Charged particle mean multiplicities measured in 4x4 kinematic bins of $Q^2$ and $y$.

Charged particle mean multiplicities measured with the additional restriction to select only particles from the current region of the Breit frame $0<\eta^{*}<4$, in 4x4 kinematic bins of $Q^2$ and $y$.

Variance of the charged particle multiplicity measured in 4x4 kinematic bins of $Q^2$ and $y$.

Variance of the charged particle multiplicity measured with the additional restriction to select only particles from the current region of the Breit frame $0<\eta^{*}<4$, in 4x4 kinematic bins of $Q^2$ and $y$.

KNO function for charged particles neasured with the additional restriction to select only particles from the current region of the Breit frame $0<\eta^{*}<4$, in 4x4 kinematic bins of $Q^2$ and $y$.

Hadron entropy for charged particles selected in a sliding pseudorapidity window of 1.4 units size with transverse momenta $P_{T lab}>150$ MeV, in the accessible kinematic bins of momentum transfer $Q^2$ and $y$. The data are presented as a function of $Q^2$ and the corresponding average $x$-Bjorken.

Hadron entropy for charged particles neasured with the additional restriction to select only particles from the current region of the Breit frame $0<\eta^{*}<4$, in 4x4 kinematic bins of $Q^2$ and $y$. The data are presented as a function of $Q^2$ and the corresponding average $x$-Bjorken.

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.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 0-1 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of pseudorapidity for the PT interval 1-10 GeV in fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity PT interval 0-1.5 in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity PT interval 1.5-5 in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 0-1.5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

Charged particle density as a function of PT in the pseudorapidity region 1.5-5 for fixed Q**2 and X intervals in the HCM frame.

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.

The neutral current reduced cross section at Q^2=90 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=120 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=150 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=200 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=250 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=300 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=400 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=500 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=650 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=800 GeV^2 for a proton energy of 460 GeV.

The neutral current reduced cross section at Q^2=35 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=45 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=60 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=90 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=120 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=150 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=200 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=250 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=300 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=400 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=500 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=650 GeV^2 for a proton energy of 575 GeV.

The neutral current reduced cross section at Q^2=800 GeV^2 for a proton energy of 575 GeV.

The proton structure functions FL and F2 measured at Q^2=1.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=2.0 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=2.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=3.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=5.0 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=6.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=8.5 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=12 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=15 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=20 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=25 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=35 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=45 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=60 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=90 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=120 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=150 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=200 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=250 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=300 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=400 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=500 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=650 GeV^2 as a function of X without model assumptions.

The proton structure functions FL and F2 measured at Q^2=800 GeV^2 as a function of X without model assumptions.

The proton structure function FL obtained by averaging the FL data from the previous tables.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0003 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0003 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0010 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=60.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0030 and Q^2=90.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=60.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=90.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=200.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0100 and Q^2=400.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=3.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=5.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=6.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=8.5 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=12.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=15.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=20.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=25.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=35.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=45.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=60.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=90.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=200.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=400.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=800.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

The reduced diffractive cross section multiplied by X_Pomeron at XP=0.0300 and Q^2=1600.0 GeV^2 . The first (sys) error is the uncorrelated systematic error and the second is the correlated systematic error.

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.

The slope of the measured T distribution for elastic PHI meson production.

Full set of spin density matrix elements for elastic electroproduction of PHI mesons for W around 75 GeV.

The value of the combination of matrix elements 2*r^5_{11}+r^{5}_{00} for three Q**2 bins.

Ratio of the longitudinal to transverse cross sections for elastic PHI meson electroproduction.

Normalised distribution in M(P=4_5) for NC and CC dijet events. M(P=4_5) is the dijet mass.

Normalised distribution in ZP for NC and CC dijet events. ZP corresponds to 0.5*MIN(1-COS(THETA*)) summed over the two jets. THETA* is the polar angle of each parton in the c.m. system of the virtual boson and the incoming parton.

Normalised distribution in XP for NC and CC dijet events. XP is the ratio X/PSI where PSI is the fraction of the protons for momentacarried by the parton entering the hard scattering process.

Normalised distribution in ET(C=FOWARD) for NC and CC dijet events. ET(C=FORWARD) is the transverse energy of the most (non-remnant) forward jet.

Normalised distribution in THETA(C=FORWARD) for NC and CC dijet events. THETA(C=FORWARD) is the polar angle of the most (non-remnant) forward jet.

Normalised distribution in dijet mass for CC and NC events with Q**2 > 5000GeV**2.

The multiplicity of charged hadrons for three intervals of mass of the charged hadron system in the forward region.

The multiplicity of charged hadrons for three intervals of mass of the charged hadron system in the backward region.

The multiplicity of positively charged hadrons for three intervals of mass of the charged hadron system in the full phase space region.

The multiplicity of negatively charged hadrons for three intervals of mass of the charged hadron system in the full phase space region.

Charged particle rapidity spectra for three intervals of the mass of the charged haron system.

The central region charged particle density.

The parameter RHO which relects the correlation between the number of particles in the forward and backward hemisphere.