Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1 & Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1 & Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1 & Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side charged hadron yield per π 0 trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Away-side isolated direct photon trigger as a function of xE, which is equivalent to zT in the collinear limit cos(∆φ) = 1.

Breakdown of syst. uncertainties (fully bin-by-bin correlated) for differential cross section for $e^+e^-\rightarrow\pi^+\pi^-\gamma$, with $50^o<\theta_\gamma<130^o$

Bare cross section for $e^+e^-\rightarrow\pi^+\pi^-$

Statistical covariance matrix for bare cross section for $e^+e^-\rightarrow\pi^+\pi^-$

Inverse statistical covariance matrix for bare cross section for $e^+e^-\rightarrow\pi^+\pi$

Breakdown of syst. uncertainties (fully bin-by-bin correlated) for the cross section for $e^+e^-\rightarrow\pi^+\pi^-$

Pion form factor $|F_\pi|^2$

Statistical covariance matrix for pion form factor $|F_\pi|^2$

Inverse statistical covariance matrix $|F_\pi|^2$

Breakdown of syst. uncertainties (fully bin-by-bin correlated) for the pion form factor $|F_\pi|^2$

Vacuum polarisation correction $\delta_{VP}(s)=(\frac{\alpha_{em}(s)}{\alpha_{em}(0)})^2$, with $\sigma^{bare} = \sigma^{dressed}/\delta$ - calculated using the routine from F.Jegerlehner: https://web.archive.org/web/20170828074416/http://www-com.physik.hu-berlin.de/~fjeger/alphaQEDn.uu (2003, archived on August 28, 2017)

Final State Radiation correction $(1.+\eta_{FSR}(s))$, evaluated using the formula in Eur. Phys. J. C 24, 51-69 (2002)

The differential radiator function cross section $H(M_{\pi\pi}^2,s)\cdot \frac{\pi \alpha^2 \beta_\pi^3}{3 M_{\pi\pi}^2 s}$, inclusive in $\theta_\gamma$, in bins of 0.01 GeV$^2$ in $M_{\pi\pi}^2$. The value used for $s$ in the Monte Carlo production is $s = 999.85\; GeV^2$, corresponding to the mean value of DA$\Phi$NE energy for data collected in 2006. Obtained with the PHOKHARA5 MC generator, see Eur. Phys. J. C 27, 563 (2003) and https://looptreeduality.csic.es/phokhara/phokhara5.0.tar.gz

The K$\pi$ pair invariant mass distribution integrated over the $K^{*0}$ $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ =62.4 GeV after mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (top left) pT = 0.4–0.6 GeV/c in Au+Au collisions at √sNN = 200 GeV after the mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (top right) pT = 0.6–0.8 GeV/c in Au+Au collisions at √sNN = 62.4 GeV after the mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (bottom left) pT = 0.8–1.0 GeV/c in Au+Au collisions at √sNN = 200 GeV after the mixed-event background subtraction.

The Kπ pair invariant mass distribution for various pT bins (bottom right) pT = 1.0–1.2 GeV/c in Au+Au collisions at √sNN = 62.4 GeV after the mixed-event background subtraction.

The signal-to-background ratio for $K^{*0}$ measurements as a function of $p_T$ for different collision centrality bins (0-10%, 10-40%, 40-60%, 60-80%) in Au+Au collisions at 200 GeV.

$K^{*0}$ mass as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

$K^{*0}$ mass as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

$K^{*0}$ mass as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

$K^{*0}$ mass as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

$K^{*0}$ width as a function of $p_T$ for minimum bias Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The $K^{*0}$ reconstruction efficiency multiplied by the detector acceptance as a function of $p_T$ in Au+Au (|$\eta$| < 0.8) collisions at 200 GeV for different collision centrality bins (0-20% ,20-40% , 40-60%)

The $K^{*0}$ reconstruction efficiency multiplied by the detector acceptance as a function of $p_T$ in Cu+Cu (|$\eta$| < 1.0) collisions at 200 GeV for different collision centrality bins (0-20% ,20-40% , 40-60%)

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%, 60-80%) in Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%) in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%, 60-80%) in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

Mid-rapidity $K^{*0}$ $p_T$ spectra for various collision centrality bins (0-20%, 20-40%, 40-60%) in Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity yields dN/dy of $K^{*0}$ as a function of the average number of participating nucleons, $⟨N_{part}⟩$, for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 62.4 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity $K^{*0}$ $⟨p_T⟩$ as a function $⟨N_{part}⟩$ for Cu+Cu collisions at $\sqrt{s_{NN}}$ = 200 GeV

The mid-rapidity $⟨p_T⟩$ of $\pi$, K, p and $K^{*0}$ as a function of $⟨N_{part}⟩$ for Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})N(K^-)$ in Au+Au collisions divided by $N(K^{*0})N(K^-)$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$.

Mid-rapidity $N(K^{*0})N(K^-)$ in Cu+Cu collisions divided by $N(K^{*0})N(K^-)$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})N(K^-)$ in d+Au collisions divided by $N(K^{*0})N(K^-)$ ratio in d+Au collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(K^{*0})/N(K^-)$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $[N(\phi)/N(K^{*0})]$ in Au+Au collisions divided by $[N(\phi)/N(K^{*0})]$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $[N(\phi)/N(K^{*0})]$ in Cu+Cu collisions divided by $[N(\phi)/N(K^{*0})]$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $[N(\phi)/N(K^{*0})]$ in d+Au collisions divided by $[N(\phi)/N(K^{*0})]$ ratio in p+p collisions at $\sqrt{s_{NN}}$=200 GeV as a function of $⟨N_{part}⟩$

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Au+Au collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias Cu+Cu collisions as a function of $\sqrt{s_{NN}}$.

Mid-rapidity $N(\phi)/N(K^{*0})$ ratio in minimum bias p+p collisions as a function of $\sqrt{s_{NN}}$.

The $K^{*0}$ $v_2$ (Run IV) as a function of $p_T$ in minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $K^{*0}$ $v_2$ (Run II) as a function of $p_T$ in minimum bias Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

The $K^{*0}$ $R_{CP}$ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

The $K^{*0}$ $R_{CP}$ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

The $K^{*0}$ $R_{CP}$ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

The $K^{*0}$ ~$R_{CP}$~ as a function of $p_T$ in Au+Au collisions at 62.4 and 200 GeV compared to the $R_{CP}$ of $K^0_S$ and $\Lambda$ at 200 GeV.

$v_2$ vs $N_{part}$ in two $p_T$ ranges and $R_{AA}$ vs $N_{part}$ in the same $p_T$ ranges.

$v_2$ vs $N_{part}$ in two $p_T$ ranges and $R_{AA}$ vs $N_{part}$ in the same $p_T$ ranges.

$v_2$ vs $N_{part}$ and $R_{AA}$ vs $N_{part}$ in two $p_T$ ranges compared with WHDG model.

$v_2$ vs $N_{part}$ in two $p_T$ ranges compared with various models.

$R_{AA}$ vs $N_{part}$ in two $p_T$ ranges compared with various models.

Total visible cross section for LAMBDA/C+ production for the two decay channels combined. The second systematic error reflects the uncertainty in the branching ratios.

Measured D+ cross section as a function of the D+ transverse momentum.

Measured D+ cross section as a function of the D+ pseudorapidity.

Measured D+ cross section as a function of Q**2.

Measured D+ cross section as a function of the Bjorken X.

Normalized differential primary charged particle yield in inelastic (INEL) events.

Normalized differential primary charged particle yield in non-single diffractive (NSD) events.

Normalized invariant primary charged particle yield in non-single diffractive (NSD) events.

Transverse momentum spectra of charged particles in inelastic (INEL) events for event multiplicity N_ACC 3.

Transverse momentum spectra of charged particles in inelastic (INEL) events for event multiplicity N_ACC 7.

Transverse momentum spectra of charged particles in inelastic (INEL) events for event multiplicity N_ACC 17.

Mean transverse momentum of charged particles in inelastic (INEL) events as a function of the accepted event multiplicity in the PT range 0 TO 4 GeV.

Mean transverse momentum of charged particles in inelastic (INEL) events as a function of the accepted event multiplicity in the PT range 0.15 TO 4 GeV.

Mean transverse momentum of charged particles in inelastic (INEL) events as a function of the accepted event multiplicity in the PT range 0.5 TO 4 GeV.

Mean transverse momentum charged particles in inelastic (INEL) events as a function of the charged particle multiplicity in the PT range 0 TO 4 GeV.

Mean transverse momentum charged particles in inelastic (INEL) events as a function of the charged particle multiplicity in the PT range 0.15 TO 4 GeV.

Mean transverse momentum charged particles in inelastic (INEL) events as a function of the charged particle multiplicity in the PT range 0.5 TO 4 GeV.

Fit to the modified Hagedorn function (1/2PI*PT)*D2N(C=CHGD)/DETARAP/DPT ~ (PT/MT)*(1+(PT/PT0))**-B for non-single diffractive (NSD) events.

Fit to the modified Hagedorn function (1/2PI*PT)*D2N(C=CHGD)/DETARAP/DPT ~ (PT/MT)*(1+(PT/PT0))**-B for inelastic (INEL) events.

Fit to the modified Hagedorn function (1/2PI*PT)*D2N(C=CHGD)/DETARAP/DPT ~ (PT/MT)*(1+(PT/PT0))**-B for inelastic (INEL) events.

Angular dependence of the differential cross section for the W range 1.160 to 1.200 GeV.

Angular dependence of the differential cross section for the W range 1.200 to 1.240 GeV.

Angular dependence of the differential cross section for the W range 1.240 to 1.280 GeV.

Angular dependence of the differential cross section for the W range 1.280 to 1.320 GeV.

Angular dependence of the differential cross section for the W range 1.320 to 1.360 GeV.

Angular dependence of the differential cross section for the W range 1.360 to 1.400 GeV.

Angular dependence of the differential cross section for the W range 1.400 to 1.440 GeV.

Angular dependence of the differential cross section for the W range 1.440 to 1.480 GeV.

Angular dependence of the differential cross section for the W range 1.480 to 1.520 GeV.

Angular dependence of the differential cross section for the W range 1.520 to 1.560 GeV.

Angular dependence of the differential cross section for the W range 1.560 to 1.600 GeV.

Angular dependence of the differential cross section for the W range 1.600 to 1.640 GeV.

Angular dependence of the differential cross section for the W range 1.640 to 1.680 GeV.

Angular dependence of the differential cross section for the W range 1.680 to 1.720 GeV.

Angular dependence of the differential cross section for the W range 1.720 to 1.760 GeV.

Angular dependence of the differential cross section for the W range 1.760 to 1.800 GeV.

Angular dependence of the differential cross section for the W range 1.800 to 1.840 GeV.

Angular dependence of the differential cross section for the W range 1.840 to 1.880 GeV.

Angular dependence of the differential cross section for the W range 1.880 to 1.920 GeV.

Angular dependence of the differential cross section for the W range 1.920 to 1.960 GeV.

Angular dependence of the differential cross section for the W range 1.960 to 2.000 GeV.

Angular dependence of the differential cross section for the W range 2.000 to 2.040 GeV.

Angular dependence of the differential cross section for the W range 2.040 to 2.080 GeV.

Angular dependence of the differential cross section for the W range 2.080 to 2.120 GeV.

Angular dependence of the differential cross section for the W range 2.120 to 2.160 GeV.

Angular dependence of the differential cross section for the W range 2.160 to 2.200 GeV.

Angular dependence of the differential cross section for the W range 2.200 to 2.240 GeV.

Angular dependence of the differential cross section for the W range 2.240 to 2.280 GeV.

Angular dependence of the differential cross section for the W range 2.280 to 2.320 GeV.

Angular dependence of the differential cross section for the W range 2.320 to 2.360 GeV.

Angular dependence of the differential cross section for the W range 2.360 to 2.400 GeV.

Angular dependence of the differential cross section for the W range 2.400 to 2.500 GeV.

Angular dependence of the differential cross section for the W range 2.500 to 2.600 GeV.

Angular dependence of the differential cross section for the W range 2.600 to 2.700 GeV.

Angular dependence of the differential cross section for the W range 2.700 to 2.800 GeV.

Angular dependence of the differential cross section for the W range 2.800 to 2.900 GeV.

Angular dependence of the differential cross section for the W range 2.900 to 3.000 GeV.

Angular dependence of the differential cross section for the W range 3.000 to 3.100 GeV.

Angular dependence of the differential cross section for the W range 3.100 to 3.200 GeV.

Angular dependence of the differential cross section for the W range 3.200 to 3.300 GeV.

PI0_PI0 invariant mass distribution at an incident kinetic energy of 1200 MeV.

PI0_PI0 invariant mass distribution at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0_PI0 opening angle (DELTA) at an incident kinetic energy of 1300 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1000 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1100 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1200 MeV.

P_PI0 invariant mass distribution at an incident kinetic energy of 1300 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1000 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1100 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1200 MeV.

P_PI0_PI0 invariant mass distribution at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the Proton centre-of-mass angle at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0 centre-of-mass angle at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0_PI0 centre-of-mass angle at an incident kinetic energy of 1300 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1000 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1100 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1200 MeV.

Distribution of the cosine of the PI0 angle in the PI0_PI0 subsystem at an incident kinetic energy of 1300 MeV.