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.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Matrix of statistical correlation coefficients of the unfolded jet cross sections at low $Q^2$.

Matrix of statistical correlation coefficients of the unfolded normalised jet cross sections at low $Q^2$.

Inclusive jet cross sections for $P_T^{\rm jet}$ = 5-7 GeV$^2$ measured as a function of $Q^2$ in the range 150-15000 GeV$^2$. The cross section values and uncertainties have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>). See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections for $P_T^{\rm jet}$ = 5-7 GeV$^2$ measured as a function of $Q^2$ in the range 150-15000 GeV$^2$. The cross section values and uncertainties have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>). See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Matrix of statistical correlation coefficients of the unfolded jet cross sections at high $Q^2$. The statistical correlations have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>).

Matrix of statistical correlation coefficients of the unfolded normalised jet cross sections at high $Q^2$. The statistical correlations have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>).

The strong coupling extracted from the normalised inclusive jet, dijet and trijet data at NLO as a function of the renormalisation scale $\mu_r$. For each $\mu_r$ the values of the strong coupling $\alpha_s(\mu_r)$ and the equivalent values $\alpha_s(M_Z)$ are given with experimental (exp) and theoretical (th) uncertainties.

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.

The combined differential $D^{*\pm}$-production cross section as a function of $Q^2$, with its uncorrelated and correlated uncertainties.

The combined differential $D^{*\pm}$-production cross section as a function of $y$, with its uncorrelated and correlated uncertainties.

The combined double-differential $D^{*\pm}$-production cross section as a function of $Q^2$ and $y$, with its uncorrelated and correlated uncertainties.

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 $Q^2$.

Inclusive Jet Cross Section ${\rm\frac{d\sigma_{jet}}{dP_T}}$.

2-Jet Cross Section ${\rm\frac{d\sigma_{2-jet}}{d\langle P_T \rangle}}$.

3-Jet Cross Section ${\rm\frac{d\sigma_{3-jet}}{d\langle P_T \rangle}}$.

Inclusive Jet Cross Section ${\rm\frac{d^2\sigma_{jet}}{dQ^2dP_T}}$.

2-Jet Cross Section ${\rm\frac{d^2\sigma_{2-jet}}{dQ^2d\langle P_T \rangle}}$.

2-Jet Cross Section ${\rm\frac{d^2\sigma_{2-jet}}{dQ^2d\xi}}$.

3-Jet Cross Section ${\rm\frac{d^2\sigma_{3-jet}}{dQ^2d\langle P_T \rangle}}$.

3-Jet to 2-Jet Cross Sections Ratio ${\rm\frac{d\sigma_{3-jet}}{dQ^2}/\frac{d\sigma_{2-jet}}{dQ^2}}$.

3-Jet to 2-Jet Cross Sections Ratio ${\rm\frac{d\sigma_{3-jet}}{d\langle P_T \rangle}/\frac{d\sigma_{2-jet}}{d\langle P_T \rangle}}$.

3-Jet to 2-Jet Cross Sections Ratio ${\rm\frac{d^2\sigma_{3-jet}}{dQ^2d\langle P_T \rangle}/\frac{d^2\sigma_{2-jet}}{dQ^2d\langle P_T \rangle}}$.

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.

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

3-jet cross section normalised to 2-jet cross section in bins of $Q^{2}$.

Normalised inclusive jet cross section in bins of $Q^{2}$ and $P_{T}$.

Normalised 2-jet cross section in bins of $Q^{2}$ and $\langle P_{T} \rangle$.

Normalised 2-jet cross sections in bins of $Q^2$ and $\xi$.

Bin averaged differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON).

Bin averaged differential cross sections of diffractive di-jet production as a function centre of mass PT of the leading jet.

Bin averaged differential cross sections of diffractive di-jet production as a function of the pseudorapidity difference.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 29 to 50 GeV.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 50 to 70 GeV.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 70 to 100 GeV.

Bin averaged double differential cross sections of diffractive di-jet production as a function of Z(NAME=POMERON) in the (Q**2 + PT(LEADING JET)**2) range 100 to 200 GeV.

Visible cross section for inclusive D*+- production with two jets.

Ratio of visible cross sections of inclusive D*+- production with and without the two jets.

Ratio of visible cross sections of inclusive D*+- production with and without the two jets.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of Q**2.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of Q**2.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of X.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of X.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of W.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of W.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of PT.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of PT.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of ETARAP.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of ETARAP.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of Z.

Differential cross section for inclusive D*+- production in the visible kinematic region as a function of Z.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Double differential cross section for inclusive D*+- production in bins of Q**2 and X.

Differential cross section for inclusive D*+- production as a function of Q**2 with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.

Differential cross section for inclusive D*+- production as a function of Q**2 with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.

Differential cross section for inclusive D*+- production as a function of X with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.

Differential cross section for inclusive D*+- production as a function of X with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.

Differential cross section for inclusive D*+- production as a function of PT with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.

Differential cross section for inclusive D*+- production as a function of PT with the constraint that the transverse momentum of the D* in the virtual photon-proton centre-of-mass frame is > 2 GeV.

Differential cross section for inclusive D*+- production as a function of ETARAP with the constraint that the transverse momentum of the D* in the virtualphoton-proton centre-of-mass frame is > 2 GeV.

Differential cross section for inclusive D*+- production as a function of ETARAP with the constraint that the transverse momentum of the D* in the virtualphoton-proton centre-of-mass frame is > 2 GeV.

Differential cross section for D*+- production with dijets as a function of Q**2.

Differential cross section for D*+- production with dijets as a function of Q**2.

Differential cross section for D*+- production with dijets as a function of X.

Differential cross section for D*+- production with dijets as a function of X.

Differential cross section for D*+- production with dijets as a function of ET(C=JET1).

Differential cross section for D*+- production with dijets as a function of ET(C=JET1).

Differential cross section for D*+- production with dijets as a function of M(C=JET2).

Differential cross section for D*+- production with dijets as a function of M(C=JET2).

Double differential cross section for D*+- production with dijets in bins of Q**2 and PHI(JET1)-PHI(JET2).

Double differential cross section for D*+- production with dijets in bins of Q**2 and PHI(JET1)-PHI(JET2).

Double differential cross section for D*+- production with dijets in bins of Q**2 and PHI(JET1)-PHI(JET2).

Double differential cross section for D*+- production with dijets in bins of Q**2 and PHI(JET1)-PHI(JET2).

Differential cross section for D*+- production with dijets as a function of pseudorapidity of the jet containing D*.

Differential cross section for D*+- production with dijets as a function of pseudorapidity of the jet containing D*.

Differential cross section for D*+- production with dijets as a function of pseudorapidity of the other jet.

Differential cross section for D*+- production with dijets as a function of pseudorapidity of the other jet.

Differential cross section for D*+- production with dijets as a function of the pseudorapidity difference of the two jets.

Differential cross section for D*+- production with dijets as a function of the pseudorapidity difference of the two jets.

Differential cross section for D*+- production with dijets as a function of X(C=GAMMA), the observed fraction of the virtual photon momentum carried by the partons.

Differential cross section for D*+- production with dijets as a function of X(C=GAMMA), the observed fraction of the virtual photon momentum carried by the partons.

Double differential cross section for D*+- production with dijets in bins of Q**2 and X(C=GAMMA), the observed fraction of the virtual photon momentum carried by the partons.

Double differential cross section for D*+- production with dijets in bins of Q**2 and X(C=GAMMA), the observed fraction of the virtual photon momentum carried by the partons.

Differential cross section for D*+- production with dijets as a function of X(C=GLUON), the observed fraction of the proton momentum carried by the gluon.

Differential cross section for D*+- production with dijets as a function of X(C=GLUON), the observed fraction of the proton momentum carried by the gluon.

Double differential cross section for D*+- production with dijets in bins of Q**2 and X(C=GLUON), the observed fraction of the proton momentum carried by the gluon.

Double differential cross section for D*+- production with dijets in bins of Q**2 and X(C=GLUON), the observed fraction of the proton momentum carried by the gluon.

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Inclusive dijet cross section for a lower ET cut off of (5+4) GeV for the highest ET jet.

Inclusive dijet cross section for a lower ET cut off of (5+7) GeV for the highest ET jet.

Inclusive dijet cross section averaged over the indicated Q**2 at ET(MAX) for a lower cut off of ET (5+2) GeV for the highest ET jet.

Inclusive dijet cross section averaged over the indicated regions of X, Q**2 and ABS(DETARAP) for a lower cut off of ET (5+2) GeV for the highest ET jet.

The dijet rate averaged over the indicated regions of Q**2 and X for a lower ET cut off of (5+0) GeV for the highest ET jet.

The dijet rate averaged over the indicated regions of Q**2 and X for a lower ET cut off of (5+1) GeV for the highest ET jet.

The dijet rate averaged over the indicated regions of Q**2 and X for a lower ET cut off of (5+2) GeV for the highest ET jet.

The dijet rate averaged over the indicated regions of Q**2 and X for a lower ET cut off of (5+4) GeV for the highest ET jet.

The dijet rate averaged over the indicated regions of Q**2 and X for a lower ET cut off of (5+7) GeV for the highest ET jet.

Dijet rate averaged over the indicated regions of Q**2, X and ET(MAX) for alower ET cut off of (5+2) GeV for the highest ET jet.

Dijet rate averaged over the indicated regions of Q**2, X and DETARAP for alower ET cut off of (5+2) GeV for the highest ET jet.

Measured ratio of the number of dijets with azimuthal separation < 120 degrees to the total number of dijet events.

The NC cross section DSIG/DX for Q**2 > 10000 GeV**2. There is an additional 1.5 PCT normalization uncertainty.

The CC cross section DSIG/DX for Q**2 > 1000 GeV**2. There is an additional 1.5 PCT normalization uncertainty.

The NC reduced cross section and the electromagnetic structure funcion F2 derived from the data. For Q**2 > 2000 GeV**2 the extraction of F2 is restricted to Y < 0.6.

The CC double differential cross section D2SIG/DX/DQ**2 and the structure function term PHI.

The NC E- P reduced cross section for the high-y analysis. All E- P data not previously reported in EPJ C19 (2001) 269 are given.. There is an additional 1.8 PCT normalization uncertainty.

The NC structure function term PHI and the structure function FL for the E-P data.

The NC structure function term PHI and the structure function FL for the E+P data.

The generalised structure function XF3.

The structure function XF3(C=GAMMA,Z) obtained by averaging over different Q**2 values and transforming to Q**2 = 1500 GeV**2.

Breakdown of errors from table 6, DSIG(C=NC)/DQ**2 as a function of Q**2. All errors are in PCT.

All errors are in PCT.

Breakdown of errors from table 8, DSIG(C=NC)/DX as a function of X. All errors are in PCT.

Breakdown of errors from table 9, DSIG(C=NC)/DX as a function of X. All errors are in PCT.

Breakdown of errors from table 10, DSIG(C=CC)/DX as a function of X. All errors are in PCT.

Breakdown of errors from table 11, F2 as a function of Q**2, X and Y. All errors are in PCT.

Breakdown of errors from table 11, F2 as a function of Q**2, X and Y. PHI(C=NC) is the NC structure function term.. Y+ = 1+(1-Y)**2. DEL(F2),DEL9F3) and DEL(FL) are the corrections to F2 as decribed in the text of the paper.

All errors are in PCT.

Breakdown of errors from table 12, SIG(C=REDUCED) as a function of Q**2 andX. All errors are in PCT.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 21 to 75 GeV and the W(C=GAMMA P) range 95 to 285 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 21 to 35 GeV and the W(C=GAMMA P) range 95 to 285 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 35 to 52 GeV and the W(C=GAMMA P) range 95 to 285 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 52 to 75 GeV and the W(C=GAMMA P) range 95 to 285 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 21 to 35 GeV and the W(C=GAMMA P) range 95 to 212 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 21 to 35 GeV and the W(C=GAMMA P) range 212 to 285 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 35 to 52 GeV and the W(C=GAMMA P) range 95 to 212 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 35 to 52 GeV and the W(C=GAMMA P) range 212 to 285 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 1 GeV**2) integrated over the ET range 52 to 75 GeV and the W(C=GAMMA P) range 212 to 285 GeV.

Measured differential E+ P cross section DSIG/DETARAP for inclusive jet photoproduction(Q**2 < 0.01 GeV**2) integrated over the ET ranges 5 to 12 GeV and 12 to 21 GeV and the W(C=GAMMA P) range 164 to 242 GeV.

Measured differential E+ P cross section DSIG/DET for inclusive jet photoproductionm, with jets defined by the cone algorithm with R = 1, for the two Q**2 ranges integrated over the jet pseudorapidity range -1 to 2.5 in the W(C=GAMMA P) range 164 to 242 GeV.

The scaled GAMMA P cross section at a mean W of 200 GeV as a function of the jet XT for the jet CM rapidity range -0.5 to 0.5. Jets are defined by the conealgorithm with R = 1.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Single differential visible cross section as a function of LOG(X).

Single differential visible cross section as a function of ETARAP.

Single differential visible cross section as a function of Q**2.

Single differential visible cross section as a function of Z.

Double differential visible cross section as a function of ETARAP and Q**2.

Double differential visible cross section as a function of PT and Q**2.

Double differential visible cross section as a function of ETARAP and Z.

Double differential visible cross section as a function of PT and ETARAP.

Double differential visible cross section as a function of PT and Z.

The inclusive visible D*+ cross section extracted in the DGLAP scheme.

The charm structure function extracted in both the DGLAP and CCFM scheme.

The NC single differential cross section, as a function of Q**2 in the range from 200 to 30000 Gev**2, for Y < 0.9 after correction (KCOR) according to theStandard Model expectation from the measured kinematic cuts y < 0.63 for Q**2 < 890 GeV**2. The first DSYS error is the uncorrelated systematic error and the second is the correlated systematic error.

No description provided.

The structure function, F2, and the reduced cross section, in NC DIS scattering at Q**2 from 150 to 30000 GeV**2 as a function if x and y. The individual corrections used to calculate F2 from the cross sections are given in the following table.

The various corrections to the cross sections used to calcuate the F2 values given in the previous table. See the text of the paper for more details.

The CC double differential cross section and the structure function term PHI(C=CC) - see text of the paper for details - at Q**2 from 150 to 1 5000 GeV**2 as a function of both x and y. Also tabulated are the QED corrections to the data, which have already been applied.

CT = The various sources of error (in percent) to the individual NC reduced cross section given in table 6 - see text of paper for more details;DTOT - TOTAL error. DSTA - STATISTICAL error. DUNC - UNCORRELATED SYSTEMATIC error. DUNC(E) - UNCORRELATED SYSTEMATIC error from the positron energy. DUNC(H) - UNCORRELATED SYSTEMATIC error from the hadronic energy. DCOR - CORRELATED SYSTEMATIC error. DCOR(E+) - CORRELATED SYSTEMATIC from one sig variation in the positron energy. DCOR(T+) - CORRELATED SYSTEMATIC from one sig variation in the positron polar angle. DCOR(H+) - CORRELATED SYSTEMATIC from one sig variation in the hadron energy. DCOR(N+) - CORRELATED SYSTEMATIC from one sig variation in the noise subtraction. DCOR(B+) - CORRELATED SYSTEMATIC from one sig variation in the background subtraction.

The various sources of error (in percent) to the individual CC double differential cross sections given in table 7 - see text of paper for more details. DTOT - TOTAL error. DSTA - STATISTICAL error. DUNC - UNCORRELATED SYSTEMATIC error. DUNC(H) - UNCORRELATED SYSTEMATIC error from the hadronic energy. DCOR - CORRELATED SYSTEMATIC error. DCOR(V+) - CORRELATED SYSTEMATIC from one sig variationin the cut on the Vap/Vp ratio. DCOR(H+) - CORRELATED SYSTEMATIC from one sig variation in the hadron energy. DCOR(N+) - CORRELATED SYSTEMATIC from one sig variation in the noise subtraction. DCOR(B+) - CORRELATED SYSTEMATIC from one sig variation in the background subtraction.

The structure function xF3 dtermined by combining the present NC E- data with previously measured E+ data at a proton enetrgy of 820 GeV. (Adloff et al. EPJ C13 (609) 2000.). The luminosity uncertainties of the E+ P and E- P data sets are included in the systematic error.

The total CC cross section in the region Q**2 > 1000 GeV**2 and Y > 0.9 after applying a small correction factor from the measured Y range from 0.03 0.85.

Inclusive di-jet cross section as a function of the di-jet mass M and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of Y (inelasticity) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and ET.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETARAP(forward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETARAP(backward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the inclusive kT alogrithm.

Inclusive single jet cross section as a function of ET and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive dijet cross section as a function Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of ET and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of the di-jet mass M and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of Y (inelasticity) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and ET.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of ETARAP(forward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive di-jet cross section as a function of ETARAP(backward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the Aachen alogrithm.

Inclusive dijet cross section as a function Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of ET and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of the di-jet mass M and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of Y (inelasticity) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and ET.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETARAP(forward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive di-jet cross section as a function of ETARAP(backward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the exclusive kT alogrithm.

Inclusive dijet cross section as a function Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of ET and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of the di-jet mass M and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XI (=XBJ/XP) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of XP and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of X (=XBJ) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of Y (inelasticity) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and ET.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of ETAPRIME ((ETARAP(P=3)-ETARAP(P=4))/2) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of ETARAP(forward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

Inclusive di-jet cross section as a function of ETARAP(backward jet in lab frame) and Q**2.. Data are analysed in the Breit frame using the Cambridge jet alogrithm.

The NC single differential cross section, as a function of Q**2 in the range from 200 to 30000 Gev**2, measured for y < 0.9 and final state electron energy> 11 Gev, and also with the same y cut but after correction for the electron en ergy cut. Also tabulated are the QED corrections to the data, which have alreadybeen applied. The first DSYS error is the uncorrelated systematic error and the second is the correlated systematic error.

The CC single differential cross section, as a function of Q**2 in the range from 300 to 15000 Gev**2, measured for 0.03 < y < 0.85 and final state electron PT > 12 Gev, and also with the same y cut but after correction for the electron PT cut. Also tabulated are the QED corrections to the data, which have alreadybeen applied. The first DSYS error is the uncorrelated systematic error and the second is the correlated systematic error.

The various sources of error (in percent) to the individual NC reduced cross section given in table 4 - see text of paper for more details. DTOT - TOTAL error. DSTA - STATISTICAL error. DUNC - UNCORRELATED SYSTEMATIC error. DUNC(E) - UNCORRELATED SYSTEMATIC error from the positron energy. DUNC(T) - UNCORRELATED SYSTEMATIC error from the polar positron angle. DUNC(H) - UNCORRELATED SYSTEMATIC error from the hadronic energy. DCOR - CORRELATED SYSTEMATIC error. DCOR(E+) - CORRELATED SYSTEMATIC from one sig variation in the positron energy. DCOR(T+) - CORRELATED SYSTEMATIC from one sig variation in the positron polar angle. DCOR(H+) - CORRELATED SYSTEMATIC from one sig variation in the hadron energy. DCOR(N+) - CORRELATED SYSTEMATIC from one sig variation in the noise subtraction. DCOR(B+) - CORRELATED SYSTEMATIC from one sig variation in the background subtraction.

The various sources of error (in percent) to the individual CC double differential cross sections given in table 5 - see text of paper for more details. DTOT - TOTAL error. DSTA - STATISTICAL error. DUNC - UNCORRELATED SYSTEMATIC error. DUNC(H) - UNCORRELATED SYSTEMATIC error from the hadronic energy. DCOR - CORRELATED SYSTEMATIC error. DCOR(V+) - CORRELATED SYSTEMATIC from one sig variationin the cut on the Vap/Vp ratio. DCOR(H+) - CORRELATED SYSTEMATIC from one sig variation in the hadron energy. DCOR(N+) - CORRELATED SYSTEMATIC from one sig variation in the noise subtraction. DCOR(B+) - CORRELATED SYSTEMATIC from one sig variation in the background subtraction.

DIS cross section as a function of the transverse D* pseudo-rapidity.

DIS cross section as a function of the four-momentum transfer squared, Q**2.

DIS cross section as a function of the observed gluon momentum fraction, X(C=GAMMA,OBS).

Differential photoproduction cross section as a function of the rapidity of the D* for the ETAG33 data sample.

Differential photoproduction cross section as a function of the transverse momentum of the D* for the ETAG33 data sample.

Differential photoproduction cross section as a function of the rapidity of the D* for the ETAG44 data sample.

Differential photoproduction cross section as a function of the transverse momentum of the D* for the ETAG44 data sample.

Double differential photoproduction cross section as a function of the rapidity of the D* for three ranges of transverse momentum at an average W 0f 194 GeV.

Differential photoproduction cross section as a function of the gluon momentum fraction from the ETAG33 data sample.

Differential photoproduction cross section as a function of the gluon momentum fraction from the ETAG44 data sample.

No description provided.

No description provided.

No description provided.

No description provided.

Effective photon parton distribution in the form X(C=GAMMA)*PDF(X,PT**2). The second systematic error is due to the uncertainty in the extraction ofthe PDF resulting from multiple parton scattering effects which was determined using the two event generators PYTHIA and PHOJET.