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.

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.

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

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

The semi-inclusive leading neutron structure function for Q**2.

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).

Measured differential photoproduction cross sections as a function of the squared transverse momentum of the J/PSI in 4 bins of elasticity.

Measured differential photoproduction cross sections as a function of the elasticity of the J/PSI in 4 bins of transverse momentum.

Measured differential electroproduction cross section as a function of Q**2.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P frame.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured differential electroproduction cross section as a function of the photon-proton centre of mass energy W.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P rest frame.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P rest frame.

Measured differential electroproduction cross section as a function of the squared transverse momentum of the J/PSI in the GAMMA* P rest frame.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured differential electroproduction cross section as a function of the elasticity of the J/PSI.

Measured polarization parameter in the Helicity Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

Measured polarization parameter in the Collins-Soper Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

Measured polarization parameter in the Helicity Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

Measured polarization parameter in the Collins-Soper Frame. Here ALPHA is given by DSIG/DCOS(THETA) ~ 1+ ALPHA COS(THETA)**2 and NU is given by DSIG/DPHI ~ 1+ ALPHA/3 + (NU/3)*COS(2THETA).

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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.

Q**2 dependence of the GAMMA* P cross section for proton dissociative PHI meson production at mean W There is an additional overall normalization uncertainty of 5.3 PCT.

Q**2 dependence of the ratio pf the PHI to RHO0 elastic cross section for mean W There is an additional overall normalization uncertainty of 4.0 PCT.

Q**2 + MASS(V)**2 dependence of the ratio pf the PHI to RHO0 elastic cross section for mean W There is an additional overall normalization uncertainty of 4.0 PCT.

Q**2 dependence of the longitudinal and transverse GAMMA* P cross sections for elastic RHO0 production at mean W There is an additional overall normalization uncertainty of 3.9 PCT.

Q**2 dependence of the longitudinal and transverse GAMMA* P cross sections for elastic PHI production at mean W There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for elastic RHO0 production for Q**2 There is an additional overall normalization uncertainty of 3.9 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production for Q**2 There is an additional overall normalization uncertainty of 4.6 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production for Q**2 There is an additional overall normalization uncertainty of 4.6 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production for Q**2 There is an additional overall normalization uncertainty of 4.6 PCT.

W dependence of the GAMMA* P cross section for elastic PHI production for Q**2 There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for elastic PHI production for Q**2 There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for elastic PHI production for Q**2 There is an additional overall normalization uncertainty of 4.7 PCT.

W dependence of the GAMMA* P cross section for dissociative PHI production for Q**2 There is an additional overall normalization uncertainty of 5.3 PCT.

T dependence of the GAMMA* P cross section for elastic RHO0 production for several values. There is an additional overall normalization uncertainty of 3.9 PCT.

T dependence of the GAMMA* P cross section for dissociative RHO0 production for several values. There is an additional overall normalization uncertainty of 4.6 PCT.

T dependence of the GAMMA* P cross section for elastic PHI production for several values. There is an additional overall normalization uncertainty of 4.7 PCT.

T dependence of the GAMMA* P cross section for dissociative PHI production for several values. There is an additional overall normalization uncertainty of 5.3 PCT.

Q**2 dependence of the slope of the T distribution in elastic RHO0 production.

Q**2 dependence of the slope of the T distribution in elastic PHI production.

Q**2 dependence of the slope of the T distribution in dissociative RHO0 production.

Q**2 dependence of the slope of the T distribution in dissociative PHI production.

W dependence of the GAMMA* P cross section for dissociative RHO0 production in four ABS(T) bins at Q**2 There is an additional normalization uncertainty of 4 PCT.

W dependence of the GAMMA* P cross section for dissociative RHO0 production in four ABS(T) bins at Q**2 There is an additional normalization uncertainty of 4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic RHO0 meson total cross section. There is an additional overall normalization uncertainty of 2.4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic PHI meson total cross section. There is an additional overall normalization uncertainty of 2.4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic RHO0 meson differential cross section at T=0. There is an additional overall normalization uncertainty of 2.4 PCT.

Q**2 dependence of the ratio of proton dissociative to elastic PHI mesondifferential cross section at T=0. There is an additional overall normalization uncertainty of 2.4 PCT.

Slope differences between elastic and proton dissociative scattering for RHO0 meson production.

Slope differences between elastic and proton dissociative scattering for PHI meson production.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of Q**2.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of W.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of PHI mesons as a function of T.

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Spin density matrix elements for diffractive electroproduction of RHO0 mesons as a function of M(PI+PI-).

Q**2 dependence of the matrix element combination RHO(JJ=5,MM=00) + 2*RHO(JJ=5,MM=11).

Q**2 dependence of the matrix element combination RHO(JJ=1,MM=00) + 2*RHO(JJ=1,MM=11).

T dependence of the matrix element combination RHO(JJ=5,MM=00) + 2*RHO(JJ=5,MM=11).

T dependence of the matrix element combination RHO(JJ=1,MM=00) + 2*RHO(JJ=1,MM=11).

Q**2 dependence of the ratio R.

Q**2 dependence of the ratio R.

W dependence of the ratio R.

W dependence of the ratio R.

W dependence of the ratio R.

T dependence of the ratio R.

T dependence of the ratio R.

Di-pion mass dependence of the ratio R.

Di-pion mass dependence of the ratio R.

Dependence of the exponential slope of the T distribution as a function of the di-pion mass for the Q**2 range 2.5 to 5 GeV**2.

Dependence of the exponential slope of the T distribution as a function of the di-pion mass for the Q**2 range 5 to 60 GeV**2.

Q**2 dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production.

Q**2 dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for PHI production.

T dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 2.5 to 5 GeV**2.

T dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 5 to 60 GeV**2.

T dependence of the ratio of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for PHI production in the Q**2 range 2.5 to 60 GeV**2.

Di-pion mass dependence of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 2.5 to 5 GeV**2.

Di-pion mass dependence of the helicity amplitudes (assumed purely imaginary) and phase difference between the T11 and T00 amplitudes for RHO0 production in the Q**2 range 5 to 60 GeV**2.