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

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

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

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

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

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

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

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

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

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

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

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 $Q^2$.

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.

The measured differential cross section based on the kT jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ET for jet ETARAP -1 TO 0 . The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the kT jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ET for jet ETARAP 0 TO 1 . The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the kT jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ET for jet ETARAP 1 TO 1.5 . The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the kT jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ET for jet ETARAP 1.5 TO 2 . The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the kT jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ET for jet ETARAP 2 TO 2.5 . The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the anti-kT jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ET for jet ETARAP -1 TO 2.5 . The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the SIScone jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ET for jet ETARAP -1 TO 2.5 . The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the anti-kT jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ETARAP for jet ET > 17 GeV. The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

The measured differential cross section based on the SIScone jet algorithm in the kinematic region Q^2<1 GeV^2 and 142 < W < 293 GeV as a function of the jet ETARAP for jet ET > 17 GeV. The first (sys) error is the uncorrelated systematic error and the second is the jet-energy scale uncertainty.

Total visible cross section for LAMBDA/C+ production for the two decay channels combined. The second systematic error reflects the uncertainty in the branching ratios.

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

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

Measured D+ cross section as a function of Q**2.

Measured D+ cross section as a function of the Bjorken X.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Measured differential cross section as a function of the muon pseudorapidity.

Measured differential cross section as a function of the jet transverse momentum.

Measured differential cross section as a function of the jet pseudorapidity.

Measured cross sections for beauty production with a muon and jet for the Q**2 bin 2 to 4 GeV**2.

Measured cross sections for beauty production with a muon and jet for the Q**2 bin 4 to 20 GeV**2.

Measured cross sections for beauty production with a muon and jet for the Q**2 bin 20 to 45 GeV**2.

Measured cross sections for beauty production with a muon and jet for the Q**2 bin 45 to 100 GeV**2.

Measured cross sections for beauty production with a muon and jet for the Q**2 bin 100 to 250 GeV**2.

Measured cross sections for beauty production with a muon and jet for the Q**2 bin 250 to 3000 GeV**2.

Extracted values of F2 for B-BBAR production at an X value of 0.00013. The second systematic error is the uncertainty on the extrapolation to the full muon and jet phase space.

Extracted values of F2 for B-BBAR production at an X value of 0.0002. The second systematic error is the uncertainty on the extrapolation to the full muon and jet phase space.

Extracted values of F2 for B-BBAR production at an X value of 0.0005. The second systematic error is the uncertainty on the extrapolation to the full muon and jet phase space.

Extracted values of F2 for B-BBAR production at an X value of 0.002. The second systematic error is the uncertainty on the extrapolation to the full muon and jet phase space.

Extracted values of F2 for B-BBAR production at an X value 0.005.

Extracted values of F2 for B-BBAR production at an X value of 0.013. The second systematic error is the uncertainty on the extrapolation to the full muon and jet phase space.