Sample correlations in $\Delta\phi$ ($|\Delta\eta|<$ 1.78) for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-95% $d$+Au at $\sqrt{s_{NN}}$ = 200 GeV, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV, 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV, and 0-12% central Au+Au at $\sqrt{s_{NN}}$ = 200 GeV. The data are averaged between positive and negative $\Delta\phi$ and reflected in the plot.

Background subtracted sample correlations for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ on the near-side for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-95% $d$+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV, 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV and 0-12% central Au+Au at $\sqrt{s_{NN}}$ = 200 GeV. The dependence of the jet-like correlation is shown as a function of $\Delta\eta$ ($|\Delta\phi|<$ 0.78). The data are averaged between positive and negative $\Delta\eta$.

Background subtracted sample correlations for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ on the near-side for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-95% $d$+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV, 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV and 0-12% central Au+Au at $\sqrt{s_{NN}}$ = 200 GeV. The dependence of the jet-like correlation is shown as a function of $\Delta\phi$ ($|\Delta\eta|<$ 1.78). The data are averaged between positive and negative $\Delta\phi$.

Dependence of jet-like yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV. 5% systematic error due to the uncertainty on the associated particle's efficiency is not shown.

Dependence of jet-like yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV. 5% systematic error due to the uncertainty on the associated particle's efficiency is not shown.

Dependence of jet-like yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for $d$+Au at $\sqrt{s_{NN}}$ = 200 GeV. 5% systematic error due to the uncertainty on the associated particle's efficiency is not shown.

Dependence of jet-like yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV. 5% systematic error due to the uncertainty on the associated particle's efficiency is not shown.

Dependence of jet-like yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV. 5% systematic error due to the uncertainty on the associated particle's efficiency is not shown.

Dependence of jet-like yield on $p_T^{\mathrm{trigger}}$ for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, 0-95% $d$+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV, 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV and 0-12% central Au+Au at $\sqrt{s_{NN}}$ = 200 GeV. The 5% systematic error due to the uncertainty on the associated particle's efficiency is not shown.

Dependence of jet-like yield on $p_T^{\mathrm{associated}}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ for 0-60% Cu+Cu and 0-80% Au+Au collisions at $\sqrt{s_{NN}}$ = 62.4 GeV and 0-95% $d$+Au, 0-60% Cu+Cu, 0-12% Au+Au and 40-80% Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The 5% systematic error due to the uncertainty on the associated particle's efficiency is not shown.

Dependence of the widths in $\Delta\phi$ on $p_T^{\mathrm{trigger}}$ for 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-95% $d$+Au, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV and $\sqrt{s_{NN}}$ = 200 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, and 0-12% and 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\phi$ on $p_T^{\mathrm{associated}}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ for 0-95% $d$+Au, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV and $\sqrt{s_{NN}}$ = 200 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, and 0-12% and 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\phi$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of the widths in $\Delta\phi$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of the widths in $\Delta\phi$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-95% $d$+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\phi$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\phi$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\eta$ on $p_T^{\mathrm{trigger}}$ for 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-95% $d$+Au, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV and $\sqrt{s_{NN}}$ = 200 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, and 0-12% and 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\eta$ on $p_T^{\mathrm{associated}}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ for 0-95% $d$+Au, 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV and $\sqrt{s_{NN}}$ = 200 GeV, 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV, and 0-12% and 40-80% Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\eta$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of the widths in $\Delta\eta$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-80% Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of the widths in $\Delta\eta$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-95% $d$+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\eta$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for 0-60% Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of the widths in $\Delta\eta$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of ridge yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of ridge yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of ridge yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of ridge yield on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Ratio of the ridge and jet-like yields on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV.

Ratio of the ridge and jet-like yields on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV.

Ratio of the ridge and jet-like yields on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV.

Ratio of the ridge and jet-like yields on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of $V_{3\Delta}/V_{2\Delta}$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of $V_{3\Delta}/V_{2\Delta}$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 62.4 GeV.

Dependence of $V_{3\Delta}/V_{2\Delta}$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for $d$+Au at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of $V_{3\Delta}/V_{2\Delta}$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Cu+Cu at $\sqrt{s_{NN}}$ = 200 GeV.

Dependence of $V_{3\Delta}/V_{2\Delta}$ on $N_{part}$ for 3 $<$ $p_T^{trigger}$ $<$ 6 GeV/$c$ and 1.5 GeV/$c$ $<$ $p_T^{associated}$ $<$ $p_T^{trigger}$ for Au+Au at $\sqrt{s_{NN}}$ = 200 GeV.

The acceptance-corrected excess dielectron mass spectra, normalized to the charged particle multiplicity at mid-rapidity dNch/dy, in Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV. The dNch/dy values in Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV are from Ref. [38]. The normalization uncertainty from the STAR measured dN/dy is about 10%, which is not shown in the table.

The acceptance-corrected excess dielectron mass spectra, normalized to the charged particle multiplicity at mid-rapidity dNch/dy, in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV. The dNch/dy values in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV are from Ref. [39]. The normalization uncertainty from the STAR measured dN/dy is about 10%, which is not shown in the table.

Integrated yields of the normalized dilepton excesses for 0.4 < $M^{ll}$ < 0.75 GeV/c$^2$ as a function of dNch/dy. From top to bottom: 0-80% Au+Au collisions at $\sqrt{s_{NN}}$ = 19.6 GeV, then 0-10%, 10-40%, 40-80% and 0-80% Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Representative results on $v_3^2\{2\}$ from Au+Au collisions as a function of $\Delta\eta$ for charged hadrons with pT > 0.2 GeV/c and |$\eta$| < 1.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

Npart values are for the corresponding centrality at 200 GeV.

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Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Pion HBT radii for the 5% most central collisions.

Pion HBT radii for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.;.

Pion HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

Product of the three HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

The decoupling time extracted from R_long(KT) as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The fitted exponential slope of the T distribution as a function of X(NAME=POMERON).

The differential cross section as a function of PHI, the angle between the positron scattering plane and the proton scattering plane for the LRG and the LPS data samples.

The azimuthal asymmetries ALT and ATT as a function of X(NAME=POMERON).

The azimuthal asymmetries ALT and ATT as a function of BETA.

The azimuthal asymmetries ALT and ATT as a function of ABS(T).

The azimuthal asymmetries ALT and ATT as a function of Q**2.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 3.9 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 7.1 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 14 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and ABS(T) = 0.09 to 0.19 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 3.9 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 7.1 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 14 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and ABS(T) = 0.19 to 0.55 GeV**2 for M(X) values of 3, 7, 15 and 30 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 3.9 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 7.1 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 14 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LPS data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 2.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 3.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 4.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 5.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 6.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 8.5 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 12 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 16 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 22 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 30 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 40 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 50 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 65 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 85 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 110 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 140 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 185 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

The reduced diffractive cross sections obtained from the LRG data as a function of X(NAME=POMERON) for Q**2 = 255 GeV**2 and M(X) values of 3, 6, 11, 19 and 32 GeV.

Transverse mass spectra for kaon production in the central rapidity region for collisions at 20 GeV per nucleon.

Transverse mass spectra for kaon production in the central rapidity region for collisions at 30 GeV per nucleon.

Rapidity distribution of PI- production.

Rapidity distribution of K- production.

Rapidity distribution of K+ production.

Energy dependence of the mean K+ to PI+ and K- to PI- multiplicity ratio with the full phase space.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the mean K+ to PI+ and K- to PI- multiplicity ratio mid rapidity regions.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the inverse slope parameter of the transverse mass spectra in K+ and K- production.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the mean transverse mass measured at mid rapidity in PI+ and PI- production.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Energy dependence of the mean transverse mass measured at mid rapidity in K+ and K- production.. The data below 6 GeV are from the AGS and above 100 GeV from RHIC.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production for the full DIS sample. Statistical errors only are given.

The intercepts and slope for the exponential parameterisation of the differential cross section of the form A exp(-B*PT**2). Errors do not contain additional 2.1 PCT uncertainty on the intercepts.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in the photoproduction sample. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

Normalized double differential cross sections for leading neutron production in three regions of Q**2. Statistical errors only are given.

The intercepts and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the photoproduction sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the low-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the mid-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

The intercept and slope for the exponential parameterisation of the differential cross section of the form Aexp(-B*PT**2) for the high-Q**2 DIS sample. The errors do not contain the additional 2.1 PCT uncertainty on the DIS intercepts, nor the additional 5.1 PCT uncertainty on the photoproduction intercepts.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of pseudorapidity.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of PT.

Differential inclusive charged hadron production cross section as a function of PT.

Measurement of the proton structure function F2 at Q**2 = 8.0 GeV**2.

Measurement of the proton structure function F2 at Q**2 = 14.0 GeV**2.

Measurement of the proton structure function F2 at Q**2 = 27.0 GeV**2.

Measurement of the proton structure function F2 at Q**2 = 55.0 GeV**2.

Measurement of the proton total cross section for GAMMA* P scattering at Q**2 = 2.7 GeV.

Measurement of the proton total cross section for GAMMA* P scattering at Q**2 = 4.0 GeV.

Measurement of the proton total cross section for GAMMA* P scattering at Q**2 = 6.0 GeV.

Measurement of the proton total cross section for GAMMA* P scattering at Q**2 = 8.0 GeV.

Measurement of the proton total cross section for GAMMA* P scattering at Q**2 = 14.0 GeV.

Measurement of the proton total cross section for GAMMA* P scattering at Q**2 = 27.0 GeV.

Measurement of the proton total cross section for GAMMA* P scattering at Q**2 = 55.0 GeV.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 1.2 GeV and Q**2 = 2.7 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 1.2 GeV and Q**2 = 4.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 1.2 GeV and Q**2 = 6.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 1.2 GeV and Q**2 = 8.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 1.2 GeV and Q**2 = 14.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 1.2 GeV and Q**2 = 27.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 1.2 GeV and Q**2 = 55.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 3.0 GeV and Q**2 = 2.7 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 3.0 GeV and Q**2 = 4.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 3.0 GeV and Q**2 = 6.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 3.0 GeV and Q**2 = 8.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 3.0 GeV and Q**2 = 14.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 3.0 GeV and Q**2 = 27.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 3.0 GeV and Q**2 = 55.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 6.0 GeV and Q**2 = 2.7 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 6.0 GeV and Q**2 = 4.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 6.0 GeV and Q**2 = 6.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 6.0 GeV and Q**2 = 8.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 6.0 GeV and Q**2 = 14.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 6.0 GeV and Q**2 = 27.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 6.0 GeV and Q**2 = 55.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 11.0 GeV and Q**2 = 2.7 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 11.0 GeV and Q**2 = 4.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 11.0 GeV and Q**2 = 6.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 11.0 GeV and Q**2 = 8.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 11.0 GeV and Q**2 = 14.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 11.0 GeV and Q**2 = 27.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 11.0 GeV and Q**2 = 55.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 20.0 GeV and Q**2 = 2.7 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 20.0 GeV and Q**2 = 4.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 20.0 GeV and Q**2 = 6.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 20.0 GeV and Q**2 = 8.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 20.0 GeV and Q**2 = 14.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 20.0 GeV and Q**2 = 27.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 20.0 GeV and Q**2 = 55.0 GeV**2.

Cross section for the diffractive scattering process GAMMA* P --> DD X for a diffractive mass of 30.0 GeV and Q**2 = 2.7 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 0.28 to 2 GeV, to the total cross section for Q**2 = 2.7 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 0.28 to 2 GeV, to the total cross section for Q**2 = 4.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 0.28 to 2 GeV, to the total cross section for Q**2 = 6.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 0.28 to 2 GeV, to the total cross section for Q**2 = 8.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 0.28 to 2 GeV, to the total cross section for Q**2 = 14.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 0.28 to 2 GeV, to the total cross section for Q**2 = 27.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 0.28 to 2 GeV, to the total cross section for Q**2 = 55.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 2 to 4 GeV, to the total cross section for Q**2 = 2.7 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 2 to 4 GeV, to the total cross section for Q**2 = 4.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 2 to 4 GeV, to the total cross section for Q**2 = 6.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 2 to 4 GeV, to the total cross section for Q**2 = 8.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 2 to 4 GeV, to the total cross section for Q**2 = 14.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 2 to 4 GeV, to the total cross section for Q**2 = 27.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 2 to 4 GeV, to the total cross section for Q**2 = 55.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 4 to 8 GeV, to the total cross section for Q**2 = 2.7 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 4 to 8 GeV, to the total cross section for Q**2 = 4.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 4 to 8 GeV, to the total cross section for Q**2 = 6.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 4 to 8 GeV, to the total cross section for Q**2 = 8.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 4 to 8 GeV, to the total cross section for Q**2 = 14.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 4 to 8 GeV, to the total cross section for Q**2 = 27.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 4 to 8 GeV, to the total cross section for Q**2 = 55.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 8 to 15 GeV, to the total cross section for Q**2 = 2.7 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 8 to 15 GeV, to the total cross section for Q**2 = 4.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 8 to 15 GeV, to the total cross section for Q**2 = 6.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 8 to 15 GeV, to the total cross section for Q**2 = 8.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 8 to 15 GeV, to the total cross section for Q**2 = 14.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 8 to 15 GeV, to the total cross section for Q**2 = 27.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 8 to 15 GeV, to the total cross section for Q**2 = 55.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 15 to 25 GeV, to the total cross section for Q**2 = 2.7 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 15 to 25 GeV, to the total cross section for Q**2 = 4.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 15 to 25 GeV, to the total cross section for Q**2 = 6.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 15 to 25 GeV, to the total cross section for Q**2 = 8.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 15 to 25 GeV, to the total cross section for Q**2 = 14.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 15 to 25 GeV, to the total cross section for Q**2 = 27.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 15 to 25 GeV, to the total cross section for Q**2 = 55.0 GeV**2.

Ratio of the cross sections for diffractive scattering GAMMA* P --> DD X integrated over the diffractive mass 25 to 35 GeV, to the total cross section for Q**2 = 2.7 GeV**2.

Ratio of the total diffractive cross section observed to the total cross section.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 2.7 GeV**2 and BETA = 0.6522.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 2.7 GeV**2 and BETA = 0.2308.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 2.7 GeV**2 and BETA = 0.0698.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 2.7 GeV**2 and BETA = 0.0218.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 2.7 GeV**2 and BETA = 0.0067.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 2.7 GeV**2 and BETA = 0.0030.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 4.0 GeV**2 and BETA = 0.7353.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 4.0 GeV**2 and BETA = 0.3077.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 4.0 GeV**2 and BETA = 0.1000.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 4.0 GeV**2 and BETA = 0.0320.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 4.0 GeV**2 and BETA = 0.0099.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 4.0 GeV**2 and BETA = 0.0044.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 6.0 GeV**2 and BETA = 0.8065.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 6.0 GeV**2 and BETA = 0.4000.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 6.0 GeV**2 and BETA = 0.1429.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 6.0 GeV**2 and BETA = 0.0472.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 6.0 GeV**2 and BETA = 0.0148.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 6.0 GeV**2 and BETA = 0.0066.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 8.0 GeV**2 and BETA = 0.8475.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 8.0 GeV**2 and BETA = 0.4706.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 8.0 GeV**2 and BETA = 0.1818.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 8.0 GeV**2 and BETA = 0.0620.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 8.0 GeV**2 and BETA = 0.0196.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 8.0 GeV**2 and BETA = 0.0088.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 14.0 GeV**2 and BETA = 0.9067.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 14.0 GeV**2 and BETA = 0.6087.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 14.0 GeV**2 and BETA = 0.2800.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 14.0 GeV**2 and BETA = 0.1037.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 14.0 GeV**2 and BETA = 0.0338.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 14.0 GeV**2 and BETA = 0.0153.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 27.0 GeV**2 and BETA = 0.9494.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 27.0 GeV**2 and BETA = 0.7500.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 27.0 GeV**2 and BETA = 0.4286.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 27.0 GeV**2 and BETA = 0.1824.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 27.0 GeV**2 and BETA = 0.0632.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 27.0 GeV**2 and BETA = 0.0291.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 55.0 GeV**2 and BETA = 0.9745.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 55.0 GeV**2 and BETA = 0.8594.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 55.0 GeV**2 and BETA = 0.6044.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 55.0 GeV**2 and BETA = 0.3125.

The diffractive structure function F2(NAME=D3) multiplied by X(NAME=POMERON), for Q**2 = 55.0 GeV**2 and BETA = 0.1209.

The diffractive structure function of the proton multiplied by X(NAME=POMERON) at the point X(POMERON) = 0.01 and Q**2 = 2.7 GeV**2.

The diffractive structure function of the proton multiplied by X(NAME=POMERON) at the point X(POMERON) = 0.01 and Q**2 = 4.0 GeV**2.

The diffractive structure function of the proton multiplied by X(NAME=POMERON) at the point X(POMERON) = 0.01 and Q**2 = 6.0 GeV**2.

The diffractive structure function of the proton multiplied by X(NAME=POMERON) at the point X(POMERON) = 0.01 and Q**2 = 8.0 GeV**2.

The diffractive structure function of the proton multiplied by X(NAME=POMERON) at the point X(POMERON) = 0.01 and Q**2 = 14.0 GeV**2.

The diffractive structure function of the proton multiplied by X(NAME=POMERON) at the point X(POMERON) = 0.01 and Q**2 = 27.0 GeV**2.

The diffractive structure function of the proton multiplied by X(NAME=POMERON) at the point X(POMERON) = 0.01 and Q**2 = 55.0 GeV**2.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 172.3 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 182.8 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 188.6 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 194.4 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 200.2 GeV.

Jet fractions using the JADE algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 130.1 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 136.1 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 161.3 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 172.3 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 182.8 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 188.6 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 194.4 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 200.2 GeV.

Jet fractions using the KT(Durham) algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Jet fractions using the Cambridge algorithm as a function of the jet resolution parameter YCUT at c.m. energy 202.2 GeV.

Jet fractions using the Cambridge algorithm as a function of the jet resolution parameter YCUT at c.m. energy 206.2 GeV.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for event thrust.

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for the scaled heavy jet mass (RHO(C=HEAVY)).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for total jet broadening (BT).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for wide jet broadening (BW).

Differential distributions for the C-Parameter.

Differential distributions for the C-Parameter.

Differential distributions for the C-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the D-Parameter.

Differential distributions for the THRUST at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the RHO(C=HEAVY) at c.m. energy 91.2 GeV forlight quark (udsc) and b quark events.

Differential distributions for the BT at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the BW at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the C-PARAM at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Differential distributions for the D-PARAM at c.m. energy 91.2 GeV for light quark (udsc) and b quark events.

Mean values (first moment) and dispersion (second moment) of the THRUST distribution as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the scaled heavy jet mass (RHO(C=HEAVY)) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the total jet broadening (BT) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the wide jet broadening (BW) as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the C-PARAM as a function of c.m. energy.

Mean values (first moment) and dispersion (second moment) of the D-PARAM as a function of c.m. energy.

Charged particle multiplicities at c.m. energy 91.2 GeV for all flavour, light quark (udsc) and bottom (b) flavour events.

Charged particle multiplicity.

Charged particle multiplicity.

Charged particle multiplicity.

First and second moment of the charged particle multiplicity distribution at c.m. energy 91.2 GeV for all flavours and for udsc an b flavours.

First and second moment of the charged particle multiplicity distribution at c.m. energy.

Distribution of LN(1/X) at c.m. energy 91.2 GeV.

Distribution of LN(1/X) at higher c.m. energies.

Distribution of LN(1/X) at higher c.m. energies.

Distribution of LN(1/X) at higher c.m. energies.

The J/PSI photoproduction cross section as a function of W for the ABS(T) range 10 to 30 GeV**2.

The values of POWER obtained in the fit of the form W**POWER to the J/PSI photoproduction cross section.

The density matrix elements for the J/PSI photoproduction data.

Ratio of cross section for PSI(2S) to J/PSI production. as a function of Z. Statistical errors only.

The measured J/PSI differential cross section DSIG/DZ for different PT cuts.

The measured J/PSI differential cross section DSIG/DPT**2.

The J/PSI cross section versus W.

The measured J/PSI differential cross section DSIG/DYRAP.

J/PSI helicity parameter 'ALPHA', defined as DN/DCOS(THETA) ~ 1 + ALPHA*COS(THETA)**2, as a function of PT in the target frame.The uncertainties are due to the total experimental uncertainties.

J/PSI helicity parameter 'ALPHA', defined as DN/DCOS(THETA) ~ 1 + ALPHA*COS(THETA)**2, as a function of PT in the helicity basis.The uncertainties are due to the total experimental uncertainties.

J/PSI leptoproduction differential cross section as a function of the laboratory frame PT**2.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame rapidity Y*.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame PT**2.

J/PSI leptoproduction differential cross section as a function of the laboratory frame rapidity Y.

J/PSI leptoproduction differential cross section as a function of Q**2 for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of Z for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of W for laboratort PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of the laboratory frame PT**2 for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame rapidity Y* for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction differential cross section as a function of the centre-of-mass frame PT**2 for laboratory PT**2 > 6.4 GeV**2 and Q**2 > 12 GeV**2.

J/PSI leptoproduction double differential cross section as a function of the centre-of-mass frame PT**2 and Z for the Z range 0.3 to 0.6.

J/PSI leptoproduction double differential cross section as a function of the centre-of-mass frame PT**2 and Z for the Z range 0.6 to 0.75.

J/PSI leptoproduction double differential cross section as a function of the centre-of-mass frame PT**2 and Z for Z range 0.75 to 0.9.

J/PSI leptoproduction double differential cross section as a function of Q**2 and Z for the Z range 0.3 to 0.6.

J/PSI leptoproduction double differential cross section as a function of Q**2 and Z for the Z range 0.6 to 0.75.

J/PSI leptoproduction double differential cross section as a function of Q**2 and Z for the Z range 0.75 to 0.9.

J/PSI photoproduction cross section at a mean Q**2 of 10.6 GeV**2.

J/PSI leptoproduction differential cross section as a function of COS(THETA*). for the Z range 0.75 to 0.9.

J/PSI leptoproduction differential cross section as a function of COS(THETA*) in the Q**2 range 2 to 6.5 GeV**2.

J/PSI leptoproduction differential cross section as a function of COS(THETA*) in the Q**2 range 6.5 to 100 GeV**2.

The inelastic J/PSI production cross section as a function of PT**2.

Low Z inelastic J/PSI cross section as a function of W.

Low Z inelastic J/PSI cross section as a function of PT**2.

Inelastic J/PSI cross section for the full Z range. The data come from two different data sets with the points at Z = 0.38 being statistically correlated.

The mean values of the five event shape variable distributions.

The corrected distributions of (1-TRUST).

The corrected distributions for the scaled heavy jet mass, RHO.

The corrected distributions for the total jet broadening, BT.

The corrected distributions for the wide jet broadening, BW.

The corrected distributions for the C-parameter, C-PARAM.

Distribution for Wide Jet Broadening at c.m. energy 189 GeV.

Distribution for C-Parameter at c.m. energy 189 GeV.

Mean values (first moments) of the 1-THRUST distributions as a function of c.m. energy.

Mean values (first moments) of the Heavy Jet Mass distributions as a function of c.m. energy.

Mean values (first moments) of the Total Jet Broadening distributions as a function of c.m. energy.

Mean values (first moments) of the Wide Jet Broadening distributions as a function of c.m. energy.

Mean values (first moments) of the C-Parameter distributions as a function of c.m. energy.

Dispersion values (second moments) of the 1-THRUST distributions as a function of c.m. energy.

Dispersion values (second moments) of the Heavy Jet Mass distributions as afunction of c.m. energy.

Dispersion values (second moments) of the Total Jet Broadening distributions as a function of c.m. energy.

Dispersion values (second moments) of the Wide Jet Broadening distributionsas a function of c.m. energy.

Dispersion values (second moments) of the C-Parameter distributions as a function of c.m. energy.

Values of the strong coupling constant ALPHA-s at the Z0 mass, from fits tothe first moments of the various event shape distribution.

The strong coupling constant, ALPHA-s, measured at different c.m. energies from a fit to the 1-THRUST distribution. The second DSYS error is the uncertainty in the theory.

The strong coupling constant, ALPHA-s, measured at different c.m. energies from a fit to the Heavy Jet Mass distribution. The second DSYS error is the uncertainty in the theory.

The strong coupling constant, ALPHA-s, measured at different c.m. energies from a fit to the Total Jet Broadening distribution. The second DSYS error is the uncertainty in the theory.

The strong coupling constant, ALPHA-s, measured at different c.m. energies from a fit to the Wide Jet Broadening distribution. The second DSYS error is theuncertainty in the theory.

The strong coupling constant, ALPHA-s, measured at different c.m. energies from a fit to the C-Parameter distribution. The second DSYS error is the uncertainty in the theory.

The strong coupling constant, ALPHA-s, as determined from the combined event shape variables as a function of c.m. energy. The values for c.m. energy belowthe Z0 mass were determined only for four event shape variables.

Q**2 dependence of the elastic J/PSI photoproduction cross section.

Slope of the elastic J/PSI photoproduction T distribution.

Slope of the elastic J/PSI photoproduction T distribution.

Spin density matrices of the angular distribution in J/PSI electroproduction.

Ratio of longitudinal to transverse J/PSI electroproduction cross section determined under the assumption of SCHC.

Inclusive and inelastic (MX>10) J/PSI electroproduction cross sections.

Inclusive and inelastic (MX>10) J/PSI electroproduction cross sections.

Inclusive and inelastic (MX>10) J/PSI electroproduction cross sections.

Inclusive and inelastic (MX>10) J/PSI electroproduction cross sections.

Inclusive and inelastic (MX>10) J/PSI electroproduction cross sections.

Inclusive and inelastic (MX>10GEV) differential cross section for J/PSI electroproduction.

Inclusive and inelastic (MX>10GEV) differential cross section for J/PSI electroproduction.

Inclusive and inelastic (MX>10GEV) differential cross section for J/PSI electroproduction.

W dependence of the inclusive and inelastic (Z<0.9) J/PSI photoproduction cross section.

No description provided.

No description provided.

No description provided.

Inverse slope parameter.

Inverse slope parameter.

Rapidity distributions of negatively charged hadrons (pion mass assumed) produced in central S+Au collisions.

Rapidity distributions of negatively charged hadrons produced in central S+S collisions.

Rapidity distributions of net protons (p-pbar) for minimum bias p+Au collisions at 200 GeV/nucleon.

Rapidity distributions of net protons (p-pbar) for minimum bias p+S collisions at 200 GeV/nucleon.

Rapidity distributions of net protons (p-pbar) for central S+Au collisions at 200 GeV/nucleon.

Rapidity distributions of net protons (p-pbar) for central d+Au collisions at 200 GeV/nucleon.

Rapidity distributions of net protons (p-pbar) for central O+Au collisions at 200 GeV/nucleon.

Rapidity distributions of net protons (p-pbar) for central S+Ag collisions at 200 GeV/nucleon.

Rapidity distributions of net protons (p-pbar) for central S+S collisions at 200 GeV/nucleon.

Rapidity distributions of net hyperons (Lambda-Lambdabar) for minimum bias p+Au (1.4 < y < 4.4) collisions at 200 GeV/nucleon.

Rapidity distributions of net hyperons (Lambda-Lambdabar) for minimum bias p+S (1.0 < y < 5.0) collisions at 200 GeV/nucleon.

Rapidity distributions of net hyperons (Lambda-Lambdabar) for central S+Ag (0.5 < y < 3.0) collisions at 200 GeV/nucleon.

Rapidity distributions of net hyperons (Lambda-Lambdabar) for central S+Au (3.0 < y < 5.0) collisions at 200 GeV/nucleon.

Rapidity distributions of net hyperons (Lambda-Lambdabar) for central S+S (0.5 < y < 3.0) collisions at 200 GeV/nucleon.

Transverse momentum distributions of net protons for minimum bias p+AU collisions.

Transverse momentum distributions of net protons for minimum bias p+S collisions.

Transverse momentum distributions of net protons for central S+Au collisions.

Transverse momentum distributions of net protons for central d+Au collisions.

Transverse momentum distributions of net protons for central O+Au collisions.

Transverse momentum distributions of net protons for central S+Ag collisions.

Transverse momentum distributions of net protons for central S+S collisions.

Rapidity distributions of negatively charged hadrons produced in minimum bias nucleon-nucleon collisions.

Rapidity distributions of negatively charged hadrons produced in p+S collisions.

Rapidity distributions of negatively charged hadrons produced in minimum bias nucleon-nucleon collisions.

Rapidity distributions of negatively charged hadrons produced in central d+Au collisions.

Rapidity distributions of negatively charged hadrons produced in central O+Au collisions.

Rapidity distributions of negatively charged hadrons produced in central S-nucleus collisions.

Transverse momentum distributions of negatively charged hadrons produced inp+S a interactions for different rapidity regions.

Transverse momentum distributions of negatively charged hadrons produced inp+Au a interactions for different rapidity regions.

Transverse momentum distributions of negatively charged hadrons produced incentral d+Au a collisions for the rapidity interval (0.8 < y < 2.0).

Transverse momentum distributions of negatively charged hadrons produced incentral d+Au a collisions for different rapidity regions.

Transverse momentum distributions of negatively charged hadrons produced incentral O+Au a collisions for different rapidity regions.

Transverse momentum distributions of negatively charged hadrons produced incentral S+Au a collisions for different rapidity regions.

Transverse momentum distributions of negatively charged hadrons produced incentral S+S a collisions for different rapidity regions.

Transverse momentum distributions of negatively charged hadrons produced incentral S+Ag a collisions for different rapidity regions.

Cross section for the MU+ MU- decay channel.

Cross section for the E+ E- decay channel.

Cross section for the E+ E- decay channel.

Cross section for the E+ E- decay channel.

Cross section for the E+ E- decay channel.

Direct inelastic J/PSI photoproduction cross section for both decay channels combined (except W = 50-90 which is MU+ MU- only).

Direct inelastic J/PSI photoproduction cross section for both decay channels combined (except 50<W<110 which is MU+ MU- only).

PT**2 distribution for the J/PSI --> MU+ MU- sample.

Z distribution for the J/PSI --> MU+ MU- sample.

Data fitted with the form DSIG/DPT**2=CONST*EXP(-SLOPE*PT**2).

Cross section from PSI(3685) --> J/PSI(1S) < MU+ MU- > PI+ PI- mode.

Cross section from PSI(3685) --> E+ E- + MU+ MU- mode.

Cross section from PSI(3685) --> J/PSI(1S) < E+ E- > PI+ PI- mode.

Cross section from PSI(3685) --> J/PSI(1S) < MU+ MU- > PI+ PI- mode.

Cross section from PSI(3685) --> E+ E- + MU+ MU- mode.

Second systematic error is due to uncertainties in the PSI(2S) partial widths. J/PSI cross section 119.5+-11.2+-12.0 nb is from NP B472, 3. Extrapolation to Q2=0.

No description provided.

No description provided.