Integrated away-side $\gamma_{dir}$-h per-trigger $I_{AA}$ and $I_{dA}$ of Au+Au, d+Au, and p+p, as a function of $\xi$.

$I_{AA}$ vs $\xi$ for direct photon $p_{T}^{\gamma}$ of 5-7 GeV/$c$, 7-9 GeV/$c$, and 9-12 GeV/$c$.

$I_{AA}$ vs $\xi$ for direct photon $p_{T}^{\gamma}$ of 5-7 GeV/$c$, 7-9 GeV/$c$, and 9-12 GeV/$c$.

$I_{AA}$ vs $\xi$ for direct photon $p_{T}^{\gamma}$ of 5-7 GeV/$c$, 7-9 GeV/$c$, and 9-12 GeV/$c$.

$I_{AA}$ as a function of $\xi$ for direct photon $p_{T}^{\gamma}$ of 5-7, 7-9, and 9-12 GeV/$c$. Three away-side integration ranges are chosen to calculate the per-trigger yield and the corresponding $I_{AA}$, $|\Delta\phi-\pi|<\pi/2$, $|\Delta\phi-\pi|<\pi/3$, and $|\Delta\phi-\pi|<\pi/6$.

$I_{AA}$ as a function of $\xi$ for direct photon $p_{T}^{\gamma}$ of 5-7, 7-9, and 9-12 GeV/$c$. Three away-side integration ranges are chosen to calculate the per-trigger yield and the corresponding $I_{AA}$, $|\Delta\phi-\pi|<\pi/2$, $|\Delta\phi-\pi|<\pi/3$, and $|\Delta\phi-\pi|<\pi/6$.

$I_{AA}$ as a function of $\xi$ for direct photon $p_{T}^{\gamma}$ of 5-7, 7-9, and 9-12 GeV/$c$. Three away-side integration ranges are chosen to calculate the per-trigger yield and the corresponding $I_{AA}$, $|\Delta\phi-\pi|<\pi/2$, $|\Delta\phi-\pi|<\pi/3$, and $|\Delta\phi-\pi|<\pi/6$.

Ratios of $I_{AA}$ as a function of direct photon $p_T$ for three different away-side integration ranges.

Measured $I_{AA}$ for direct photon $p_T$ of 5-7, 7-9, and 9-12 GeV/$c$, as a function of $\xi$, are compared with theoretical model calculations.

Measured $I_{AA}$ for direct photon $p_T$ of 5-7, 7-9, and 9-12 GeV/$c$, as a function of $\xi$, are compared with theoretical model calculations.

Measured $I_{AA}$ for direct photon $p_T$ of 5-7, 7-9, and 9-12 GeV/$c$, as a function of $\xi$, are compared with theoretical model calculations.

Nuclear modification factors Rcp for $\pi^{+}$ + $\pi^{-}$ and p + $\bar{p}$ in 200 GeV AuAu collisions.

Nuclear modification factors Rcp for $\pi^{+}$ + $\pi^{-}$ and p + $\bar{p}$ in 200 GeV AuAu collisions.

Nuclear modification factors Rcp for $\pi^{+}$ + $\pi^{-}$ and p + $\bar{p}$ in 200 GeV AuAu collisions.

The $\pi^{-}$/$\pi{+}$ and $\bar{p}$/p ratios in 12 $\%$ central, MB Au+Au and d+Au collisions at $\sqrt{s}_{NN}$ = 200 GeV. Errors are statistical and point-to-point systematic.

The p/$\pi^{+}$ and $\bar{p}$/$\pi^{-}$ ratios from d+Au and Au+Au collisions at $\sqrt{s}_{NN}$ = 200 GeV. The systematic uncertainties for 60-80$\%$ Au+Au collisions are similar.

$E\frac{dN^3}{dp^3}$ 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

Integrated per-trigger yields as a function of associated particle angle relative to $\psi_2$ event plane $\phi^a - \psi_2$ integrated over the near side $|\Delta\phi|<\pi/4$.

Integrated per-trigger yields as a function of associated particle angle relative to $\psi_2$ event plane $\phi^a - \psi_2$ integrated over the away side $|\Delta\phi|<\pi/4$.

Integrated per-trigger yields as a function of associated particle angle relative to $\psi_2$ event plane for near-side $|\Delta\phi|<\pi/4$ and for away-side $|\Delta\phi|<\pi/4$.

Integrated per-trigger yields as a function of associated particle angle relative to $\psi_2$ event plane for near-side $|\Delta\phi|<\pi/4$ and for away-side $|\Delta\phi|<\pi/4$.

Per-trigger yields $Y(\Delta\phi)$ of dihadrons pairs measured in Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200~{\rm GeV}$ after subtracting the underlying event model with several $p_T$ selections. Systematic uncertainties due to track matching are given.

Per-trigger yields $Y(\Delta\phi)$ of dihadrons pairs measured in Au$+$Au collisions at $\sqrt{s_{_{NN}}}=200~{\rm GeV}$ after subtracting the underlying event model with several $p_T$ selections. Systematic uncertainties due to track matching are given.

$\Psi_{2}$-dependent $C(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $1<p_{T}^{assoc}<2$ GeV/c.

$\Psi_{2}$-dependent $C(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $2<p_{T}^{assoc}<4$ GeV/c.

$\Psi_{2}$-dependent $C(\Delta\phi)$ for $4<p_{T}^{trig}<10$ GeV/c and $2<p_{T}^{assoc}<4$ GeV/c.

$\Psi_{3}$-dependent $C(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $1<p_{T}^{assoc}<2$ GeV/c.

$\Psi_{3}$-dependent $C(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $2<p_{T}^{assoc}<4$ GeV/c.

$\Psi_{3}$-dependent $C(\Delta\phi)$ for $4<p_{T}^{trig}<10$ GeV/c and $1<p_{T}^{assoc}<2$ GeV/c.

$\Psi_{2}$-dependent $Y(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $1<p_{T}^{assoc}<2$ GeV/c.

$\Psi_{2}$-dependent $C(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $2<p_{T}^{assoc}<4$ GeV/c.

$\Psi_{2}$-dependent $C(\Delta\phi)$ for $4<p_{T}^{trig}<10$ GeV/c and $2<p_{T}^{assoc}<4$ GeV/c.

$\Psi_{3}$-dependent $C(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $1<p_{T}^{assoc}<2$ GeV/c.

$\Psi_{3}$-dependent $C(\Delta\phi)$ for $2<p_{T}^{trig}<4$ GeV/c and $2<p_{T}^{assoc}<4$ GeV/c.

$\Psi_{3}$-dependent $C(\Delta\phi)$ for $4<p_{T}^{trig}<10$ GeV/c and $2<p_{T}^{assoc}<4$ GeV/c.

$\Psi_2$-dependent C for 2 $< p_T^t <$ 4 and 1 $< p_T^a <$ 2 GeV/c.

$\Psi_2$-dependent C for 2 $< p_T^t <$ 4 and 2 $< p_T^a <$ 4 GeV/c.

$\Psi_2$-dependent C for 4 $< p_T^t <$ 10 and 2 $< p_T^a <$ 4 GeV/c.

$\Psi_2$-dependent Y for 2 $< p_T^t <$ 4 and 1 $< p_T^a <$ 2 GeV/c.

$\Psi_2$-dependent Y for 2 $< p_T^t <$ 4 and 2 $< p_T^a <$ 4 GeV/c.

$\Psi_2$-dependent Y for 4 $< p_T^t <$ 10 and 2 $< p_T^a <$ 4 GeV/c.

$\Psi_3$-dependent C for 2 $< p_T^t <$ 4 and 1 $< p_T^a <$ 2 GeV/c.

$\Psi_3$-dependent C for 2 $< p_T^t <$ 4 and 2 $< p_T^a <$ 4 GeV/c.

$\Psi_3$-dependent C for 4 $< p_T^t <$ 10 and 2 $< p_T^a <$ 4 GeV/c.

$\Psi_3$-dependent Y for 2 $< p_T^t <$ 4 and 1 $< p_T^a <$ 2 GeV/c.

$\Psi_3$-dependent Y for 2 $< p_T^t <$ 4 and 2 $< p_T^a <$ 4 GeV/c.

$\Psi_3$-dependent Y for 4 $< p_T^t <$ 10 and 2 $< p_T^a <$ 4 GeV/c.

Identified hadron $v_2$ in midcentral (20–60%, right panels) Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. Panels (a) and (b) show $v_2$ as a function of transverse momentum $p_T$. The $v_2$ of all species for centrality 0–20% has been scaled up by a factor of 1.6 for better comparison with results of 20–60% centrality. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

Identified hadron $v_2$ in midcentral (20–60%, right panels) Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. Panels (a) and (b) show $v_2$ as a function of transverse momentum $p_T$. The $v_2$ of all species for centrality 0–20% has been scaled up by a factor of 1.6 for better comparison with results of 20–60% centrality. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

Identified hadron $v_2$ in midcentral (20–60%, right panels) Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. Panels (a) and (b) show $v_2$ as a function of transverse momentum $p_T$. The $v_2$ of all species for centrality 0–20% has been scaled up by a factor of 1.6 for better comparison with results of 20–60% centrality. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 0–10% centrality [panel (a)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 0–10% centrality [panel (a)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 0–10% centrality [panel (a)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 10–20% centrality [panel (b)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 10–20% centrality [panel (b)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 10–20% centrality [panel (b)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 20–40% centrality [panel (c)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 20–40% centrality [panel (c)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 20–40% centrality [panel (c)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 40–60% centrality [panel (d)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 40–60% centrality [panel (d)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 40–60% centrality [panel (d)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The error bars (shaded boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 10–40% centrality [panel (b)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The $v_2$ of $\Lambda$ and K$^0_S$ are measured by STAR collaboration [21]. The error bars (open boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown on the results from this study are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 10–40% centrality [panel (b)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The $v_2$ of $\Lambda$ and K$^0_S$ are measured by STAR collaboration [21]. The error bars (open boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown on the results from this study are type A and B only.

The quark-number-scaled $v_2$ ($v_2/n_q$) of identified hadrons are shown as a function of the kinetic energy per quark, KE$_T/n_q$ in 10–40% centrality [panel (b)] in Au + Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The $v_2$ of $\Lambda$ and K$^0_S$ are measured by STAR collaboration [21]. The error bars (open boxes) represent the statistical (systematic) uncertainties. The systematic uncertainties shown on the results from this study are type A and B only.

Transverse single-spin asymmetry of $J/\psi$ mesons plotted against $J/\psi$ transverse momentum. Systematic uncertainties $\delta$$A^f_N$ Type B and $\delta$$A^P_N$ Type B are due to the geometric scale factor and the polarization, respectively.

Transverse single-spin asymmetry of $J/\psi$ mesons plotted against $J/\psi$ transverse momentum. Systematic uncertainties $\delta$$A^f_N$ Type B and $\delta$$A^P_N$ Type B are due to the geometric scale factor and the polarization, respectively.

Transverse single-spin asymmetry of $J/\psi$ mesons plotted against $J/\psi$ transverse momentum. Systematic uncertainties $\delta$$A^f_N$ Type B and $\delta$$A^P_N$ Type B are due to the geometric scale factor and the polarization, respectively.

$J/\psi$ $R_{CP}$ for 0-20%, 20-40%, and 40-60% (central) relative to 60-86% (peripheral) Au+Au collisions at 62.4 GeV. Type A errors are point-to-point uncorrelated, Type B errors are point-to-point correlated, and Type C are global systematic from the uncertainty in the peripheral $<N_{coll}>$ value.

$J/\psi$ $R_{CP}$ for 0-40% (central) relative to 40-86% (peripheral) Au+Au collisions at 39 GeV. Type A errors are point-to-point uncorrelated, Type B errors are point-to-point correlated, and Type C are global systematic from the uncertainty in the peripheral $<N_{coll}>$ value.

$J/\psi$ $R_{AA}$ at $\sqrt{s_{NN}}$ = 39 and 62.4 GeV. Type A errors are point-to-point uncorrelated, Type B errors are point-to-point correlated, and Type C are global systematic from the uncertainty in the peripheral $<N_{coll}>$ value.

$J/\psi$ $R_{AA}$ at $\sqrt{s_{NN}}$ = 39 and 62.4 GeV.

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.