The $v_{dyn}$ and the three terms of $v_{dyn}$ vs $\sqrt{\langle N_{ch}\rangle \langle N_{\gamma}\rangle }$ for mixed events. $Corr_{\gamma\,-ch}^{real}$ is plotted.

The $v_{dyn}$ and the three terms of $v_{dyn}$ vs $\sqrt{\langle N_{ch}\rangle \langle N_{\gamma}\rangle }$ for mixed events. $Corr_{\gamma\,-ch}^{mixed}$ is plotted.

The $v_{dyn}$ and the three terms of $v_{dyn}$ vs $\sqrt{\langle N_{ch}\rangle \langle N_{\gamma}\rangle }$ for mixed events. $\omega_{\gamma}^{real}$ is plotted.

The $v_{dyn}$ and the three terms of $v_{dyn}$ vs $\sqrt{\langle N_{ch}\rangle \langle N_{\gamma}\rangle }$ for mixed events. $\omega_{\gamma}^{mixed}$ is plotted.

The $v_{dyn}$ and the three terms of $v_{dyn}$ vs $\sqrt{\langle N_{ch}\rangle \langle N_{\gamma}\rangle }$ for mixed events. $v_{dyn}^{real}$ is plotted.

The $v_{dyn}$ and the three terms of $v_{dyn}$ vs $\sqrt{\langle N_{ch}\rangle \langle N_{\gamma}\rangle }$ for mixed events. $v_{dyn}^{mixed}$ is plotted.

The values of the observable $v_{dyn}^{ch-\gamma}$ for the same side.

The values of the observable $v_{dyn}^{ch-\gamma}$ for the same side.

The values of the observable $v_{dyn}^{ch-\gamma}$ for the away-side.

The values of the observable $v_{dyn}^{ch-\gamma}$ for the away-side.

The correlation between positive and negative charged particles measured by the FTPC and photons measured by the PMD using $v_{dyn}$ for real events.

$r_{m,1}$ vs multiplicity for first order of m.

$r_{m,1}$ vs multiplicity for first order of m.

$r_{m,1}$ vs multiplicity for second order of m.

$r_{m,1}$ vs multiplicity for second order of m.

$r_{m,1}$ vs multiplicity for third order of m.

$r_{m,1}$ vs multiplicity for third order of m.

The moments $r_{m,1}$(m=1-3) for real and mixed events as a function of order m in a fixed multiplicity bin of 47$\langle \sqrt{\langle N_{ch}\rangle \langle N_{\gamma}\rangle }\langle 54$.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 0% to 20% centrality $Au+Au$. 90% Limit on 18-20 and 20-22 GeV/c bins.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 20% to 40% centrality $Au+Au$. 90% Limit for 20-22 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 40% to 60% centrality $Au+Au$. 90% Limit for 18-20 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 20% to 60% centrality $Au+Au$. 90% Limit for 18-20 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 60% to 92% centrality $Au+Au$. 90% Limit for 18-20 GeV/c bin.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, 0% to 92% centrality $Au+Au$.

$E\frac{dN^3}{dp^3}$ vs. $p_T$, $p+p$.

${\eta}$ $R_{AA}$, 0% to 5% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 0% to 10% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 10% to 20% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 0% to 20% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 20% to 40% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 40% to 60% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 20% to 60% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 60% to 92% centrality $Au+Au$.

${\eta}$ $R_{AA}$, 0% to 92% centrality $Au+Au$.

${\pi^{0}}$ $R_{AA}$, 0% to 92% centrality $Au+Au$.

${\eta}$ ${R_{AA}}$, 0% to 92% centrality $Au+Au$.

${\eta}$ $R_{AA}$ vs centrality ($p_T>$20 GeV/c).

${\eta}$ $R_{AA}$ vs centrality ($p_T>$5 GeV/c).

Slope ${\eta}$ $R_{AA}$ ($5<p_T<$ 18 GeV/c) vs centrality.

$\chi^{2}/{NDF}$, Prob%, ${\eta}$ $R_{AA}$ ($5<p_T<$ 18 GeV/c) Prob, $R_{AA}$ ($p_T>$ 5 GeV/c) Prob vs centrality