Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $p_{\rm T,ee}$ for 0.14 < $m_{\rm ee}$ < 0.7 GeV/$c^{2}$.

Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $p_{\rm T,ee}$ for 0.7 < $m_{\rm ee}$ < 1.1 GeV/$c^{2}$.

Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $\rm DCA_{ee}$ for 0.14 < $m_{\rm ee}$ < 1.1 GeV/$c^{2}$.

Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $p_{\rm T,ee}$ for 1.1 < $m_{\rm ee}$ < 2.7 GeV/$c^{2}$.

Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $\rm DCA_{ee}$ for 1.1 < $m_{\rm ee}$ < 2.7 GeV/$c^{2}$.

Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $p_{\rm T,ee}$ for 2.7 < $m_{\rm ee}$ < 3.3 GeV/$c^{2}$.

Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $\rm DCA_{ee}$ for 2.7 < $m_{\rm ee}$ < 3.3 GeV/$c^{2}$.

Ratio of inclusive to decay photon cross sections extracted from the dielectron spectra measured in pp collisions at $\sqrt{s}$ = 7 TeV in the ALICE acceptance as a function of $p_{\rm T,ee}$.

The dielectron cross section in inelastic pp collisions at $\sqrt{s}$ = 13 TeV as a function of pair transverse momentum for 0.7 < $m_{\rm ee}$ < 1.03 GeV/$c^{2}$.

Ratio of dielectron spectra in HM and INEL events scaled by the charged-particle multiplicity as a function of invariant mass for $p_{\rm T,ee}$ < 6.0 GeV/$c$.

Ratio of dielectron spectra in HM and INEL events scaled by the charged-particle multiplicity as a function of invariant mass for $p_{\rm T,ee}$ < 1.0 GeV/$c$.

Ratio of dielectron spectra in HM and INEL events scaled by the charged-particle multiplicity as a function of invariant mass for 1.0 < $p_{\rm T,ee}$ < 2.0 GeV/$c$.

Ratio of dielectron spectra in HM and INEL events scaled by the charged-particle multiplicity as a function of invariant mass for 2.0 < $p_{\rm T,ee}$ < 3.0 GeV/$c$.

Ratio of dielectron spectra in HM and INEL events scaled by the charged-particle multiplicity as a function of invariant mass for 3.0 < $p_{\rm T,ee}$ < 6.0 GeV/$c$.

The dielectron cross section in inelastic pp collisions at $\sqrt{s}$ = 13 TeV as a function of pair transverse momentum for 1.03 < $m_{\rm ee}$ < 2.86 GeV/$c^{2}$.

The dielectron cross section in inelastic pp collisions at $\sqrt{s}$ = 13 TeV as a function of invariant mass for $p_{\rm T,ee}$ < 1.0 GeV/$c$.

The dielectron cross section in inelastic pp collisions at $\sqrt{s}$ = 13 TeV as a function of invariant mass for 1.0 < $p_{\rm T,ee}$ < 2.0 GeV/$c$.

The dielectron cross section in inelastic pp collisions at $\sqrt{s}$ = 13 TeV as a function of invariant mass for 2.0 < $p_{\rm T,ee}$ < 3.0 GeV/$c$.

The dielectron cross section in inelastic pp collisions at $\sqrt{s}$ = 13 TeV as a function of invariant mass for 3.0 < $p_{\rm T,ee}$ < 6.0 GeV/$c$.

Ratio of direct to inclusive photon cross sections extracted from the dielectron spectra in inelastic pp collisions at $\sqrt{s}$ = 13 TeV.

Ratio of direct to inclusive photon cross sections extracted from the dielectron spectra in high-multiplicity pp collisions at $\sqrt{s}$ = 13 TeV.

Dielectron excess spectra as in pp collisions at $\sqrt{s}$ = 13 TeV as a function of $m_{\rm ee}$ after subtraction of the hadronicdecay cocktail. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.075$ GeV/$c$.

Dielectron excess spectra as in pp collisions at $\sqrt{s}$ = 13 TeV in the invariant mass interval 0.15<$m_{\rm ee}$<0.6 as a function of $p_{\rm T,ee}$ after subtraction of the hadronicdecay cocktail. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.075$ GeV/$c$.

Exclusive J/psi photoproduction cross section in gamma-p.

Dissociative J/psi photoproduction gamma-p.

Cross section ratio, dissociative J/psi photoproduction gamma-p over exclusive J/psi photoproduction gamma-p.

Inclusive $e^+e^-$ cross section in p-Pb collisions at $\sqrt{s}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for $0.5 < m_{\rm ee} < 1.1$ GeV/$c$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Inclusive $e^+e^-$ cross section in pp collisions at $\sqrt{s}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for $1.1 < m_{\rm ee} < 2.7$ GeV/$c$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Inclusive $e^+e^-$ cross section in p-Pb collisions at $\sqrt{s}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for $1.1 < m_{\rm ee} < 2.7$ GeV/$c$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Dielectron nuclear modification factor $R_{\rm pPb}$ at $\sqrt{s}$ = 5.02 TeV as a function of $m_{\rm ee}$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Dielectron nuclear modification factor $R_{\rm pPb}$ at $\sqrt{s}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for $0.5 < m_{\rm ee} < 1.1$ GeV/$c$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

Dielectron nuclear modification factor $R_{\rm pPb}$ at $\sqrt{s}$ = 5.02 TeV as a function of $p_{\rm T,ee}$ for $1.1 < m_{\rm ee} < 2.7$ GeV/$c$. Electrons are measured within $|\eta_{\rm e}| < 0.8$ and $p_{\rm T,e} > 0.2$ GeV/$c$.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Measured unfolded differential cross-section as a function of the dilepton transverse momentum $p^{ll}_{\mathrm{T}}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Measured unfolded differential cross-section as a function of the the four-body transverse momentum $p^{ll\gamma\gamma}_{\mathrm{T}}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Measured unfolded differential cross-section as a function of the diphoton invariant mass $m_{\gamma\gamma}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Measured unfolded differential cross-section as a function of the four-body invariant mass $m_{ll\gamma\gamma}$. NLO predictions from Sherpa 2.2.10 and MadGraph5_aMC@NLO 2.7.3 are also shown. The uncertainty in the predictions is divided into statistical and theoretical uncertainties (scale and PDF+$\alpha_{s}$).

Expected and observed $95\%$ confidence intervals for the coupling parameters $f_{T,j}/\Lambda^{4}$ of transverse dimension-8 operators. All parameter values outside of the stated range are excluded at the chosen confidence level. No unitarity constraints are applied.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,8}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,0}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,1}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,2}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,5}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,6}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,7}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

Expected and observed unitarised $95\%$ confidence intervals for the coupling parameter $f_{T,9}/\Lambda^{4}$ in the clipping energy range between 1.1 and 5 TeV. The non-unitarised limits ($E_c = \infty$) are also shown. All parameter values outside of the stated range are excluded at the chosen confidence level.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 220-300 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 300-450 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 450-500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed filtered AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 220-300 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 300-450 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 450-500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed trimmed AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 220-300 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 300-450 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 450-500 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 500-600 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 600-800 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 800-1000 GeV/c.

The unfolded distributions (x1000) for the mean mass of the two leading jets in in dijet events for reconstructed pruned AK7 jets, for the mean PT of the two leading jets in the range 1000-1500 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 125-150 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 150-220 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 220-300 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for Z->LEPTON LEPTON events for the jet PT range 300-450 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 trimmed jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded AK7 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 125-150 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded CA8 pruned jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 150-220 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 220-300 GeV/c.

Unfolded CA12 filtered jet mass distribution (x1000) for W->LEPTON NU events for the jet PT range 300-450 GeV/c.

The DY pre-FSR cross section measurements for the combined dimuon and dielectron channels normalized to the Z-peak region in the full acceptance.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 20-30 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 30-45 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 45-60 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 60-120 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 120-200 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.

The DY dimuon rapidity spectrum within the detector acceptance, normalized to the Z-peak region, for the mass bin 200-1500 GeV. The two columns correspond to pre-FSR and post-FSR. The uncertainties are the total experimental uncertainties.