The cross-section in bins of the di-$J/\psi$ transverse momentum in the forward rapidity region, assuming unpolarised $J/\psi$ mesons and excluding the $J/\psi$ spin-alignment systematic uncertainty. The branching fraction and luminosity uncertainties are not included in the systematic uncertainty as they are constant at 1.1$\%$ and 1.9$\%$ respectively.

The cross-section in bins of the di-$J/\psi$ invariant mass in the central rapidity region, assuming unpolarised $J/\psi$ mesons and excluding the $J/\psi$ spin-alignment systematic uncertainty. The branching fraction and luminosity uncertainties are not included in the systematic uncertainty as they are constant at 1.1$\%$ and 1.9$\%$ respectively.

The cross-section in bins of the di-$J/\psi$ invariant mass in the forward rapidity region, assuming unpolarised $J/\psi$ mesons and excluding the $J/\psi$ spin-alignment systematic uncertainty. The branching fraction and luminosity uncertainties are not included in the systematic uncertainty as they are constant at 1.1$\%$ and 1.9$\%$ respectively.

The total cross-section, DPS cross-section, $f_{\mathrm{DPS}}$, and average acceptance correction in the muon fiducial volume for the $\Delta y$ distribution. The branching fraction and luminosity uncertainties are not included in the systematic uncertainty as they are constant at 1.1$\%$ and 1.9$\%$ respectively.

The total cross-section, DPS cross-section, $f_{\mathrm{DPS}}$, and average acceptance correction in the muon fiducial volume for the $\Delta \phi$ distribution. The branching fraction and luminosity uncertainties are not included in the systematic uncertainty as they are constant at 1.1$\%$ and 1.9$\%$ respectively.

The total cross-section, DPS cross-section, $f_{\mathrm{DPS}}$, and average acceptance correction in the muon fiducial volume for the $m$($J/\psi$ $J/\psi$) distribution. The branching fraction and luminosity uncertainties are not included in the systematic uncertainty as they are constant at 1.1$\%$ and 1.9$\%$ respectively.

The total cross-section, DPS cross-section, $f_{\mathrm{DPS}}$, and average acceptance correction in the muon fiducial volume for the $p_{\mathrm{T}}$($J/\psi$ $J/\psi$) distribution. The branching fraction and luminosity uncertainties are not included in the systematic uncertainty as they are constant at 1.1$\%$ and 1.9$\%$ respectively.

The average acceptance weight for each spin-alignment scenario relative to the unpolarised case in bins of the sub-leading $J/\psi$ transverse momentum in the central rapidity region.

The average acceptance weight for each spin-alignment scenario relative to the unpolarised case in bins of the sub-leading $J/\psi$ transverse momentum in the forward rapidity region.

The average acceptance weight for each spin-alignment scenario relative to the unpolarised case in bins of the di-$J/\psi$ transverse momentum in the central rapidity region.

The average acceptance weight for each spin-alignment scenario relative to the unpolarised case in bins of the di-$J/\psi$ transverse momentum in the forward rapidity region.

The average acceptance weight for each spin-alignment scenario relative to the unpolarised case in bins of the di-$J/\psi$ invariant in the central rapidity region.

The average acceptance weight for each spin-alignment scenario relative to the unpolarised case in bins of the di-$J/\psi$ invariant in the forward rapidity region.

Ratios of integrated fiducial CC and NC cross sections obtained from the combination of electron and muon channels with statistical (stat) and systematic (syst) uncertainties. The common fiducial regions are defined in Section 2.3.

Total cross sections times leptonic branching ratios obtained from the combination of electron and muon channels with statistical and systematic uncertainties, for $W^+$, $W^-$, their sum and the $Z/\gamma^*$ process measured at $\sqrt{s}=7$ TeV. The $Z/\gamma^*$ cross section is defined for the dilepton mass window $m_{\ell\ell} = 66 - 116$ GeV. The uncertainties denote the statistical (stat), the experimental systematic (syst), the luminosity (lumi), and acceptance extrapolation (acc) contributions.

Ratios of total CC and NC cross sections obtained from the combination of electron and muon channels with statistical and systematic uncertainties. The $Z/\gamma^*$ cross section is defined for the dilepton mass window $m_{\ell\ell} = 66 - 116$ GeV. The uncertainties denote the statistical (stat), the experimental systematic (syst), and acceptance extrapolation (acc) contributions.

The correlation coefficients of the $W^+$, $W^-$ and $Z$ fiducial cross-section measurements.

Measurement of the electron-to-muon cross-section ratios for the $W$ and $Z$ production, $R_W$ and $R_Z$. The uncertainties denote the statistical (stat) and the experimental systematic (syst) contributions.

Differential cross section for the $W^+ \to \ell^+\nu$ processes combined from $\ell = e, \mu$ decays extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the $W^- \to \ell^-\bar{\nu}$ processes combined from $\ell = e, \mu$ decays extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $46 < m_{\ell\ell} < 66$ GeV combined from $\ell = e, \mu$ decays extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV combined from $\ell = e, \mu$ decays extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV combined from $\ell = e, \mu$ decays extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the forward $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV combined from $\ell = e, \mu$ decays extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the forward $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV combined from $\ell = e, \mu$ decays extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the $W^- \to e^-\bar{\nu}$ process extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the $W^+ \to e^+\nu$ process extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to ee$ process in the invariant mass region $46 < m_{\ell\ell} < 66$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to ee$ process in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the forward $Z/\gamma^* \to ee$ process in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to ee$ process in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the forward $Z/\gamma^* \to ee$ process in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the $W^- \to \mu^-\bar{\nu}$ process extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the $W^+ \to \mu^+\nu$ process extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to \mu\mu$ process in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to \mu\mu$ process in the invariant mass region $46 < m_{\ell\ell} < 66$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Differential cross section for the central $Z/\gamma^* \to \mu\mu$ process in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV extrapolated to the common fiducial region. The statistical, uncorrelated systematic, correlated systematic and luminosity uncertainties are given in percent.

Values of $E(W[Z])$ and $A(W[Z])$ correction factors for integrated $W\to\ell\nu$ and $Z\to\ell\ell$ measurements together with the total estimated uncertainties in percent. The separate electron and muon measurements are divided by the $E(W[Z])$ factors, as defined in Eq.(8), to correct them to the corresponding common fiducial region. The $A(W[Z])$ factors, defined in Eq. (9), are used to extract a total cross section. Finally, the ratios of $A(W[Z])$ correction factors are given for four combinations of $W^+$, $W^-$ and $Z$ treating all components of the $A(W[Z])$ uncertainties as correlated between processes, which is relevant for the acceptance uncertainties on the total cross-section ratios.

Values of $E(W)$ correction factors for the differential $W\to\ell\nu$ measurements together with the total estimated uncertainties in percent. The separate electron and muon measurements are divided by the $E(W)$ factors, as defined in Eq.(8), to correct them to the corresponding common fiducial region. This only affects the bin of highest $\eta_\ell$, all other $E(W)$ factors are exactly 1 without uncertainties.

Values of $E(Z)$ correction factors for the differential $Z/\gamma^*\to e^+e^-$ measurements together with the total estimated uncertainties in percent. The separate electron and muon measurements are divided by the $E(Z)$ factors, as defined in Eq.(8), to correct them to the corresponding common fiducial region.

Values of $E(Z)$ correction factors for the differential $Z/\gamma^*\to \mu^+\mu^-$ measurements together with the total estimated uncertainties in percent. The separate electron and muon measurements are divided by the $E(Z)$ factors, as defined in Eq.(8), to correct them to the corresponding common fiducial region.

Values of $E(Z)$ correction factors for the differential forward $Z/\gamma^*\to e^+e^-$ measurements together with the total estimated uncertainties in percent. The separate electron and muon measurements are divided by the $E(Z)$ factors, as defined in Eq.(8), to correct them to the corresponding common fiducial region.

Correlation coefficients between integrated cross sections extrapolated to the total phase space, $\sigma^\mathrm{tot}_{W \to \ell\nu}$ and $\sigma^\mathrm{tot}_{Z/\gamma^* \to \ell\ell}$ for four combinations of $W^+, W^-, W^{\pm}$ and $Z$. Values are given including and excluding the luminosity uncertainties.

Correlation coefficients between integrated fiducial cross sections in electron and muon channels for $W^{\pm}$ and $Z$. Values are given including and excluding the luminosity uncertainties.

The differential W charge asymmetry $A_{\ell}$ as defined in Eq. (19) from the combined electron and muon channel measurements. All uncertainties are quoted in % with respect to the $A_{\ell}$ values. The statistical (stat), uncorrelated (uncor) and correlated (cor) systematic uncertainties are reported.

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the integrated common fiducial cross sections using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups.

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial cross sections for the $W^+ \to \ell^+\nu$ process using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups.

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial cross sections for the $W^- \to \ell^-\bar{\nu}$ process$ using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups.

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial W charge asymmetry $A_{\ell}$ using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups.

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial cross sections for the central $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $46 < m_{\ell\ell} < 66$ GeV using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups. The term 'EW' quantifies the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised ($\pm$). All predictions are corrected for leading two-loop EW contributions.

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial cross sections for the central $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups. The term 'EW' quantifies the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised ($\pm$).

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial cross sections for the central $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups. The term 'EW' quantifies the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised ($\pm$).

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial cross sections for the forward $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups. The term 'EW' quantifies the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised ($\pm$).

Combined NNLO QCD and NLO EW predictions as defined in Eq. (15), c.f. Section 6.1.2 and Ref. [110] Chapter III.2.3, for the differential common fiducial cross sections for the forward $Z/\gamma^* \to \ell\ell$ processes in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV using Table 15 input parameters and various NNLO PDFs. The given uncertainties correspond to the statistical accuracy from the numerical DYNNLO 1.5 integration (stat) and the PDF uncertainties, where the latter are evaluated following the different prescriptions of the PDF groups. The term 'EW' quantifies the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised ($\pm$).

Nominal NNLO QCD + NLO EW $K_f$-factors as defined in Eq. (20) for the differential $W^+ \to \ell^+\nu$ process. The $K_f$-factor is calculated as ratio of the best NNLO QCD + NLO EW prediction to the NLO QCD calculation using the MCFM/APPLGRID calculation, both using the ATLAS-epWZ12 NNLO PDF set, c.f. Section 7.1. In addition to the nominal $K_f$-factor, a full set of alternative $K$-factors is presented reflecting the following systematic variations, c.f. Tables 19 and 21. The factor $K_{FEWZ}$ uses FEWZ 3.1.b2 for the NNLO QCD prediction, combined with NLO EW. The factors $K_\mu$ reflect the variation of the renormalisation and factorisations scales ($\mu_R, \mu_F$ up/down) by factors of 2 and 0.5, respectively. The statistical uncertainty on each $K_f$-factor (stat) is obtained from the NNLO QCD calculation, while the numerical uncertainties from all other contributions are negligible.

Nominal NNLO QCD + NLO EW $K_f$-factors as defined in Eq. (20) for the differential $W^- \to \ell^-\bar{\nu}$ process. The $K_f$-factor is calculated as ratio of the best NNLO QCD + NLO EW prediction to the NLO QCD calculation using the MCFM/APPLGRID calculation, both using the ATLAS-epWZ12 NNLO PDF set, c.f. Section 7.1. In addition to the nominal $K_f$-factor, a full set of alternative $K$-factors is presented reflecting the following systematic variations, c.f. Tables 19 and 21. The factor $K_{FEWZ}$ uses FEWZ 3.1.b2 for the NNLO QCD prediction, combined with NLO EW. The factors $K_\mu$ reflect the variation of the renormalisation and factorisations scales ($\mu_R, \mu_F$ up/down) by factors of 2 and 0.5, respectively. The statistical uncertainty on each $K_f$-factor (stat) is obtained from the NNLO QCD calculation, while the numerical uncertainties from all other contributions are negligible.

Nominal NNLO QCD + NLO EW $K_f$-factors as defined in Eq. (20) for the differential central $Z/\gamma^* \to \ell\ell$ process in the invariant mass region $46 < m_{\ell\ell} < 66$ GeV. The $K_f$-factor is calculated as ratio of the best NNLO QCD + NLO EW prediction to the NLO QCD calculation using the MCFM/APPLGRID calculation, both using the ATLAS-epWZ12 NNLO PDF set, c.f. Section 7.1. In addition to the nominal $K_f$-factor, a full set of alternative $K$-factors is presented reflecting the following systematic variations, c.f. Tables 19 and 21. The factor $K_{FEWZ}$ uses the FEWZ 3.1.b2 NNLO QCD prediction, combined with NLO EW. The factors $K_\mu$ reflect the variation of the renormalisation and factorisations scales ($\mu_R, \mu_F$ up/down) by factors 2 and 0.5, respectively. The factors $K_{EW}$ quantify the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised (EW up/down). The statistical uncertainty on each $K_f$-factor (stat) is obtained from the NNLO QCD calculation, while the numerical uncertainties from all other contributions is negligible.

Nominal NNLO QCD + NLO EW $K_f$-factors as defined in Eq. (20) for the differential central $Z/\gamma^* \to \ell\ell$ process in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV. The $K_f$-factor is calculated as ratio of the best NNLO QCD + NLO EW prediction to the NLO QCD calculation using the MCFM/APPLGRID calculation, both using the ATLAS-epWZ12 NNLO PDF set, c.f. Section 7.1. In addition to the nominal $K_f$-factor, a full set of alternative $K$-factors is presented reflecting the following systematic variations, c.f. Tables 19 and 21. The factor $K_{FEWZ}$ uses the FEWZ 3.1.b2 NNLO QCD prediction, combined with NLO EW. The factors $K_\mu$ reflect the variation of the renormalisation and factorisations scales ($\mu_R, \mu_F$ up/down) by factors 2 and 0.5, respectively. The factors $K_{EW}$ quantify the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised (EW up/down). The statistical uncertainty on each $K_f$-factor (stat) is obtained from the NNLO QCD calculation, while the numerical uncertainties from all other contributions is negligible.

Nominal NNLO QCD + NLO EW $K_f$-factors as defined in Eq. (20) for the differential central $Z/\gamma^* \to \ell\ell$ process in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV. The $K_f$-factor is calculated as ratio of the best NNLO QCD + NLO EW prediction to the NLO QCD calculation using the MCFM/APPLGRID calculation, both using the ATLAS-epWZ12 NNLO PDF set, c.f. Section 7.1. In addition to the nominal $K_f$-factor, a full set of alternative $K$-factors is presented reflecting the following systematic variations, c.f. Tables 19 and 21. The factor $K_{FEWZ}$ uses the FEWZ 3.1.b2 NNLO QCD prediction, combined with NLO EW. The factors $K_\mu$ reflect the variation of the renormalisation and factorisations scales ($\mu_R, \mu_F$ up/down) by factors 2 and 0.5, respectively. The factors $K_{EW}$ quantify the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised (EW up/down). The statistical uncertainty on each $K_f$-factor (stat) is obtained from the NNLO QCD calculation, while the numerical uncertainties from all other contributions is negligible.

Nominal NNLO QCD + NLO EW $K_f$-factors as defined in Eq. (20) for the differential forward $Z/\gamma^* \to \ell\ell$ process in the invariant mass region $66 < m_{\ell\ell} < 116$ GeV. The $K_f$-factor is calculated as ratio of the best NNLO QCD + NLO EW prediction to the NLO QCD calculation using the MCFM/APPLGRID calculation, both using the ATLAS-epWZ12 NNLO PDF set, c.f. Section 7.1. In addition to the nominal $K_f$-factor, a full set of alternative $K$-factors is presented reflecting the following systematic variations, c.f. Tables 19 and 21. The factor $K_{FEWZ}$ uses the FEWZ 3.1.b2 NNLO QCD prediction, combined with NLO EW. The factors $K_\mu$ reflect the variation of the renormalisation and factorisations scales ($\mu_R, \mu_F$ up/down) by factors 2 and 0.5, respectively. The factors $K_{EW}$ quantify the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised (EW up/down). The statistical uncertainty on each $K_f$-factor (stat) is obtained from the NNLO QCD calculation, while the numerical uncertainties from all other contributions is negligible.

Nominal NNLO QCD + NLO EW $K_f$-factors as defined in Eq. (20) for the differential forward $Z/\gamma^* \to \ell\ell$ process in the invariant mass region $116 < m_{\ell\ell} < 150$ GeV. The $K_f$-factor is calculated as ratio of the best NNLO QCD + NLO EW prediction to the NLO QCD calculation using the MCFM/APPLGRID calculation, both using the ATLAS-epWZ12 NNLO PDF set, c.f. Section 7.1. In addition to the nominal $K_f$-factor, a full set of alternative $K$-factors is presented reflecting the following systematic variations, c.f. Tables 19 and 21. The factor $K_{FEWZ}$ uses the FEWZ 3.1.b2 NNLO QCD prediction, combined with NLO EW. The factors $K_\mu$ reflect the variation of the renormalisation and factorisations scales ($\mu_R, \mu_F$ up/down) by factors 2 and 0.5, respectively. The factors $K_{EW}$ quantify the deviation in case of using the NNLO QCD and NLO EW combination procedure as defined in Eq. (13) from the nominal prescription in Eq. (15), where the effect is symmetrised (EW up/down). The statistical uncertainty on each $K_f$-factor (stat) is obtained from the NNLO QCD calculation, while the numerical uncertainties from all other contributions is negligible.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the integrated common fiducial cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties are negligible on these correction factors.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the differential common fiducial $W^+ \to e^+\nu$ cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties (stat) are given.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the differential common fiducial $W^- \to e^-\bar{\nu}$ cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties (stat) are given.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the differential common fiducial $W^+ \to \mu^+\nu$ cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties (stat) are given.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the differential common fiducial $W^- \to \mu^-\bar{\nu}$ cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties (stat) are given.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the differential common fiducial central $Z/\gamma^* \to ee$ cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties (stat) are given.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the differential common fiducial central $Z/\gamma^* \to \mu\mu$ cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties (stat) are given.

Correction factors estimated from Powheg+Pythia6+Photos samples, c.f. Section 2.2, to convert the differential common fiducial forward $Z/\gamma^* \to ee$ cross-section measurements from Born QED level, c.f. Section 6.1.2, to a "dressed" and "bare" QED FSR definition. The "dressed" level is obtained from the charged final-state lepton(s) combined with all FSR photons within a cone R, as defined in Footnote 1, of R<0.1. The "bare" level is obtained from the charged final-state lepton(s) after QED FSR losses. The factors $C_{dressed}$ ($C_{bare}$) are defined as the ratio of the dressed (bare) to the Born QED level cross sections. The statistical uncertainties (stat) are given.

Values of $g_1^{NS}$ for the COMPASS data in ($x$, $Q^2$) bins.

Parameters of two solutions of the QCD fit. The assumed functional form at $Q^2_0 = 1 ($GeV$/c)^2$ is $q(x) = \eta x^\alpha (1-x)^\beta (1 + \gamma x)/N$ where N is the normalisation. The parametrisation is used for the singlet and gluon helicity distribution and the two non-singlet distributions $\Delta q_3$ and $\Delta q_8$.

Normalisations of the different data sets used in the QCD fit.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $467 < m^{\gamma-\rm jet1} < 510$ GeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $510 < m^{\gamma-\rm jet1} < 590$ GeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $590 < m^{\gamma-\rm jet1} < 670$ GeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $670 < m^{\gamma-\rm jet1} < 760$ GeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $760 < m^{\gamma-\rm jet1} < 850$ GeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $850 < m^{\gamma-\rm jet1} < 950$ GeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $0.95 < m^{\gamma-\rm jet1} < 1.05$ TeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $1.05 < m^{\gamma-\rm jet1} < 1.25$ TeV.

Measured cross sections for isolated-photon plus 1jet production as a function of $|\cos\theta^{\star}|$ for the range $1.25 < m^{\gamma-\rm jet1} < 2.45$ TeV.

Measured cross sections for isolated-photon plus 2jet production as a function of $E_{\rm T}^{\gamma}$.

Measured cross sections for isolated-photon plus 2jet production as a function of $p_{\rm T}^{\rm jet2}$.

Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm \gamma-jet2}$.

Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm jet1-jet2}$.

Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm \gamma-jet2}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.

Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm \gamma-jet2}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.

Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm jet1-jet2}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.

Measured cross sections for isolated-photon plus 2jet production as a function of $\Delta\phi^{\rm jet1-jet2}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.

Measured cross sections for isolated-photon plus 2jet production as a function of $\beta^{\rm jet1}$.

Measured cross sections for isolated-photon plus 2jet production as a function of $\beta^{\gamma}$.

Ratio of measured cross sections for isolated-photon plus 2jet production as a function of $\beta$.

Measured cross sections for isolated-photon plus 3jet production as a function of $E_{\rm T}^{\gamma}$.

Measured cross sections for isolated-photon plus 3jet production as a function of $p_{\rm T}^{\rm jet3}$.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm \gamma-jet3}$.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet1-jet3}$.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet2-jet3}$.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm \gamma-jet3}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm \gamma-jet3}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet1-jet3}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet1-jet3}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet2-jet3}$ for the range $130< E_{\rm T}^{\gamma} <300$ GeV.

Measured cross sections for isolated-photon plus 3jet production as a function of $\Delta\phi^{\rm jet2-jet3}$ for the range $E_{\rm T}^{\gamma} >300$ GeV.

HT inclusive distribution in SRZ.

Jet multiplicity distribution in SRZ.

B-tagged jet multiplicity distribution in SRZ.

Dilepton invariant mass distribution in SRMedium.

Dilepton invariant mass distribution in SRMedium.

Dilepton invariant mass in SRHigh.

Expected 95% exclusion contour for the gluino simplified model with fixed N1 mass and decays to quarks and Z bosons in SRZ.

Observed 95% exclusion contour for the gluino simplified model with fixed N1 mass and decays to quarks and Z bosons in SRZ.

Expected 95% exclusion contour for the squark simplified model with fixed N1 mass and decays to quarks and Z bosons in SRZ.

Observed 95% exclusion contour for the squark simplified model with fixed N1 mass and decays to quarks and Z bosons in SRZ.

Expected 95% exclusion contour for the gluino simplified model with varying N1 mass and decays to quarks and Z bosons in SRZ.

Observed 95% exclusion contour for the gluino simplified model with varying N1 mass and decays to quarks and Z bosons in SRZ.

Expected 95% exclusion contour for the gluino simplified model with sleptons in the edge SRs.

Observed 95% exclusion contour for the gluino simplified model with sleptons in the edge SRs.

Expected 95% exclusion contour for the gluino simplified model with decays to on- or off-shell Z bosons in the edge SRs.

Observed 95% exclusion contour for the gluino simplified model with decays to on- or off-shell Z bosons in the edge SRs.

Expected 95% exclusion contour for the gluino simplified model with decays to on- or off-shell Z bosons in SRZ.

Observed 95% exclusion contour for the gluino simplified model with decays to on- or off-shell Z bosons in SRZ.

Cutflow table for three benchmark signal points from the $\tilde{g}$--$\chi_{2}^{0}$ on-shell grid in SRZ for the $ee$ and $\mu\mu$ channels separately. The number of generated events is N RAW, while N WEIGHTED corresponds to the number of events expected in 14.7/fb, after all MC simulation corrections have been applied.

Cutflow table for three benchmark signal points for the slepton model in SR-low, SR-medium and SR-high for the $ee$ and $\mu\mu$ channels separately. The number of generated events is N RAW, while N WEIGHTED corresponds to the number of events expected in 14.7/fb, after all MC simulation corrections have been applied. The event generation was filtered to require at least two leptons (electrons or muons) with $p_{T}>5$ GeV and $|\eta|<2.8$, with 20000 events required to pass the filter. The corresponding number of unfiltered events is provided in the ``Pre-filter events'' row of the table.

Signal acceptance for the gluino simplified model with decays to quarks and Z bosons in SRZ.

Signal efficiency for the gluino simplified model with decays to quarks and Z bosons in SRZ.

Signal acceptance for the gluino simplified model with decays via sleptons in SRLow.

Signal efficiency for the gluino simplified model with decays via sleptons in SRLow.

Signal acceptance for the gluino simplified model with decays via sleptons in SRMedium.

Signal efficiency for the gluino simplified model with decays via sleptons in SRMedium.

Signal acceptance for the gluino simplified model with decays via sleptons in SRHigh.

Signal efficiency for the gluino simplified model with decays via sleptons in SRHigh.

Upper limits on the signal cross-section at 95% CL for the gluino simplified model with fixed N1 mass and decays to quarks and Z bosons in SRZ.

Upper limits on the signal cross-section at 95% CL for the squark simplified model with fixed N1 mass and decays to quarks and Z bosons in SRZ.

Upper limits on the signal cross-section at 95% CL for the gluino simplified model with varying N1 mass and decays to quarks and Z bosons in SRZ.

Upper limits on the signal cross-section at 95% CL for the gluino simplified model with decays via sleptons.

Upper limits on the signal cross-section at 95% CL for the gluino simplified model with decays to on-shell or off-shell Z bosons.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 1$^\text{st}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 2$^\text{nd}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_2)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 2$^\text{nd}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_2)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 3$^\text{rd}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_3)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 3$^\text{rd}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_3)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 4$^\text{th}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_4)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 4$^\text{th}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_4)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 5$^\text{th}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_5)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 5$^\text{th}$ jet $p_{\text{T}}$, $p_{\text{T}}(\text{j}_5)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 1$^\text{st}$ jet $|y|$, $|y(\text{j}_1)|$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 1$^\text{st}$ jet $|y|$, $|y(\text{j}_1)|$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 2$^\text{nd}$ jet $|y|$, $|y(\text{j}_2)|$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 2$^\text{nd}$ jet $|y|$, $|y(\text{j}_2)|$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 3$^\text{rd}$ jet $|y|$, $|y(\text{j}_3)|$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 3$^\text{rd}$ jet $|y|$, $|y(\text{j}_3)|$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 4$^\text{th}$ jet $|y|$, $|y(\text{j}_4)|$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 4$^\text{th}$ jet $|y|$, $|y(\text{j}_4)|$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 5$^\text{th}$ jet $|y|$, $|y(\text{j}_5)|$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the 5$^\text{th}$ jet $|y|$, $|y(\text{j}_5)|$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the Z boson $|y|$, $|y(\text{Z})|$, for events with at least one jet and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the Z boson $|y|$, $|y(\text{Z})|$, for events with at least one jet.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the Z boson $|y|$, $|y(\text{Z})|$ for events with at least one jet and $p_\text{T}(\text{Z}) > 150\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the Z boson $|y|$, $|y(\text{Z})|$ for events with at least one jet and $p_\text{T}(\text{Z}) > 150\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the Z boson $|y|$, $|y(\text{Z})|$ for events with at least $p_\text{T}(\text{Z}) > 300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the Z boson $|y|$, $|y(\text{Z})|$ for events with at least $p_\text{T}(\text{Z}) > 300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_1)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 150\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 150\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the 2$^\text{nd}$leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_2)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the 2$^\text{nd}$leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_2)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the 3$^\text{rd}$leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_3)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the 3$^\text{rd}$leading jet, $y_{\text{diff}}(\text{Z}, \text{j}_3)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the system constituted of the two leading jets, $y_{\text{diff}}(\text{Z}, \text{dijet})$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the Z boson and the system constituted of the two leading jets, $y_{\text{diff}}(\text{Z}, \text{dijet})$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the two leading jets, $y_{\text{diff}}(\text{j}_1, \text{j}_2)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{diff}}$ of the two leading jets, $y_{\text{diff}}(\text{j}_1, \text{j}_2)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the two leading jets, $y_{\text{sum}}(\text{j}_1, \text{j}_2)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the two leading jets, $y_{\text{sum}}(\text{j}_1, \text{j}_2)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_1)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 150\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 150\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_1)$ for events with $p_{\text{T}}(\text{Z}) > 300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the 2$^\text{nd}$leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_2)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the 2$^\text{nd}$leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_2)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the 3$^\text{rd}$leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_3)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the 3$^\text{rd}$leading jet, $y_{\text{sum}}(\text{Z}, \text{j}_3)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the system constituted of the two leading jets, $y_{\text{sum}}(\text{Z}, \text{dijet})$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the $y_{\text{sum}}$ of the Z boson and the system constituted of the two leading jets, $y_{\text{sum}}(\text{Z}, \text{dijet})$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least one jet, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least one jet.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least two jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least two jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least four jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least four jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least five jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of $H_\text{T}$ for events with at least five jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet for events with at least ine jet, $\Delta\Phi(\text{Z},\text{j}_1)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet for events with at least ine jet, $\Delta\Phi(\text{Z},\text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet for events with at least two jets, $\Delta\Phi(\text{Z},\text{j}_1)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet for events with at least two jets, $\Delta\Phi(\text{Z},\text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet for events with at least three jets, $\Delta\Phi(\text{Z},\text{j}_1)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet for events with at least three jets, $\Delta\Phi(\text{Z},\text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^\text{nd}$ leading jet for events with at least three jets, $\Delta\Phi(\text{Z},\text{j}_1)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^\text{nd}$ leading jet for events with at least three jets, $\Delta\Phi(\text{Z},\text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^\text{rd}$ leading jet for events with at least three jets, $\Delta\Phi(\text{Z},\text{j}_1)$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^\text{rd}$ leading jet for events with at least three jets, $\Delta\Phi(\text{Z},\text{j}_1)$.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet$\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least two jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet$\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least two jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet$\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least two jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet$\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least two jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet$\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet$\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^{\text{nd}}$ leading jet$\Delta\Phi(\text{Z},\text{j}_2)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^{\text{nd}}$ leading jet$\Delta\Phi(\text{Z},\text{j}_2)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^{\text{rd}}$ leading jet$\Delta\Phi(\text{Z},\text{j}_3)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^{\text{rd}}$ leading jet$\Delta\Phi(\text{Z},\text{j}_3)$, for events with $p_{\text{T}}(\text{Z})>150\,$GeV and at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV and at least one jet, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV and at least one jet.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV and at least two jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV and at least two jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV and at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV and at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^{\text{nd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_2)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^{\text{nd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_2)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^{\text{rd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_3)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^{\text{rd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_3)$, for events with $p_{\text{T}}(\text{Z})>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with at least three jets, $p_{\text{T}}(\text{Z})>150\,$GeV, and $H_{\text{T}}>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with at least three jets, $p_{\text{T}}(\text{Z})>150\,$GeV, and $H_{\text{T}}>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^{\text{nd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_2)$, for events with at least three jets, $p_{\text{T}}(\text{Z})>150\,$GeV, and $H_{\text{T}}>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 2$^{\text{nd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_2)$, for events with at least three jets, $p_{\text{T}}(\text{Z})>150\,$GeV, and $H_{\text{T}}>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^{\text{rd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with at least three jets, $p_{\text{T}}(\text{Z})>150\,$GeV, and $H_{\text{T}}>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the Z boson and the 3$^{\text{rd}}$ leading jet, $\Delta\Phi(\text{Z},\text{j}_1)$, for events with at least three jets, $p_{\text{T}}(\text{Z})>150\,$GeV, and $H_{\text{T}}>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two leading jets, $\Delta\Phi(\text{j}_1,\text{j}_2)$, for events with at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two leading jets, $\Delta\Phi(\text{j}_1,\text{j}_2)$, for events with at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two 1$^{\text{st}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two 1$^{\text{st}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two 2$^{\text{nd}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two 2$^{\text{nd}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two leading jets, $\Delta\Phi(\text{j}_1,\text{j}_2)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>150\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the two leading jets, $\Delta\Phi(\text{j}_1,\text{j}_2)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>150\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 1$^{\text{st}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>150\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 1$^{\text{st}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>150\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 2$^{\text{nd}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_2,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>150\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 2$^{\text{nd}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_2,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>150\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 1$^{\text{st}}$ and 2$^{\text{nd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_2)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 1$^{\text{st}}$ and 2$^{\text{nd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_2)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 1$^{\text{st}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 1$^{\text{st}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 2$^{\text{nd}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>300\,$GeV, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the azimuthal angle between the 2$^{\text{nd}}$ and 3$^{\text{rd}}$ leading jets, $\Delta\Phi(\text{j}_1,\text{j}_3)$, for events with at least three jets and $p_{\text{T}}(\text{Z})>300\,$GeV.

The cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the mass of the system made of the two leading jets, $m_{\text{j}_1\text{j}_1}$, and breakdown of the relative uncertainty.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production measured as a function of the mass of the system made of the two leading jets, $m_{\text{j}_1\text{j}_1}$.

The cross section for Z($\rightarrow\ell\ell$) + jets production as a function of the leading jet transverse momentum and rapidity

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production as a function of the leading jet transverse momentum and rapidity

The cross section for Z($\rightarrow\ell\ell$) + jets production as a function of the Z boson and leading jet rapidities

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production as a function of the Z boson and leading jet rapidities

The cross section for Z($\rightarrow\ell\ell$) + jets production as a function of the rapidities of the Z boson and leading jet, and of the transverse momentum of the jet for the same configuration.

Bin-to-bin correlation in the the cross section for Z($\rightarrow\ell\ell$) + jets production as a function of the rapidities of the Z boson and leading jet, and of the transverse momentum of the jet for the same configuration.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 6 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 7 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 8 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections measured as a function of $P_T^{\rm jet}$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 9 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised dijet cross sections measured as a function of $\langle P_T \rangle_2$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 10 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 5.5-8.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 8.0-11.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 11.0-16.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 16.0-22.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 22.0-30.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 30.0-42.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 42.0-60.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised trijet cross sections measured as a function of $\langle P_T \rangle_3$ for $Q^2$ = 60.0-80.0 GeV$^2$. The correction factors on the theoretical cross sections $c^{\rm had}$ are listed together with their uncertainties. The radiative correction factors $c^{\rm rad}$ are already included in the quoted cross sections. Note that the uncertainties labelled $\delta^{E_{e^\prime}}$ and $\delta^{\theta_{e^\prime}}$ in Table 11 of the paper (arXiv:1611.03421v3) should be swapped. See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Matrix of statistical correlation coefficients of the unfolded jet cross sections at low $Q^2$.

Matrix of statistical correlation coefficients of the unfolded normalised jet cross sections at low $Q^2$.

Inclusive jet cross sections for $P_T^{\rm jet}$ = 5-7 GeV$^2$ measured as a function of $Q^2$ in the range 150-15000 GeV$^2$. The cross section values and uncertainties have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>). See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Normalised inclusive jet cross sections for $P_T^{\rm jet}$ = 5-7 GeV$^2$ measured as a function of $Q^2$ in the range 150-15000 GeV$^2$. The cross section values and uncertainties have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>). See Table 5 of arXiv:1406.4709v2 for details of the correlation model.

Matrix of statistical correlation coefficients of the unfolded jet cross sections at high $Q^2$. The statistical correlations have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>).

Matrix of statistical correlation coefficients of the unfolded normalised jet cross sections at high $Q^2$. The statistical correlations have been determined in the scope of the analysis of an earlier H1 publication (<a href="https://inspirehep.net/record/1301218">INSPIRE</a>, <a href="https://www.hepdata.net/record/ins1301218">HEPData</a>).

The strong coupling extracted from the normalised inclusive jet, dijet and trijet data at NLO as a function of the renormalisation scale $\mu_r$. For each $\mu_r$ the values of the strong coupling $\alpha_s(\mu_r)$ and the equivalent values $\alpha_s(M_Z)$ are given with experimental (exp) and theoretical (th) uncertainties.

Multiplicity of additional jets with pt>80GeV

Transverse momentum of leading b-jet

Transverse momentum of sub-leading b-jet

Transverse momentum of leading (highest pt) additional jet

Measured Gap fraction within |y|<0.8 as a function of Q0

Measured Gap fraction within 0.8<|y|<1.5 as a function of Q0

Measured Gap fraction within 1.5<|y|<2.1 as a function of Q0

Measured Gap fraction within |y|<2.1 as a function of Q0

Measured Gap fraction within |y|<2.1 as a function of Q0 for invariant mass region m_{emubb} < 300GeV

Measured Gap fraction within |y|<2.1 as a function of Q0 for invariant mass region 300 GeV < m_{emubb} < 425GeV

Measured Gap fraction within |y|<2.1 as a function of Q0 for invariant mass region 425 GeV< m_{emubb} < 600GeV

Measured Gap fraction within |y|<2.1 as a function of Q0 for invariant mass region m_{emubb} > 600GeV

Measured Gap fraction within |y|<0.8 as a function of QSUM

Measured Gap fraction within 0.8<|y|<1.5 as a function of QSUM

Measured Gap fraction within 1.5<|y|<2.1 as a function of QSUM

Measured Gap fraction within |y|<2.1 as a function of QSUM

Measured Gap fraction within |y|<2.1 as a function of QSUM for invariant mass region m_{emubb} < 300GeV

Measured Gap fraction within |y|<2.1 as a function of QSUM for invariant mass region 300 GeV < m_{emubb} < 425 GeV

Measured Gap fraction within |y|<2.1 as a function of QSUM for invariant mass region 425GeV< m_{emubb} < 600GeV

Measured Gap fraction within |y|<2.1 as a function of QSUM for invariant mass region m_{emubb} > 600GeV

Measured prompt $X(3872) / \psi(2S)$ production ratio using the two-lifetime fit model.

Measured non-prompt $X(3872) / \psi(2S)$ production ratio using the two-lifetime fit model.

Measured short-lived non-prompt $X(3872)$ / total non-prompt $\psi(2S)$ production ratio using the two-lifetime fit model.

Measured long-lived non-prompt $X(3872)$ / total non-prompt $\psi(2S)$ production ratio using the two-lifetime fit model.

Measured cross section times branching fractions as a function of pT for prompt $\psi$(2S) production.

Measured cross section times branching fractions as a function of pT for non-prompt $\psi$(2S) production.

Measured cross section times branching fractions as a function of pT for prompt X(3872) production.

Measured cross section times branching fractions as a function of pT for non-prompt X(3872) production.

Measured non-prompt fraction for $\psi(2S)$ production.

Measured non-prompt fraction for X(3872) production.

Normalised differential decay width of $\psi(2S) \rightarrow J/\psi \pi\pi$ in bins of $m_{\pi\pi}$.

Normalised differential decay width of $X(3872) \rightarrow J/\psi \pi\pi$ in bins of $m_{\pi\pi}$.