'The relative dynamical correlation as a function of $N_{part}$'

'The relative dynamical correlation as a function of $N_{part}$'

'The relative dynamical correlation as a function of $N_{part}$'

'The relative dynamical correlation as a function of $N_{part}$'

'The relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'ratios of the measured data to the power law as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The ratios of the measured data to UrQMD calculations as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'The UrQMD calculations of relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'Comparison of a model incorporating a Boltzmann-Langevin approach to the calculation of thermalization effects for the relative dynamical correlation as a function of $N_{part}$'

'relative dynamical correlation as a function of $N_{part}$'

'relative dynamical correlation as a function of $N_{part}$'

'relative dynamical correlation as a function of $N_{part}$'

'relative dynamical correlation as a function of collision energy for the 0-5\% centrality bin'

'relative dynamical correlation as a function of collision energy for the 0-5\% centrality bin'

'relative dynamical correlation as a function of collision energy for the 0-5\% centrality bin'

'relative dynamical correlation as a function of collision energy for the 0-5\% centrality bin'

'relative dynamical correlation as a function of collision energy for the 0-5\% centrality bin'

(a) Centrality dependence of $v^{even}_{1}$ for $0.4 \lt p_{T} \lt 0.7$ GeV/c for Au+Au collisions at $\sqrt{s_{_{NN}}} = 200, 39$ and $19.6$ GeV; (b) $K$ vs. $\langle N_{ch} \rangle^{-1}$ for the $v^{even}_{1}$ values shown in (a). The $\langle N_{ch} \rangle$ values correspond to the centrality intervals indicated in panel (a).

Comparison of the $\sqrt{s_{_{NN}}}$ dependence of $v^{even}_{1}$ and $v_3$ for $0.4 \lt p_{T} \lt 0.7$ GeV/c in 0-10 central Au+Au collisions.

Raw $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 27 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 39 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Raw $\Delta N_k$ distributions in Au+Au collisions at 200 GeV for 0–5%, 30–40%, and 70–80% collision centralities at midrapidity. The distributions are not corrected for the finite centrality bin width effect nor the reconstruction efficiency.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of cumulants (C1, C2, C3, and C4) of $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $M/\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $S\sigma$ for $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 7.7 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 11.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 14.5 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 19.6 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 27 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 39 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 62.4 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collision centrality dependence of the $\kappa\sigma^2$ for $\Delta N_k$ distributions in Au+Au collisions at 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collisions energy dependence of $M/\sigma^2$ for $\Delta N_k$ multiplicity distributions from 0–5% most central and 70–80% peripheral collisions in Au+Au collisions at \sqrt{s_{NN}} = 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collisions energy dependence of $S\sigma$ for $\Delta N_k$ multiplicity distributions from 0–5% most central and 70–80% peripheral collisions in Au+Au collisions at \sqrt{s_{NN}} = 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Collisions energy dependence of $\kappa\sigma^2$ for $\Delta N_k$ multiplicity distributions from 0–5% most central and 70–80% peripheral collisions in Au+Au collisions at \sqrt{s_{NN}} = 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV. The error bars are statistical uncertainties and the caps represent systematic uncertainties.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{+}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, and 39 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $p$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{+}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $p$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{+}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{p}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{p}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, and 39 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{p}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{p}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{+}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{+}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, and 39 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{+}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{+}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{-}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{-}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, and 39 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{-}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\pi^{-}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{+}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{+}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, and 39 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{+}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{+}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 11.5, 14.5, 19.6, 27, 39 and 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K^{-}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 11.5, 14.5, 19.6, 27, 39 and 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $K_0^s$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 11.5, 14.5, 19.6, 27, 39 and 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Directed flow $v_1$ as a function of rapidity $y$ for $\Lambda$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\bar{\Lambda}$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7, 11.5, 14.5, 19.6, 27, 39, 62.4 and 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 11.5, 14.5, 19.6, 27, 39 and 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 5%–10% central Au+Au collisions at $\sqrt{s_{NN}} =$ 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 11.5, 14.5, 19.6, 27, 39 and 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 10%–40% central Au+Au collisions at $\sqrt{s_{NN}} =$ 200 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 7.7 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 11.5, 14.5, 19.6, 27, 39 and 62.4 GeV.

Directed flow $v_1$ as a function of rapidity $y$ for $\phi$ in 40%–80% central Au+Au collisions at $\sqrt{s_{NN}} =$ 200 GeV.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Directed flow slope $dv_1/dy$ as a function of beam energy in 10%–40% central Au+Au collisions.

Identified particle (Kaon Plus) RCP for RHIC BES energies. The colored shaded boxes describe the point-to-point systematic uncertainties. The uncertainty bands at unity on the right side of the plot correspond to the pT -independent uncertainty in Ncoll scaling with the color in the band corresponding to the color of the data points for that energy.

Identified particle (Kaon Minus) RCP for RHIC BES energies. The colored shaded boxes describe the point-to-point systematic uncertainties. The uncertainty bands at unity on the right side of the plot correspond to the pT -independent uncertainty in Ncoll scaling with the color in the band corresponding to the color of the data points for that energy.

Identified particle (Proton) RCP for RHIC BES energies. The colored shaded boxes describe the point-to-point systematic uncertainties. The uncertainty bands at unity on the right side of the plot correspond to the pT -independent uncertainty in Ncoll scaling with the color in the band corresponding to the color of the data points for that energy.

Identified particle (Antiproton) RCP for RHIC BES energies. The colored shaded boxes describe the point-to-point systematic uncertainties. The uncertainty bands at unity on the right side of the plot correspond to the pT -independent uncertainty in Ncoll scaling with the color in the band corresponding to the color of the data points for that energy.

Charged hadron Y(<Npart>) for two ranges of pT (pT 3.0 - 3.5 GeV/c). Statistical uncertainty bars are included, mostly smaller than point size, as well as shaded bands to indicate systematic uncertainties.

Charged hadron Y(<Npart>) for two ranges of pT (pT 4.0 - 4.5 GeV/c). Statistical uncertainty bars are included, mostly smaller than point size, as well as shaded bands to indicate systematic uncertainties.

Glauber Fit Parameters

Nch at each Collision Energy (GeV)

Ncoll at each Collision Energy (GeV)

Npart at each Collision Energy (GeV)

The value of $\sigma^{NN}_{inel}$ used in the Monte Carlo Glauber simulation at each collision energy

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

Charged hadron $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\\p$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\overline{p}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$K^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$K^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\pi^{+}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 7.7 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 11.5 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 14.5 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 19.6 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 27 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 39 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

$\pi^{-}$ $\frac{1}{2\pi p_{T}}$ * $\frac{d^{2}N}{d\eta dp_{T}}$ $\pm$ stat. $\pm$ sys. $(GeV/c)^{-2}$ for $\sqrt{s_{NN}}$ = 62.4 GeV/c

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

The intercepts and slope for the exponential parameterisation of the differential cross section of the form A exp(-B*PT**2). Errors do not contain additional 2.1 PCT uncertainty on the intercepts.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

The intercepts and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the photoproduction sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the low-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the mid-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the high-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

$\sqrt{s_{NN}}$ dependence of $<p_t>$ fluctuations for central collisions and STAR full acceptance. CERES fluctuation data (12.3 and 17.3 GeV) were linearly extrapolated to the STAR $\eta$ acceptance

Hijing-1.37 $<p_t>$ fluctuations for central collisions and the STAR acceptance at three energies, for quench-on, quench-off and jets-off collisions.

(Color Online) Variation of $N_{ch}$ normalized to the number of collisions in the FTPC coverage $(2.9 \leq \eta \leq 3.9)$ and $N_{\gamma}$ normalized to number of collisions, in the PMD coverage $(2.3 \leq \eta \leq 3.7)$ as a function of $N_{coll}$. The lower band shows the uncertainty in the ratio due to uncertainties in $N_{coll}$ calculations.

(Color Online) $dN/d\eta$ for charged particles and photons for Au + Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV for various event centrality classes.

(Color Online) $dN/d\eta$ for charged particles and photons for Au + Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV for various event centrality classes.

(Color Online) Half width at half maximum of the pseudorapidity distributions ($\eta_{h}$) of charged particles as a function of total charged particle multiplicity ($N_{T}$) normalized to the center of mass energy. The Au + Au collision data are from the PHOBOS [8] experiment and p + p collision data are from the ISR [31] experiments.

(Color Online) Half width at half maximum of the pseudorapidity distributions ($\eta_{h}$) of charged particles as a function of total charged particle multiplicity ($N_{T}$) normalized to the center of mass energy. The Au + Au collision data are from the PHOBOS [8] experiment and p + p collision data are from the ISR [31] experiments.

(Color Online) Variation of $dN_{ch}/d\eta$ normalized to $N_{part}$ with $\eta – y_{beam}$ for central and peripheral collisions for positively charged hadrons ($h^{+}$) and negatively charged hadrons ($h^{−}$).

(Color Online) The top panel shows the variation of pion rapidity density normalized to $N_{part}$ with $y – y_{beam}$ for central collisions at various collision energies. Also shown is the estimated $dN_{\pi^{0}}/dy$ obtained from $dN\_{\gamma}/dy$ normalized to $N_{part}$. The bottom panel shows the variation of net proton rapidity density normalized to $N_{part}$ with $y – y_{beam}$ for central collisions at various collision energies.

(Color Online) The top panel shows the variation of pion rapidity density normalized to $N_{part}$ with $y – y_{beam}$ for central collisions at various collision energies. Also shown is the estimated $dN_{\pi^{0}}/dy$ obtained from $dN\_{\gamma}/dy$ normalized to $N_{part}$. The bottom panel shows the variation of net proton rapidity density normalized to $N_{part}$ with $y – y_{beam}$ for central collisions at various collision energies.

Directed flow of charged particles as a function of pseudorapidity, for centrality 10%-70%.

Directed flow of charged particles as a function of pseudorapidity, for centrality 10%-70%.

Directed flow of charged particles as a function of pseudorapidity, for centrality 10%-70%.

$v_1$ versus rapidity for charged particles.

$v_1$ versus rapidity for pions.

$v_1$ versus rapidity for protons.

Directed flow of charged particles as a function of pseudorapidity for the 60-70% and 70-80% centrality classes.

Directed flow of charged particles as a function of pseudorapidity for the 10-20%, 20-30%, 30-40%, 40-50% and 50-60% centrality classes.

Directed flow of charged particles as a function of pseudorapidity for the 5-10% centrality class.

Directed flow of charged particles as a function of pseudorapidity for the 0-5% centrality class.

$v_1${3} versus $p_t$ measured in the main TPC (|$\eta$| < 1.3), for centrality 10%-70%.

$v_1${3} versus $p_t$ measured in the Forward TPC (2.5 < |$\eta$| < 4.0), for different centralities.

Directed flow of charged particles as a function of impact parameter for the mid-pseudorapidity region (|$\eta$| < 1.3) and the forward pseudorapidity region (2.5 < |$\eta$| < 4.0.

Charged particle $v_1$ for Au+Au collisions (10%-70%) at 200 GeV as a function of $\eta-y_{beam}$.

Charged particle $v_1$ for Au+Au collisions (10%-70%) at 62.4 GeV as a function of $\eta-y_{beam}$.

Charged particle $v_1$ for Pb+Pb collisions (12.5%-33.5%) at 17.2 GeV as a function of $y-y_{beam}$.

Average transverse momentum per event for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV for the 5% most central collisions.

$<\Delta p_{t,i}\Delta p_{t,j}>$ as a function of centrality and incident energy for Au+Au collisions compared with HIJING results.

(d$N/\textrm{d}\eta)<\Delta p_{t,i}\Delta p_{t,j}>$ as a function of centrality and incident energy for Au+Au collisions compared with HIJING results.

$(<\Delta p_{t,i}\Delta p_{t,j}>)^{1/2}/<<p_{t}>>$ as a function of centrality and incident energy for Au+Au collisions compared with HIJING results.

$(<\Delta p_{t,i}\Delta p_{t,j}>)^{1/2}/<<p_{t}>>$ as a function of incident energy for 0-5% most central Au+Au collisions compared with CERES results.