Measured unfolded differential cross-section as a function of the dilepton transverse momentum $p^{ll}_{\mathrm{T}}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Measured unfolded differential cross-section as a function of the the four-body transverse momentum $p^{ll\gamma\gamma}_{\mathrm{T}}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Measured unfolded differential cross-section as a function of the diphoton invariant mass $m_{\gamma\gamma}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Measured unfolded differential cross-section as a function of the four-body invariant mass $m_{ll\gamma\gamma}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Expected and observed $95\%$ confidence intervals for the coupling parameters $f_{T,j}/\Lambda^{4}$ of transverse dimension-8 operators. All parameter values outside of the stated range are excluded at the chosen confidence level. No unitarity constraints are applied.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,8}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,0}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,1}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,2}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,5}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,6}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,7}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,9}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction off protons with a Soeding-inspired analytic function --- statistical correlations only. Only one half of the (symmetric) matrix is stored.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction off protons, differential in the dipion mass and in bins of $W$. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction off protons, differential in the dipion mass and in bins of $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, in bins of the photon-proton energy $W$. The cross section is defined as the integral of the relativistic Breit Wigner resonance in the dipion mass over the range $2m_\pi<m_{\pi\pi}<1.53$ GeV. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons in bins of the photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction cross sections off protons as a function of energy. Parameters with subscript "el" and "pd" correspond to elastic and proton-dissociative cross sections, respectively.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction cross sections off protons as a function of energy --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of elastic $\rho^0(770)$ photoproduction cross section off protons as a function of energy (various experiments)

Fit of elastic $\rho^0(770)$ photoproduction cross sections off protons as a function of energy (various experiments) --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction cross section off protons, double-differential in the dipion mass and the momentum transfer $\vert t\vert$. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction cross section off protons, double-differential in the dipion mass and the momentum transfer $\vert t\vert$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, single-differential in the momentum transfer $\vert t\vert$. The cross section is defined as the integral of the relativistic Breit Wigner resonance in the dipion mass over the range $2m_\pi<m_{\pi\pi}<1.53$ GeV. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, single differential in the momentum transfer $\vert t\vert$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$. Parameters with subscript "el" and "pd" correspond to elastic and proton-dissociative cross sections, respectively.

Fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction double-differenial cross section off protons, as a function of the dipion mass and the momentum transfer $\vert t\vert$, in bins of the photon-proton energy $W$ The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\pi^{+}\pi^{-}$ photoproduction double-differenial cross section off protons, as a function of the dipion mass and the momentum transfer $\vert t\vert$, in bins of the photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction off protons, single-differential in the momentum transfer $\vert t\vert$, in bins of the photon-proton energy $W$. The cross section is defined as the integral of the relativistic Breit Wigner resonance in the dipion mass over the range $2m_\pi<m_{\pi\pi}<1.53$ GeV. The tabulated cross sections are $\gamma p$ cross sections but can be converted to $ep$ cross sections using the effective photon flux $\Phi_{\gamma/e}$.

Elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction cross section off protons, single differential in the momentum transfer $\vert t\vert$ and in bins of the photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Regge fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ and photon-proton energy $W$. Parameters with subscript "el" and "pd" correspond to elastic and proton-dissociative cross sections, respectively.

Regge fit of elastic ($m_Y=m_p$) and proton-dissociative ($1<m_Y<10$ GeV) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ and photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of $b$-slopes in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$.

Fit of $b$-slopes in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Fit of Pomeron trajectories in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$.

Fit of Pomeron trajectories in elastic ($m_Y=m_p$) $\rho^0(770)$ photoproduction single-differential cross sections off protons as a function of momentum transfer $t$ in bins of photon-proton energy $W$ --- statistical correlations coefficients $\rho_{ij}$ only. Only one half of the (symmetric) matrix is stored. Bins are identified by their global bin number.

Bin averaged hadron level differential cross sections as a function of the variable $z_{I\!\!P}$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections as a function of the variable $x_{I\!\!P}$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections as a function of the variable $y$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections as a function of the variable $Q^2$ for diffractive dijet DIS. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $E_T^{*\text{jet1}}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $M_X$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $\vert\Delta\eta^{\text{jets}}\vert$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential cross sections for diffractive dijet DIS as a function of the variable $\langle\eta^{\text{jets}}\rangle$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations and the the radiative corrections ($1+\delta_{\text{rad}}$) are also listed. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $z_{I\!\!P}$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $x_{I\!\!P}$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $y$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections as a function of the variable $x_\gamma$ for the dijet photoproduction kinematic range. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $E_T^{*\text{jet1}}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $M_X$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $\vert\Delta\eta^{\text{jets}}\vert$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Bin averaged hadron level differential diffractive dijet $ep$ cross sections in the photoproduction kinematic range as a function of the variable $\langle\eta^{\text{jets}}\rangle$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given. The overall normalisation uncertainty of $6\%$ is not included in the table.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $\vert\Delta\eta^{\text{jets}}\vert$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $y$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $z_{I\!\!P}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Ratios of differential diffractive dijet $ep$ cross sections, measured in photoproduction, to measurements in DIS as a function of the variable $E_T^{*\text{jet1}}$. The hadronisation correction factors ($1+\delta_{\text{hadr}}$) applied to the NLO calculations are given.

Diphoton production cross section as a function of the diphoton rapidity.

Diphoton production cross section differential in the cosine of the polar angle in the Collins-Soper frame.

Diphoton production cross section differential in the sub-leading to leading photon transverse momentum ratio (z).

Bin averaged hadron level differential cross section for diffractive dijet production as a function of X(C=POMERON). The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level differential cross section for diffractive dijet production as a function of Z(C=POMERON). The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level differential cross section for diffractive dijet production as a function of the average pseudorapidity of the dijet system. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level differential cross section for diffractive dijet production as a function of the absolute difference of the pseudorapidities of the two jets. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level differential cross section for diffractive dijet production as a function of W. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level differential cross section for diffractive dijet production as a function of the dijet invariant mass. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level differential cross section for diffractive dijet production as a function of mass of the diffractive system. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level double-differential cross section for diffractive dijet production as a function of X(GAMMA) for 3 ranges of ET of jet 1. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Bin averaged hadron level double-differential cross section for diffractive dijet production as a function of Z(POMERON) for 2 ranges of X(GAMMA). The first systematic error is the uncorrelated and the second the correlated uncertainty.

Ratios of the diffractive to the inclusive single-differential hadron level dijet cross sections as a function of X(C=GAMMA). The first systematic error is the uncorrelated and the second the correlated uncertainty.

Ratios of the diffractive to the inclusive single-differential hadron level dijet cross sections as a function of ET of jet 1. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Ratios of the diffractive to the inclusive single-differential hadron level dijet cross sections as a function of the average pseudorapidity of the dijet system. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Ratios of the diffractive to the inclusive single-differential hadron level dijet cross sections as a function of the absolute difference in the pseudorapidities of the 2 jets. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Ratios of the diffractive to the inclusive single-differential hadron level dijet cross sections as a function of the invariant mass of the dijet system. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Ratios of the diffractive to the inclusive single-differential hadron level dijet cross sections as a function of W. The first systematic error is the uncorrelated and the second the correlated uncertainty.

Proton structure function F2 at Q**2 = 55 GeV**2.

Proton structure function F2 at Q**2 = 70 GeV**2.

Proton structure function F2 at Q**2 = 90 GeV**2.

Proton structure function F2 at Q**2 = 120 GeV**2.

Proton structure function F2 at Q**2 = 190 GeV**2.

Proton structure function F2 at Q**2 = 320 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 25 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 35 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 45 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 55 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 70 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 90 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 120 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 190 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 190 GeV**2.

The diffractive cross section multiplied by (Q**2)*(Q**2+M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 1.2 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 3 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 6 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 11 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 20 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 30 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 35 GeV for W = 220 GeV.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9455 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7353 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4098 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1712 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0588 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0270 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9605 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7955 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4930 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2244 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0805 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0374 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9690 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8333 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.5556 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2711 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1011 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0476 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9745 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8594 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6044 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3125 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1209 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0576 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9798 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8861 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6604 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3665 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1489 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0722 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9843 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9091 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7143 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4265 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1837 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0909 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9881 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9302 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7692 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4979 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2308 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9925 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9548 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8407 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6109 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3220 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1743 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9726 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8989 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7256 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4444 and Q**2 = 320 GeV**2.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.00015 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.00015 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0050 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0050 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.005.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.005.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.040.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.060 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Differential polarized inclusive jet cross sections as a function of jet transverse energy.

Differential polarized inclusive jet cross sections as a function of photon virtuality, Q**2.

Differential polarized inclusive jet cross sections as a function of photon virtuality, Q**2.

Differential polarized inclusive jet cross sections as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Differential polarized inclusive jet cross sections as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Integrated polarized inclusive-jet cross section in the given kinematical range for the E- beam.

Integrated polarized inclusive-jet cross section in the given kinematical range for the E+ beam.

Differential unpolarized cross section for single jet production as a function of the jet pseudorapidity.

Differential unpolarized cross section for two jet production as a function of the mean jet pseudorapidity.

Differential unpolarized cross section for three jet production as a function of the mean jet pseudorapidity.

Differential unpolarized cross section for single jet production as a function of the jet transverse energy.

Differential unpolarized cross section for two jet production as a function of the mean jet transverse energy.

Differential unpolarized cross section for three jet production as a function of the mean jet transverse energy.

Differential unpolarized cross section for single jet production as a function of photon virtuality, Q**2.

Differential unpolarized cross section for two jet production as a function of photon virtuality, Q**2.

Differential unpolarized cross section for three jet production as a function of photon virtuality, Q**2.

Differential unpolarized inclusive-jet cross section as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Integrated unpolarized jet cross section in the given kinemetical region.

Differential unpolarized dijet cross section as a function of the dijet mass.

Differential unpolarized three-jet cross section as a function of the three-jet mass.

Distribution of D(SIG)/DM(P=6) as a function of M(P=6) .

Distribution of D(SIG)/DBETA as a function of BETA .

Distribution of D(SIG)/DX(NAME=POMERON) as a function of X(NAME=POMERON) .

Distribution of D(SIG)/DET(P=4,5,RF=CM) as a function of ET(P=4,5,RF=CM) .

Distribution of D(SIG)/DETARAP(P=4,5,RF=CM) as a function of ETARAP(P=4,5,RF=CM) .

Distribution of D(SIG)/DZ(NAME=POMERON) as a function of Z(NAME=POMERON) .

Distribution of D(SIG)/DX(NAME=GAMMA) as a function of X(NAME=GAMMA) .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DET(P=4,RF=CM) as a function of Z(NAME=POMERON) for ET(P=4,RF=CM) from 5 to 6.5 GeV). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DET(P=4,RF=CM) as a function of Z(NAME=POMERON) for ET(P=4,RF=CM) from 6.5 to 8 GeV). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DET(P=4,RF=CM) as a function of Z(NAME=POMERON) for ET(P=4,RF=CM) from 8 to 16 GeV). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 5 to 12 GeV**2). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 12 to 25 GeV**2). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 25 to 50 GeV**2). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 50 to 100 GeV**2). .

Cross section D(SIG)/X(C=GAMMA,OBS) as a function of X(C=GAMMA,OBS) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/Y as a function of Y in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/Y as a function of Y in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=4) as a function of ET(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=5) as a function of ET(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=6) as a function of ET(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=4) as a function of ET(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=5) as a function of ET(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=6) as a function of ET(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=7) as a function of ET(P=7) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=4) as a function of ETARAP(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=5) as a function of ETARAP(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=6) as a function of ETARAP(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=4) as a function of ETARAP(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=5) as a function of ETARAP(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=6) as a function of ETARAP(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=7) as a function of ETARAP(P=7) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/COS(PSI(3)) as a function of COS(PSI(3)) in two jet invariant mass regions, 25 to 50 and > 50 GeV . PSI(3) is the angle in the 3-jet CM frame between the plane containing the highest energy jet (P=4) and the beam, and the plane containing the three jets .