Signal region detector-level distribution for the observable $p_{\mathrm{T}}^{\mathrm{lead}\, \ell}$.

Signal region detector-level distribution for the observable $m_{e\mu}$.

Signal region detector-level distribution for the observable $p_{\mathrm{T}}^{e\mu}$.

Measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|y_{e\mu}|$

Relative systematic uncertainties for the fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|y_{e\mu}|$

Measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|\Delta \phi(e \mu)|$

Relative systematic uncertainties for the fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|\Delta \phi(e \mu)|$

Measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $ \cos\theta^{\ast}$

Relative systematic uncertainties for the fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $ \cos\theta^{\ast}$

Measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{\mathrm{lead}\, \ell}$

Relative systematic uncertainties for the fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{\mathrm{lead}\, \ell}$

Measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $m_{e\mu}$

Relative systematic uncertainties for the fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $m_{e\mu}$

Measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{e\mu}$

Relative systematic uncertainties for the fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{e\mu}$

The statistical correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|y_{e\mu}|$

The total correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|y_{e\mu}|$

The statistical correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|\Delta \phi(e \mu)|$

The total correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $|\Delta \phi(e \mu)|$

The statistical correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $ \cos\theta^{\ast}$

The total correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $ \cos\theta^{\ast}$

The statistical correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{\mathrm{lead}\, \ell}$

The total correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{\mathrm{lead}\, \ell}$

The statistical correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $m_{e\mu}$

The total correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $m_{e\mu}$

The statistical correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{e\mu}$

The total correlation coefficients (in percentage) between bins for the measured fiducial differential cross-section of $WW \rightarrow e^{\pm}\nu\mu^{\mp}\nu$ production for the observable $p_{\mathrm{T}}^{e\mu}$

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. 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. 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. 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 di-jet cross section as a function of the mean transverse energy of thedi-jet system for the region where either X(C=GAMMA+) or X(C=GAMMA-) are < 0.75 .

The di-jet cross section as a function of the mean transverse energy of thedi-jet system for the region where both X(C=GAMMA+) and X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of X(C=GAMMA) for transverse energy from 5 TO 7 GeV for the full X(C=GAMMA+) and X(C=GAMMA-) region.

The di-jet cross section as a function of X(C=GAMMA) for mean transverse energy 7 TO 11 GeV for the full X(C=GAMMA+)-X(C=GAMMA-) region.

The di-jet cross section as a function of X(C=GAMMA) for mean transverse energy 11 TO 25 for the full X(C=GAMMA+)-X(C=GAMMA-) region.

The di-jet cross section as a function of X(C=GAMMA) for mean transverse energy 5 TO 7 GeV in the region where either X(C=GAMMA+) or X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of X(C=GAMMA) for mean transverse energy 7 TO 11 GeV in the region where either X(C=GAMMA+) or X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of X(C=GAMMA) for mean transverse energy 5 TO 7 GeV in the region where both X(C=GAMMA+) and X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of X(C=GAMMA) for mean transverse energy 7 TO 11 GeV in the region where both X(C=GAMMA+) and X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of LOG10(X(C =GAMMA)) for mean transverse energy 5 TO 7 GeV for the full X(C=GAMMA+)-X(C=GAMMA-) region.

The di-jet cross section as a function of LOG10(X(C =GAMMA)) for mean transverse energy 5 TO 7 for the region where either X(C=GAMMA+) or X(C=GAMMA-) are <0.75.

The di-jet cross section as a function of LOG10(X(C =GAMMA)) for mean transverse energy 5 to 7 GeV for the region where both X(C=GAMMA+) and X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of the absolute pseudorapidity difference of the two leading jets for the region where either X(C=GAMMA+) or X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of the absolute pseudorapidity difference of the two leading jets for the region where both X(C=GAMMA+) and X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of the pseudorapidity of the jet with the lower pseudorapidity in the region where either X(C=GAMMA+) or X(C=GAMMA-)are < 0.75.

The di-jet cross section as a function of the pseudorapidity of the jet with the lower pseudorapidity in the region where both X(C=GAMMA+) and X(C=GAMMA-) are < 0.75.

The di-jet cross section as a function of the pseudorapidity of the jet with the lower pseudorapidity in the region where either X(C=GAMMA+) or X(C=GAMMA-)are < 0.75.

The di-jet cross section as a function of the pseudorapidity of the jet with the lower pseudorapidity in the region where both X(C=GAMMA+) and X(C=GAMMA-) are < 0.75.

Correlation matrix of negative systematic uncertainties.

The measured values of the X distribution.

The measured values of the LN(1/X) distribution.

The measured value of F2 and DSIG/DX for the SW data sample in the Q**2 range 15 to 30 GeV**2.

The measured value of F2 and DSIG/DX for the FD data sample in the Q**2 range 30 to 50 GeV**2.

The measured value of F2 and DSIG/DX for the FD data sample in the Q**2 range 50 to 150 GeV**2.

The measured value of F2 and DSIG/DX for the EE data sample in the Q**2 range 400 to 2350 GeV**2.

Statistical correlation between the bins for mean Q**2 value 12.1 GeV**2.

Statistical correlation between the bins for mean Q**2 value 19.9 GeV**2.

Statistical correlation between the bins for mean Q**2 value 39.7 GeV**2.

Statistical correlation between the bins for mean Q**2 value 76.4 GeV**2.

Statistical correlation between the bins for mean Q**2 value 780 GeV**2.

F2 and DSIG/DX over the full X range 0.10 to 0.60 as a function of Q**2.

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)).

Distribution of Aplanarity.

Distribution of Oblateness.

Distribution of the C-parameter.

Distribution of Heavy Jet Mass.

Distribution of Sphericity.

Distribution of Total Jet Broadening.

Distribution of Wide Jet Broadening.

Distribution of the Transition value between 2- and 3-jets, Y23.

Weighted mean values of ALPHAS derived from the six event shape distribution using order (alpha**2) +NLLA QCD calculation with x(mu)=1 and the ln(R)-matching scheme. Results are also given evolved to M(Z0). The 187 GeV entry corresponds to the luminosity weighted mean c.m. energy.

Charged particle multiplicity (in percent).

Mean values of the charged particle multiplicity and higher order moments. D is defined as SQRT(MEAN(MULT)-MEAN(MULT))**2. C2 is defined as MEAN(MULT**2)/MEAN(MULT)**2. R2 is defined as MEAN(MULT(MULT-1))/MEAN(MULT)**2.

Measured value of the momentum spectra of charged particles (PTIN) in the event plane.

Measured value of the momentum spectra of charged particles (PTOUT) out of the event plane.

Measured value of the rapidity (YRAP).

Measured value of the fragmentation functions.

Measured valueS of the 1/LN(X) distribution.

Mean values of the momentum parameter.

Inclusive cross section for PI0 production in two-jet events.

Inclusive cross section for ETA production in two-jet events.

Inclusive cross section for ETAPRIME production in two-jet events.

Inclusive cross section for PI0 production in three-jet events where the PI0 comes from JET1.

Inclusive cross section for PI0 production in three-jet events where the PI0 comes from JET2.

Inclusive cross section for PI0 production in three-jet events where the PI0 comes from JET3.

Inclusive cross section for ETA production in three-jet events where the ETA comes from JET1.

Inclusive cross section for ETA production in three-jet events where the ETA comes from JET2.

Inclusive cross section for ETA production in three-jet events where the ETA comes from JET3.

Inclusive cross section for ETAPRIME production in three-jet events where the ETAPRIME comes from JET1.

Inclusive cross section for ETAPRIME production in three-jet events where the ETAPRIME comes from JET2.

Inclusive cross section for ETAPRIME production in three-jet events where the ETAPRIME comes from JET3.

Inclusive cross section for K0S production in hadronic events as a functionof 1/LN(XP).

Inclusive cross section for LAMBDA production in hadronic events as a function of 1/LN(XP).

Inclusive cross section for K0S production in two-jet events as a function of 1/LN(XP).

Inclusive cross section for LAMBDA production in two-jet events as a function of 1/LN(XP).

Inclusive cross section for K0S production in three-jet events where the K0S comes from JET1.

Inclusive cross section for K0S production in three-jet events where the K0S comes from JET2.

Inclusive cross section for K0S production in three-jet events where the K0S comes from JET3.

Inclusive cross section for LAMBDA production in three-jet events where theLAMBDA comes from JET1.

Inclusive cross section for LAMBDA production in three-jet events where theLAMBDA comes from JET2.

Inclusive cross section for LAMBDA production in three-jet events where theLAMBDA comes from JET3.