C(k*)/(quadratic baseline) for K0s K+ and all kT, systematic uncertainties negligible for k*>0.06 GeV/c

C(k*)/(quadratic baseline) for K0s K+ and kT < 0.85 GeV/c, systematic uncertainties negligible for k*>0.06 GeV/c

C(k*)/(quadratic baseline) for K0s K+ and kT > 0.85 GeV/c, systematic uncertainties negligible for k*>0.06 GeV/c

C(k*)/(quadratic baseline) for K0s K- and all kT, systematic uncertainties negligible for k*>0.06 GeV/c

C(k*)/(quadratic baseline) for K0s K- and kT < 0.85 GeV/c, systematic uncertainties negligible for k*>0.06 GeV/c

C(k*)/(quadratic baseline) for K0s K- and kT > 0.85 GeV/c, systematic uncertainties negligible for k*>0.06 GeV/c

R vs. kT for 7 TeV pp averaged over K0s K+ and K0s K- with Achasov2 parameters

R vs. kT for 2.76 TeV/nucleon Pb Pb averaged over K0s K+ and K0s K- with Achasov2 parameters

lambda/purity vs. kT for 7 TeV pp averaged over K0s K+ and K0s K- with Achasov2 parameters

lambda/purity vs. kT for 2.76 TeV/nucleon Pb Pb averaged over K0s K+ and K0s K- with Achasov2 parameters

R vs. kT for 7 TeV pp averaged over K0s K+ and K0s K- and with Achasov2 parameters

R vs. kT for 7 TeV pp --> K0s K0s averaged over event multiplicity

R vs. kT for 7 TeV pp --> K+- K+- averaged over event multiplicity and averaged between K+ and K-

lambda/purity vs. kT for 7 TeV pp averaged over K0s K+ and K0s K- and with Achasov2 parameters

lambda/purity vs. kT for 7 TeV pp --> K0s K0s averaged over event multiplicity

lambda/purity vs. kT for 7 TeV pp --> K+- K+- averaged over event multiplicity and averaged between K+ and K-

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

Fully corrected $p_{\rm T} D$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $p_{\rm T} D$ distributions pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 Tune 4C simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Ratio of fully corrected $p_{\rm T} D$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Fully corrected $LeSub$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$.

Ratio of fully corrected $LeSub$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 Tune 4C simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

Ratio of fully corrected $LeSub$ distributions in pp collisions at $\sqrt{s} = 7$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

Fully corrected $g$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $g$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 Tune 4C simulations. The systematic uncertainty of $g$ is propagated to the ratio.

Ratio of fully corrected $g$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $g$ is propagated to the ratio.

Fully corrected $p_{\rm T} D$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $p_{\rm T} D$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Ratio of fully corrected $p_{\rm T} D$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $p_{\rm T} D$ is propagated to the ratio.

Fully corrected $LeSub$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$. The results are compared to PYTHIA.

Ratio of fully corrected $LeSub$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA 8 simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

Ratio of fully corrected $LeSub$ distributions in $0$--$10\%$ central Pb--Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$\,TeV for $R = 0.2$ in the range of jet $p_{\mathrm{T,jet}}^{\rm ch}$ of $40$--$60$\,GeV$/c$ and PYTHIA Perugia 11 simulations. The systematic uncertainty of $LeSub$ is propagated to the ratio.

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

Data-to-cocktail ratio as a function of the invariant-mass. In the hadronic cocktail, random correlations of dielectrons from charm decays are assumed to simulate the effects of the interaction between charm quarks and the medium. The statistical and systematic uncertainties of data are represented by vertical bars and boxes.

Dielectron invariant-mass spectrum measured in central Pb-Pb collisions for the transverse-momentum interval 1.0 < $p_{\rm T,ee}$ < 2.0 GeV/$c. The statistical and systematic uncertainties of the data are represented by vertical bars and boxes.

Dielectron invariant-mass spectrum measured in central Pb--Pb collisions for the transverse-momentum interval 2.0 < $p_{\rm T,ee}$ < 4.0 GeV/$c. The statistical and systematic uncertainties of the data are represented by vertical bars and boxes.

Direct photon ratio $R_{\gamma^{(*)}}=1+\gamma^{(*)}_{\mathrm{dir}}/\gamma^{(*)}_{\mathrm{decay}}$ measured using virtual photons in the centrality range 0$-$10$\%$. The statistical and systematic uncertainties of the data are represented by vertical bars and boxes.

V2{GAMMA,DECAY} as function of $p_\text{T}$, collision centrality 20-40%, for Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

V2{GAMMA,INCLUSIVE} as function of $p_\text{T}$, collision centrality 0-20%, for Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

V2{GAMMA,INCLUSIVE} as function of $p_\text{T}$, collision centrality 20-40%, for Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

V2{GAMMA,DIRECT} as function of $p_\text{T}$, collision centrality 0-20%, for Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

V2{GAMMA,DIRECT} as function of $p_\text{T}$, collision centrality 20-40%, for Pb-Pb collisions at $\sqrt{s_{\rm NN}} = 2.76$ TeV.

$\langle p_{\rm T} \rangle$ of $\Lambda$(1520) (sum of particle and anti-particle states) at midrapidity as a function of $\langle {\rm d}N_{\rm ch}/{\rm d}\eta \rangle^{1/3}$. The uncertainty 'syst,uncorrelated' indicates the systematic uncertainty after removing the contributions common to all centrality classes

$\Lambda$(1520) (sum of particle and anti-particle states) to $\Lambda$ (defined as 2 $\Lambda$) $p_{\rm T}$-integrated yield ratio at midrapidity as a function of $\langle {\rm d}N_{\rm ch}/{\rm d}\eta \rangle^{1/3}$. The uncertainty 'syst,uncorrelated' indicates the systematic uncertainty after removing the contributions common to all centrality classes

Reconstructed mass of $\rho^{0}$ meson in 40-60$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Reconstructed mass of $\rho^{0}$ meson in 60-80$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Yield of $\rho^{0}$ meson normalized to the number of inelastic pp collisions at $\sqrt{s}=2.76~{\rm TeV}$.

Yield of $\rho^{0}$ meson in 0-20$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Yield of $\rho^{0}$ meson in 20-40$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Yield of $\rho^{0}$ meson in 40-60$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Yield of $\rho^{0}$ meson in 60-80$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Ratio of integrated yields $2\rho^{0}/(\pi^{+}+\pi^{-})$ as a function of $(dN_{ch}/d\eta)^{1/3}$ in pp and 0-20$\%$, 20-40$\%$, 40-60$\%$, 60-80$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Mean transverse momentum of $\rho^{0}$ meson as a function of $(dN_{ch}/d\eta)^{1/3}$ in pp and 0-20$\%$, 20-40$\%$, 40-60$\%$, 60-80$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Ratio $2\rho^{0}/(\pi^{+}+\pi^{-})$ as a function of $p_{T}$ in pp collisions at $\sqrt{s}=2.76~{\rm TeV}$.

Ratio $2\rho^{0}/(\pi^{+}+\pi^{-})$ as a function of $p_{T}$ in 0-20$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

Ratio $2\rho^{0}/(\pi^{+}+\pi^{-})$ as a function of $p_{T}$ in 60-80$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

$R_{AA}$ as a function of $p_{T}$ in 0-20$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

$R_{AA}$ as a function of $p_{T}$ in 20-40$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

$R_{AA}$ as a function of $p_{T}$ in 40-60$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

$R_{AA}$ as a function of $p_{T}$ in 60-80$\%$ central Pb-Pb collisions at $\sqrt{s_{\rm NN}}=2.76~{\rm TeV}$.

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

Raa vs $\langle dNch/d\eta \rangle$.

Raa vs $\langle dNch/d\eta \rangle$.

Raa vs $\langle dNch/d\eta \rangle$.

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

Direct photon spectra(Nucl. Part. Phys. 23, A1 (1997)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in p+p at $\sqrt{s_{NN}}$= 63 GeV.

Direct photon spectra(Sov. J. Nucl. Phys. 51, 836 (1990)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in p+p at $\sqrt{s_{NN}}$= 63 GeV.

Direct photon spectra normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 62.4 GeV.

Direct photon spectra normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 39.0 GeV.

Direct photon spectra(Physical Review C91, 064904 (2015)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review Letters 104, 132301 (2010)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review Letters 109, 152302 (2012)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review C98, 054902 (2018)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Cu+Cu at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physics Letters B754 235 (2016)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Pb+Pb at $\sqrt{s_{NN}}$= 2760 GeV.

Number of binary collisions N_{coll} vs. Charged particle multiplicity in Au+Au at various cm energies.

Charged particle multiplicity vs. centrality in Au+Au at various cm energies.

Number of binary collisions N_{coll} vs. centrality in Au+Au at various cm energies.

Integrated direct photon yield vs. Charged particle multiplicity in various systems at various cm energies.

Charged particle multiplicity vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. Charged particle multiplicity in various systems at various cm energies.

Charged particle multiplicity vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. centrality in various systems at various cm energies.