Ratio of inclusive $\psi(2{\rm S})$ over J/$\psi$ yields times their branching ratios as a function of $y_{\rm cms}$ in p--Pb collisions at $\sqrt{s_{\rm NN}}$ = 8.16 TeV .The first uncertainty is statistical, while the second is the systematic.

Ratio of inclusive $\psi(2{\rm S})$ over J/$\psi$ yields times their branching ratios as a function of $p_{\rm T}$ in p--Pb collisions at $\sqrt{s_{\rm NN}}$ = 8.16 TeV at forward rapidity.The first uncertainty is statistical, while the second is the systematic.

Ratio of inclusive $\psi(2{\rm S})$ over J/$\psi$ yields times their branching ratios as a function of $p_{\rm T}$ in p--Pb collisions at $\sqrt{s_{\rm NN}}$ = 8.16 TeV at backward rapidity.The first uncertainty is statistical, while the second is the systematic.

Inclusive $\psi(2{\rm S})$ $R_{\rm pPb}$ values as a function of $y_{\rm {cms}}$ at $\sqrt{s_{\rm NN}}$ = 8.16 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a correlated systematic uncertainty.

Inclusive $\psi(2{\rm S})$ $R_{\rm pPb}$ values as a function of $p_{\rm T}$ at $\sqrt{s_{\rm NN}}$ = 8.16 TeV at forward rapidity. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a correlated systematic uncertainty.

Inclusive $\psi(2{\rm S})$ $R_{\rm pPb}$ values as a function of $p_{\rm T}$ at $\sqrt{s_{\rm NN}}$ = 8.16 TeV at backward rapidity. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a correlated systematic uncertainty.

Double ratio of $\psi$(2S) and J/$\psi$ cross sections in p--Pb and pp collisions as a function of rapidity, at $\sqrt{s_{\mathrm{NN}}} = 8.16$ TeV. The first uncertainty is statistical, while the second is the systematic.

Double ratio of $\psi$(2S) and J/$\psi$ cross sections in p--Pb and pp collisions as a function of $p_{\rm T}$, at $\sqrt{s_{\mathrm{NN}}} = 8.16$ TeV at forward rapidity. The first uncertainty is statistical, while the second is the systematic.

Double ratio of $\psi$(2S) and J/$\psi$ cross sections in p--Pb and pp collisions as a function of $p_{\rm T}$, at $\sqrt{s_{\mathrm{NN}}} = 8.16$ TeV at backward rapidity. The first uncertainty is statistical, while the second is the systematic.

Inclusive $\psi(2{\rm S})$ cross section times branching ratio for backward and forward rapidity, in p--Pb collisions at $\sqrt{s_{\rm NN}}$ = 8.16 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a correlated systematic uncertainty.

Inclusive $\psi(2{\rm S})$ $R_{\rm pPb}$ values for backward and forward rapidity at $\sqrt{s_{\rm NN}}$ = 8.16 TeV. The first uncertainty is statistical, the second is the uncorrelated systematic, while the third one is a correlated systematic uncertainty.

Summary of results for bottom muon v2 as a function of pT for different centrality. Uncertainties are statistical and systematic, respectively.

Summary of results for charm muon v3 as a function of pT for different centrality. Uncertainties are statistical and systematic, respectively.

Summary of results for bottom muon v3 as a function of pT for different centrality. Uncertainties are statistical and systematic, respectively.

Transverse momentum distributions of deuterons in the IV+V V0M multiplicity class

Transverse momentum distributions of deuterons in the VI V0M multiplicity class

Transverse momentum distributions of deuterons in the VII V0M multiplicity class

Transverse momentum distributions of deuterons in the IIX V0M multiplicity class

Transverse momentum distributions of deuterons in the IX V0M multiplicity class

Transverse momentum distributions of deuterons in the X V0M multiplicity class

Transverse momentum distributions of deuterons in the INEL>0 pp collisions

Transverse momentum distributions of deuterons in the INEL pp collisions

Transverse momentum distributions of anti-deuterons in the I V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the II V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the III V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the IV+V V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the VI V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the VII V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the IIX V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the IX V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the X V0M multiplicity class

Transverse momentum distributions of anti-deuterons in the INEL>0 pp collisions

Transverse momentum distributions of anti-deuterons in the INEL pp collisions

$\bar{d}$/d ratio as a function of transverse momentum in I V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in II V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in III V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in IV+V V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in VI V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in VII V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in IIX V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in IX V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in X V0M multiplicity class

$\bar{d}$/d ratio as a function of transverse momentum in INEL>0 pp collisions

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the I V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the II V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the III V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the IV+V V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the VI V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the VII V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the IIX V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the IX V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the X V0M multiplicity class V0M multiplicity class

Coalescence parameter $B_2$ as a function of $p_{\mathrm{T}}$ in the INEL>0 pp collisions V0M multiplicity class

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

$K^{+} + K^{-}$ transverse momentum spectra in V0M multilpicity classes

$p + \bar{p}$ transverse momentum spectra in V0M multilpicity classes

$p + \bar{p}$ transverse momentum spectra in V0M multilpicity classes

$\pi^{+} + \pi^{-}$ transverse momentum spectra ratios, V0M multiplicity classes to INEL>0

$\pi^{+} + \pi^{-}$ transverse momentum spectra ratios, V0M multiplicity classes to INEL>0

$K^{+} + K^{-}$ transverse momentum spectra ratios, V0M multiplicity classes to INEL>0

$K^{+} + K^{-}$ transverse momentum spectra ratios, V0M multiplicity classes to INEL>0

$p + \bar{p}$ transverse momentum spectra ratios, V0M multiplicity classes to INEL>0

$p + \bar{p}$ transverse momentum spectra ratios, V0M multiplicity classes to INEL>0

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

Blast-wave fit parameters

$p_{T}$-integrated ($K^{+} + K^{-}$)/($\pi^{+} + \pi^{-}$) and ($p + \bar{p}$)/($\pi^{+} + \pi^{-}$) ratios in pp collisions as a function of $\langle dN_{ch}/d\eta\rangle_{|\eta|<0.5}$

$p_{T}$-integrated (multi)strange hadron to pion ratios in pp collisions as a function of $\langle dN_{ch}/d\eta\rangle_{|\eta|<0.5}$

$p_{T}$-integrated ($\Omega^{-} + \bar{\Omega}^{+}$)/($\pi^{+} + \pi^{-}$) ratios in pp collisions as a function of $\langle dN_{ch}/d\eta\rangle_{|\eta|<0.5}$

Average transverse momentum of $\pi^{+} + \pi^{-}$, $K^{+} + K^{-}$, and $p + \bar{p}$ as a function of $\langle dN_{ch}/d\eta\rangle_{|\eta|<0.5}$

Transverse momentum spectra ratios ($K^{+} + K^{-}$)/($\pi^{+} + \pi^{-}$) in V0M multiplicity classes

Transverse momentum spectra ratios ($K^{+} + K^{-}$)/($\pi^{+} + \pi^{-}$) in V0M multiplicity classes

Transverse momentum spectra ratios ($p + \bar{p}$)/($\pi^{+} + \pi^{-}$) in V0M multiplicity classes

Transverse momentum spectra ratios ($p + \bar{p}$)/($\pi^{+} + \pi^{-}$) in V0M multiplicity classes

Efficiency and N2LO volume-corrected proton cumulant ratio $K_4/K_2$ plotted as a function of the rapidity acceptance

Efficiency and N2LO volume-corrected proton cumulant ratio $K_2/K_1$ plotted as a function of the mean number of participants $<N_{part}>$ for two rapidity acceptances

Efficiency and N2LO volume-corrected proton cumulant ratio $K_3/K_2$ plotted as a function of the mean number of participants $<N_{part}>$ for two rapidity acceptances

Efficiency and N2LO volume-corrected proton cumulant ratio $K_4/K_2$ plotted as a function of the mean number of participants $<N_{part}>$ for two rapidity acceptances

Efficiency and N2LO volume-corrected proton cumulant $K_2$ plotted as a function of $\Delta y$

Efficiency and N2LO volume-corrected proton cumulant $K_3$ plotted as a function of $\Delta y$

Efficiency and N2LO volume-corrected proton cumulant $K_4$ plotted as a function of $\Delta y$

Efficiency and N2LO volume-corrected proton correlator $C_3$ plotted as a function of $\Delta y$

Efficiency and N2LO volume-corrected proton correlator $C_4$ plotted as a function of $\Delta y$

Efficiency and N2LO volume-corrected proton correlator $C_2$ plotted as a function of maximum $p_t$

Efficiency and N2LO volume-corrected proton correlator $C_3$ plotted as a function of maximum $p_t$

Efficiency and N2LO volume-corrected proton correlator $C_4$ plotted as a function of maximum $p_t$

Efficiency and N2LO volume-corrected proton correlator $C_2$ plotted as a function of the mean number of protons.

Efficiency and N2LO volume-corrected proton correlator $C_3$ plotted as a function of the mean number of protons.

Efficiency and N2LO volume-corrected proton correlator $C_4$ plotted as a function of the mean number of protons.

Efficiency and N2LO volume-corrected proton cumulant ratio $K_3/K_2$ plotted as a function of the center-of-mass energy for two centrality bins (0-10% and 30-40%).

Efficiency and N2LO volume-corrected proton cumulant ratio $K_4/K_2$ plotted as a function of the center-of-mass energy for two centrality bins (0-10% and 30-40%).

Centrality dependence of flow harmonics from $v_2$ to $v_9$.

Centrality dependence of flow harmonics from $v_2$ to $v_9$.

Centrality dependence of flow harmonics from $v_2$ to $v_9$.

Centrality dependence of flow harmonics from $v_2$ to $v_9$.

Centrality dependence of flow harmonics from $v_2$ to $v_9$.

Centrality dependence of linear and non-linear flow modes.

Centrality dependence of linear and non-linear flow modes.

Centrality dependence of linear and non-linear flow modes.

Centrality dependence of linear and non-linear flow modes.

Centrality dependence of linear and non-linear flow modes.

Centrality dependence of linear and non-linear flow modes.

Centrality dependence of symmetry-plane correlations.

Centrality dependence of symmetry-plane correlations.

Centrality dependence of symmetry-plane correlations.

Centrality dependence of symmetry-plane correlations.

Centrality dependence of non-linear flow mode coefficients.

Centrality dependence of non-linear flow mode coefficients.

Centrality dependence of non-linear flow mode coefficients.

Centrality dependence of non-linear flow mode coefficients.

Centrality dependence of non-linear flow mode coefficients.

Centrality dependence of single cumulants C1, of net-lambda multiplicity distributions at Au + Au collision 62.4 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C1, of net-lambda multiplicity distributions at Au + Au collision 200 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C2, of net-lambda multiplicity distributions at Au + Au collision 19.6 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C2, of net-lambda multiplicity distributions at Au + Au collision 27 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C2, of net-lambda multiplicity distributions at Au + Au collision 39 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C2, of net-lambda multiplicity distributions at Au + Au collision 62.4 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C2, of net-lambda multiplicity distributions at Au + Au collision 200 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C3, of net-lambda multiplicity distributions at Au + Au collision 19.6 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C3, of net-lambda multiplicity distributions at Au + Au collision 27 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C3, of net-lambda multiplicity distributions at Au + Au collision 39 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C3, of net-lambda multiplicity distributions at Au + Au collision 62.4 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of single cumulants C3, of net-lambda multiplicity distributions at Au + Au collision 200 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C2/C1, as a function of net-lambda multiplicity distributions at Au + Au collision 19.6 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C2/C1, as a function of net-lambda multiplicity distributions at Au + Au collision 27 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C2/C1, as a function of net-lambda multiplicity distributions at Au + Au collision 39 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C2/C1, as a function of net-lambda multiplicity distributions at Au + Au collision 62.4 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C2/C1, as a function of net-lambda multiplicity distributions at Au + Au collision 200 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C3/C2, as a function of net-lambda multiplicity distributions at Au + Au collision 19.6 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C3/C2, as a function of net-lambda multiplicity distributions at Au + Au collision 27 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C3/C2, as a function of net-lambda multiplicity distributions at Au + Au collision 39 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C3/C2, as a function of net-lambda multiplicity distributions at Au + Au collision 62.4 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Centrality dependence of net-lambda cumulant ratio C3/C2, as a function of net-lambda multiplicity distributions at Au + Au collision 200 GeV. Values are shown with NBD, Poisson and UrQMD predictions.Npart values are from Phys. Rev. C 104, 024902 (2021) and they are little different than the values shown in the original paper.

Beam-energy dependence of net-lambda cumulant ratios C2/C1 in most central (0-5%) and peripheral (50-60%). Values are shown with NBD, Poisson and UrQMD predictions.

Beam-energy dependence of net-lambda cumulant ratios C3/C2 in most central (0-5%) and peripheral (50-60%). Values are shown with NBD, Poisson and UrQMD predictions.

Beam-energy dependence of net-lambda, net-proton and net-kaon cumulant ratios C2/C1 in most central (0-5%) collision.

Beam-energy dependence of net-lambda, net-proton and net-kaon cumulant ratios C3/C2 in most central (0-5%) collision.

Beam-energy dependence of net-lambda cumulant ratios C2/C1 in most central (0-5%) collision, along with results from HRG.

Beam-energy dependence of net-lambda cumulant ratios C3/C2 in most central (0-5%) collision, along with results from HRG.

Rapidity dependence of net-lambda cumulant ratios C2/C1 in most central (0-5%) collision, along with results from NBD.

Rapidity dependence of net-lambda cumulant ratios C3/C2 in most central (0-5%) collision, along with results from NBD.

Rapidity dependence of normalized C2 in most central (0-5%) collision at Au+Au 19.6 GeV.

Rapidity dependence of normalized C2 in most central (0-5%) collision at Au+Au 200 GeV.

Numerical values of double-differential yields $d^{2}n/dydp_{T}$ presented in Fig. 10, given in units of $10^{−3} (GeV/c)^{−1}$. The first uncertainty is statistical, while the second one is systematic

Numerical values of double-differential yields $1/m_T d^{2}n/dm_{T}dy$ given in units of $10^{−3}(GeV)^{−2}$ and presented in Fig. 11; the values of $m_T−m_0$ specify the bin centers. The first uncertainty is statistical, while the second one is systematic

Numerical values of double-differential yields $1/m_T d^{2}n/dm_{T}dy$ given in units of $10^{−3}(GeV)^{−2}$ and presented in Fig. 11; the values of $m_T−m_0$ specify the bin centers. The first uncertainty is statistical, while the second one is systematic

Numerical values of double-differential yields $1/m_T d^{2}n/dm_{T}dy$ given in units of $10^{−3}(GeV)^{−2}$ and presented in Fig. 11; the values of $m_T−m_0$ specify the bin centers. The first uncertainty is statistical, while the second one is systematic

Numerical values of the $p_T$-integrated and extrapolated $dn/dy$ distribution presented in Fig. 12. The first uncertainty is statistical, while the second one is systematic. Additionally, the width of the Gaussian fit to the $dn/dy$ distribution, as well as the mean multiplicity of $K^{*}(892)^0$ mesons are shown (see the text for details)

The mean multiplicities $\langle K^{*}(892)^0\rangle$ and the widths of the rapidity distributions $\sigma_y$ obtained from $dn/dy$ distributions (see the text for details). The first uncertainty is statistical and the second systematic

The mean multiplicity of $K^{*}(892)^0$ mesons for 158 GeV/$c$ inelastic p+p interactions compared to theoretical multiplicities obtained within Hadron Gas Models

The mean multiplicities of different particle species measured in nucleus-nucleus collisions at 158$A$ GeV/$c$ by NA49 and NA61/SHINE. The total uncertainties of $\langle K^{*}(892)^0\rangle$, $\langle K^{+}\rangle$ and $\langle K^{-}\rangle$ were taken as the square roots of the sums of squares of statistical and systematic uncertainties. For NA49 p+p data, the $\langle K^{+}\rangle$ and $\langle K^{-}\rangle$ results include statistical uncertainties only($\langle K^{+}\rangle$ =0.2267$\pm$0.0006 and $\langle K^{-}\rangle$=0.1303$\pm$0.0004), whereas systematic uncertainties for total yields were not reported. Therefore, NA61/SHINE $\langle K^{+}\rangle$ and $\langle K^{-}\rangle$ values were used in the $\langle K^{*}(892)^0 \rangle / \langle K^{+} \rangle$ and $\langle K^{*}(892)^{0}\rangle / \langle K^{-} \rangle$ ratios. The numbers of $\langle K^{+} \rangle$ and $\langle K^{−}\rangle$ and their uncertainties for the 5% most central Pb+Pb collisions were multiplied by a factor 262/362 in orderto estimate charged kaon multiplicities in the 23.5% most central Pb+Pb reactions

Parameters of the polynomial fit of net-proton C3/C2 and C4/C2 vs energy in 0-5$\%$ central Au+Au collisions. Polynomial of order 5 and 4 are used to fit C3/C2 and C4/C2 ratio vs energies, respectively.

Cumulant ratios C3/C2 and C4/C2 of net-proton distributions in STAR Au+Au collisions for nine energies from $\sqrt{s_{NN}} = 7.7 - 200 GeV for 0-5$\%$ and 70-80$\%$ centrality.

Cumulant ratios C3/C2 and C4/C2 of net-proton distributions in Au+Au collisions from UrQMD for 0-5$\%$ centrality.

Cumulant ratios C3/C2 and C4/C2 of net-proton distributions from HRG GCE, HRG GEC excluded volume, HRG CE model.

Cumulants and their ratios up to fourth order in Au+Au collisions at $\sqrt{s_{NN}} = 200 GeV using conventional analytical efficiency corrections and unfolding approaches with various cases of distribution of detector response.

Rapidity dependence of cumulant ratio C4/C2 of net-proton distributions for 0-5$\%$ central Au+Au collisions at nine energies from $\sqrt{s_{NN}} = 7.7 - 200 GeV.

Significance of deviations in net-proton C4/C2 (or kappa*sigma^2) for central 0-5$\%$ Au+Au collisions and those from UrQMD, HRG and peripheral 70-80$\%$ data.