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.

Nuclear modicifation factor vs. N_coll $J\psi$ with|y|<1 and pT < 3 GeV/c in d Au collisions.

The invariant cross section versus transverse momentum for J/$\psi$ with $|y|\lt 1$ in $p+p$ collisions.

The invariant yield versus transverse momentum for $J/\Psi$ with |y| < 1 in 0 - 100 percent central d+Au collisions.

The effective exponential slope, $b_n$, obtained from the fit of double differential photoproduction cross sections ${\rm d^2}\sigma_{\gamma p}/{\rm d}x_L{\rm d}p_{T,n}^2$ to a single exponential function in bins of $x_L$. The first uncertainty represents the fit error from the statistical and uncorrelated systematic uncertainty and the second one is due to the correlated systematic uncertainty.

Energy dependence of the exclusive photoproduction of a $\rho^0$ meson associated with a leading neutron, $\gamma p \to \rho^0 n \pi^+$. The first uncertainty is statistical and the second is systematic. The global normalisation uncertainty of $4.4\%$ is not included. $\Phi_{\gamma}$ is the integral of the photon flux, Eq. (3) of paper, in a given $W_{\gamma p}$ bin.

Differential photoproduction cross section ${\rm d}\sigma_{\gamma p}/{\rm d}\eta$ for the exclusive process $\gamma p \to \rho^0 n \pi^+$ as a function of the $\rho^0$ pseudorapidity in the kinematic range $0.35 < x_L < 0.95$, $\theta_n < 0.75$ mrad and $20 < W_{\gamma p} < 100$ GeV. The statistical, uncorrelated and correlated systematic uncertainties, $\delta_{stat}$, $\delta_{sys}^{unc}$ and $\delta_{sys}^{cor}$ respectively, are given, which does not include the global normalisation error of $4.4\%$.

Differential photoproduction cross section ${\rm d}\sigma_{\gamma p}/{\rm d}t^{\prime}$ for the exclusive process $\gamma p \to \rho^0 n \pi^+$ as a function of the $\rho^0$ four-momentum transfer squared, $t^{\prime}$, in the kinematic range $0.35 < x_L < 0.95$, $\theta_n < 0.75$ mrad and $20 < W_{\gamma p} < 100$ GeV. The statistical, uncorrelated and correlated systematic uncertainties, $\delta_{stat}$, $\delta_{sys}^{unc}$ and $\delta_{sys}^{cor}$ respectively, are given, which does not include the global normalisation error of $4.4\%$.

Exponential slopes, $b_1$ and $b_2$, and the ratio $\sigma_1/\sigma_2$, obtained from the components of fit, Eq. (14) of paper, to the differential cross section ${\rm d}\sigma_{\gamma p}/{\rm d}t^{\prime}$ in bins of $x_L$. The errors represent the statistical and systematic uncertainties added in quadrature.

Exponential slopes, $b_1$ and $b_2$, and the ratio $\sigma_1/\sigma_2$, obtained from the components of fit, Eq. (14) of paper, to the differential cross section ${\rm d}\sigma_{\gamma p}/{\rm d}t^{\prime}$ in bins of $p_{T,n}^2$. The errors represent the statistical and systematic uncertainties added in quadrature.

Energy dependence of elastic $\rho^0$ photoproduction on the pion, $\gamma \pi^+ \to \rho^0 \pi^+$, extracted in the one-pion-exchange approximation using OPE1 sample. The first uncertainty represents the full experimental error and the second is the model error coming from the pion flux uncertainty (see text). $\Gamma_\pi(x_L)$ represents the value of the pion flux, Eqs. (5-6) of paper, integrated over the $p_{T,n}<0.2$ GeV range, at a given $x_L$.

Cross section of elastic $\rho^0$ photoproduction on the pion, $\gamma \pi^+ \to \rho^0 \pi^+$, extracted in the one-pion-exchange approximation using three different samples: full sample, OPE1 and OPE2. The first uncertainty represents the full experimental error and the second is the model error coming from the pion flux uncertainty (see text). $\Gamma_\pi$ represents the value of the pion flux, Eqs. (5-6) of paper, integrated over the corresponding $(x_L,p_{T,n})$ range.

HERA combined reduced cross sections $\sigma_{r,\rm NC}^{+}$ for NC $e^{+}p$ scattering at $\sqrt{s} = 225$ GeV; $\delta_{\rm stat}$, $\delta_{\rm uncor}$ and $\delta_{\rm cor}$ represent the statistical, uncorrelated systematic and correlated systematic uncertainties, respectively; $\delta_{\rm rel}$, $\delta_{\gamma p}$, $\delta_{\rm had}$ and $\delta_{1}$ to $\delta_{4}$ are the correlated sources of uncertainties arising from the combination procedure. The uncertainties are quoted in percent relative to $\sigma_{r,\rm NC}^{+}$.

HERA combined reduced cross sections $\sigma_{r,\rm NC}^{-}$ for NC $e^{-}p$ scattering at $\sqrt{s} = 318$ GeV; $\delta_{\rm stat}$, $\delta_{\rm uncor}$ and $\delta_{\rm cor}$ represent the statistical, uncorrelated systematic and correlated systematic uncertainties, respectively; $\delta_{\rm rel}$, $\delta_{\gamma p}$, $\delta_{\rm had}$ and $\delta_{1}$ to $\delta_{4}$ are the correlated sources of uncertainties arising from the combination procedure. The uncertainties are quoted in percent relative to $\sigma_{r,\rm NC}^{-}$.

HERA combined reduced cross sections $\sigma_{r,\rm CC}^{+}$ for CC $e^{+}p$ scattering at $\sqrt{s} = 318$ GeV; $\delta_{\rm stat}$, $\delta_{\rm uncor}$ and $\delta_{\rm cor}$ represent the statistical, uncorrelated systematic and correlated systematic uncertainties, respectively; $\delta_{\rm rel}$, $\delta_{\gamma p}$, $\delta_{\rm had}$ and $\delta_{1}$ to $\delta_{4}$ are the correlated sources of uncertainties arising from the combination procedure. The uncertainties are quoted in percent relative to $\sigma_{r,\rm CC}^{+}$.

HERA combined reduced cross sections $\sigma_{r,\rm CC}^{-}$ for CC $e^{-}p$ scattering at $\sqrt{s} = 318$ GeV; $\delta_{\rm stat}$, $\delta_{\rm uncor}$ and $\delta_{\rm cor}$ represent the statistical, uncorrelated systematic and correlated systematic uncertainties, respectively; $\delta_{\rm rel}$, $\delta_{\gamma p}$, $\delta_{\rm had}$ and $\delta_{1}$ to $\delta_{4}$ are the correlated sources of uncertainties arising from the combination procedure. The uncertainties are quoted in percent relative to $\sigma_{r,\rm CC}^{-}$.

Structure function $xF_3^{\gamma Z}$ for different values of $Q^2$ and $x_{\rm Bj}$.

Structure function $xF_3^{\gamma Z}$ averaged over $Q^2 \ge 1000$ GeV$^2$ at the scale 1000 GeV$^2$.

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.

Diffractive DIS dijet cross section measured differentially as a function of $\log x_P$. The global normalisation uncertainty of $7.8\%$ is not listed explicitly but is included in the total systematic uncertainty. The last two column show the correction factors for hadronisation and QED radiation, respectively. (Note: assume typo in Table 2 that $x_P$ really means $\log x_P$.).

Diffractive DIS dijet cross section measured differentially as a function of $z_P$. The global normalisation uncertainty of $7.8\%$ is not listed explicitly but is included in the total systematic uncertainty. The last two column show the correction factors for hadronisation and QED radiation, respectively.

Diffractive DIS dijet cross section measured differentially as a function of $p^{\ast}_{T,1}$.

Diffractive DIS dijet cross section measured differentially as a function of $p^{\ast}_{T,2}$.

Diffractive DIS dijet cross section measured differentially as a function of $\langle p^{\ast}_{T}\rangle$.

Diffractive DIS dijet cross section measured differentially as a function of $\Delta\eta^{\ast}$.

Diffractive DIS dijet cross section measured differentially as a function of $z_P$ and $Q^2$.

Diffractive DIS dijet cross section measured differentially as a function of $p^{\ast}_{\rm T,1}$ and $Q^2$.

Double-differential trijet cross sections measured as a function of Q**2 and MEAN(PT(3JET)) using the kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential trijet cross sections measured as a function of Q**2 and XI(3) using the kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential inclusive jet cross sections measured as a function of Q**2 and PT(JET) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.5% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential dijet cross sections measured as a function of Q**2 and MEAN(PT(2JET)) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.6% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential dijet cross sections measured as a function of Q**2 and XI(2) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.6% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential trijet cross sections measured as a function of Q**2 and MEAN(PT(3JET)) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential trijet cross sections measured as a function of Q**2 and XI(3) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised inclusive jet cross sections measured as a function of Q**2 and PT(JET) using the kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.5% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised dijet cross sections measured as a function of Q**2 and MEAN(PT(2JET)) using the kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.6% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised inclusive dijet cross sections measured as a function of Q**2 and XI(2) using the kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.6% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised trijet cross sections measured as a function of Q**2 and MEAN(PT(3JET)) using the kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised trijet cross sections measured as a function of Q**2 and XI(3) using the kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised inclusive jet cross sections measured as a function of Q**2 and PT(JET) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.5% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised dijet cross sections measured as a function of Q**2 and MEAN(PT(2JET)) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.6% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised inclusive dijet cross sections measured as a function of Q**2 and XI(2) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.6% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised trijet cross sections measured as a function of Q**2 and MEAN(PT(3JET)) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Double-differential normalised trijet cross sections measured as a function of Q**2 and XI(3) using the anti-kT jet algorithm. The total systematic uncertainty sums all systematic uncertainties in quadrature, including the uncertainty due to the LAr noise of 0.9% and the total normalisation uncertainty of 2.9%. The correction factors on the theoretical cross sections C(HAD) and C(EW) are listed in the rightmost columns.

Differential cross sections for inclusive jet production in charm events as a function of ETARAP(JET) for -1.6 < ETARAP(JET) < 2.2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in beauty events as a function of Q**2 for 5 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in beauty events as a function of Q**2 for 5 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in beauty events as a function of XB. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in charm events as a function of XB. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 5 < Q**2 < 20 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 20 < Q**2 < 60 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 60 < Q**2 < 120 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 120 < Q**2 < 400 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 400 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 5 < Q**2 < 20 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 20 < Q**2 < 60 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 60 < Q**2 < 120 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 120 < Q**2 < 400 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 400 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=17 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=24 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=32 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=45 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=60 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=80 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=110 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=5 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=7 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=9 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=12 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=17 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=24 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=32 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=45 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=60 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=80 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 318 GeV and Q^2=110 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=7 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=9 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=12 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=17 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=24 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=32 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=45 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=60 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=80 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=110 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=5 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=7 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=9 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=12 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=17 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=24 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=32 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=45 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=60 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=80 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 251 GeV and Q^2=110 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=7 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=9 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=12 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=17 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=24 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=32 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=45 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=60 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=80 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=110 GeV^2 for the central-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=5 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=7 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=9 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=12 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=17 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=24 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=32 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=45 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=60 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=80 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 225 GeV and Q^2=110 GeV^2 for the shifted-vertex region. The (sys) error shown in the table is the total systematic uncertainty, excluding the normalisation uncertainties shown separately below.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=9 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=12 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=17 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=24 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=32 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=45 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=60 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=80 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

The reduced cross section for the reaction E+ P --> E+ X at a centre-of-mass energy 300 GeV and Q^2=110 GeV^2 for the years 1996 and 1997, after adjustment for FL extraction.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=9 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=12 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=17 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=24 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=32 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=45 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=60 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=80 GeV^2.

Extracted values of F2 and FL for both unconstrained and constrained fits for Q^2=110 GeV^2.

Extracted values of F2 and R at nine Q^2 points.

D(SIG)/DQ**2 IN NB/GEV**2 as a function of Q**2 IN GEV**2.

D(SIG)/DY IN NB as a function of Y.

D(SIG)/DX IN NB as a function of X.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 5-9 GeV^2.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 9-14 GeV^2.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 14-23 GeV^2.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 23-45 GeV^2.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 45-100 GeV^2.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 100-158 GeV^2.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 158-251 GeV^2.

SIG(C=VIS) IN PB as a function of Y for the Q^2 range 251-1000 GeV^2.

Reduced cross section as a function of X for Q^2 = 7 GeV^2.

Reduced cross section as a function of X for Q^2 = 12 GeV^2.

Reduced cross section as a function of X for Q^2 = 18 GeV^2.

Reduced cross section as a function of X for Q^2 = 32 GeV^2.

Reduced cross section as a function of X for Q^2 = 60 GeV^2.

Reduced cross section as a function of X for Q^2 = 120 GeV^2.

Reduced cross section as a function of X for Q^2 = 200 GeV^2.

Reduced cross section as a function of X for Q^2 = 350 GeV^2.

The single-differential cross section DSIG/DX (Y<0.9,Y(1-x)**2>0.004) at Q^2=3000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The single-differential cross section DSIG/DY (Y<0.9,Y(1-x)**2>0.004) at Q^2=185 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The single-differential cross section DSIG/DY (Y<0.9,Y(1-x)**2>0.004) at Q^2=3000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=200 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=250 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=350 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=450 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=650 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=800 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=1200 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=1500 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=2000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=3000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=5000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=8000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=12000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=20000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The reduced cross section SIG(Reduced) at Q^2=30000 GeV^2, corrected to the electroweak Born level, for zero (Pe=0), positive (Pe=+0.32) and negative (Pe=-0.36) polarisations.

The structure function xF3 at Q^2=1500, 2000 and 3000 GeV^2 extracted using this data at Pe=0 and previously published NC E-P DIS data.

The structure function xF3 at Q^2=5000, 8000 and 12000 GeV^2 extracted using this data at Pe=0 and previously published NC E-P DIS data.

The structure function xF3 at Q^2=20000 and 30000 GeV^2 extracted using this data at Pe=0 and previously published NC E-P DIS data.

The interference structure function XF3(gammaZ) evaulated at Q^2=1500 GeV^2 in X centred bins.

The polarisation asymmetry measured using the positively and negatively polarised positron beams.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of -25.8 % for Q^2 values of 8000, 12000, 20000, 30000 and 50000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 8000, 12000, 20000, 30000 and GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 8000, 12000, 20000, and GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 8000, 12000, 20000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of -25.8 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of -25.8 % for Q^2 values of 5000, 8000, 15000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of +36.0 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of -37.0 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of +32.5 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 90, 120, 150, 200 and 250 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 300, 400, 500, 650 and 800 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 90, 120, 150, 200 and 250 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 300, 400, 500, 650 and 800 GeV^2.

The Neutral Current Reduced Cross Section for E+- P interactions with a beam polarisation of 0 % as a function of Q^2 at Y=0.75.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 8000, 12000, 20000, 30000 and 50000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 120, 150, 200, 250 and 300 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 400, 500, 650, 800 and 1000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 1200, 1500, 2000, 3000 and 5000 GeV^2.

The Neutral Current Reduced Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 8000, 12000, 20000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E- P interactions with a beam polarisation of 0 % for Q^2 values of 5000, 8000, 15000, 30000 and GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 300, 500, 1000, 2000 and 3000 GeV^2.

The Charged Current Double Differential Cross Section for E+ P interactions with a beam polarisation of 0 % for Q^2 values of 5000, 8000, 15000, and GeV^2.

The combined HERA I+II Neutral Current Reduced Cross Section and F2 for E- P interactions with a beam polarisation of 0 %.

The combined HERA I+II Neutral Current Reduced Cross Section and F2 for E+ P interactions with a beam polarisation of 0 %.

The combined HERA I+II Charged Current Double Differential Cross Section and Reduced Cross Section for E- P interactions with a beam polarisation of 0 %.

The combined HERA I+II Charged Current Double Differential Cross Section and Reduced Cross Section for E+ P interactions with a beam polarisation of 0 %.

The Neutral Current DSIG/DQ**2 for E- P interactions with a beam polarisation of -25.8% and +36.0% as a function of Q^2 at Y<0.9.

The Neutral Current DSIG/DQ**2 for E+ P interactions with a beam polarisation of -37.0% and +32.5% as a function of Q^2 at Y<0.9.

The Charged Current DSIG/DQ**2 for E- P interactions with a beam polarisation of -25.8% and +36.0% as a function of Q^2 at Y<0.9.

The Charged Current DSIG/DQ**2 for E+ P interactions with a beam polarisation of -37.0% and +32.5% as a function of Q^2 at Y<0.9.

The Neutral Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The Charged Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The Combined HERA I+ II Neutral Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The Combined HERA I+ II Neutral Current DSIG/DQ**2 for E+- P interactions with a beam polarisation of 0% as a function of Q^2 at Y<0.9.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 200, 250, 300 and 400 GeV^2.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 500, 650, 800 and 1000 GeV^2.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 1200, 1500, 2000 and 3000 GeV^2.

The measured structure function F2(gZ) determined using the polarised HERA II data set for Q^2 values of 5000, 8000, 12000 and 20000 GeV^2.

Averaged structure function F2(gz) for a Q^2 value of 1500 GeV^2 determined using the polarised HERA II data set.

The measured structure function xF3(gZ) determined using the polarised HERA II data set for Q^2 values of 5000, 8000, 12000, 20000 and 30000 GeV^2.

The measured structure function xF3(gZ) determined using the polarised HERA II data set for Q^2 values of 1200, 1500, 2000, 3000 and GeV^2.

Averaged structure function xF3(gz) for a Q^2 value of 1500 GeV^2 determined using the polarised HERA II data set.

Bin averaged differential cross section as a function of ET in the defined phase space.

Bin averaged double differential cross section for inclusive prompt photon production in bins of ET and the pseudorapidity range -1.00 to -0.57.

Bin averaged double differential cross section for inclusive prompt photon production in bins of ET and the pseudorapidity range -0.57 to 0.20.

Bin averaged double differential cross section for inclusive prompt photon production in bins of ET and the pseudorapidity range 0.20 to 0.94.

Bin averaged double differential cross section for inclusive prompt photon production in bins of ET and the pseudorapidity range 0.94 to 1.42.

Bin averaged double differential cross section for inclusive prompt photon production in bins of ET and the pseudorapidity range 1.42 to 2.43.

Bin averaged differential cross section for prompt photon plus jet as a function of the photon transverse energy.

Bin averaged differential cross section for prompt photon plus jet as a function of the photon pseudorapidity.

Bin averaged differential cross section for prompt photon plus jet as a function of the jet transverse energy.

Bin averaged differential cross section for prompt photon plus jet as a function of the jet pseudorapidity.

Bin averaged differential cross section for prompt photon plus jet as a function of X(C=GAMMA,LO) thelongitudinal momentum fraction of the partons in the photon in LO approximation.

Bin averaged differential cross section for prompt photon plus jet as a function of X(C=P,LO) thelongitudinal momentum fraction of the partons in the proton in LO approximation.

Bin averaged differential cross section for prompt photon plus jet as a function of the photons transverse momentum perpendicular to the jet direction separated into two regions of X(C=GAMMA,LO).

Bin averaged differential cross section for prompt photon plus jet as a function of the difference in azimuthal angle between the photon and the jet separated into two regions of X(C=GAMMA,LO).

Single differential cross section DSIG/DZ for D*+- production. The DSYS errors are the uncorrelated and correlated systematicuncertainties respectively.

Single differential cross section DSIG/DLOG(Q**2) for D*+- production. The DSYS errors are the uncorrelated and correlated systematicuncertainties respectively.

Single differential cross section DSIG/DX for D*+- production. The DSYS errors are the uncorrelated and correlated systematicuncertainties respectively.

Double differential cross section for D*+- production in the LOG(Q**2) binfrom 2.0 to 2.2. The DSYS errors are the uncorrelated and correlated systematicuncertainties respectively.

Double differential cross section for D*+- production in the LOG(Q**2) binfrom 2.2 to 2.4. The DSYS errors are the uncorrelated and correlated systematicuncertainties respectively.

Double differential cross section for D*+- production in the LOG(Q**2) binfrom 2.4 to 3.0. The DSYS errors are the uncorrelated and correlated systematicuncertainties respectively.

Measured values of the charm contributions to F2 for a mean Q**2 of 120GeV. The third DSYS error is the model uncertainty.

Measured values of the charm contributions to F2 for a mean Q**2 of 200GeV. The third DSYS error is the model uncertainty.

Measured values of the charm contributions to F2 for a mean Q**2 of 400GeV. The third DSYS error is the model uncertainty.

Measured differential cross section DSIG/DQ**2.

Measured differential cross section DSIG/DX.

Pseudorapidity distribution with additional kinematical restraints on Q**2 and ET.

The DVCS cross section DSIG/DT in three different regions of Q**2.

The DVCS cross section DSIG/DT in three regions of W.

Overall value of the SLOPE parameter of the fit to the DSIG/DT distribution.

Overall value of the fit to the W distribution of the form W**POWER.

Value of the power of the fit to the W distribution of the form W**POWER in three Q**2 regions.

Value of the fitted slope parameter in three Q**2 regions.

Value of the fitted slope parameter in three W regions.

The measured beam charge asymmetry defined as the difference in the DSIG/DPHI distributions between E+ P and E- P collisions.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 318.

The reduced cross section at Q**2 = 24 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 32 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 45 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 251.

The reduced cross section at Q**2 = 24 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 32 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 45 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 60 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 80 GeV**2 for centre-of-mass energy 225.

The reduced cross section at Q**2 = 110 GeV**2 for centre-of-mass energy 225.

FL and F2 at Q**2 = 24 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 32 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 45 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 60 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 80 GeV**2 with no constraints on FL or F2.

FL and F2 at Q**2 = 110 GeV**2 with no constraints on FL or F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and F2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2.

FL and R as a function of Q**2 with no constraints on F2 or FL. The quantites are quoted such that Q**2/X is constant for each value which correspinds to Y = 0.71 at Ecm=225 GeV.

FL and R as a function of Q**2 with the additional constraints that F2 >= 0 and 0 <= FL <= F2. The quantites are quoted such that Q**2/X is constant for each value which correspinds to Y = 0.71 at Ecm=225 GeV.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 318.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 251.

Percentage contributions of the various sources of systematic error for Q**2 = 24 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 32 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 45 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 60 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 80 GeV**2 for centrof-mass energy 225.

Percentage contributions of the various sources of systematic error for Q**2 = 110 GeV**2 for centrof-mass energy 225.

Differential cross section DSIG/DX for the two values of longitudinal polarization of the electron beam.

Differential cross section DSIG/DY for the two values of longitudinal polarization of the electron beam.

Values of the differential cross section DSIG/DQ**2 with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DX with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DY with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DQ**2 with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DX with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the differential cross section DSIG/DY with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlation between cross section bins.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 280 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 530 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 950 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 1700 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 3000 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 5300 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 9500 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 17000 GeV**2.

Values of the reduced cross section for 3 values of longitudinal polarization of the electron beam for Q**2 = 30000 GeV**2.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Values of the reduced cross section with detailed statistical and systematic errors.. The first DSYS is the uncorrelated systematic error and the second is the calorimeter energy scale uncertainty which has significant correlationS between cross section bins.

Differential K0S cross section as a function of Q**2 in the laboratory frame.

Differential K0S cross section as a function of X in the laboratory frame.

Differential K0S cross section as a function of PT in the laboratory frame.

Differential K0S cross section as a function of ETARAP in the laboratory frame.

Differential LAMBDA cross section as a function of Q**2 in the laboratory frame.

Differential LAMBDA cross section as a function of X in the laboratory frame.

Differential LAMBDA cross section as a function of PT in the laboratory frame.

Differential LAMBDA cross section as a function of ETARAP in the laboratoryframe.

Differential K0S cross section as a function of PT in the target hemisphere of the Breit frame.

Differential K0S cross section as a function of PT in the current hemisphere of the Breit frame.

Differential K0S cross section as a function of XP(Breit) in the target hemisphere of the Breit frame.

Differential K0S cross section as a function of XP(Breit) in the current hemisphere of the Breit frame.

Differential LAMBDA cross section as a function of PT in the target hemisphere of the Breit frame.

Differential LAMBDA cross section as a function of PT in the current hemisphere of the Breit frame.

Differential LAMBDA cross section as a function of XP(Breit) in the target hemisphere of the Breit frame.

Differential LAMBDA cross section as a function of XP(Breit) in the currenthemisphere of the Breit frame.

Value of the LAMBDA/K0S cross section ratio as a function of Q**2.

Value of the LAMBDA/K0S cross section ratio as a function of X.

Value of the LAMBDA/K0S cross section ratio as a function of PT.

Value of the LAMBDA/K0S cross section ratio as a function of ETARAP.

Value of the LAMBDA/K0S cross section ratio as a function of PT in the target hemisphere of the Breit frame.

Value of the LAMBDA/K0S cross section ratio as a function of PT in the current hemisphere of the Breit frame.

Value of the LAMBDA/K0S cross section ratio as a function of X in the target hemisphere of the Breit frame.

Value of the LAMBDA/K0S cross section ratio as a function of X in the current hemisphere of the Breit frame.

Value of the HADRON+-/K0S cross section ratio as a function of Q**2.

Value of the HADRON+-/K0S cross section ratio as a function of X.

Value of the HADRON+-/K0S cross section ratio as a function of PT.

Value of the HADRON+-/K0S cross section ratio as a function of ETARAP.

e+e- production cross section at mid rapidity for ultra peripheral Au+Au reactions.The results are given for 3 intervals of masses of the electron pair : 2.0 to 2.3, 2.3 to 2.8 and 2.0 to 2.8 Gev/c2.

Invariant cross section of electrons from charm decay versus PT These values has been obtained using g3data software which to extract the data from the plot and should therefore be used with caution. The values in the last column indicate the level of uncertainty intoduced by g3data.

Invariant cross section of electrons from bottom decay versus PT These values has been obtained using g3data software which to extract the data from the plot and should therefore be used with caution. The values in the last column indicate the level of uncertainty intoduced by g3data.

Total bottom cross section To obtain the total bottom cross section, the differential charm cross section has been extrapolated to the whole rapidity range, using a HVQMNR rapidity distribution with aCTEQ5M PDF.

Inclusive non-diffractive photoproduction single differential cross sections as a function of rapidity in the specified kinematic range.

Reduced cross section as measured in the SVX data sample for Q**2 = 0.50 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the SVX data sample for Q**2 = 0.65 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the SVX data sample for Q**2 = 0.85 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the SVX data sample for Q**2 = 1.20 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the SVX data sample for Q**2 = 1.50 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the SVX data sample for Q**2 = 2.00 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the SVX data sample for Q**2 = 2.50 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the SVX data sample for Q**2 = 3.50 GeV**2. Additional 3 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 0.50 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 0.65 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 0.85 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 1.20 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 1.50 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 2.00 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 2.50 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 3.50 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 5.00 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 6.50 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 8.50 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-BST data sample for Q**2 = 12.00 GeV**2.. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Reduced cross section as measured in the NVX-S9 data sample. Additional 1.1 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 0.2 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 0.25 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 0.35 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 0.5 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 0.65 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 0.85 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 1.2 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 1.5 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 2.0 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 2.5 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 3.5 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 5.0 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 6.5 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 8.5 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Combined H1 reduced cross section and F2 measurement for Q**2 = 12.0 GeV**2. Additional 0.5 PCT luminosity uncertainty not included in the total error.

Measured D+- cross section as a function of X.

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

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

Measured D0/DBAR0 cross section as a function of Q**2.

Measured D0/DBAR0 cross section as a function of X.

Measured D0/DBAR0 cross section as a function of the transverse momentum of the D meson.

Measured D0/DBAR0 cross section as a function of the pseudorapidity of the D meson.

Measured cross section for D+- mesons in Q**2 and Y bins.

Measured cross section for D0/DBAR0 mesons in Q**2 and Y bins.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D+- mesons.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D+- mesons.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D+- mesons.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D0/DBAR0 mesons not coming from D*+- decays.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D0/DBAR0 mesons not coming from D*+- decays.. The second systematic error is from the extrapolation to the full phase space.

The extracted values of the F2(NAME=CHARM) structure function from the production cross section of D0/DBAR0 mesons not coming from D*+- decays.. The second systematic error is from the extrapolation to the full phase space.

The combined F2(NAME=CHARM) structure function from the production cross section of D+- and D0/DBAR0 mesons.. The second systematic error is from the extrapolation to the full phase space.. The additional error from the branching ratio is 3.3 PCT.

The combined F2(NAME=CHARM) structure function from the production cross section of D+- and D0/DBAR0 mesons.. The second systematic error is from the extrapolation to the full phase space.. The additional error from the branching ratio is 3.3 PCT.

The combined F2(NAME=CHARM) structure function from the production cross section of D+- and D0/DBAR0 mesons.. The second systematic error is from the extrapolation to the full phase space.. The additional error from the branching ratio is 3.3 PCT.

Data from the 2000 running period at Q**2 There is an additional 1.2 PCT overall normalisation uncertainty not included.

Data from the 2000 running period at Q**2 There is an additional 1.2 PCT overall normalisation uncertainty not included.

Data from the 2000 running period at Q**2 There is an additional 1.2 PCT overall normalisation uncertainty not included.

Data from the 2000 running period at Q**2 There is an additional 1.2 PCT overall normalisation uncertainty not included.

Data from the 2000 running period at Q**2 There is an additional 1.2 PCT overall normalisation uncertainty not included.

Data from the 2000 running period at Q**2 There is an additional 1.2 PCT overall normalisation uncertainty not included.

Data from the 2000 running period at Q**2 There is an additional 1.2 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Data from the 1996/1997 running period at Q**2 There is an additional 1.7 PCT overall normalisation uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Combined data at Q**2 There is an additional 0.5 PCT correlated uncertainty not included.

Details of the bin-to-bin correlated systematic uncertainties from the 2000 running period.

Details of the bin-to-bin correlated systematic uncertainties from the 1996/1997 running period.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

Details of the bin-to-bin correlated systematic uncertainties from the combined data sets after diagonisation for Q**2.

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.

Cross section for the process GAMMA P --> GAMMA DD as a function of T.

Differential cross sections as a function of X(C=GAMMA) from beauty and charm quarks.

Differential cross sections for the most energetic jet as a function of ET from beauty and charm quarks.

Differential cross sections for the most energetic jet as a function of ET from beauty and charm quarks.

Differential cross sections as a function of the electron ET for the jet associated to the electron from beauty or charm decays.

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.

Differential cross section as a function of the photon ETARAP.

Differential cross section as a function of Q**2.

Differential cross section as a function of the photon ET in the ETARAP bins -1.2 to -0.6.

Differential cross section as a function of the photon ET in the ETARAP bins -0.6 to 0.2.

Differential cross section as a function of the photon ET in the ETARAP bins 0.2 to 0.9.