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.

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.

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.

Inclusive trijet cross section as a function of the jet psuedorapidity in the lab frame for the jet with the highest transverse energy.

Inclusive trijet cross section as a function of the jet psuedorapidity in the lab frame for the jet with the second highest transverse energy.

Inclusive trijet cross section as a function of the jet psuedorapidity in the lab frame for the jet with the third highest transverse energy.

The Inclusive dijet cross section as a function of Q**2 for jets in the Breit frame.

The Inclusive trijet cross section as a function of Q**2 for jets in the Breit frame.

The ratio of the inclusive trijet to dijet cross sections for jets in the Breit frame as a function of Q**2.

Values of the strong coupling constant ALPHAS at the Z mass as determined from this analysis. The second DSYS error here is from the theoretical systematic uncertainty.

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.

Cross sections for exclusive J/PSI production as a function of W in the Q**2 region 10 to 100 GeV**2.

Cross sections for exclusive J/PSI photoproduction as a function of W in the Q**2 region 0.15 to 0.18 GeV**2.

Cross sections for exclusive J/PSI photoproduction as a function of W in the Q**2 region 2 to 5 GeV**2.

Cross sections for exclusive J/PSI photoproduction as a function of W in the Q**2 region 5 to 10 GeV**2.

Cross sections for exclusive J/PSI photoproduction as a function of W in the Q**2 region 10 to 100 GeV**2.

Cross sections of exclusive J/PSI production as a function of Q**2 separating for the J/PSI --> E+ E- and MU+ MU- decay channels.

Cross sections of exclusive J/PSI photoproduction as a function of Q**2.

Cross sections for exclusive J/PSI photoproduction as a function of T in 4 Q**2 bins.

Parameters of fits to the W and Q**2 dependence of the exclusive J/PSI cross section.

Measured values of the differential cross section DSIG/DT as a function of W for T in the range 0.0 to 0.1 GeV**2.

Measured values of the differential cross section DSIG/DT as a function of W for T in the range 0.1 to 0.3 GeV**2.

Measured values of the differential cross section DSIG/DT as a function of W for T in the range 0.3 to 0.9 GeV**2.

Measured values of the differential cross section DSIG/DT as a function of W for T in the range 0.9 to 2.0 GeV**2.

Measured values of the Pomeron trajectory as a function of T in the Q**2 range 2 to 100 GeV**2.

Spin density matrices and ratio of cross sections of longitudinally and transversely polarized photons as a function of Q**2.

Spin density matrices and ratio of cross sections of longitudinally and transversely polarized photons as a function of W.

Spin density matrices and ratio of cross sections of longitudinally and transversely polarized photons as a function of T.

Inclusive jet cross section DSIG/DETARAP for jets in the lab. frame. Data from the 1995-1997 data sample.

Inclusive jet cross section DSIG/DETARAP for jets in the lab. frame. Data from the 1999-2000 data sample.

Inclusive jet cross section DSIG/DETARAP for jets in the lab. frame. Data from the combined data sample.

Inclusive jet cross section DSIG/DET for jets in the lab. frame. Data from the 1995-1997 running period.

Inclusive jet cross section DSIG/DET for jets in the lab. frame. Data from the 1999-2000 running period.

Inclusive jet cross section DSIG/DET for jets in the lab. frame. Data from the combined running period.

Inclusive di-jet cross section DSIG/DQ**2 for jets in the lab. frame. Data from the 1995-1997 data sample.

Inclusive di-jet cross section DSIG/DQ**2 for jets in the lab. frame. Data from the 1999-2000 data sample.

Inclusive di-jet cross section DSIG/DQ**2 for jets in the lab. frame. Data from the combined data sample.

Inclusive di-jet cross section DSIG/DM for jets in the lab. frame. Data from the 1995-1997 sample.

Inclusive di-jet cross section DSIG/DM for jets in the lab. frame. Data from the 1999-2000 sample.

Inclusive di-jet cross section DSIG/DM for jets in the lab. frame. Data from the combined sample.

Mean subjet multiplicity as a function of the YCUT parameter used in defining the jet for the inclusive jet sample with ET 14 to 17 GeV and 17 to 21 GeV.

Mean subjet multiplicity as a function of the YCUT parameter used in defining the jet for the inclusive jet sample with ET 21 to 25 GeV and 25 to 35 GeV.

Mean subjet multiplicity as a function of the YCUT parameter used in defining the jet for the inclusive jet sample with ET 35 to 55 GeV and 55 to 119 GeV.

Measured values of the mean subjet multiplicity at YCUT = 0.01 as a function of Q**2.

Value of ALPHAS at the Z0 mass obtained from the data with ET(C=JET) > 25 GeV.. The second DSYS error is due to the uncertainty in the theory.