$\pi^0$ spectra from figure 2a from 40-60% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ spectra from figure 2a from 60-80% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 2b from minimum bias U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 2b from 0-20% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 2b from 20-40% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 2b from 40-60% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 2b from 60-80% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

Ratio of $\pi^0$ yield to the fit from figure 2c from minimum bias U+U collisions. Sys. uncertainties include B and C uncertainties from data points.

Ratio of $\pi^0$ yield to the fit from figure 2c from 0-20% U+U collisions. Sys. uncertainties include B and C uncertainties from data points.

Ratio of $\pi^0$ yield to the fit from figure 2c from 60-80% U+U collisions. Sys. uncertainties include B and C uncertainties from data points.

Ratio of $\eta$ yield to the fit from figure 2d from minimum bias U+U collisions. Sys. uncertainties include B and C uncertainties from data points.

Ratio of $\eta$ yield to the fit from figure 2d from 0-20% U+U collisions. Sys. uncertainties include B and C uncertainties from data points.

Ratio of $\eta$ yield to the fit from figure 2d from 40-60% U+U collisions. Sys. uncertainties include B and C uncertainties from data points.

$\eta/\pi^0$ ratio from figure 3 from minimum bias U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 3 from 0-20% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 3 from 20-40% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 3 from 40-60% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 3 from 60-80% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 3 from minimum bias Au+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\pi^0$ $R_{AA}$ from figure 4a from 0-20% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\eta$ $R_{AA}$ from figure 4a from 0-20% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\pi^0$ $R_{AA}$ from figure 4b from 20-40% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\eta$ $R_{AA}$ from figure 4b from 20-40% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\pi^0$ $R_{AA}$ from figure 4c from 40-60% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\eta$ $R_{AA}$ from figure 4c from 40-60% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\pi^0$ $R_{AA}$ from figure 4d from minimum bias U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\eta$ $R_{AA}$ from figure 4d from minimum bias U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\pi^0$ $R_{AA}$ from figure 5a from 0-20% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 2 set.

$\pi^0$ $R_{AA}$ from figure 5a from 0-5% Au+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AA}$ from figure 5a from 40-60% U+U collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 2 set.

$\pi^0$ $R_{AA}$ from figure 5a from 40-50% Au+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ integrated $R_{AA}$ for $p_T>5$ GeV/$c$ in U+U collisions as a function of centrality from figure 6a. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\eta$ integrated $R_{AA}$ for $p_T>5$ GeV/$c$ in U+U collisions as a function of centrality from figure 6a. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 1 set.

$\pi^0$ integrated $R_{AA}$ for $p_T>5$ GeV/$c$ in Au+Au collisions as a function of centrality from figure 6a. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ integrated $R_{AA}$ for $p_T>5$ GeV/$c$ in U+U collisions as a function of centrality from figure 6b. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data. Calculation is carried out for Glauber 2 set.

Number of participant nucleons of in dep U$+$U collisions

Number of participant nucleons of in dep U$+$U collisions

Number of participant nucleons of in dep Au$+$Au collisions

$\pi^0$ spectra from figure 3a from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ spectra from figure 3a from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ spectra from figure 3a from 40-60% semi-peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ spectra supplemental to figure 3a from 60-90% peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

Ratio of $\pi^0$ spectra from the PbSc to the combined spectra from figure 3b from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\pi^0$ spectra from the PbGl to the combined spectra from figure 3b from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\pi^0$ spectra from the PbSc to the combined spectra from figure 3c from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\pi^0$ spectra from the PbGl to the combined spectra from figure 3c from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\pi^0$ spectra from the PbSc to the combined spectra from figure 3d from 40-60% semi-peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\pi^0$ spectra from the PbGl to the combined spectra from figure 3d from 40-60% semi-peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

$\eta$ spectra from figure 3e from minimum bias Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 3e from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 3e from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra from figure 3e from 40-60% semi-peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ spectra supplemental to figure 3e from 60-90% peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

Ratio of $\eta$ spectra from the PbSc to the combined spectra from figure 3f from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\eta$ spectra from the PbGl to the combined spectra from figure 3f from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\eta$ spectra from the PbSc to the combined spectra from figure 3g from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\eta$ spectra from the PbGl to the combined spectra from figure 3g from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\eta$ spectra from the PbSc to the combined spectra from figure 3h from 40-60% semi-peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

Ratio of $\eta$ spectra from the PbGl to the combined spectra from figure 3h from 40-60% semi-peripheral Au+Cu collisions. Type A uncertainties are uncorrelated point-to-point. Systematic noncorr. uncertainties are uncorrelated between PbSc and PbGl subsystems.

$\eta/\pi^0$ ratio from figure 4 from minimum bias Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 4 from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 4 from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio from figure 4 from 40-60% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\eta/\pi^0$ ratio supplemental to figure 4 from 60-90% peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point.

$\pi^0$ $R_{AB}$ from figure 5a from 0-10% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ from figure 5b from 10-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ from figure 5c from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ $R_{AB}$ from figure 5a from 0-20% central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ from figure 5d from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ $R_{AB}$ from figure 5b from 20-40% semi-central Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ from figure 5e from 40-60% semi-peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ $R_{AB}$ from figure 5c from 40-60% semi-peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ from figure 5f from minimum bias Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ $R_{AB}$ from figure 5f from minimum bias Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ supplemental to figure 5 from 60-90% peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\eta$ $R_{AB}$ supplemental to figure 5 from 60-90% peripheral Cu+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ supplemental to figure 6a from 20-30% central Au+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ supplemental to figure 6b from 0-10% central Cu+Cu collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ $R_{AB}$ supplemental to figure 6b from 40-50% semi-central Au+Au collisions. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ for $p_T>5$ GeV/$c$ in Cu+Au collisions as a function of centrality from figure 7a. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ for $p_T>5$ GeV/$c$ in Au+Au collisions as a function of centrality from figure 7a. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ for $p_T>10$ GeV/$c$ in Cu+Au collisions as a function of centrality from figure 7b. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

$\pi^0$ for $p_T>10$ GeV/$c$ in Au+Au collisions as a function of centrality from figure 7b. Type A uncertainties are uncorrelated point-to-point. Type B uncertainties are correlated point-to-point. Type C uncertainties affect the scale of the data.

Multiplicity in Au+Au collisions at $\sqrt{s_{NN}}$ = 130 GeV

Transverse energy in Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Multiplicity in Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Transverse energy in Au+Au collisions at $\sqrt{s_{NN}}$ = 39 GeV

Multiplicity in Au+Au collisions at $\sqrt{s_{NN}}$ = 39 GeV

Transverse energy in Au+Au collisions at $\sqrt{s_{NN}}$ = 27 GeV

Multiplicity in Au+Au collisions at $\sqrt{s_{NN}}$ = 27 GeV

Transverse energy in Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV

Multiplicity in Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV

Transverse energy in Au+Au collisions at $\sqrt{s_{NN}}$ = 14.5 GeV

Multiplicity in Au+Au collisions at $\sqrt{s_{NN}}$ = 14.5 GeV

Transverse energy in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 GeV

Multiplicity in Au+Au collisions at $\sqrt{s_{NN}}$ = 7.7 GeV

Transverse energy in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

Multiplicity in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

Transverse energy in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Multiplicity in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Transverse energy in Cu+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

Multiplicity in Cu+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

Transverse energy in U+U collisions at $\sqrt{s_{NN}}$ = 193 GeV

Multiplicity in U+U collisions at $\sqrt{s_{NN}}$ = 193 GeV

Transverse energy in d+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

Multiplicity in d+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

Transverse energy in He+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

Multiplicity in He+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

$\pi^0$ meson $v_4, 20-40\%$ centrality

$\pi^0$ meson $v_4, 40-60\%$ centrality

$\pi^0$ meson $v_4, 20-60\%$ centrality

$\pi^0$ meson $v_4/v_2^2, 0-20\%$ centrality

$\pi^0$ meson $v_4/v_2^2, 20-40\%$ centrality

$\pi^0$ meson $v_4/v_2^2, 40-60\%$ centrality

$\pi^0$ meson $v_4/v_2^2, 20-60\%$ centrality

$\Eta/ \pi^0 ratios

$\pi^0$ nuclear modification factors

$\pi^0$ nuclear modification factors

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 0^{\circ}-15^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 0^{\circ}-15^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 15^{\circ}-30^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 15^{\circ}-30^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 30^{\circ}-45^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 30^{\circ}-45^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 45^{\circ}-60^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 45^{\circ}-60^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 60^{\circ}-75^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 60^{\circ}-75^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 75^{\circ}-90^{\circ}$

$pi^0$ nuclear modification factors vs reaction plane, $\Delta \phi = 75^{\circ}-90^{\circ}$

Centrality dependence of $p_T$ ingetrated $R_{AA}(\Delta \phi)$

Centrality dependence of $p_T$ ingetrated $R_{AA}(\Delta \phi)$

INVARIANT YIELDS

RAA

RAA

RAA

RAA

pT AVERAGE RAA

Sloss

Sloss

Sloss

n_eff(xT)

n_eff(xT)

n_eff(xT)

n_eff(xT)

Data for the number of reconstructed photon conversions as a function of conversion location plots

Corrected photon spectra, pT

Corrected photon spectra, y

Data for the two-photon invariant mass plots

π0 transverse momentum spectra

π0 contribution in the photon spectra spectra

Rapidity distributions of the fiducial yields and integrated $<p_{\perp}>$ for the $0-5\%$ and $70-80\%$ Au+Au collisions. Pion yields are scaled down by a factor of 5. Errors shown are those propagated from Fig.1. Systematic errors on the fiducial yields are $5\%$; those on $<p_{\perp}>$ are $5\%$ for pions and $5-10\%$ for kaons and antiprotons.

Rapidity distributions of the fiducial yields and integrated $<p_{\perp}>$ for the $0-5\%$ and $70-80\%$ Au+Au collisions. Pion yields are scaled down by a factor of 5. Errors shown are those propagated from Fig.1. Systematic errors on the fiducial yields are $5\%$; those on $<p_{\perp}>$ are $5\%$ for pions and $5-10\%$ for kaons and antiprotons.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

Mean transverse momentum of negative particles and (b) $K^-/\pi^-$ and $\bar{p}/\pi^-$ ratios as function of the charged hadron multiplicity. Open symbols are for pp, and filled ones are for Au+Au data. (c) Mid-rapidity $K^-/\pi^-$ ratio as function of $\frac{(dN/dy)_{\pi}}{S}$. Systematic errors are shown for STAR data, and statistical errors for other data.

$\frac{(dN/dy)_{\pi}}{S}$ (stars), $T_{ch}$ (circles) and $T_{kin}$ (triangles) and (b) $<\beta>$ as a function of the charged hadron multiplicity. Errors are systematic.

$\frac{(dN/dy)_{\pi}}{S}$ (stars), $T_{ch}$ (circles) and $T_{kin}$ (triangles) and (b) $<\beta>$ as a function of the charged hadron multiplicity. Errors are systematic.

The ratios Anti-Λ/Λ, K+/K-, and Anti-Ξ+/Ξ- as a function of pT

Anti-baryon to baryon ratios measured by STAR

The mid-rapidity kaon multiplicity densities ($dN/dy$) and mT exponential inverse slopes (T in MeV) as a function of negative hadron multiplicity with $|η|<0.5$ ($dNh-/dη$). Quoted errors are uncorrelated errors (first) and correlated systematic errors (second). Systematic error on $dNh-/dη$ is $7\%$.

The mid-rapidity kaon multiplicity densities ($dN/dy$) and mT exponential inverse slopes (T in MeV) as a function of negative hadron multiplicity with $|η|<0.5$ ($dNh-/dη$). Quoted errors are uncorrelated errors (first) and correlated systematic errors (second). Systematic error on $dNh-/dη$ is $7\%$.

Central 0-6% K/π yield ratios.