Raw primary antitriton-to-triton ratio as a function of the momentum p_primary in MC (sigma_inel x 4.0).

Raw TPC/TOF ratio for antitriton as a function of the momentum p_primary in exp. data.

Raw TPC/TOF ratio for antitriton as a function of the momentum p_primary in MC (sigma_inel x 0.5).

Raw TPC/TOF ratio for antitriton as a function of the momentum p_primary in MC (sigma_inel x 1.0).

Raw TPC/TOF ratio for antitriton as a function of the momentum p_primary in MC (sigma_inel x 1.5).

Inelastic interaction cross section of antitriton on an averaged material element of the ALICE detector.

Inelastic interaction cross section of antitriton on an averaged material element of the ALICE detector.

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).

Antihelium-3 cosmic-ray flux from background before the solar modulation

Antihelium-3 cosmic-ray flux from dark matter before the solar modulation

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

Antihelium-3 cosmic-ray flux from background after the solar modulation

Antihelium-3 cosmic-ray flux from dark matter after 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.

K p (same charge) correlation function for centrality 5-10% from Pb-Pb collisions at 5020 GeV

K p correlation function for centrality 10-20% from Pb-Pb collisions at 5020 GeV

K p (same charge) correlation function for centrality 10-20% from Pb-Pb collisions at 5020 GeV

K p correlation function for centrality 20-30% from Pb-Pb collisions at 5020 GeV

K p (same charge) correlation function for centrality 20-30% from Pb-Pb collisions at 5020 GeV

K p correlation function for centrality 30-40% from Pb-Pb collisions at 5020 GeV

K p (same charge) correlation function for centrality 30-40% from Pb-Pb collisions at 5020 GeV

K p correlation function for centrality 40-50% from Pb-Pb collisions at 5020 GeV

K p (same charge) correlation function for centrality 40-50% from Pb-Pb collisions at 5020 GeV

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

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

The $\langle x_{\mathrm{j}\gamma} \rangle$ and $R_{\mathrm{j}\gamma}$, the number of associated jets per photon, in 0-30% and 30-100% centrality PbPb collisions. The smeared pp data are added for comparison. A value of 999 in the bin range indicates that there is no upper limit.

The $I_{\mathrm{AA}}^{\mathrm{jet}}$ vs. $p_{\mathrm{T}}^{\mathrm{jet}}$ for 0-30% and 30-100% centrality PbPb collisions. Bins for which there are no data points are denoted as 'empty'.

The centrality dependence of $x_{\mathrm{j}\gamma}$ of photon+jet pairs normalized by the number of photons for PbPb and smeared pp data. Empty bins are denoted as 'empty' in the table.

The $\langle x_{\mathrm{j}\gamma} \rangle$ and $R_{\mathrm{j}\gamma}$ as a function of $\langle N_{\mathrm{part}} \rangle$ for $p_{\mathrm{T}}^{\gamma} > 60$ and 80 GeV. The PbPb results are compared to pp results smeared by the relative jet energy resolution corresponding to each centrality interval.