Flux-integrated differential $\nu_{e}$ CCQE-like cross section versus electron angle.

Covariance matrix for flux-integrated differential $\nu_{e}$ CCQE-like cross section versus electron angle.

The flux-integrated differential $\nu_{e}$ CCQE-like cross section versus $Q^{2}_{\rm QE}$.

Covariance matrix for the flux-integrated differential $\nu_{e}$ CCQE-like cross section versus $Q^{2}_{\rm QE}$.

The ratio of the MINERvA $\nu_{e}$ CCQE differential cross section as a function of $Q^2_{\rm QE}$ to the analogous result from MINERvA for $\nu_{\mu}$ [Phys.Rev.Lett. 111 (2013) 022502].

Covariance matrix for the ratio of the MINERvA $\nu_{e}$ CCQE differential cross section as a function of $Q^2_{\rm QE}$ to the analogous result from MINERvA for $\nu_{\mu}$ [Phys.Rev.Lett. 111 (2013) 022502].

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 $Q^2$.

Differential cross sections for inclusive jet production in charm events as a function of ETARAP(JET) for -1.6 < ETARAP(JET) < 2.2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in beauty events as a function of Q**2 for 5 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in beauty events as a function of Q**2 for 5 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in beauty events as a function of XB. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Differential cross sections for inclusive jet production in charm events as a function of XB. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 5 < Q**2 < 20 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 20 < Q**2 < 60 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 60 < Q**2 < 120 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 120 < Q**2 < 400 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in beauty events as a function of XB for 400 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 5 < Q**2 < 20 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 20 < Q**2 < 60 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 60 < Q**2 < 120 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 120 < Q**2 < 400 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

Double-differential cross sections for inclusive jet production in charm events as a function of XB for 400 < Q**2 < 1000 GeV**2. The measurements are given together with their statistical and systematic uncertainties. Hadronisation and QED radiative corrections, CHAD and CRAD, respectively, are also shown.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(BOTTOM BOTTOMBAR) and the reduced beauty cross sections SIGR(BOTTOM BOTTOMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

The structure function F2(CHARM CHARMBAR) and the reduced charm cross sections SIGR(CHARM CHARMBAR), both as functions of XB and Q**2. The measurements are given together with their statistical, systematic and extrapolation uncertainties.

Production cross section for two-photon data as a function of W.

Production cross section for two-photon data as a function of W.

Measured production cross section for the E+ E- process as a function of W for Q**2 from 1.2 to 8.5 GeV**2 for the Z-pole data.

Measured production cross section for the E+ E- process as a function of W for Q**2 from 8.8 to 30 GeV**2 for the high energy data.

Measured production cross section cross section for the two photon process as a function of W for Q**2 from 1.2 to 8.5 GeV**2 for the Z-pole data.

Measured production cross section cross section for the two photon process as a function of W for Q**2 from 8.8 to 30 GeV**2 for the high energy data.

Measured production cross section for the two-photon process as a function of W for Q**2 from 1.2 to 8.5 GeV**2 for the Z-pole data.

Measured production cross section for the two-photon process as a function of W for Q**2 from 8.8 to 30 GeV**2 for the high energy data.

The differential cross section as a function of pseudorapidity.

The differential cross section as a function of log(M(P=5)**2).

The differential cross section as a function of X(C=D*).

The differential cross section as a function of BETA.

The differential cross section as a function of LOG(BETA).

The differential cross section as a function of LOG(Q**2).

The differential cross section as a function of W.

Overall ratio of diffractively produced D*+- mesons to inclusive D*+- mesons.

Ratio of diffractively produced D*+- mesons to inclusive D*+- mesons as a function of transverse momentum.

Ratio of diffractively produced D*+- mesons to inclusive D*+- mesons as a function of pseudorapidity.

Ratio of diffractively produced D*+- mesons to inclusive D*+- mesons as a function of X(C=D*).

Ratio of diffractively produced D*+- mesons to inclusive D*+- mesons as a function of LOG(Q**2).

Ratio of diffractively produced D*+- mesons to inclusive D*+- mesons as a function of W.

Differential cross section as a function of LOG(BETA) in different regions of Q**2 and X(NAME=POMERON).

The measured charm contribution to the diffractive structure function of the proton F2(C=D(3),CHARM).

Differential cross section as a function of the ratio of the virtualities of the two photons.

Differential cross section as a function of the acolinearity angle PHI between the scattered electrons.

Differential cross section as a function of the acolinearity angle DEL(PHI) between the scattered electrons.

Differential cross section as a function of W of the hadronic system.

Differential cross section as a function of the Bjorken X.

Differential cross section as a function of the DIS Y variable.

Differential cross section as a function of LOG(S/S0).

Cross sections as a function of W for the lower Q**2, Z pole, data.

Cross sections as a function of W for the high Q**2 data.

Cross sections for the two photon RHO0 RHO0 and non-resonance data for the lower Q**2, Z pole, data.

Cross sections for the two photon RHO0 RHO0 and non-resonance data for the higher Q**2 data.