The fraction of the direct photon component as a function of $p_T$.

The fraction of the direct photon component as a function of $p_T$.

Invariant yield (Au+Au) of direct photons as a function of $p_T$.

Invariant yield (Au+Au) of direct photons as a function of $p_T$.

Invariant yield (Au+Au) of direct photons as a function of $p_T$.

Invariant cross section ($p$+$p$) of direct photons as a function of $p_T$.

Experimental correlation moments $R^2_{x2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^2_{x2}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^2_{y2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^2_{y2}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x6}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x6}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{y6}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{y6}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x2y2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x2y2}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x4}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{x}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{y4}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^4_{y4}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x2y4}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x2y4}(q)$ Fit. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x4y2}(q)$ Data. Systematic errors are less than the statistical errors.

Experimental correlation moments $R^6_{x4y2}(q)$ Fit. Systematic errors are less than the statistical errors.

Source function profile $S(r_x)$ Image in the PCMS.

Source function profile $S(r_x)$ Fit in the PCMS. The blue line represents the Hump fit.

Source function profile $S(r_y)$ Image in the PCMS.

Source function profile $S(r_y)$ Fit in the PCMS. The blue line represents the Hump fit.

Source function profile $S(r_z)$ Image in the PCMS.

Source function profile $S(r_z)$ Fit in the PCMS. The blue line represents the Hump fit.

Associated correlation profile $C(q_x)$ Image in the PCMS.

Associated correlation profile $C(q_x)$ Fit in the PCMS.

Associated correlation profile $C(q_y)$ Image in the PCMS.

Associated correlation profile $C(q_y)$ Fit in the PCMS.

Associated correlation profile $C(q_z)$ Image in the PCMS.

Associated correlation profile $C(q_z)$ Fit in the PCMS.

Source function comparison between Therminator calculation and image for $S(r_x)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_x)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_y)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_y)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_z)$ in PCMS.

Source function comparison between Therminator calculation and image for $S(r_z)$ in PCMS.

$\Delta$$t_{LCM}$ from Therminator events compared with various assumptions for $\Delta\tau$ and resonance emissions.

$\Delta$$t_{LCM}$ from Therminator events compared with various assumptions for $\Delta\tau$ and resonance emissions.

$\pi^0$ invariant yields for different centralities. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

$\pi^0$ invariant yields for different centralities. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Nuclear modification factor ($R_{AA}$) for $\pi^0$s. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

$\pi^0$ $R_{AA}$ for the most central (0-5%) Au+Au collisions and PQM model calculations for different values of $<\bar{q}>$. The bin range is not an uncertainty in the x-axis because the actual uncertainty by having the finite bin width is corrected for by the bin-shift correction. These bins were constructed using the corrected finite values as centers.

Integrated nuclear modification factor ($R_{AA}$) for $\pi^0$ as a function of collision centrality.

Measured $C_2$($q_{inv}$) and restored $C_2$($q_{inv}$) from imaged $S(r)$, compared with angle-averaged Gaussian $C_2$($q_{inv}$) for charged kaon pairs measured for 0.3 < $k_T$ < 0.9 GeV/$c$ at 0-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Measured $C_2$($q_{inv}$) and restored $C_2$($q_{inv}$) from imaged $S(r)$, compared with angle-averaged Gaussian $C_2$($q_{inv}$) for charged kaon pairs measured for 0.3 < $k_T$ < 0.9 GeV/$c$ at 0-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Measured $C_2$($q_{inv}$) and restored $C_2$($q_{inv}$) from imaged $S(r)$, compared with angle-averaged Gaussian $C_2$($q_{inv}$) for charged kaon pairs measured for 0.3 < $k_T$ < 0.9 GeV/$c$ at 0-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Measured $C_2$($q_{inv}$) and restored $C_2$($q_{inv}$) from imaged $S(r)$, compared with angle-averaged Gaussian $C_2$($q_{inv}$) for charged kaon pairs measured for 0.3 < $k_T$ < 0.9 GeV/$c$ at 0-30% central Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

$m^2$ (signal+background) distribution for $\bar{d}$,$d$ for $p_T$ = 1.6-2.9 GeV/$c$.

$m^2$ (background) distribution for $\bar{d}$,$d$ for $p_T$ = 1.6-2.9 GeV/$c$.

$m^2$ (signal) distribution for $\bar{d}$,$d$ for $p_T$ = 1.6-2.9 GeV/$c$.

Comparison of differential $v_2(p_T)$ for $\pi^{\pm}$. Results are shown for 20-60% central Au+Au collisions.

Comparison of differential $v_2(p_T)$ for $K^{\pm}$. Results are shown for 20-60% central Au+Au collisions.

Comparison of differential $v_2(p_T)$ for $(\bar{p})p$. Results are shown for 20-60% central Au+Au collisions.

Comparison of differential $v_2(p_T)$ for $\phi$ mesons. Results are shown for 20-60% central Au+Au collisions.

Comparison of differential $v_2(p_T)$ for $(\bar{d})d$. Results are shown for 20-60% central Au+Au collisions.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$v_2$ vs $KE_T$ for several identified particle species obtained in mid-central Au+Au collisions, and ${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for the same particle species.

$R_{cp}$ as a function of $\eta$ for 1.5 < $p_T$ < 4.0 GeV/$c$ for different centrality classes. Systematic uncertainties which are point-to-point uncorrelated (sys-uncorr) and correlated (sys-corr) are shown.

$1/{N_{trig}}$ ${dN}/{d\Delta\phi}$ distributions for charge selected $\bar{p}$ and $p$ triggers both with associated $p$ for six centrality bins. Triggers have 2.5 < $p_T$ < 4.0 GeV/$c$ and associated particles have 1.8 < $p_T$ < 2.5 GeV/$c$.

$1/{N_{trig}}$ ${dN}/{d\Delta\phi}$ distributions for charge selected $\bar{p}$ and $p$ triggers both with associated $p$ for six centrality bins. Triggers have 2.5 < $p_T$ < 4.0 GeV/$c$ and associated particles have 1.8 < $p_T$ < 2.5 GeV/$c$.

$1/{N_{trig}}$ ${dN}/{d\Delta\phi}$ distributions for charge-inclusive baryon and meson triggers and associated mesons for six centrality bins. Triggers have 2.5 < $p_T$ < 4.0 GeV/$c$ and associated particles have 1.8 < $p_T$ < 2.5 GeV/$c$.

Conditional yields per trigger on the near side for charge selected and charge selected $p$ and $\bar{p}$ correlations. Triggers have 2.5 < $p_T$ < 4.0 GeV/$c$ and associated particles have 1.8 < $p_T$ < 2.5 GeV/$c$. There is an 11.4% additional normalization error on baryon associated particle points and 8.9% each on the $p$ and $\bar{p}$ associated particle points.

Conditional yields per trigger on the away side for charge selected and charge selected $p$ and $\bar{p}$ correlations. Triggers have 2.5 < $p_T$ < 4.0 GeV/$c$ and associated particles have 1.8 < $p_T$ < 2.5 GeV/$c$.

Conditional yields per trigger for baryon and meson triggers with associated mesons. Triggers have 2.5 < $p_T$ < 4.0 GeV/$c$ and associated particles have 1.8 < $p_T$ < 2.5 GeV/$c$. There is an additional 13.6% normalization error.

$v_2$ vs $p_T$ for identified particle species obtained in minimum bias Au+Au collisions.

$v_2$ vs $p_T$ for identified particle species obtained in minimum bias Au+Au collisions.

$v_2$ vs $p_T$ for identified particle species obtained in minimum bias Au+Au collisions.

$v_2$ vs $KE_T$ for identified particle species obtained in minimum bias Au+Au collisions.

$v_2$ vs $KE_T$ for identified particle species obtained in minimum bias Au+Au collisions.

$v_2$ vs $KE_T$ for identified particle species obtained in minimum bias Au+Au collisions.

${v_2}/{n_q}$ vs ${p_T}/{n_q}$ for identified particle species obtained in minimum bias Au+Au collisions.

${v_2}/{n_q}$ vs ${p_T}/{n_q}$ for identified particle species obtained in minimum bias Au+Au collisions.

${v_2}/{n_q}$ vs ${p_T}/{n_q}$ for identified particle species obtained in minimum bias Au+Au collisions.

${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for identified particle species obtained in minimum bias Au+Au collisions.

${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for identified particle species obtained in minimum bias Au+Au collisions.

${v_2}/{n_q}$ vs ${KE_T}/{n_q}$ for identified particle species obtained in minimum bias Au+Au collisions.

$I_{AA}$ versus $p_T^B$ for four trigger $p_T$ bins in HR+SR ($|\Delta\phi - \pi|$ < $\pi/2$) and HR ($|\Delta\phi - \pi|$ < $\pi/6$).

$I_{AA}$ versus $p_T^B$ for four trigger $p_T$ bins in HR+SR ($|\Delta\phi - \pi|$ < $\pi/2$) and HR ($|\Delta\phi - \pi|$ < $\pi/6$).

Truncated mean $<p_T^{\prime}>$ in 1 < $p_T^B$ < 5 GeV/$c$ versus $N_{part}$ for the near-side, away-side shoulder, and head regions for Au+Au and $p$+$p$ for three trigger $p_T$ bins.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Charged hadron $v_2$($p_T$) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV from the two-particle cumulant method, the BBC event plane, and the ZDC-SMD event plane for the indicated centralities.

Anisotropy parameter $v_2$ as a function of pseudorapidity within the PHENIX central arms using event planes from the BBC and ZDC-SMD, and from the two-particle cumulant method for centrality 20–40%. The results are shown for three $p_T$ bins, which are from top to bottom: 2.0–3.0, 1.2–1.4 and 0.6–0.8 GeV/$c$.

Comparison of the $v_2${BBC} and $v_2${ZDC-SMD} obtained from the S-N and ZDC-BBC-CNT subevents as a function of pT in the 20–60% centrality range.

Charged hadron $v_2${2} for the PHENIX experiment as a function of $p_T$ in centrality 20–60%.

The PHENIX $v_2${BBC} and $v_2${ZDC-SMD} from the modified event-plane method for charged hadrons as a function of $p_T$ in different centralities.

The PHENIX $v_2${BBC} and $v_2${ZDC-SMD} from the modified event-plane method for charged hadrons as a function of $p_T$ in different centralities.

The PHENIX $v_2${BBC} and $v_2${ZDC-SMD} from the modified event-plane method for charged hadrons as a function of $p_T$ in different centralities.

The PHENIX $v_2${BBC} and $v_2${ZDC-SMD} from the modified event-plane method for charged hadrons as a function of $p_T$ in different centralities.

The PHENIX $v_2${BBC} and $v_2${ZDC-SMD} from the modified event-plane method for charged hadrons as a function of $p_T$ in different centralities.

The PHENIX $v_2${BBC} and $v_2${ZDC-SMD} from the modified event-plane method for charged hadrons as a function of $p_T$ in different centralities.