Muons and jets from beauty photoproduction, energy fraction of the exchanged photon entering the hard subprocess

Muons and jets from beauty in deep-inelastic scattering, negative momentum transfer squared $Q^2$. Jets are reconstructed in the Breit frame of reference.

Muons and jets from beauty in deep-inelastic scattering, Bjorken-x. Jets are reconstructed in the Breit frame of reference.

Muons and jets from beauty in deep-inelastic scattering, muon pseudorapidity. Jets are reconstructed in the Breit frame of reference.

Muons and jets from beauty in deep-inelastic scattering, muon transverse momentum. Jets are reconstructed in the Breit frame of reference.

Muons and jets from beauty in deep-inelastic scattering, leading jet transverse momentum. Jets are reconstructed in the Breit frame of reference.

Muons and jets from beauty in photoproduction and deep-inelastic scattering. in photoproduction, two jets are required, with transverse momentum above 7 and 6 GeV, respectively. In Deep-inelastic scattering, jets are reconstructed in the Breit frame of reference, and only one jet is required, with transverse momentum above 6 GeV.

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.

<K+>/<PI>+.

Inverse slope parameter T.

Inverse slope parameter T.

Inverse slope parameter T.

Inverse slope parameter T.

K-/PI- at y=0.

K-/PI- at y=0.

<K->/<PI->.

<K->/<PI->.

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.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

$\rm dN_{ch}/dy$ versus y distribution derived from the $\rm dN_{ch}/d\eta$ distribution along with pt distributions and particle ratios measured in ALICE. Errors are systematic.

The ratio of the standard deviation of the rapidity distribution of charged particles to that expected from Landau hydrodynamics versus versus $\sqrt{s}$/nucleon-pair. The standard deviation for data for all charged particles is derived from the $\rm dN_{ch}/d\eta$ distributions measured at various energies and converted to $\rm dN_{ch}/dy$ in a consistent manner. The data from the BRAHMS and PHOBOS experiments derived by the present authors from these experiments $dN/d\eta$ distributions.

The measured differential cross section as a function of the pseudorapidity of the photon.

The measured differential cross section as a function of the transverse energy of the jet.

The measured differential cross section as a function of the pseudorapidity of the jet.

Inclusive dijet cross-sections ${d\sigma/dM_{jj}}$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\eta^{*}}$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\log_{10}\left(\xi\right)}$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\log_{10}\left(\xi\right)}$ for ${Q^{2}}$ between 125 and 250 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\log_{10}\left(\xi\right)}$ for ${Q^{2}}$ between 250 and 500 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\log_{10}\left(\xi\right)}$ for ${Q^{2}}$ between 500 and 1000 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\log_{10}\left(\xi\right)}$ for ${Q^{2}}$ between 1000 and 2000 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\log_{10}\left(\xi\right)}$ for ${Q^{2}}$ between 2000 and 5000 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\log_{10}\left(\xi\right)}$ for ${Q^{2}}$ between 5000 and 20000 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\overline{E^{jet}_{T,B}}}$ for ${Q^{2}}$ between 125 and 250 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\overline{E^{jet}_{T,B}}}$ for ${Q^{2}}$ between 250 and 500 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\overline{E^{jet}_{T,B}}}$ for ${Q^{2}}$ between 500 and 1000 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\overline{E^{jet}_{T,B}}}$ for ${Q^{2}}$ between 1000 and 2000 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\overline{E^{jet}_{T,B}}}$ for ${Q^{2}}$ between 2000 and 5000 GeV$^2$. Other details as in the caption to Table 1.

Inclusive dijet cross-sections ${d\sigma/d\overline{E^{jet}_{T,B}}}$ for ${Q^{2}}$ between 5000 and 20000 GeV$^2$. Other details as in the caption to Table 1.

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

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 $\xi$.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Normalised cross sections of forward neutron production in DIS as a function of XF. For each measurement, the statistical, the uncorrelated systematic uncertainties and the bin-to-bin correlated systematic uncertainties due to the FNC absolute energy scale (EFNC), the measurement of the particle impact position in the FNC (XYFNC) and the model dependence of the data correction (model) are given.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Projections of the correlation function C.

Pion HBT radii for the 5% most central collisions.

Pion HBT radii for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions.

Ratio of Pion HBT radii for the OUT projection to that for the SIDE projection for the 5% most central collisions from the STAR experiment at 200 GeV taken from Adams et al. PR C71(2005)044906.;.

Pion HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

Product of the three HBT radii at KT=0.3 for the 5% most central collisions as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

The decoupling time extracted from R_long(KT) as a function of the central charged multiplicity. Data from other experiments is shown for comparison.

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).

The measured differential cross section DSIG/DQ**2 for inclusive jet production using the SIScone jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 125 to 250 GeV for the anti-KT jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 250 to 500 GeV for the anti-KT jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 500 to 1000 GeV for the anti-KT jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 1000 to 2000 GeV for the anti-KT jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 2000 to 5000 GeV for the anti-KT jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 5000 to 100000 GeV for the anti-KT jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 125 to 250 GeV for the SIScone jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 250 to 500 GeV for the SIScone jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 500 to 1000 GeV for the SIScone jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 1000 to 2000 GeV for the SIScone jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 2000 to 5000 GeV for the SIScone jet algorithm.

The measured differential cross section DSIG/DET for inclusive jet production in the Q**2 region 5000 to 100000 GeV for the SIScone jet algorithm.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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