Differential cross sections of the Y(2S) meson as a function of pT for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of pT for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of pT for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Differential cross sections of the Y(1S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(1S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(2S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(2S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(3S) meson as a function of rapidity for pp collisions. The global uncertainty arises from the integrated luminosity uncertainty in pp collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(1S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(2S) meson as a function of pT for PbPb collisions. Global uncertainties arise from the number of minimum bias events and TAA uncertainties for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Differential cross sections of the Y(3S) meson as a function of pT for PbPb collisions.

Nuclear modification factor of the Y(1S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(1S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of pT. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(3S) meson as a function of pT.

Nuclear modification factor of the Y(3S) meson as a function of pT.

Nuclear modification factor of the Y(1S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(1S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(2S) meson as a function of rapidity. Global uncertainty combines the uncertainties from TAA, pp luminosity, and number of minimum bias events in PbPb collisions.

Nuclear modification factor of the Y(3S) meson as a function of rapidity.

Nuclear modification factor of the Y(3S) meson as a function of rapidity.

Nuclear modification factor of the Y(1S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(1S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(1S) state.

Nuclear modification factor of the Y(1S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(1S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(1S) state.

Nuclear modification factor of the Y(2S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(2S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(2S) state.

Nuclear modification factor of the Y(2S) meson as a function of collision centrality. Global uncertainty combines the pp luminosity and number of minimum bias events in PbPb collisions. The PP Y(2S) global uncertainty consists of the statistical and systematic uncertainties of pp yield for Y(2S) state.

Confidence intervals on the nuclear modification factors of the Y(3S) mesons as a function of collision centrality.

Confidence intervals on the nuclear modification factors of the Y(3S) mesons as a function of collision centrality.

Confidence intervals on the nuclear modification factors of the Y(2S) mesons as a function of collision centrality.

Confidence intervals on the nuclear modification factors of the Y(2S) mesons as a function of collision centrality.

Nuclear modification factors of the Y(1S) and Y(2S) mesons in the integrated pT, rapidity and centrality.

Nuclear modification factors of the Y(1S) and Y(2S) mesons in the integrated pT, rapidity and centrality.

MG/PTJET for SD (0.5,1.5) in PP collision

MG/PTJET for SD (0.1,0.0) in PbPb collision and PP collision smeared for PTJET 160-180

Ratio of MG/PTJET for SD (0.1,0.0) between PbPb collision and PP collision smeared for PTJET 160-180

MG/PTJET for SD (0.5,1.5) in PbPb collision and PP collision smeared for PTJET 160-180

Ratio of MG/PTJET for SD (0.5,1.5) between PbPb collision and PP collision smeared for PTJET 160-180

MG/PTJET for SD (0.1,0.0) in PbPb collision and PP collision smeared for centrality class 0-10%

Ratio of MG/PTJET for SD (0.1,0.0) between PbPb collision and PP collision smeared for centrality class 0-10%

MG/PTJET for SD (0.5,1.5) in PbPb collision and PP collision smeared for centrality class 0-10%

Ratio of MG/PTJET for SD (0.5,1.5) between PbPb collision and PP collision smeared for centrality class 0-10%

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV.

The ratio of pPb to pp $\eta_{\mathrm{dijet}}$ spectra for dijets in the range $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV.

The ratio of theory to data, for the ratio of the pPb to pp $\eta_{\mathrm{dijet}}$ spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV. The total uncertainties on the data points are provided in the column entitled 'DATA UNCERTAINTIES'. The theory points are from the NLO pQCD calculations of DSSZ, EPS09, nCTEQ15, and EPPS16 nPDFs, using CT14 as the baseline PDF.

The ratio of theory to data, for the ratio of the pPb to pp $\eta_{\mathrm{dijet}}$ spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV. The total uncertainties on the data points are provided in the column entitled 'DATA UNCERTAINTIES'. The theory points are from the NLO pQCD calculations of DSSZ, EPS09, nCTEQ15, and EPPS16 nPDFs, using CT14 as the baseline PDF.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pp dijet pseudorapidity spectra, shifted to match the $\eta_{\mathrm{dijet}}$ range of the pPb collisions, for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the CT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $55 < p_{\mathrm{T}}^{\mathrm{ave}} < 75$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $75 < p_{\mathrm{T}}^{\mathrm{ave}} < 95$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $95 < p_{\mathrm{T}}^{\mathrm{ave}} < 115$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $115 < p_{\mathrm{T}}^{\mathrm{ave}} < 150$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the MMHT14 as the baseline PDF.

The measured pPb dijet pseudorapidity spectra for $p_{\mathrm{T}}^{\mathrm{ave}} > 150$ GeV using the MMHT14 as the baseline PDF.

$\pi^0$ 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.

Direct photon spectra(Nucl. Part. Phys. 23, A1 (1997)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in p+p at $\sqrt{s_{NN}}$= 63 GeV.

Direct photon spectra(Sov. J. Nucl. Phys. 51, 836 (1990)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in p+p at $\sqrt{s_{NN}}$= 63 GeV.

Direct photon spectra normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 62.4 GeV.

Direct photon spectra normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 39.0 GeV.

Direct photon spectra(Physical Review C91, 064904 (2015)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review Letters 104, 132301 (2010)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review Letters 109, 152302 (2012)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Au+Au at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physical Review C98, 054902 (2018)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Cu+Cu at $\sqrt{s_{NN}}$= 200 GeV.

Direct photon spectra(Physics Letters B754 235 (2016)) normalized by $(dN_{ch}/d\eta)^{1.25}$ for in Pb+Pb at $\sqrt{s_{NN}}$= 2760 GeV.

Number of binary collisions N_{coll} vs. Charged particle multiplicity in Au+Au at various cm energies.

Charged particle multiplicity vs. centrality in Au+Au at various cm energies.

Number of binary collisions N_{coll} vs. centrality in Au+Au at various cm energies.

Integrated direct photon yield vs. Charged particle multiplicity in various systems at various cm energies.

Charged particle multiplicity vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. Charged particle multiplicity in various systems at various cm energies.

Charged particle multiplicity vs. centrality in various systems at various cm energies.

Integrated direct photon yield vs. centrality in various systems at various cm energies.

Rapidity dependence of $R_{\mathrm{pPb}}$ for prompt $\psi$(2S) mesons at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, in three $p_{\mathrm{T}}$ ranges. The fully correlated global uncertainty of 4.2% is not included in the point-by-point uncertainty.

Transverse momentum dependence of $R_{\mathrm{pPb}}$ for prompt $\psi$(2S) mesons at $\sqrt(s_{\textrm{NN}})=5.02 $ TeV, in seven $y_{\mathrm{CM}}$ ranges. The fully correlated global uncertainty of 4.2% is not incuded in the point-by-point uncertainty.