.00$ (GeV/c).