Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the inclusive jet multiplicity.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the inclusive jet multiplicity.

Differential cross section for the production of W bosons as a function of H_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of H_T for events with N_jets ≥ 1.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the H_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the H_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the H_T for events with N_jets ≥ 1.

Differential cross section for the production of W bosons as a function of the W p_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the W p_T for events with N_jets ≥ 1.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the W p_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the W p_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the W p_T for events with N_jets ≥ 1.

Differential cross section for the production of W bosons as a function of the leading jet p_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the leading jet p_T for events with N_jets ≥ 1.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the leading jet p_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the leading jet p_T for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the leading jet p_T for events with N_jets ≥ 1.

Differential cross section for the production of W bosons as a function of the leading jet rapidity for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the leading jet rapidity for events with N_jets ≥ 1.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the leading jet rapidity for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the leading jet rapidity for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the leading jet rapidity for events with N_jets ≥ 1.

Differential cross section for the production of W bosons as a function of second leading jet p_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of second leading jet p_T for events with N_jets ≥ 2.

Differential cross section for the production of W bosons as a function of second leading jet rapidity for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of second leading jet rapidity for events with N_jets ≥ 2.

Differential cross section for the production of W bosons as a function of Δ R_jet1,jet2 for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of Δ R_jet1,jet2 for events with N_jets ≥ 2.

Differential cross section for the production of W bosons as a function of dijet invariant mass for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of dijet invariant mass for events with N_jets ≥ 2.

Cross section for the production of W bosons as a function of exclusive jet multiplicity.

Statistical correlation between bins in data for the cross section for the production of W bosons as a function of exclusive jet multiplicity.

Differential cross section for the production of W bosons as a function of the H_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the H_T for events with N_jets ≥ 2.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the H_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the H_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the H_T for events with N_jets ≥ 2.

Differential cross section for the production of W bosons as a function of the W p_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the W p_T for events with N_jets ≥ 2.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the W p_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the W p_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the W p_T for events with N_jets ≥ 2.

Differential cross section for the production of W bosons as a function of the leading jet p_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the leading jet p_T for events with N_jets ≥ 2.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the leading jet p_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the leading jet p_T for events with N_jets ≥ 2.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the leading jet p_T for events with N_jets ≥ 2.

Differential cross section for the production of W bosons as a function of the electron η for events with N_jets ≥ 0.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the electron η for events with N_jets ≥ 0.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the electron η for events with N_jets ≥ 0.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the electron η for events with N_jets ≥ 0.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the electron η for events with N_jets ≥ 0.

Differential cross section for the production of W bosons as a function of the electron η for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the electron η for events with N_jets ≥ 1.

Differential cross sections for the production of W⁺ bosons, W^- bosons and the W⁺/W^- cross section ratio as a function of the electron η for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W⁺ bosons as a function of the electron η for events with N_jets ≥ 1.

Statistical correlation between bins in data for the differential cross sections for the production of W^- bosons as a function of the electron η for events with N_jets ≥ 1.

List of experimentally considered systematic uncertainties for the W+jets cross section measurement

Non-perturbative corrections for the cross section for the production of W bosons for different inclusive jet multiplicities.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the inclusive jet multiplicity.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of H_T for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the H_T for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the W p_T for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the W p_T for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the leading jet p_T for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the leading jet p_T for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the leading jet rapidity for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the leading jet rapidity for events with N_jets ≥ 1.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of second leading jet p_T for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of second leading jet rapidity for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of Δ R_jet1,jet2 for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of dijet invariant mass for events with N_jets ≥ 2.

Non-perturbative corrections for the cross section for the production of W bosons as a function of exclusive jet multiplicity.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the H_T for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the H_T for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the W p_T for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the W p_T for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the leading jet p_T for events with N_jets ≥ 2.

Non-perturbative corrections for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the leading jet p_T for events with N_jets ≥ 2.

NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the H_T for events with N_jets ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].

NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the W p_T for events with N_jets ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].

NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the leading jet p_T for events with N_jets ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].

NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W⁺ bosons and W^- bosons as a function of the leading jet rapidity for events with N_jets ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].

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.

Measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_\text{T}^{\text{lead }\ell}$.

Statistical correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_\text{T}^{\text{lead }\ell}$.

Total correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_\text{T}^{\text{lead }\ell}$.

Measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $m_{e\mu}$.

Statistical correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $m_{e\mu}$.

Total correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $m_{e\mu}$.

Measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_{T}^{e\mu}$.

Statistical correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_{T}^{e\mu}$.

Total correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_{T}^{e\mu}$.

Measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|y_{e\mu}|$.

Statistical correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|y_{e\mu}|$.

Total correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|y_{e\mu}|$.

Measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $\Delta\phi_{e\mu}$.

Statistical correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $\Delta\phi_{e\mu}$.

Total correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $\Delta\phi_{e\mu}$.

Measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|cos(\theta^*)|$.

Statistical correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|cos(\theta^*)|$.

Total correlation between bins in data for the measured fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|cos(\theta^*)|$.

Measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_\text{T}^{\text{lead }\ell}$.

Statistical correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_\text{T}^{\text{lead }\ell}$.

Total correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_\text{T}^{\text{lead }\ell}$.

Measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $m_{e\mu}$.

Statistical correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $m_{e\mu}$.

Total correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $m_{e\mu}$.

Measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_{T}^{e\mu}$.

Statistical correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_{T}^{e\mu}$.

Total correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $p_{T}^{e\mu}$.

Measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|y_{e\mu}|$.

Statistical correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|y_{e\mu}|$.

Total correlation between bins in data for the measured normalized fiducial cross-section of $WW\rightarrow e\mu$ production for the observable $|y_{e\mu}|$.

Measured normalized fiducial cross section of $WW\rightarrow e\mu$ production for the observable $\Delta\phi_{e\mu}$.

Statistical correlation between bins in data for the measured normalized fiducial cross section of $WW\rightarrow e\mu$ production for the observable $\Delta\phi_{e\mu}$.

Total correlation between bins in data for the measured normalized fiducial cross section of $WW\rightarrow e\mu$ production for the observable $\Delta\phi_{e\mu}$.

Measured normalized fiducial cross section of $WW\rightarrow e\mu$ production for the observable $|cos(\theta^*)|$.

Statistical correlation between bins in data for the measured normalized fiducial cross section of $WW\rightarrow e\mu$ production for the observable $|cos(\theta^*)|$.

Total correlation between bins in data for the measured normalized fiducial cross section of $WW\rightarrow e\mu$ production for the observable $|cos(\theta^*)|$.

List of experimentally considered systematic uncertainties for the WW cross section measurement.

Extrapolated unfolded fiducial cross-section of $WW\rightarrow e\mu$ production as a function of $p_\text{T}^{\text{lead }\ell}$.

Extrapolated unfolded fiducial cross-section of $WW\rightarrow e\mu$ production as a function of $m_{e\mu}$.

Extrapolated unfolded fiducial cross-section of $WW\rightarrow e\mu$ production as a function of $p_{T}^{e\mu}$.

XP distribution at c.m. energy 172.0 GeV.

XP distribution at c.m. energy 183.0 GeV.

XP distribution at c.m. energy 189.0 GeV.

XP distribution at c.m. energy 196.0 GeV.

XP distribution at c.m. energy 200.0 GeV.

XP distribution at c.m. energy 206.0 GeV.

Peak position in XI distribution for different c.m. energies.

XI distribution at c.m. energy 133.0 GeV.

XI distribution at c.m. energy 161.0 GeV.

XI distribution at c.m. energy 172.0 GeV.

XI distribution at c.m. energy 183.0 GeV.

XI distribution at c.m. energy 189.0 GeV.

XI distribution at c.m. energy 196.0 GeV.

XI distribution at c.m. energy 200.0 GeV.

XI distribution at c.m. energy 206.0 GeV.

XE distribution at c.m. energy 133.0 GeV.

XE distribution at c.m. energy 161.0 GeV.

XE distribution at c.m. energy 172.0 GeV.

XE distribution at c.m. energy 183.0 GeV.

XE distribution at c.m. energy 189.0 GeV.

XE distribution at c.m. energy 196.0 GeV.

XE distribution at c.m. energy 200.0 GeV.

XE distribution at c.m. energy 206.0 GeV.

PTIN distribution at c.m. energy 133.0 GeV.

PTIN distribution at c.m. energy 161.0 GeV.

PTIN distribution at c.m. energy 172.0 GeV.

PTIN distribution at c.m. energy 183.0 GeV.

PTIN distribution at c.m. energy 189.0 GeV.

PTIN distribution at c.m. energy 196.0 GeV.

PTIN distribution at c.m. energy 200.0 GeV.

PTIN distribution at c.m. energy 206.0 GeV.

PTOUT distribution at c.m. energy 206.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 133.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 161.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 172.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 183.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 189.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 196.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 200.0 GeV.

RAPIDITY W.R.T THRUST AXIS distribution at c.m. energy 206.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 133.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 161.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 172.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 183.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 189.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 196.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 200.0 GeV.

RAPIDITY W.R.T. SPHERICITY AXIS distribution at c.m. energy 206.0 GeV.

Combined results for ALPHAS.

Event shape means.

THRUST distribution at c.m. energy 91.20 GeV.

1-THRUST distribution at c.m. energy 133.00 GeV.

1-THRUST distribution at c.m. energy 161.00 GeV.

1-THRUST distribution at c.m. energy 172.00 GeV.

1-THRUST distribution at c.m. energy 183.00 GeV.

1-THRUST distribution at c.m. energy 189.00 GeV.

1-THRUST distribution at c.m. energy 200.00 GeV.

1-THRUST distribution at c.m. energy 206.00 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 91.20 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 133.00 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 161.00 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 172.00 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 183.00 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 189.00 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 200.00 GeV.

Heavy Jet Mass (RHO) distribution at c.m. energy 206.00 GeV.

Total jet broadening distribution at c.m. energy 91.20 GeV.

Total jet broadening distribution at c.m. energy 133.00 GeV.

Total jet broadening distribution at c.m. energy 161.00 GeV.

Total jet broadening distribution at c.m. energy 172.00 GeV.

Total jet broadening distribution at c.m. energy 183.00 GeV.

Total jet broadening distribution at c.m. energy 189.00 GeV.

Total jet broadening distribution at c.m. energy 200.00 GeV.

Total jet broadening distribution at c.m. energy 206.00 GeV.

Wide jet broadening distribution at c.m. energy 91.20 GeV.

Wide jet broadening distribution at c.m. energy 133.00 GeV.

Wide jet broadening distribution at c.m. energy 161.00 GeV.

Wide jet broadening distribution at c.m. energy 172.00 GeV.

Wide jet broadening distribution at c.m. energy 183.00 GeV.

Wide jet broadening distribution at c.m. energy 189.00 GeV.

Wide jet broadening distribution at c.m. energy 200.00 GeV.

Wide jet broadening distribution at c.m. energy 206.00 GeV.

C-PARAMETER distribution at c.m. energy 91.20 GeV.

C-PARAMETER distribution at c.m. energy 133.00 GeV.

C-PARAMETER distribution at c.m. energy 161.00 GeV.

C-PARAMETER distribution at c.m. energy 172.00 GeV.

C-PARAMETER distribution at c.m. energy 183.00 GeV.

C-PARAMETER distribution at c.m. energy 189.00 GeV.

C-PARAMETER distribution at c.m. energy 200.00 GeV.

C-PARAMETER distribution at c.m. energy 206.00 GeV.

Thrust Major distribution at c.m. energy 91.20 GeV.

Thrust Major distribution at c.m. energy 133.00 GeV.

Thrust Major distribution at c.m. energy 161.00 GeV.

Thrust Major distribution at c.m. energy 172.00 GeV.

Thrust Major distribution at c.m. energy 183.00 GeV.

Thrust Major distribution at c.m. energy 189.00 GeV.

Thrust Major distribution at c.m. energy 200.00 GeV.

Thrust Major distribution at c.m. energy 206.00 GeV.

Thrust Minor distribution at c.m. energy 91.20 GeV.

Thrust Minor distribution at c.m. energy 133.00 GeV.

Thrust Minor distribution at c.m. energy 161.00 GeV.

Thrust Minor distribution at c.m. energy 172.00 GeV.

Thrust Minor distribution at c.m. energy 183.00 GeV.

Thrust Minor distribution at c.m. energy 189.00 GeV.

Thrust Minor distribution at c.m. energy 200.00 GeV.

Thrust Minor distribution at c.m. energy 206.00 GeV.

Jet Mass Difference distribution at c.m. energy 91.20 GeV.

Jet Mass Difference distribution at c.m. energy 133.00 GeV.

Jet Mass Difference distribution at c.m. energy 161.00 GeV.

Jet Mass Difference distribution at c.m. energy 172.00 GeV.

Jet Mass Difference distribution at c.m. energy 183.00 GeV.

Jet Mass Difference distribution at c.m. energy 189.00 GeV.

Jet Mass Difference distribution at c.m. energy 200.00 GeV.

Jet Mass Difference distribution at c.m. energy 206.00 GeV.

Aplanarity distribution at c.m. energy 91.20 GeV.

Aplanarity distribution at c.m. energy 133.00 GeV.

Aplanarity distribution at c.m. energy 161.00 GeV.

Aplanarity distribution at c.m. energy 172.00 GeV.

Aplanarity distribution at c.m. energy 183.00 GeV.

Aplanarity distribution at c.m. energy 189.00 GeV.

Aplanarity distribution at c.m. energy 200.00 GeV.

Aplanarity distribution at c.m. energy 206.00 GeV.

Planarity distribution at c.m. energy 133.00 GeV.

Planarity distribution at c.m. energy 161.00 GeV.

Planarity distribution at c.m. energy 172.00 GeV.

Planarity distribution at c.m. energy 183.00 GeV.

Planarity distribution at c.m. energy 189.00 GeV.

Planarity distribution at c.m. energy 200.00 GeV.

Planarity distribution at c.m. energy 206.00 GeV.

Oblateness distribution at c.m. energy 91.20 GeV.

Oblateness distribution at c.m. energy 133.00 GeV.

Oblateness distribution at c.m. energy 161.00 GeV.

Oblateness distribution at c.m. energy 172.00 GeV.

Oblateness distribution at c.m. energy 183.00 GeV.

Oblateness distribution at c.m. energy 189.00 GeV.

Oblateness distribution at c.m. energy 200.00 GeV.

Oblateness distribution at c.m. energy 206.00 GeV.

Sphericity distribution at c.m. energy 91.20 GeV.

Sphericity distribution at c.m. energy 133.00 GeV.

Sphericity distribution at c.m. energy 161.00 GeV.

Sphericity distribution at c.m. energy 172.00 GeV.

Sphericity distribution at c.m. energy 183.00 GeV.

Sphericity distribution at c.m. energy 189.00 GeV.

Sphericity distribution at c.m. energy 200.00 GeV.

Sphericity distribution at c.m. energy 206.00 GeV.

LN(Y12) distribution at c.m. energy 91.20 GeV.

LN(Y12) distribution at c.m. energy 133.00 GeV.

LN(Y12) distribution at c.m. energy 161.00 GeV.

LN(Y12) distribution at c.m. energy 172.00 GeV.

LN(Y12) distribution at c.m. energy 183.00 GeV.

LN(Y12) distribution at c.m. energy 189.00 GeV.

LN(Y12) distribution at c.m. energy 200.00 GeV.

LN(Y12) distribution at c.m. energy 206.00 GeV.

LN(Y23) distribution at c.m. energy 91.20 GeV.

LN(Y23) distribution at c.m. energy 133.00 GeV.

LN(Y23) distribution at c.m. energy 161.00 GeV.

LN(Y23) distribution at c.m. energy 172.00 GeV.

LN(Y23) distribution at c.m. energy 183.00 GeV.

LN(Y23) distribution at c.m. energy 189.00 GeV.

LN(Y23) distribution at c.m. energy 200.00 GeV.

LN(Y23) distribution at c.m. energy 206.00 GeV.

LN(Y34) distribution at c.m. energy 91.20 GeV.

LN(Y34) distribution at c.m. energy 133.00 GeV.

LN(Y34) distribution at c.m. energy 161.00 GeV.

LN(Y34) distribution at c.m. energy 172.00 GeV.

LN(Y34) distribution at c.m. energy 183.00 GeV.

LN(Y34) distribution at c.m. energy 189.00 GeV.

LN(Y34) distribution at c.m. energy 200.00 GeV.

LN(Y34) distribution at c.m. energy 206.00 GeV.

LN(Y45) distribution at c.m. energy 91.20 GeV.

LN(Y45) distribution at c.m. energy 133.00 GeV.

LN(Y45) distribution at c.m. energy 161.00 GeV.

LN(Y45) distribution at c.m. energy 172.00 GeV.

LN(Y45) distribution at c.m. energy 183.00 GeV.

LN(Y45) distribution at c.m. energy 189.00 GeV.

LN(Y45) distribution at c.m. energy 206.00 GeV.

LN(Y56) distribution at c.m. energy 91.20 GeV.

LN(Y56) distribution at c.m. energy 133.00 GeV.

LN(Y56) distribution at c.m. energy 161.00 GeV.

LN(Y56) distribution at c.m. energy 172.00 GeV.

LN(Y56) distribution at c.m. energy 183.00 GeV.

LN(Y56) distribution at c.m. energy 189.00 GeV.

LN(Y56) distribution at c.m. energy 206.00 GeV.

1-jet fraction at c.m. energy 91.20 GeV.

1-jet fraction at c.m. energy 133.00 GeV.

1-jet fraction at c.m. energy 161.00 GeV.

1-jet fraction at c.m. energy 172.00 GeV.

1-jet fraction at c.m. energy 183.00 GeV.

1-jet fraction at c.m. energy 189.00 GeV.

1-jet fraction at c.m. energy 200.00 GeV.

1-jet fraction at c.m. energy 206.00 GeV.

2-jet fraction at c.m. energy 91.20 GeV.

2-jet fraction at c.m. energy 133.00 GeV.

2-jet fraction at c.m. energy 161.00 GeV.

2-jet fraction at c.m. energy 172.00 GeV.

2-jet fraction at c.m. energy 183.00 GeV.

2-jet fraction at c.m. energy 189.00 GeV.

2-jet fraction at c.m. energy 200.00 GeV.

2-jet fraction at c.m. energy 206.00 GeV.

3-jet fraction at c.m. energy 91.20 GeV.

3-jet fraction at c.m. energy 133.00 GeV.

3-jet fraction at c.m. energy 161.00 GeV.

3-jet fraction at c.m. energy 172.00 GeV.

3-jet fraction at c.m. energy 183.00 GeV.

3-jet fraction at c.m. energy 189.00 GeV.

3-jet fraction at c.m. energy 200.00 GeV.

3-jet fraction at c.m. energy 206.00 GeV.

4-jet fraction at c.m. energy 91.20 GeV.

4-jet fraction at c.m. energy 133.00 GeV.

4-jet fraction at c.m. energy 161.00 GeV.

4-jet fraction at c.m. energy 172.00 GeV.

4-jet fraction at c.m. energy 183.00 GeV.

4-jet fraction at c.m. energy 189.00 GeV.

4-jet fraction at c.m. energy 200.00 GeV.

4-jet fraction at c.m. energy 206.00 GeV.

5-jet fraction at c.m. energy 91.20 GeV.

5-jet fraction at c.m. energy 133.00 GeV.

5-jet fraction at c.m. energy 161.00 GeV.

5-jet fraction at c.m. energy 172.00 GeV.

5-jet fraction at c.m. energy 183.00 GeV.

5-jet fraction at c.m. energy 189.00 GeV.

5-jet fraction at c.m. energy 200.00 GeV.

5-jet fraction at c.m. energy 206.00 GeV.

>=6-jet fraction at c.m. energy 91.20 GeV.

>=6-jet fraction at c.m. energy 133.00 GeV.

>=6-jet fraction at c.m. energy 161.00 GeV.

>=6-jet fraction at c.m. energy 172.00 GeV.

>=6-jet fraction at c.m. energy 183.00 GeV.

>=6-jet fraction at c.m. energy 189.00 GeV.

>=6-jet fraction at c.m. energy 200.00 GeV.

>=6-jet fraction at c.m. energy 206.00 GeV.

Differential cross section, as a function of pseudo-rapidity, from channel (1).

Differential cross section for two jet production with associated D* production, from channel (1). The quoted cross sections correspond to the centres of the bins. The second systematic error is that associated with the energy scale.

Differential cross section for two jet production with associated D* production, from channel (1). The quoted cross sections correspond to the centres of the bins. The second systematic error is that associated with the energy scale.

PT Differential cross section.

Pseudo rapidity distribution.

W differential cross section.

Q**2 differential cross section.

Charm contribution to the proton structure function F2.

Charm contribution to the proton structure function F2.

Charm contribution to the proton structure function F2.

Charm contribution to the proton structure function F2.

Charged particle Thrust(minor) distribution.

Charged particle Two-jet resolution variable, Y3 distribution.

Charged particle Heavy Jet Mass distribution.

Charged particle C-Parameter distribution.

Charged particle Oblateness distribution.

Charged particle XP distribution.

Charged particle rapidity distribution.

Charged particle PTIN distribution.

Charged particle PTOUT distribution.

Measure n-jet rates using the Durham cluster algorithm as a function of thejet-resolution parameter YCUT.

Measure n-jet rates using the Durham cluster algorithm as a function of thejet-resolution parameter YCUT.

Measure n-jet rates using the Durham cluster algorithm as a function of thejet-resolution parameter YCUT.

Measure n-jet rates using the Durham cluster algorithm as a function of thejet-resolution parameter YCUT.

Charged particle inclusive distribution of -LN(1/X).

Unfolded charged particle multiplicity distribution giving the probability to have a hadronic Z0 decay with N charged particles.

Values of the mean values of the leading moments of the charged particle multiplicity distribution. R2 is the second binomial moment defined as MEAN(N*(N-1))/MULT**2.

Unfolded values of the the mean multiplicity and dispersion of the multiplicity distributions integaretd over the rapidity region -0.5 to 0.5.

Unfolded values of the the mean multiplicity and dispersion of the multiplicity distributions integrated over the rapidity region -1.0 to 1.0.

Unfolded values of the the mean multiplicity and dispersion of the multiplicity distributions integrated over the rapidity region -1.5 to 1.5.

Unfolded values of the the mean multiplicity and dispersion of the multiplicity distributions integrated over the rapidity region -2.0 to 2.0.

Unfolded values of the the mean multiplicity and dispersion of the multiplicity distribution integrated over the full rapidity region.

Differential cross sections for the inclusive production of PI+-. Additional 3pct systematic uncertainty.

Differential cross sections for the inclusive production of K+-. Additionalsystematic uncertainty 3% above and 5% below X = 0.010.

Differential cross sections for the inclusive production of P PBAR. Additional systematic uncertainty 3% above and 5% below X = 0.018.

Measured inclusive photon cross section. Errors contain both statistical and systematic uncertainties.

Measured differential cross section for PI0 production.

Measured fragmentation function at the ETA meson. Additional 6pct systematic error.

Measured fragmentation function at the ETAPRIME meson. Additional 8pct systematic error.

Inclusive K0 spectrum. Additional 2pct normalization error.

Inclusive LAMBDA spectrum. Additional 4pct normalization error.

Fragmentation distribution for XI production.

Fragmentation distribution for SIGMA(1385) production.

Fragmentation distribution for XI(1530) production.

Differential cross section for RHO0 production.

Differential cross section for OMEGA production.

Differential cross section for K*0 production.

Differential cross section for PHI production.

Differential cross section for K*0 production as a function of the transverse momentum with respect to the Thrust axis.

Differential cross section for PHI production as a function of the transverse momentum with respect to the Thrust axis.

Fragmentation distribution for K*+- production.

Mean Multiplicities. Where a second systematic error is given, this is due to the uncertainty in the extrapolation to X = 0. Note that the ETA and ETAPRIMEvalues are for X > 0.1.

Corrected production rates from the etaprime --> rho0 gamma decay mode. Extrapolation to full x range.

Differential cross section for inclusive omega production from the omega --> pi+ pi- p0 decay mode data. The mean x values are the appropriate x position to plot the data according to the method of Lafferty et al (NIM A 355(95)541).

Differential cross section for inclusive omega production from the omega --> pi+ pi- p0 decay mode data. The mean x values are the appropriate x position to plot the data according to the method of Lafferty et al (NIM A 355(95)541).

Differential cross section for inclusive etaprime production from the etaprime --> pi+ pi- eta decay mode data. The mean x values are the appropriate x position to plot the data according to the method of Lafferty et al (NIM A 355(95)541).

Differential cross section for inclusive etaprime production from the etaprime --> pi+ pi- eta decay mode data. The mean x values are the appropriate x position to plot the data according to the method of Lafferty et al (NIM A 355(95)541).

Differential cross section for inclusive etaprime production from the etaprime --> rho0 gamma decay mode data. The mean x values are the appropriate x position to plot the data according to the method of Lafferty et al (NIM A 355(95)541).

Differential cross section for inclusive etaprime production from the etaprime --> rho0 gamma decay mode data. The mean x values are the appropriate x position to plot the data according to the method of Lafferty et al (NIM A 355(95)541).

Differential cross section for inclusive etaprime production obtained by combining the two etaprime decay modes.

Differential cross section for inclusive etaprime production obtained by combining the two etaprime decay modes.