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.

e+e- production cross section at mid rapidity for ultra peripheral Au+Au reactions.The results are given for 3 intervals of masses of the electron pair : 2.0 to 2.3, 2.3 to 2.8 and 2.0 to 2.8 Gev/c2.

Rebinned $R_{AA}$ for $\Delta \phi$, $p_T$, and path length dependence,

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 12<$p_{T}^{\gamma}$<15 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 5<$p_{T}^{\gamma}$<7 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 7<$p_{T}^{\gamma}$<9 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 9<$p_{T}^{\gamma}$<12 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 12<$p_{T}^{\gamma}$<15 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 5<$p_{T}^{\gamma}$<7 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 7<$p_{T}^{\gamma}$<9 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 9<$p_{T}^{\gamma}$<12 GeV/c.

direct $\gamma$-hadron yields per trigger p+p and Au+Au at 12<$p_{T}^{\gamma}$<15 GeV/c.

Ratio of $I_{AA}$ of Au+Au to p+p yields at 5<$p_{T}^{\gamma}$<7 GeV/c.

Ratio of $I_{AA}$ of Au+Au to p+p yields at 7<$p_{T}^{\gamma}$<9 GeV/c.

Ratio of $I_{AA}$ of Au+Au to p+p yields at 9<$p_{T}^{\gamma}$<12 GeV/c.

Ratio of $I_{AA}$ of Au+Au to p+p yields at 12<$p_{T}^{\gamma}$<15 GeV/c.

$I_{AA}(Z_T)$ for the 20% most central Au+Au data at 5<$p_{T}^{\gamma}$<7 GeV/c compared to predictions from an energy loss calculation.

$I_{AA}(Z_T)$ for the 20% most central Au+Au data at 7<$p_{T}^{\gamma}$<9 GeV/c compared to predictions from an energy loss calculation.

$I_{AA}(Z_T)$ for the 20% most central Au+Au data at 9<$p_{T}^{\gamma}$<12 GeV/c compared to predictions from an energy loss calculation.

$I_{AA}(Z_T)$ for the 20% most central Au+Au data at 12<$p_{T}^{\gamma}$<15 GeV/c compared to predictions from an energy loss calculation.

direct $\gamma$-hadron yields per trigger p+p at 5<$p_{T}^{\gamma}$<7 GeV/c.

direct $\gamma$-hadron yields per trigger p+p at 7<$p_{T}^{\gamma}$<9 GeV/c.

direct $\gamma$-hadron yields per trigger p+p at 9<$p_{T}^{\gamma}$<12 GeV/c.

direct $\gamma$-hadron yields per trigger p+p at 12<$p_{T}^{\gamma}$<15 GeV/c.

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.

Additional information containing number of events which were used to reconstruct the numvers matching to Figure 1 and 2.

Additional information containing number of events which were used to reconstruct the numvers matching to Figure 1 and 2.

Additional information containing number of events which were used to reconstruct the numvers matching to Figure 1 and 2.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Au+Au collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 62.4 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 22.5 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 22.5 GeV Cu+Cu collisions.

The uncorrected multiplicity distributions of charged hadrons with 0.2 < $p_T$ < 2.0 GeV/$c$ for 200 GeV $p$+$p$ collisions.

The mean from the NBD fit as a function of $N_{part}$ for 200 GeV Au+Au collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 62.4 GeV Au+Au collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 200 GeV Cu+Cu collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 62.4 GeV Cu+Cu collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The mean from the NBD fit as a function of $N_{part}$ for 22.5 GeV Cu+Cu collisions over the range 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of centrality for 200 GeV Au+Au collisions in the range 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 200 GeV Au+Au collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 62.4 GeV Au+Au collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 200 GeV Cu+Cu collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 62.4 GeV Cu+Cu collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Fluctuations expressed as the scaled variance as a function of $N_{part}$ for 22.5 GeV Cu+Cu collisions for 0.2 < $p_T$ < 2.0 GeV/$c$.

Scaled variance for 200 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Au+Au collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 200 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

Scaled variance for 62.4 GeV Cu+Cu collisions plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Au+Au collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 200 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The inverse of the parameter $k_{NBD}$ from the Negative Binomial Distribution fits for 62.4 GeV Cu+Cu collisions. The fluctuations are plotted as a function of $N_{part}$ for several $p_T$ ranges.

The scaled variance as a funciton of $N_{part}$ for 200 GeV Au+Au collisions in the range 0.2 < $p_T$ < 2.0 GeV/$c$.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

The correlation of the clan model parameters $\bar{n_c}$ and $\bar{N_c}$ for all of the collision species measured as a function of centrality.

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 $p_T$.

Per-trigger yield versus $\Delta\phi$ for various trigger and partner $p_T$ ($p^a_T \otimes p^b_T$), arranged by increasing pair proxy energy (sum of $p^a_T$ and $p^b_T$), in Au + Au collisions for 5-10 $\otimes$ 2-3, 4-5 $\otimes$ 4-5, 5-10 $\otimes$ 3-5, and 5-10 $\otimes$ 5-10 GeV/c.

RHS versus $p^b_T$ for p + p collisions for four trigger selections.

RHS versus $p^b_T$ for Au + Au collisions for four trigger selections.

RHS versus $N_{part}$ for 2-3 $\otimes$ 2-3 GeV/$c$. Shaded bars (brackets) represent $p_T$ -correlated uncertainties due to elliptic flow (ZYAM procedure). The most left point is from p+p.

Per-trigger yield $\Delta\phi$ distribution and corresponding fits for 2-3 $\otimes$ 2-3 GeV/c in 0-5% Au+Au collisions.

a) D versus centrality from FIT 1 and FIT2 for 2 - 3 GeV/$c$ bin. The error bars are the statistical errors; The shaded bars and brackets are the systematic errors due to $v_2$. b) The fraction of the shoulder Gaussian yield relative to the total away-side yield as function of centrality determined from FIT2.

Values of D determined from FIT1 as function of partner $p_T$ for 2-3 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT1 as function of partner $p_T$ for 3-4 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT1 as function of partner $p_T$ for 4-5 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT2 as function of partner $p_T$ for 2-3 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT2 as function of partner $p_T$ for 3-4 GeV/c $p_T$ range in 0-20% Au+Au.

Values of D determined from FIT2 as function of partner $p_T$ for 4-5 GeV/c $p_T$ range in 0-20% Au+Au.

Per-trigger yield as function of partner $p_T$ for the HR region for the 0-20% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the 20-40% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the 40-60% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the 60-92% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the HR region for the p + p collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 0-20% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 20-40% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 40-60% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the 60-92% Au + Au collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Per-trigger yield as function of partner $p_T$ for the SR region for the p + p collisions. Results for four trigger pT in 2-3, 3-4, 4-5, 5-10 GeV/c are shown.

Near-side Gaussian widths versus partner $p_T$ for four trigger $p_T$ ranges for 0-20 % Au + Au.

Near-side Gaussian widths versus partner $p_T$ for four trigger $p_T$ ranges for 0-20 % p + p.

Near-side Gaussian widths versus $N_{part}$ for five successively increasing $p^a_T$ $\otimes$ $p^b_T$. The most left point in each panel represents the value from p + p.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% p + p.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Near-side yield in $\lvert \Delta\phi \rvert$ < $\pi$/3 versus partner $p_T$ for four trigger $p_T$ selections for 0-20% Au + Au.

Per-trigger yield versus $\Delta\eta$ for 0-20% central Au + Au collisions. Results are shown for four $p^a_T \otimes p^b_T$ selections as indicated.

Per-trigger yield versus $\Delta\eta$ for 0-20% central p + p collisions. Results are shown for four $p^a_T \otimes p^b_T$ selections as indicated.

The projection of 2-D per-trigger yield in $\lvert \Delta\eta \rvert$ < 0.7 $\otimes$ $\lvert \Delta\phi \rvert$ < 0.7 and 0-20% central Au+Au collisions onto $\Delta\eta$ for four $p^a_T \otimes p^b_T$ selections.

The projection of 2-D per-trigger yield in $\lvert \Delta\eta \rvert$ < 0.7 $\otimes$ $\lvert \Delta\phi \rvert$ < 0.7 and 0-20% central Au+Au collisions onto $\Delta\phi$ for four $p^a_T \otimes p^b_T$ selections.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the head region for Au + Au for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the away-side shoulder region for Au + Au for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the near-side region for Au + Au for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the head region for p + p for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the away-side shoulder region for p + p for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, in 1 <pbT < 5 GeV/c versus centrality for the near-side region for p + p for four trigger $p_T$ bins.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 3-4 GeV/c.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 4-5 GeV/c.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 3-4 GeV/c.

Truncated mean $p_T$, $\langle p_T \rangle$, calculated for five partner pT ranges in the HR. Results for triggers in 4-5 GeV/c.

The near-side pair suppression factor $J_{AA}$ in 0-20% Au + Au collisions as function of $p^b_T$ for various ranges of $p^a_T$.

The near-side $J_{AA}$ as function of $p^b_T$ and $p^{sum}_T$ for four $p^a_T$ bins and three centrality bins. Data for 20-40%.

The near-side $J_{AA}$ as function of $p^b_T$ and $p^{sum}_T$ for four $p^a_T$ bins and three centrality bins. Data for 40-60%.

The near-side $J_{AA}$ as function of $p^b_T$ and $p^{sum}_T$ for four $p^a_T$ bins and three centrality bins. Data for 60-92%.

The pair suppression factor $J_{AA}$ for the away-side HR in 0-20% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

The pair suppression factor $J_{AA}$ for the away-side HR in 20-40% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

The pair suppression factor $J_{AA}$ for the away-side HR in 40-60% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

The pair suppression factor $J_{AA}$ for the away-side HR in 60-92% Au + Au collisions as function of $p_b^T$ for various ranges of $p_a^T$.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 0-20 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 20-40 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 40-60 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in 60-92 % Au + Au collisions.

Per-trigger yield versus $\Delta\phi$ for successively increasing trigger and partner $p_T$ ($p^a_T \otimes p^b_T$) in p + p collisions.

$\pi^0$ 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.