Differential fiducial cross section of the Z boson $|y|$ in events with $Z(\rightarrow ll)\ge+1$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the leading b-jet $|y|$ in events with $Z(\rightarrow ll)\ge+1$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the $\Delta \phi$ between Z boson and leading $b$-jet in events with $Z(\rightarrow ll)\ge+1$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the $\Delta y$ between Z boson and leading $b$-jet in events with $Z(\rightarrow ll)\ge+1$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the $\Delta R$ between Z boson and leading $b$-jet in events with $Z(\rightarrow ll)\ge+1$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the $\Delta \phi$ between the first two leading $b$-jets in events with $Z(\rightarrow ll)\ge+2$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the $\Delta y$ between the first two leading $b$-jets in events with $Z(\rightarrow ll)\ge+2$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the $\Delta R$ between the first two leading $b$-jets in events with $Z(\rightarrow ll)\ge+2$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the invariant mass of the first two leading $b$-jets in events with $Z(\rightarrow ll)\ge+2$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the Z boson $p_{\text{T}}$ in events with $Z(\rightarrow ll)\ge+2$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the $p_{\text{T}}$ of the first two leading $b$-jets in events with $Z(\rightarrow ll)\ge+2$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

Differential fiducial cross section of the ratio between the $p_{\text{T}}$ and the invariant mass of the first two leading $b$-jets in events with $Z(\rightarrow ll)\ge+2$ b-jets. The statistical uncertainties and the individual components of systematic uncertainty are given in each bin. Statistical uncertainties are bin-to-bin uncorrelated.

The measured fiducial cross section vs $E_{\mathrm{T}}^\gamma$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with Sherpa 2.2.2 at NLO. The uncertainty is defined as Max(stat error, systematic difference between Sherpa LO and Sherpa 2.2.2 NLO), and cannot be considered correlated bin-to-bin. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $|\eta^\gamma|$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with SHERPA 2.2.2 at NLO. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $|\eta^\gamma|$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with Sherpa 2.2.2 at NLO. The uncertainty is defined as Max(stat error, systematic difference between Sherpa LO and Sherpa 2.2.2 NLO), and cannot be considered correlated bin-to-bin. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $m(\ell\ell\gamma)$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with SHERPA 2.2.2 at NLO. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $m(\ell\ell\gamma)$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with Sherpa 2.2.2 at NLO. The uncertainty is defined as Max(stat error, systematic difference between Sherpa LO and Sherpa 2.2.2 NLO), and cannot be considered correlated bin-to-bin. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $p_{\mathrm{T}}^{\ell\ell\gamma}$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with SHERPA 2.2.2 at NLO. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $p_{\mathrm{T}}^{\ell\ell\gamma}$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with Sherpa 2.2.2 at NLO. The uncertainty is defined as Max(stat error, systematic difference between Sherpa LO and Sherpa 2.2.2 NLO), and cannot be considered correlated bin-to-bin. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $\Delta\phi(ll,\gamma)$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with SHERPA 2.2.2 at NLO. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $\Delta\phi(ll,\gamma)$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with Sherpa 2.2.2 at NLO. The uncertainty is defined as Max(stat error, systematic difference between Sherpa LO and Sherpa 2.2.2 NLO), and cannot be considered correlated bin-to-bin. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $p_{\mathrm{T}}^{\ell\ell\gamma}/m(\ell\ell\gamma)$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with SHERPA 2.2.2 at NLO. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

The measured fiducial cross section vs $p_{\mathrm{T}}^{\ell\ell\gamma}/m(\ell\ell\gamma)$. The central values are provided along with the statistical and systematic uncertainties together with the sign information. The statistical and "Uncor" uncertainty should be treated as uncorrelated bin-to-bin, while the rest are correlated between bins, and they are written as signed NP variations. The parton-to-particle correction factor $C_{theory}$ is the ratio of the cross-section predicted by Sherpa LO samples at particle level within the fiducial phase-space region defined in Table 4 to the predicted cross-section at parton level within the same fiducial region but with the smooth-cone isolation prescription defined above replacing the particle-level photon isolation criterion, and with Born-level leptons in place of dressed leptons. This correction should be applied on fixed order parton-level calculations. The systematic uncertainty is evaluated from a comparison with the correction factor obtained using events generated with Sherpa 2.2.2 at NLO. The uncertainty is defined as Max(stat error, systematic difference between Sherpa LO and Sherpa 2.2.2 NLO), and cannot be considered correlated bin-to-bin. In the case that the calculations are valid for dressed leptons, a modified correction factor excluding the Born-to-dressed lepton correction should be applied instead. This correction only takes into account the particle-level isolation criteria, and is provided separately here. The Sherpa 2.2.8 NLO cross-sections given below include a small contribution from EW $Z\gamma jj$ production.

Diphoton production cross section as a function of the diphoton rapidity.

Diphoton production cross section differential in the cosine of the polar angle in the Collins-Soper frame.

Diphoton production cross section differential in the sub-leading to leading photon transverse momentum ratio (z).

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.

Proton structure function F2 at Q**2 = 55 GeV**2.

Proton structure function F2 at Q**2 = 70 GeV**2.

Proton structure function F2 at Q**2 = 90 GeV**2.

Proton structure function F2 at Q**2 = 120 GeV**2.

Proton structure function F2 at Q**2 = 190 GeV**2.

Proton structure function F2 at Q**2 = 320 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 25 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 35 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 45 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 55 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 70 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 90 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 120 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 190 GeV**2.

Total GAMMA* P cross section as a function of W at Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 1.2 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 3 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 6 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 11 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 120 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 190 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 20 GeV for Q**2 = 320 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 25 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 35 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 45 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 55 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 70 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 90 GeV**2.

Cross section for diffractive scattering GAMMA* P --> DD X where M(DD) < 2.3 GeV and M(X) = 30 GeV for Q**2 = 190 GeV**2.

The diffractive cross section multiplied by (Q**2)*(Q**2+M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 1.2 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 3 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 6 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 11 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 20 GeV.

The diffractive cross section multiplied by (Q**2)*(Q**2 M(X)**2) as a function of Q**2 for W=220 GeV and M(X) = 30 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 2 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 2 to 4 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 4 to 8 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 8 to 15 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 15 to 25 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 25 to 35 GeV.

Ratio of the cross section for diffractive scattering to total cross section integrated over the interval M(X) = 0.28 to 35 GeV for W = 220 GeV.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9455 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7353 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4098 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1712 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0588 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0270 and Q**2 = 25 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9605 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7955 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4930 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2244 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0805 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0374 and Q**2 = 35 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9690 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8333 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.5556 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2711 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1011 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0476 and Q**2 = 45 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9745 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8594 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6044 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3125 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1209 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0576 and Q**2 = 55 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9798 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8861 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6604 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3665 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1489 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0722 and Q**2 = 70 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9843 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9091 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7143 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4265 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1837 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.0909 and Q**2 = 90 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9881 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9302 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7692 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4979 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.2308 and Q**2 = 120 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9925 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9548 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8407 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.6109 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.3220 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.1743 and Q**2 = 190 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.9726 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.8989 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.7256 and Q**2 = 320 GeV**2.

The diffractive structure function F2(NAME=D3) as a function of X(NAME=POMERON) for BETA = 0.4444 and Q**2 = 320 GeV**2.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.00015 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.00015 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0003 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0006 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0012 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0025 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0050 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.0050 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.005 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.005.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.010 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.005.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.400.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.020 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.025.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.125.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.040.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.700.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.900.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.030 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Diffractive structure function F2(NAME=D3) for fixed X(NAME=POMERON) = 0.060 and BETA = 0.970.. Statistical and systematic errors added in quadrature.

Differential polarized inclusive jet cross sections as a function of jet transverse energy.

Differential polarized inclusive jet cross sections as a function of photon virtuality, Q**2.

Differential polarized inclusive jet cross sections as a function of photon virtuality, Q**2.

Differential polarized inclusive jet cross sections as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Differential polarized inclusive jet cross sections as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Integrated polarized inclusive-jet cross section in the given kinematical range for the E- beam.

Integrated polarized inclusive-jet cross section in the given kinematical range for the E+ beam.

Differential unpolarized cross section for single jet production as a function of the jet pseudorapidity.

Differential unpolarized cross section for two jet production as a function of the mean jet pseudorapidity.

Differential unpolarized cross section for three jet production as a function of the mean jet pseudorapidity.

Differential unpolarized cross section for single jet production as a function of the jet transverse energy.

Differential unpolarized cross section for two jet production as a function of the mean jet transverse energy.

Differential unpolarized cross section for three jet production as a function of the mean jet transverse energy.

Differential unpolarized cross section for single jet production as a function of photon virtuality, Q**2.

Differential unpolarized cross section for two jet production as a function of photon virtuality, Q**2.

Differential unpolarized cross section for three jet production as a function of photon virtuality, Q**2.

Differential unpolarized inclusive-jet cross section as a function of X. Update: contrary to the publication, this is D(SIG)/DLOG10(X) not D(SIG)/DX.

Integrated unpolarized jet cross section in the given kinemetical region.

Differential unpolarized dijet cross section as a function of the dijet mass.

Differential unpolarized three-jet cross section as a function of the three-jet mass.

Distribution of D(SIG)/DM(P=6) as a function of M(P=6) .

Distribution of D(SIG)/DBETA as a function of BETA .

Distribution of D(SIG)/DX(NAME=POMERON) as a function of X(NAME=POMERON) .

Distribution of D(SIG)/DET(P=4,5,RF=CM) as a function of ET(P=4,5,RF=CM) .

Distribution of D(SIG)/DETARAP(P=4,5,RF=CM) as a function of ETARAP(P=4,5,RF=CM) .

Distribution of D(SIG)/DZ(NAME=POMERON) as a function of Z(NAME=POMERON) .

Distribution of D(SIG)/DX(NAME=GAMMA) as a function of X(NAME=GAMMA) .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DET(P=4,RF=CM) as a function of Z(NAME=POMERON) for ET(P=4,RF=CM) from 5 to 6.5 GeV). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DET(P=4,RF=CM) as a function of Z(NAME=POMERON) for ET(P=4,RF=CM) from 6.5 to 8 GeV). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DET(P=4,RF=CM) as a function of Z(NAME=POMERON) for ET(P=4,RF=CM) from 8 to 16 GeV). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 5 to 12 GeV**2). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 12 to 25 GeV**2). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 25 to 50 GeV**2). .

Distribution of D2(SIG)/DZ(NAME=POMERON)/DQ**2) as a function of Z(NAME=POMERON) for Q**2 from 50 to 100 GeV**2). .

Cross section D(SIG)/X(C=GAMMA,OBS) as a function of X(C=GAMMA,OBS) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/Y as a function of Y in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/Y as a function of Y in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=4) as a function of ET(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=5) as a function of ET(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=6) as a function of ET(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=4) as a function of ET(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=5) as a function of ET(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=6) as a function of ET(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ET(P=7) as a function of ET(P=7) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=4) as a function of ETARAP(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=5) as a function of ETARAP(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=6) as a function of ETARAP(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=4) as a function of ETARAP(P=4) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=5) as a function of ETARAP(P=5) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=6) as a function of ETARAP(P=6) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/ETARAP(P=7) as a function of ETARAP(P=7) in two jet invariant mass regions, 25 to 50 and > 50 GeV .

Cross section D(SIG)/COS(PSI(3)) as a function of COS(PSI(3)) in two jet invariant mass regions, 25 to 50 and > 50 GeV . PSI(3) is the angle in the 3-jet CM frame between the plane containing the highest energy jet (P=4) and the beam, and the plane containing the three jets .

Differential cross sections for diffractive photoproduction of D*+- mesons as a function of M(C=X).

Differential cross sections for diffractive photoproduction of D*+- mesons as a function of PT(C=D*).

Ratio of cross sections for Diffractive to Inclusive photoproduction of D*+- mesons as a function of PT(C=D*).

Differential cross sections for diffractive photoproduction of D*+- mesons as a function of ETARAP(C=D*).

Ratio of cross sections for Diffractive to Inclusive photoproduction of D*+- mesons as a function of ETARAP(C=D*).

Differential cross sections for diffractive photoproduction of D*+- mesons as a function of Z(C=D*).

Ratio of cross sections for Diffractive to Inclusive photoproduction of D*+- mesons as a function of Z(C=D*).

Differential cross sections for diffractive photoproduction of D*+- mesons as a function of W.

Ratio of cross sections for Diffractive to Inclusive photoproduction of D*+- mesons as a function of W.