c$\bar{c}$ production cross section as a function of rapidity in $p$+$p$ collisions, measured using semileptonic decay to electrons (closed square) and to muons (closed circle).

Transverse momentum distribution of $R_{AA}$ for negative muons from heavy-flavor mesons decay in Cu+Cu collisions in the following centrality classes: 40-94% (top panel), 20-40% (middle panel) and 0-20% (bottom panel). Also shown in the bottom panel is a theoretical calculation from [39,40], discussed in Section V.

Comparison of $R_{AA}$ as a function of $N_{part}$ between heavy-flavor muons reconstructed at forward rapidity ($1.4<y<1.9$) and $p_T >$ 2 GeV in Cu+Cu collisions (red squares) and nonphotonic electrons reconstructed at midrapidity and $p_T>$ 3 GeV in Au+Au collisions (blue circles).

Comparison of $R_{AA}$ as a function of $N_{part}$ between heavy-flavor muons reconstructed at forward rapidity ($1.4<y<1.9$) and $p_T >$ 2 GeV in Cu+Cu collisions (red squares) and nonphotonic electrons reconstructed at midrapidity and $p_T>$ 3 GeV in Au+Au collisions (blue circles).

Invariant transverse momentum spectra of $\omega$ production in $p$+$p$ and $d$+Au collisions at $\sqrt{s}$=200 GeV.

Invariant transverse momentum spectra of $\omega$ production in $p$+$p$ and $d$+Au collisions at $\sqrt{s}$=200 GeV.

Invariant transverse momentum spectra of $\omega$ production in Cu+Cu (left) and Au+Au (right) collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel for three centrality bins and minimum bias.

Invariant transverse momentum spectra of $\omega$ production in Cu+Cu (left) and Au+Au (right) collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel for three centrality bins and minimum bias.

Invariant transverse momentum spectra of $\omega$ production in Cu+Cu (left) and Au+Au (right) collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel for three centrality bins and minimum bias.

Invariant transverse momentum spectra of $\omega$ production in Cu+Cu (left) and Au+Au (right) collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel for three centrality bins and minimum bias.

Invariant transverse momentum spectra of $\omega$ production in Cu+Cu (left) and Au+Au (right) collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel for three centrality bins and minimum bias.

Invariant transverse momentum spectra of $\omega$ production in Cu+Cu (left) and Au+Au (right) collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel for three centrality bins and minimum bias.

Measured ${\omega}/{\pi}$ ratio as a function of $p_T$ in $p$ + $p$ collisions at $\sqrt{s}$=200 GeV.

Measured ${\omega}/{\pi}$ ratio as a function of $p_T$ in $p$ + $p$ collisions at $\sqrt{s}$=200 GeV.

Measured ${\omega}/{\pi}$ ratio as a function of $p_T$ in $p$ + $p$ collisions at $\sqrt{s}$=200 GeV.

${\omega}/{\pi}$ ratio versus transverse momentum in $d$+Au (0–88%) for $\omega \rightarrow {e}^{+}{e}^{-}$.

${\omega}/{\pi}$ ratio versus transverse momentum in $d$+Au (0–88%) for $\omega \rightarrow {\pi}^{+}{\pi}^{-}\pi^0$.

${\omega}/{\pi}$ ratio versus transverse momentum in $d$+Au (0–88%) for $\omega \rightarrow {\pi}^{0}\gamma$.

${\omega}/{\pi}$ ratio versus transverse momentum in Cu+Cu (0–94%) for $\omega \rightarrow {\pi}^{0}\gamma$.

${\omega}/{\pi}$ ratio versus transverse momentum in Au+Au (0–92%) for $\omega \rightarrow {\pi}^{0}\gamma$.

${\omega}/{\pi}$ ratio versus transverse momentum in Au+Au (0–92%) for $\omega \rightarrow {\pi}^{0}\gamma$.

Nuclear modification factor, RdAu, measured for the ${R}_{dAu}$ in 0–88, 0–20, 20-40, and 40-60% centrality bins in $d$+Au collisions at $\sqrt{s}$=200 GeV.

Nuclear modification factor, RdAu, measured for the ${R}_{dAu}$ in 60–88% centrality bins in $d$+Au collisions at $\sqrt{s}$=200 GeV.

Nuclear modification factor, RdAu, measured for the ${R}_{dAu}$ in 0–88, 20-40, and 40–60% centrality bins in $d$+Au collisions at $\sqrt{s}$=200 GeV.

Nuclear modification factor, RdAu, measured for the ${R}_{dAu}$ in 0–20 and 60–88% centrality bins in $d$+Au collisions at $\sqrt{s}$=200 GeV.

Nuclear modification factor, RdAu, measured for the ${R}_{dAu}$ in 0–88, 0–20, 20-40, 40-60, and 60–88% centrality bins in $d$+Au collisions at $\sqrt{s}$=200 GeV.

$R_{AA}$ of the $\omega$ in Cu+Cu collisions from the $\omega \rightarrow \pi^0\gamma$ decay channel.

$R_{AA}$ of the $\omega$ in Au+Au collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel.

$R_{AA}$ of the $\omega$ in Au+Au collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel.

$R_{AA}$ of the $\omega$ in Au+Au collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel.

$R_{AA}$ of the $\omega$ in Au+Au collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel.

$R_{AA}$ of the $\omega$ in and Au+Au collisions from the $\omega \rightarrow \pi^0 \gamma$ decay channel.

($R_{AA}$) of the $\omega \rightarrow \pi^+\pi^-\pi^0$ collision for the $\omega$ meson integrated over the range $p_T$ > 7 $\mathrm{GeV}$/$c$ as a function of the number participating nucleons ($N_{part}$).

($R_{AA}$) of the $\omega \rightarrow \pi^0 \gamma$ collision for the $\omega$ meson integrated over the range $p_T$ > 7 $\mathrm{GeV}$/$c$ as a function of the number participating nucleons ($N_{part}$).

$R_{AA}$ of the $\omega \rightarrow \pi^0 \gamma$ collision for the $\omega$ meson integrated over the range $p_T$ > 7 $\mathrm{GeV}$/$c$ as a function of the number participating nucleons ($N_{part}$).

Parameters of the Tsallis fit with parameter $n$ constrained to a fixed linear dependence on mass (for mesons). Cross sections are in $\mu$b for $J/\psi$ and $\psi^{\prime}$ and in mb for all other particles.

Constant and linear fits to the Tsallis parameter $T$ of mesons with fixed parameter $n$. The last column (Prob.) gives the probability estimated by the $\chi^2$/$n.d.f.$ of the fit.

Parameters of the Tsallis fit with Eq. 8 in the paper with parameters $n$ and $T$ constrained to have a fixed linear dependence on mass (for mesons). Cross sections are in $\mu$b for $J/\psi$ and $\psi^{\prime}$ and in mb for all other particles.

Cross sections in mb and $<p_T>$ in GeV/$c$ of different particles in $p$+$p$ collisions at $\sqrt{s}$ = 200 GeV. PHENIX columns show the values obtained by fits to the experiment spectra with the Tsallis functional form as described in the text. One should state explicitly that these values do not supersede values given in the ”Published” column by the experiments, in their publications listed in the last column, or elsewhere. An additional 9.7% systematic uncertainty should be added to all $d\sigma$/$dy$ values listed in the column “PHENIX” to account for the trigger uncertainties. Values in the column “Published” are also given without these systematic uncertainties. The column “S.M.” is the prediction of the statistical model discussed in the text. The characteristic widths of the particle spectra are $\langle p_T \rangle$ for all species except for $J/\psi$ and $\psi^{\prime}$ for which the values given in the Table are $\langle p_T^2 \rangle$. For $\psi^{\prime}$ the integration is done in the $p_T$ regionbelow 5 GeV/$c$. All errors are the combined statistical and systematic uncertainties.

Cross sections in mb and $<p_T>$ in GeV/$c$ of different particles in $p$+$p$ collisions at $\sqrt{s}$ = 200 GeV. PHENIX columns show the values obtained by fits to the experiment spectra with the Tsallis functional form as described in the text. One should state explicitly that these values do not supersede values given in the ”Published” column by the experiments, in their publications listed in the last column, or elsewhere. An additional 9.7% systematic uncertainty should be added to all $d\sigma$/$dy$ values listed in the column “PHENIX” to account for the trigger uncertainties. Values in the column “Published” are also given without these systematic uncertainties. The column “S.M.” is the prediction of the statistical model discussed in the text. The characteristic widths of the particle spectra are $\langle p_T \rangle$ for all species except for $J/\psi$ and $\psi^{\prime}$ for which the values given in the Table are $\langle p_T^2 \rangle$. For $\psi^{\prime}$ the integration is done in the $p_T$ regionbelow 5 GeV/$c$. All errors are the combined statistical and systematic uncertainties.

The invariant differential cross section ${d^2 \sigma}$/${2\pi p_T dy p_T}$ of $\omega$ meson production measured in the indicated decay channel. Type A uncertainties are $p_T$ independent. Type C & B systematic uncertainties are residual with Type B having an unknown $p_T$ dependence. For each $y$-coordinate in each $p_T$ bin was varied by the same amount according to the uncertainty Type C.

The invariant differential cross section ${d^2 \sigma}$/${2\pi p_T dy p_T}$ of $\omega$ meson production measured in the indicated decay channel. Type A uncertainties are $p_T$ independent. Type C & B systematic uncertainties are residual with Type B having an unknown $p_T$ dependence. For each $y$-coordinate in each $p_T$ bin was varied by the same amount according to the uncertainty Type C.

The invariant differential cross section ${d^2 \sigma}$/${2\pi p_T dy p_T}$ of $\omega$ meson production measured in the indicated decay channel. Type A uncertainties are $p_T$ independent. Type C & B systematic uncertainties are residual with Type B having an unknown $p_T$ dependence. For each $y$-coordinate in each $p_T$ bin was varied by the same amount according to the uncertainty Type C.

The invariant differential cross section ${d^2 \sigma}$/${2\pi p_T dy p_T}$ of $\omega$ meson production measured in the indicated decay channel. Type A uncertainties are $p_T$ independent. Type C & B systematic uncertainties are residual with Type B having an unknown $p_T$ dependence. For each $y$-coordinate in each $p_T$ bin was varied by the same amount according to the uncertainty Type C.

The invariant differential cross section ${d^2 \sigma}$/${2\pi p_T dy p_T}$ of $\omega$ meson production measured in the indicated decay channel. Type A uncertainties are $p_T$ independent. Type C & B systematic uncertainties are residual with Type B having an unknown $p_T$ dependence. For each $y$-coordinate in each $p_T$ bin was varied by the same amount according to the uncertainty Type C.

The invariant differential cross section ${d^2 \sigma}$/${2\pi p_T dy p_T}$ of $\omega$ meson production measured in the indicated decay channel. Type A uncertainties are $p_T$ independent. Type C & B systematic uncertainties are residual with Type B having an unknown $p_T$ dependence. For each $y$-coordinate in each $p_T$ bin was varied by the same amount according to the uncertainty Type C.

The invariant differential cross section ${d^2 \sigma}$/${2\pi p_T dy p_T}$ of $\omega$ meson production measured in the indicated decay channel. Type A uncertainties are $p_T$ independent. Type C & B systematic uncertainties are residual with Type B having an unknown $p_T$ dependence. For each $y$-coordinate in each $p_T$ bin was varied by the same amount according to the uncertainty Type C.

Differential invariant yield of electrons (($N_{e^+}$+$N_{e^-}$)/2) from heavy-flavor decays for different centrality classes.

Differential invariant yield of electrons (($N_{e^+}$+$N_{e^-}$)/2) from heavy-flavor decays for different centrality classes.

Differential invariant yield of electrons (($N_{e^+}$+$N_{e^-}$)/2) from heavy-flavor decays for different centrality classes.

Differential invariant yield of electrons (($N_{e^+}$+$N_{e^-}$)/2) from heavy-flavor decays for different centrality classes.

$R_{AuAu}(p^e_T)$ for different centrality classes.

$R_{AuAu}(p^e_T)$ for different centrality classes.

$R_{AuAu}(p^e_T)$ for different centrality classes.

$p^e_T$-integrated nuclear modification factors $R_{AuAu}$.

Nonphotonic electron $v_2$ as a function of $p_T$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

$R_{AA}$ for $\phi$ integrated at $p_T$ > 2.2 GeV/$c$ in Cu+Cu and Au+Au collisions vs. $N_{part}$. The global uncertainty related to the $p$+$p$ reference normalization is shown as a box on the right in the figure from the paper.

$R_{AA}$ for $\phi$ integrated at $p_T$ > 2.2 GeV/$c$ in Cu+Cu and Au+Au collisions vs. $N_{part}$. The global uncertainty related to the $p$+$p$ reference normalization is shown as a box on the right in the figure from the paper.

$R_{dA}$ vs. $p_T$ for $\phi$, $\pi^0$, and ($p$+$\bar{p}$) for 0-20% centrality $d$+Au collisions, and $R_{dA}$ vs. $p_T$ for $\phi$, $\pi^0$, and ($p$+$\bar{p}$) for 60-88% peripheral $d$+Au collisions. The global uncertainty of ~ 10% related to the $p$+$p$ reference normalization is not shown.

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 $p_T$.

$I_{AA}$ 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.