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 $p_{T}^{e\mu}$.

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].

Differential cross sections for D0 production from the (K- PI+ PI+ PI-) decay mode.

Differential cross sections for D*+ production from the ((K- PI+) PI+) decay mode.

Differential cross sections for D*+ production from the ((K- PI+ PI+ PI-) PI+) decay mode.

Differential cross sections for D*0 production from the ((K- PI+) PI0) decay mode.

Differential cross sections for D*0 production from the ((K- PI+ PI+ PI-) PI0) decay mode.

Averaged differential cross sections for the four different processes. The error is the quadratic combination of statistical and systematic error, excluding those errors common to all momenta which affect the total cross section but not the shape.

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 W.

Differential cross section as a function of DELTA(PHI), where DELTA(PHI) is the angle between the azimuthal angles of the two virtual photons.

Differential cross section as a function of YBAR, where YBAR is defined as LN(W**2/SQRT(Q1**2 * Q2**2)).

Cross section as a function of X where X is the maximum value of X1 or X2, the upper and lower vertex values.

Cross section as a function of Q**2 where Q**2 is the maximum value of Q1**2 or Q2**2, the upper and lower vertex values.

Cross section as a function of W.

Cross section as a function of DELTA(PHI), where DELTA(PHI) is the angle between the azimuthal angles of the two virtual photons.

Cross section as a function of YBAR, where YBAR is defined as LN(W**2/SQRT(Q1**2 * Q2**2)).

The B quark cross section at fixed PT min of 5 GeV, extrapolated using the HERWIG MC generator and corrected for the branching ratio (10.73 +- 0.35 PCT) for the process B --> E-. The second DSYS error is due to the uncertainty in the extrapolation procedure.

The total production rates of LAMBDA(1520). The first error is the fit error and the second DSYS error is due to the extrapolation to the full x-range.

The differential cross section w.r.t. W the virtual photon centre of mass energy from the K2PI final state. The asymmetric errors are the quadratic sum of the statistical and systematic errors. The statistical errors are also shown separately.

The differential cross section w.r.t. X(C=D*), the fractional momentum of the D* in the virtual photon-proton centre of mass system, from the K2PI final state. The asymmetric errors are the quadratic sum of the statistical and systematic errors. The statistical errors are also shown separately.

The differential cross section w.r.t. to transverse momentum of the D* fromthe K2PI final state. The asymmetric errors are the quadratic sum of the statistical and systematic errors. The statistical errors are also shown separately.

The differential cross section w.r.t. to transverse momentum of the D* fromthe K4PI final state. The asymmetric errors are the quadratic sum of the statistical and systematic errors. The statistical errors are also shown separately.

The differential cross section w.r.t. the pseudorapidity of the D* from theK2PI data. The asymmetric errors are the quadratic sum of the statistical and systematic errors. The statistical errors are also shown separately.

The differential cross section w.r.t. the pseudorapidity of the D* from theK4PI data. The asymmetric errors are the quadratic sum of the statistical and systematic errors. The statistical errors are also shown separately.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K2PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K4PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K4PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K4PI final state as a function of Q**2 and Y.

The cross sections for D* production from the K4PI final state as a function of Q**2 and Y.

The charmed structure function F2(C=CHARM) derived from a combination of the K2PI and K4PI data. There are additional systematic uncertainties described in the text of the paper which include the 1.65 PCT luminosity uncertainty and a 9 PCT uncertainty in the charm hadronization fraction to D*+-.