Transverse momentum spectra of charged particles in V0M IV multiplicity class

Transverse momentum spectra of charged particles in V0M V multiplicity class

Transverse momentum spectra of charged particles in V0M VI multiplicity class

Transverse momentum spectra of charged particles in V0M VII multiplicity class

Transverse momentum spectra of charged particles in V0M VIII multiplicity class

Transverse momentum spectra of charged particles in V0M IX multiplicity class

Transverse momentum spectra of charged particles in V0M X multiplicity class

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class I

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class II

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class III

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class IV

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class V

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class VI

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class VII

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class VIII

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class IX

Transverse momentum spectra of $\pi^{+} + \pi^{-}$ in V0M multiplicity class X

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class I

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class II

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class III

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class IV

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class V

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class VI

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class VII

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class VIII

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class IX

Transverse momentum spectra of $K^{+} + K^{-}$ in V0M multiplicity class X

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class I

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class II

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class III

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class IV

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class V

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class VI

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class VII

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class VIII

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class IX

Transverse momentum spectra of $p + \bar{p}$ in V0M multiplicity class X

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class I

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class II

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class III

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class IV + V

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class VI

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class VII

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class VIII

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class IX

Transverse momentum spectra of $K* + \bar{K}*$ in V0M multiplicity class X

Transverse momentum spectra of $\phi$ in V0M multiplicity class I

Transverse momentum spectra of $\phi$ in V0M multiplicity class II

Transverse momentum spectra of $\phi$ in V0M multiplicity class III

Transverse momentum spectra of $\phi$ in V0M multiplicity class IV + V

Transverse momentum spectra of $\phi$ in V0M multiplicity class VI

Transverse momentum spectra of $\phi$ in V0M multiplicity class VII

Transverse momentum spectra of $\phi$ in V0M multiplicity class VIII

Transverse momentum spectra of $\phi$ in V0M multiplicity class IX

Transverse momentum spectra of $\phi$ in V0M multiplicity class X

Unidentified particle spectral modification in V0M Class IX pp collisions.

$\pi^{+}+\pi^{-}$ spectral modification in V0M Class IX pp collisions.

$K^{+}+K^{-}$ spectral modification in V0M Class IX pp collisions.

$p+\bar{p}$ spectral modification in V0M Class IX pp collisions.

$\Lambda + \bar{\Lambda}$ spectral modification in V0M Class IX pp collisions.

$\Xi^{-} + \bar{\Xi}^{+}$ spectral modification in V0M Class IX pp collisions.

$K* + \bar{K}*$ spectral modification in V0M Class IX pp collisions.

$\phi$ spectral modification in V0M Class IX pp collisions.

Unidentified particle spectral modification in V0M Class I pp collisions.

$\pi^{+}+\pi^{-}$ spectral modification in V0M Class I pp collisions.

$K^{+}+K^{-}$ spectral modification in V0M Class I pp collisions.

$p+\bar{p}$ spectral modification in V0M Class I pp collisions.

$\Lambda + \bar{\Lambda}$ spectral modification in V0M Class I pp collisions.

$\Xi^{-} + \bar{\Xi}^{+}$ spectral modification in V0M Class I pp collisions.

$K* + \bar{K}*$ spectral modification in V0M Class I pp collisions.

$\phi$ spectral modification in V0M Class I pp collisions.

Transverse momentum dependence of $(p + \bar{p})/\phi$ yield ratios in low multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $(K^{+} + K^{-})/(\pi^{+} + \pi^{-})$ yield ratios in low multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $(p + \bar{p})/(\pi^{+} + \pi^{-})$ yield ratios in low multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $\Lambda/K^{0}_{s}$ yield ratios in low multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $(p + \bar{p})/\phi$ yield ratios in high multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $(K^{+} + K^{-})/(\pi^{+} + \pi^{-})$ yield ratios in high multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $(p + \bar{p})/(\pi^{+} + \pi^{-})$ yield ratios in high multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $\Lambda/K^{0}_{s}$ yield ratios in high multiplicity pp collisions at $\sqrt{s} = 7$ (TeV).

Transverse momentum dependence of $(p + \bar{p})/\phi$ ratio in low-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(K^{+} + K^{-})/(\pi^{+} + \pi^{-})$ ratio in low-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(p + \bar{p})/(\pi^{+} + \pi^{-})$ ratio in low-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $\Lambda/K^{0}_{s}$ ratio in low-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(p + \bar{p})/\phi$ ratio in mid-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(K^{+} + K^{-})/(\pi^{+} + \pi^{-})$ ratio in mid-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(p + \bar{p})/(\pi^{+} + \pi^{-})$ ratio in mid-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $\Lambda/K^{0}_{s}$ ratio in mid-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(p + \bar{p})/\phi$ ratio in high-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(K^{+} + K^{-})/(\pi^{+} + \pi^{-})$ ratio in high-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $(p + \bar{p})/(\pi^{+} + \pi^{-})$ ratio in high-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Transverse momentum dependence of $\Lambda/K^{0}_{s}$ ratio in high-$p_{T}$ interval in pp collisions as a function of $\langle dN_{ch}/d\eta \rangle_{|\eta|<0.5}$.

Integrated $(K^{+} + K^{-})$/$(\pi^{+} + \pi^{-})$ ratios as a function of $\langle dN_{ch}/d\eta\rangle$ in pp collisions at $\sqrt{s} = 7$ TeV.

Integrated $(K^{*} + \bar{K}^{*})$/$(\pi^{+} + \pi^{-})$ ratios as a function of $\langle dN_{ch}/d\eta\rangle$ in pp collisions at $\sqrt{s} = 7$ TeV.

Integrated $\phi$/$(\pi^{+} + \pi^{-})$ ratios as a function of $\langle dN_{ch}/d\eta\rangle$ in pp collisions at $\sqrt{s} = 7$ TeV.

$\langle\beta_{T}\rangle$ from blast-wave fit to PbPb collisions at $\sqrt{s}$ = 2.76 TeV

$T_{kin}$ from blast-wave fit to PbPb collisions at $\sqrt{s}$ = 2.76 TeV

$n$ from blast-wave fit to PbPb collisions at $\sqrt{s}$ = 2.76 TeV

$\langle\beta_{T}\rangle$ from blast-wave fit to pPb collisions at $\sqrt{s}$ = 5.02 TeV

$T_{kin}$ from blast-wave fit to pPb collisions at $\sqrt{s}$ = 5.02 TeV

$n$ from blast-wave fit to pPb collisions at $\sqrt{s}$ = 5.02 TeV

$\langle\beta_{T}\rangle$ from blast-wave fit to pp collisions at $\sqrt{s}$ = 7 TeV

$T_{kin}$ from blast-wave fit to pp collisions at $\sqrt{s}$ = 7 TeV

$n$ from blast-wave fit to pp collisions at $\sqrt{s}$ = 7 TeV

Observed (solid line) and expected (dashed line) 95\% CL limits on the product of the production cross section times the branching ratio of a narrow width spin-0 resonance $X$ produced via gluon-gluon initial states decaying to a $Z$ boson and a photon, $\sigma(pp\to X)\cdot\mathcal{B}(X\to Z\gamma)$, as a function of the resonance mass $m_{X}$. Observed (expected) results are derived from ensemble tests for $m_{X}>1850 (900)$~\GeV. The green and yellow solid bands correspond to the $\pm1\sigma$ and $\pm2\sigma$ intervals for the expected upper limits. The limits in the $m_{X}$ ranges from 220 GeV to 3400 GeV and are obtained from the combined $ee\gamma$ and $\mu\mu\gamma$ channels.

Observed (solid line) and expected (dashed line) 95\% CL limits on the product of the production cross section times the branching ratio of a narrow width spin-2 resonance $X$ produced via gluon-gluon initial states decaying to a $Z$ boson and a photon, $\sigma(pp\to X)\cdot\mathcal{B}(X\to Z\gamma)$, as a function of the resonance mass $m_{X}$. Observed (expected) results are derived from ensemble tests for $m_{X}>1850 (900)$~\GeV. The green and yellow solid bands correspond to the $\pm1\sigma$ and $\pm2\sigma$ intervals for the expected upper limit respectively. The limits in the $m_{X}$ ranges from 220 GeV to 3400 GeV and are obtained from the combined $ee\gamma$ and $\mu\mu\gamma$ channels..

Observed (solid line) and expected (dashed line) 95\% CL limits on the product of the production cross section times the branching ratio of a narrow width spin-2 resonance $X$ produced via $q\bar{q}$ initial states decaying to a $Z$ boson and a photon, $\sigma(pp\to X)\cdot\mathcal{B}(X\to Z\gamma)$, as a function of the resonance mass $m_{X}$. Observed (expected) results are derived from ensemble tests for $m_{X}>1850 (900)$~\GeV. The green and yellow solid bands correspond to the $\pm1\sigma$ and $\pm2\sigma$ intervals for the expected upper limit respectively. The limits in the $m_{X}$ ranges from 220 GeV to 3400 GeV and are obtained from the combined $ee\gamma$ and $\mu\mu\gamma$ channels.

The inelastic cross section differential in the forward rapidity gap size, DELTA(C=RAPGAP) for a maximum observed particle transverse momentum of 800 MeV in the gap.

The inelastic cross section excluding diffractive processes with xi_X < xi_cut, obtained by integration of the differential cross section from gap sizes zero to a variable maximum. Here xi_X is the variable (M_X)**2/S and for SD data DELTA(C=RAPGAP)~=-ln(xi_X). The errors shown are the total errors excluding the 3.4% luminosity uncertainty.

The symmetric cumulant $sc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The symmetric cumulant $sc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The symmetric cumulant $sc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The symmetric cumulant $sc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The symmetric cumulant $sc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The symmetric cumulant $sc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The symmetric cumulant $sc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The symmetric cumulant $sc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The symmetric cumulant $sc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The asymmetric cumulant $ac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The asymmetric cumulant $ac_{2}\{3\}$results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The asymmetric cumulant $ac_{2}\{3\}$results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The asymmetric cumulant $ac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The asymmetric cumulant $ac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The asymmetric cumulant $ac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The normalized symmetric cumulant $nsc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The normalized symmetric cumulant $nsc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The normalized asymmetric cumulant $nac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The normalized symmetric cumulant $nsc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The normalized symmetric cumulant $nsc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The normalized asymmetric cumulant $nac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 13 TeV

The normalized symmetric cumulant $nsc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The normalized symmetric cumulant $nsc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The normalized asymmetric cumulant $nac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The normalized symmetric cumulant $nsc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The normalized symmetric cumulant $nsc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The normalized asymmetric cumulant $nac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The normalized symmetric cumulant $nsc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The normalized symmetric cumulant $nsc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The normalized asymmetric cumulant $nac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The normalized symmetric cumulant $nsc_{2\,3}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The normalized symmetric cumulant $nsc_{2\,4}\{4\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The normalized asymmetric cumulant $nac_{2}\{3\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The $v_{2}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The $v_{3}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The $v_{4}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The $v_{2}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The $v_{3}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The $v_{4}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The $v_{2}\{2\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The $v_{3}\{2\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The $v_{4}\{2\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The $v_{2}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The $v_{3}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The $v_{4}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pp collisions at $\sqrt{s_{NN}}$ = 13 TeV

The $v_{2}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The $v_{3}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The $v_{4}\{2\}$ results as a function of multiplicity ($N_{ch}$) in pPb collisions at $\sqrt{s_{NN}}$ = 5.02 TeV

The $v_{2}\{2\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The $v_{3}\{2\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The $v_{4}\{2\}$ results as a function of multiplicity ($N_{ch}$) in PbPb collisions at $\sqrt{s_{NN}}$ = 2.76 TeV

The symmetric cumulant $ac_{2}\{3\}$ in Pb+Pb from different methods

The symmetric cumulant $ac_{2}\{3\}$ in Pb+Pb from different methods

The symmetric cumulant $ac_{2}\{3\}$ in p+Pb from different methods

The symmetric cumulant $ac_{2}\{3\}$ in p+Pb from different methods

The symmetric cumulant $ac_{2}\{3\}$ in pp from different methods

The symmetric cumulant $ac_{2}\{3\}$ in pp from different methods

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with sigma_inel(3Hebar)x1.5.

Raw primary antihelium3-to-helium3 ratio as a function of the momentum p_primary.

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with default sigma_inel(3Hebar).

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with sigma_inel(3Hebar)x0.5.

Raw primary antihelium3-to-helium3 ratio from Geant4-based MC simulations as a function of the momentum p_primary with sigma_inel(3Hebar)x1.5.

Inelastic interaction cross section of antihelium-3 on an averaged material element of the ALICE detector (ITS+TPC analysis).

Inelastic interaction cross section of antihelium-3 on an averaged material element of the ALICE detector (ITS+TPC+TOF analysis).

Inelastic interaction cross section of antihelium-3 on an averaged material element of the ALICE detector (ITS+TPC+TOF analysis).

Transparency of the galaxy to antihelium-3 nuclei from background before the solar modulation

Transparency of the galaxy to antihelium-3 nuclei from dark matter before the solar modulation

Transparency of the galaxy to antihelium-3 nuclei from background after the solar modulation

Transparency of the galaxy to antihelium-3 nuclei from dark matter after the solar modulation

Inelastic interaction cross section of antihelium-3 on proton from the fit to the ALICE data.

Inelastic interaction cross section of antihelium-3 on helium-4 from the fit to the ALICE data.

The derived hadronic total and inelastic cross sections. The quoted systematic (sys) errors are from the uncertainty in the T dependence, normalization, luminosity and rho (the ratio of the real/imaginary parts of the hadronic scattering amplitude at T=0), respectively. The statistical errors are shown as zero:.

$\Delta N_p$ multiplicity distributions in Au+Au collisions at $\sqrt{S_{NN}}=27$ GeV for 0-5 percent, 30-40 percent and 70-80 percent collision centralities at midrapidity.

$\Delta N_p$ multiplicity distributions in Au+Au collisions at $\sqrt{S_{NN}}=39$ GeV for 0-5 percent, 30-40 percent and 70-80 percent collision centralities at midrapidity.

$\Delta N_p$ multiplicity distributions in Au+Au collisions at $\sqrt{S_{NN}}=62.4$ GeV for 0-5 percent, 30-40 percent and 70-80 percent collision centralities at midrapidity.

$\Delta N_p$ multiplicity distributions in Au+Au collisions at $\sqrt{S_{NN}}=200$ GeV for 0-5 percent, 30-40 percent and 70-80 percent collision centralities at midrapidity.

Centrality dependence of the cumulants of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{S_{NN}}=7.7$ GeV.

Centrality dependence of the cumulants of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{S_{NN}}=11.5$ GeV.

Centrality dependence of the cumulants of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{S_{NN}}=19.6$ GeV.

Centrality dependence of the cumulants of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{S_{NN}}=27$ GeV.

Centrality dependence of the cumulants of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{S_{NN}}=39$ GeV.

Centrality dependence of the cumulants of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{S_{NN}}=62.4$ GeV.

Centrality dependence of the cumulants of $\Delta N_p$ distributions for Au+Au collisions at $\sqrt{S_{NN}}=200$ GeV.

Centrality dependence of $S\sigma$/Skellam and $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{S_{NN}}=7.7$ GeV.

Centrality dependence of $S\sigma$/Skellam and $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{S_{NN}}=11.5$ GeV.

Centrality dependence of $S\sigma$/Skellam and $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{S_{NN}}=19.6$ GeV.

Centrality dependence of $S\sigma$/Skellam and $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{S_{NN}}=27$ GeV.

Centrality dependence of $S\sigma$/Skellam and $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{S_{NN}}=39$ GeV.

Centrality dependence of $S\sigma$/Skellam and $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{S_{NN}}=62.4$ GeV.

Centrality dependence of $S\sigma$/Skellam and $\kappa\sigma^2$ for $\Delta N_p$ in Au+Au collisions at $\sqrt{S_{NN}}=200$ GeV.

Cumulants of net-proton distribution at $\sqrt{S_{NN}}=7.7$ GeV. (efficiency corrected).

Cumulants of net-proton distribution at $\sqrt{S_{NN}}=11.5$ GeV. (efficiency corrected).

Cumulants of net-proton distribution at $\sqrt{S_{NN}}=19.6$ GeV. (efficiency corrected).

Cumulants of net-proton distribution at $\sqrt{S_{NN}}=27$ GeV. (efficiency corrected).

Cumulants of net-proton distribution at $\sqrt{S_{NN}}=39$ GeV. (efficiency corrected).

Cumulants of net-proton distribution at $\sqrt{S_{NN}}=62.4$ GeV. (efficiency corrected).

Cumulants of net-proton distribution at $\sqrt{S_{NN}}=200$ GeV. (efficiency corrected).

Cumulants of proton distribution at $\sqrt{S_{NN}}=7.7$ GeV. (efficiency corrected).

Cumulants of proton distribution at $\sqrt{S_{NN}}=11.5$ GeV. (efficiency corrected).

Cumulants of proton distribution at $\sqrt{S_{NN}}=19.6$ GeV. (efficiency corrected).

Cumulants of proton distribution at $\sqrt{S_{NN}}=27$ GeV. (efficiency corrected).

Cumulants of proton distribution at $\sqrt{S_{NN}}=39$ GeV. (efficiency corrected).

Cumulants of proton distribution at $\sqrt{S_{NN}}=62.4$ GeV. (efficiency corrected).

Cumulants of proton distribution at $\sqrt{S_{NN}}=200$ GeV. (efficiency corrected).

Cumulants of anti-proton distribution at $\sqrt{S_{NN}}=7.7$ GeV. (efficiency corrected).

Cumulants of anti-proton distribution at $\sqrt{S_{NN}}=11.5$ GeV. (efficiency corrected).

Cumulants of anti-proton distribution at $\sqrt{S_{NN}}=19.6$ GeV. (efficiency corrected).

Cumulants of anti-proton distribution at $\sqrt{S_{NN}}=27$ GeV. (efficiency corrected).

Cumulants of anti-proton distribution at $\sqrt{S_{NN}}=39$ GeV. (efficiency corrected).

Cumulants of anti-proton distribution at $\sqrt{S_{NN}}=62.4$ GeV. (efficiency corrected).

Cumulants of anti-proton distribution at $\sqrt{S_{NN}}=200$ GeV. (efficiency corrected).