The expected 95% CL exclusion contour (-1$\sigma$) for a simplified model of dark-matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.25, $g_{\chi}$ = 1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour for a simplified model of dark-matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.25, $g_{\chi}$ = 1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The observed 95% CL exclusion contour for a simplified model of dark-matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.1 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour (+1$\sigma$) for a simplified model of dark-matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.1 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour (-1$\sigma$) for a simplified model of dark-matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.1 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour for a simplified model of dark-matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.1 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The observed 95% CL exclusion contour for a simplified model of dark-matter production involving a vector operator with couplings $g_{q}$ = 0.25, $g_{\chi}$ =1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour ($+1\sigma$) for a simplified model of dark-matter production involving a vector operator with couplings $g_{q}$ = 0.25, $g_{\chi}$ =1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour ($-1\sigma$) for a simplified model of dark-matter production involving a vector operator with couplings $g_{q}$ = 0.25, $g_{\chi}$ =1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour for a simplified model of dark-matter production involving a vector operator with couplings $g_{q}$ = 0.25, $g_{\chi}$ =1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The observed 95% CL exclusion contour for a simplified model of dark-matter production involving for a vector operator with couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.01 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour ($+1\sigma$) for a simplified model of dark-matter production involving for a vector operator with couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.01 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour ($-1\sigma$) for a simplified model of dark-matter production involving for a vector operator with couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.01 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The expected 95% CL exclusion contour for a simplified model of dark-matter production involving for a vector operator with couplings $g_{q}$ = 0.1, $g_{\chi}$ = 1 and $g_{l}$ = 0.01 as a function of the dark-matter mass $m_{\chi}$ and the mediator mass $m_{\mathrm{med}}$. The plane under the limit curve is excluded.

The 90% CL exclusion limit on the $\chi$-proton scattering cross section in a simplifed model of dark-matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.25, $g_{\chi}$ = 1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$.

The 90% CL exclusion limit on the $\chi$-nucleon scattering cross section in a simplifed model of dark-matter production involving a vector operator, Dirac DM and couplings $g_{q}$ = 0.25, $g_{\chi}$ = 1 and $g_{l}$ = 0 as a function of the dark-matter mass $m_{\chi}$.

The observed and expected 95% CL limits on M* for a dimension-7 operator EFT model with a contact interaction of type $\gamma\gamma\chi\chi$ as a function of dark-matter mass $m_{\chi}$.

The observed and expected limit at 95% CL on the production cross section of a $Z\gamma$ resonance as a function of its mass.

The observed 95% CL upper limits on signal strength $\mu$, the ratio of the experimental limit to the predicted signal cross section, for a simplified model of dark matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$ = 0.25 and $g_{\chi}$ = 1 as a function of the DM and the mediator particle masses. The bound on $\mu$ only applies for choices of couplings that yield the same kinematic distributions as the benchmark model.

Acceptance, in %, for a simplified model of dark matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$= 0.25 and $g_{\chi}$ = 1 for various $m_{\chi}$ and $m_{\textrm{med}}$ values. It is constant as a function of $m_{\chi}$ for a fixed $m_{\textrm{med}}$ in the region $m_{\textrm{med}}>2m_{\chi}$.

Fiducial reconstruction efficiencies in the three inclusive signal regions for a simplified model of dark matter production involving an axial-vector operator, Dirac DM and couplings $g_{q}$= 0.25 and $g_{\chi}$ = 1 for various $m_{\chi}$ and $m_{\textrm{med}}$ values. It is constant as a function of $m_{\chi}$ for a fixed $m_{\textrm{med}}$ in the region $m_{\textrm{med}}>2m_{\chi}$.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with two b-tags in the SR for the third MET category that is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_J with two b-tags in the SR for the fourth MET category that is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with one b-tag in the SR for the first MET category which is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with one b-tag in the SR for the second MET category which is used as input to the fit.

Distributions of the invariant mass of the Higgs boson candidates mh=m_jj with one b-tag in the SR for the third MET category which is used as input to the fit.

ATEEC function for 850 GeV < HT2 < 900 GeV

TEEC function for 900 GeV < HT2 < 1000 GeV

ATEEC function for 900 GeV < HT2 < 1000 GeV

TEEC function for 1000 GeV < HT2 < 1100 GeV

ATEEC function for 1000 GeV < HT2 < 1100 GeV

TEEC function for 1100 GeV < HT2 < 1400 GeV

ATEEC function for 1100 GeV < HT2 < 1400 GeV

TEEC function for HT2 > 1400 GeV

ATEEC function for HT2 > 1400 GeV

alphaS(mZ) values from TEEC fits

alphaS(Q) values from TEEC fits

alphaS(mZ) values from ATEEC fits

alphaS(Q) values from ATEEC fits

D(pt) distributions for pp and Pb+Pb collisions, jet rapidity 1.2 < |y| < 2.1.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 2.1.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity |y| < 0.3.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity 0.3 < |y| < 0.8.

D(z) distributions for pp and Pb+Pb collisions, jet rapidity 1.2 < |y| < 2.1.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 0.3, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with 0.3 < |y| < 0.8, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with 1.2 < |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(pt) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(pt) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 100 < pt < 126 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 126 < pt < 158 GeV.

Ratio of D(z) distributions collisions, centrality 0-10 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 20-30 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 30-40 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

Ratio of D(z) distributions collisions, centrality 60-80 PCT for jets with |y| < 2.1, 158 < pt < 398 GeV.

The difference between the total yield of particles with 1 < pt^trk < 4 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total yield of particles with 4 < pt^trk < 25 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total yield of particles with 25 < pt^trk < 100 GeV measured in 0-80 PCT Pb+Pb collisions and the total yield measured in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total transverse momentum of particles with 1 < pt^trk < 4 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total transverse momentum of particles with 4 < pt^trk < 25 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The difference between the total transverse momentum of particles with 25 < pt^trk < 100 GeV measured in 0-80 PCT Pb+Pb collisions and the total transverse momentum of particles in the same pt interval measured in pp collisions in jets with |y| < 2.1, 100 < pt < 398 GeV.

The ratio of R_D(z) distributions in three rapidity selections for 0-10 PCT Pb+Pb collisions.

The ratio of R_D(z) distributions in three rapidity selections for 10-20 PCT Pb+Pb collisions.

The ratio of R_D(z) distributions in three rapidity selections for 20-30 PCT Pb+Pb collisions.

Covariance matrix of the relative cross-section as function of the top quark pT, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix for the absolute cross-section as function of the hadronic top-quark top quark pT, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix for the absolute cross-section as function of the hadronic top-quark top quark pT, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix for the relative cross-section as function of the hadronic top-quark top quark pT, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix for the relative cross-section as function of the hadronic top-quark top quark pT, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix of the absolute cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the relative cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the relative cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix for the absolute cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix for the absolute cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix for the relative cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix for the relative cross-section as function of the absolute value of the rapidity of the top quark, accounting for the statistic and systematic uncertainties in the boosted topology.

Covariance matrix of the absolute cross-section as function of the mass of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the mass of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the relative cross-section as function of the mass of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the relative cross-section as function of the mass of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the tt̄ system pT, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the tt̄ system pT, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the relative cross-section as function of the tt̄ system pT, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the relative cross-section as function of the tt̄ system pT, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the absolute value of the rapidity of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the absolute value of the rapidity of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the absolute value of the rapidity of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Covariance matrix of the absolute cross-section as function of the absolute value of the rapidity of the tt̄ system, accounting for the statistical and systematic uncertainties in the resolved topology.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the top quark transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the top quark transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the top quark transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the top quark transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the absolute value of the top quark rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the absolute value of the top quark rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the absolute value of the top quark rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the absolute value of the top quark rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the tt̄ system transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the tt̄ system transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the tt̄ system transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the tt̄ system transverse momentum in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the absolute value of the tt̄ system rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the absolute value of the tt̄ system rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the absolute value of the tt̄ system rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the absolute value of the tt̄ system rapidity in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the mass of the tt̄ system in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the mass of the tt̄ system in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the mass of the tt̄ system in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the mass of the tt̄ system in the resolved regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the top quark transverse momentum in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the top quark transverse momentum in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the top quark transverse momentum in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the top quark transverse momentum in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the absolute value of the top quark rapidity in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the absolute differential cross-section at particle level for the absolute value of the top quark rapidity in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the absolute value of the top quark rapidity in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Table of systematic uncertainties for the relative differential cross-section at particle level for the absolute value of the top quark rapidity in the boosted regime. Note that the values shown here are obtained by propagating the individual uncertainties to the measured cross-sections, while the covariance matrices are evaluated using pseudo-experiments as described in the text.

Jet multiplicity distributions in control region CR$^{3\ell 1b}_{VV}$, after normalising the $t\bar{t}Z$ and multi-boson background processes via the simultaneous fit described in Section 5. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty in the background prediction. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

Jet multiplicity distributions in control regions CR$^{1\ell 4b}_{t\bar{t},A}$, after normalising the $t\bar{t}$ background process via the simultaneous fit described in Section 5. The $t\bar{t}$ background normalisation is constrained to the data observation for jet multiplicity values above the requirements shown in Table 6. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. The last bin in each figure contains the overflow. The lower panels show the ratio of the observed data to the total SM background prediction, with the bands representing the total uncertainty in the background prediction.

Jet multiplicity distributions in control regions CR$^{1\ell 4b}_{t\bar{t},A}$, after normalising the $t\bar{t}$ background process via the simultaneous fit described in Section 5. The $t\bar{t}$ background normalisation is constrained to the data observation for jet multiplicity values above the requirements shown in Table 6. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. The last bin in each figure contains the overflow. The lower panels show the ratio of the observed data to the total SM background prediction, with the bands representing the total uncertainty in the background prediction.

Jet multiplicity distributions in control regions CR$^{1\ell 4b}_{t\bar{t},B}$, after normalising the $t\bar{t}$ background process via the simultaneous fit described in Section 5. The $t\bar{t}$ background normalisation is constrained to the data observation for jet multiplicity values above the requirements shown in Table 6. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. The last bin in each figure contains the overflow. The lower panels show the ratio of the observed data to the total SM background prediction, with the bands representing the total uncertainty in the background prediction.

Jet multiplicity distributions in control regions CR$^{1\ell 4b}_{t\bar{t},B}$, after normalising the $t\bar{t}$ background process via the simultaneous fit described in Section 5. The $t\bar{t}$ background normalisation is constrained to the data observation for jet multiplicity values above the requirements shown in Table 6. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. The last bin in each figure contains the overflow. The lower panels show the ratio of the observed data to the total SM background prediction, with the bands representing the total uncertainty in the background prediction.

Jet multiplicity distributions in control regions CR$^{1\ell 4b}_{t\bar{t},C}$, after normalising the $t\bar{t}$ background process via the simultaneous fit described in Section 5. The $t\bar{t}$ background normalisation is constrained to the data observation for jet multiplicity values above the requirements shown in Table 6. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. The last bin in each figure contains the overflow. The lower panels show the ratio of the observed data to the total SM background prediction, with the bands representing the total uncertainty in the background prediction.

Jet multiplicity distributions in control regions CR$^{1\ell 4b}_{t\bar{t},C}$, after normalising the $t\bar{t}$ background process via the simultaneous fit described in Section 5. The $t\bar{t}$ background normalisation is constrained to the data observation for jet multiplicity values above the requirements shown in Table 6. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. The last bin in each figure contains the overflow. The lower panels show the ratio of the observed data to the total SM background prediction, with the bands representing the total uncertainty in the background prediction.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{3\ell 1b}_A$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{3\ell 1b}_A$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{3\ell 1b}_B$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{3\ell 1b}_B$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{3\ell 1b}_C$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{3\ell 1b}_C$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{1\ell 4b}_A$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{1\ell 4b}_A$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{1\ell 4b}_B$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{1\ell 4b}_B$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{1\ell 4b}_C$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $E^{T}_\text{miss}$ for events passing all the signal candidate selection requirements, except that on $E^{T}_\text{miss}$, for SR$^{1\ell 4b}_C$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the mass of the $\tilde{t}_1$ for a fixed $(\tilde{\chi}^0_1) = 0$ GeV, assuming $\text{BR}(\tilde{\chi}^0_2 \to Z\tilde{\chi}^0_1) = 0.5$ and $\text{BR}(\tilde{\chi}^0_2 \to h\tilde{\chi}^0_1) = 0.5$.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the mass of the $\tilde{t}_1$ for a fixed $(\tilde{\chi}^0_1) = 0$ GeV, assuming $\text{BR}(\tilde{\chi}^0_2 \to Z\tilde{\chi}^0_1) = 0.5$ and $\text{BR}(\tilde{\chi}^0_2 \to h\tilde{\chi}^0_1) = 0.5$.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the mass of the $\tilde{t}_1$ for a fixed $(\tilde{\chi}^0_1) = 0$ GeV, assuming $\text{BR}(\tilde{\chi}^0_2 \to Z\tilde{\chi}^0_1) = 0.5$ and $\text{BR}(\tilde{\chi}^0_2 \to h\tilde{\chi}^0_1) = 0.5$.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the mass of the $\tilde{t}_1$ for a fixed $(\tilde{\chi}^0_1) = 0$ GeV, assuming $\text{BR}(\tilde{\chi}^0_2 \to Z\tilde{\chi}^0_1) = 0.5$ and $\text{BR}(\tilde{\chi}^0_2 \to h\tilde{\chi}^0_1) = 0.5$.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to Z\tilde{t}_1) = 1$.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to Z\tilde{t}_1) = 1$.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to Z\tilde{t}_1) = 1$.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to Z\tilde{t}_1) = 1$.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to h\tilde{t}_1) = 1$.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to h\tilde{t}_1) = 1$.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to h\tilde{t}_1) = 1$.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the masses of the $\tilde{t}_2$ and $\tilde{\chi}^0_1$, for a fixed $m(\tilde{t}_1)-m(\tilde{\chi}^0_1) = 180$ GeV and assuming a $\text{BR}(\tilde{t}_2 \to h\tilde{t}_1) = 1$.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=600$ GeV $m(\tilde{\chi}^0_1)=250$ GeV.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=600$ GeV $m(\tilde{\chi}^0_1)=250$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=600$ GeV $m(\tilde{\chi}^0_1)=250$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=600$ GeV $m(\tilde{\chi}^0_1)=250$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $1\ell 4b$ selection for the model $m(\tilde{t}_2)=600$ GeV $m(\tilde{\chi}^0_1)=250$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $1\ell 4b$ selection for the model $m(\tilde{t}_2)=600$ GeV $m(\tilde{\chi}^0_1)=250$ GeV.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$. for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$. for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $3\ell 1b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $1\ell 4b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Observed exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $1\ell 4b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $1\ell 4b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Expected exclusion limits at 95% CL from the analysis of $36.1 \; \text{fb}^{-1}$ of 13 TeV $pp$ collision data as a function of the $\tilde{t}_2$ branching ratio for $\tilde{t}_2 \to \tilde{t}_1 Z$, $\tilde{t}_2 \to \tilde{t}_1 h$ and $\tilde{t}_1 \to t\tilde{\chi}^0_1$ for the $1\ell 4b$ selection for the model $m(\tilde{t}_2)=650$ GeV $m(\tilde{\chi}^0_1)=200$ GeV.

Background fit results for the control and validation regions in the 1$\ell$4$b$ selection. The nominal predictions from MC simulation are given for comparison for the $t\bar{t}$ background, which is normalised to data. The "Others" category contains the contributions from $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $tZ$, and $tWZ$ production. Combined statistical and systematic uncertainties are given. The individual uncertainties can be correlated and do not necessarily add in quadrature to the total systematic uncertainty.

Background fit results for the control and validation regions in the 1$\ell$4$b$ selection. The nominal predictions from MC simulation are given for comparison for the $t\bar{t}$ background, which is normalised to data. The "Others" category contains the contributions from $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $tZ$, and $tWZ$ production. Combined statistical and systematic uncertainties are given. The individual uncertainties can be correlated and do not necessarily add in quadrature to the total systematic uncertainty.

Summary of the main systematic uncertainties and their impact (in %) on the total SM background prediction in each of the signal regions studied. The total systematic uncertainty can be different from the sum in quadrature of individual sources due to the correlations between them resulting from the fit to the data. The quoted theoretical uncertainties include modelling and cross-section uncertainties.

Summary of the main systematic uncertainties and their impact (in %) on the total SM background prediction in each of the signal regions studied. The total systematic uncertainty can be different from the sum in quadrature of individual sources due to the correlations between them resulting from the fit to the data. The quoted theoretical uncertainties include modelling and cross-section uncertainties.

Observed and expected numbers of events the three 3$\ell$1$b$ Signal regions. The nominal predictions from MC simulation are given for comparison for those backgrounds, $t\bar{t} Z$, multi-boson that are normalised to data in dedicated control regions. For SR$^{3\ell 1b}_A$, SR$^{3\ell 1b}_B$ and SR$^{3\ell 1b}_C$, the "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. Combined statistical and systematic uncertainties are given. Signal model-independent 95% CL upper limits on the visible BSM cross-section ($\sigma_{\mathrm{vis}}$), the visible number of signal events ($S^{95}_{\rm obs}$), the number of signal events ($S^{95}_{\rm exp}$) given the expected number of background events (and $\pm1\sigma$ variations of the expected background), and the discovery $p$-value ($p(s = 0)$), all calculated with pseudo-experiments, are also shown for each signal region.

Observed and expected numbers of events the three 3$\ell$1$b$ Signal regions. The nominal predictions from MC simulation are given for comparison for those backgrounds, $t\bar{t} Z$, multi-boson that are normalised to data in dedicated control regions. For SR$^{3\ell 1b}_A$, SR$^{3\ell 1b}_B$ and SR$^{3\ell 1b}_C$, the "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production. Combined statistical and systematic uncertainties are given. Signal model-independent 95% CL upper limits on the visible BSM cross-section ($\sigma_{\mathrm{vis}}$), the visible number of signal events ($S^{95}_{\rm obs}$), the number of signal events ($S^{95}_{\rm exp}$) given the expected number of background events (and $\pm1\sigma$ variations of the expected background), and the discovery $p$-value ($p(s = 0)$), all calculated with pseudo-experiments, are also shown for each signal region.

Observed and expected numbers of events in the three 1$\ell$4$b$ signal regions. The nominal predictions from MC simulation are given for comparison for those backgrounds, $t\bar{t}$, are normalised to data in dedicated control regions. For SR$^{1\ell 4b}_A$, SR$^{1\ell 4b}_B$ and SR$^{1\ell 4b}_C$, the "Others" category contains the contributions from $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $tZ$, and $tWZ$ production. Combined statistical and systematic uncertainties are given. Signal model-independent 95% CL upper limits on the visible BSM cross-section ($\sigma_{\mathrm{vis}}$), the visible number of signal events ($S^{95}_{\rm obs}$), the number of signal events ($S^{95}_{\rm exp}$) given the expected number of background events (and $\pm1\sigma$ variations of the expected background), and the discovery $p$-value ($p(s = 0)$), all calculated with pseudo-experiments, are also shown for each signal region.

Observed and expected numbers of events in the three 1$\ell$4$b$ signal regions. The nominal predictions from MC simulation are given for comparison for those backgrounds, $t\bar{t}$, are normalised to data in dedicated control regions. For SR$^{1\ell 4b}_A$, SR$^{1\ell 4b}_B$ and SR$^{1\ell 4b}_C$, the "Others" category contains the contributions from $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $tZ$, and $tWZ$ production. Combined statistical and systematic uncertainties are given. Signal model-independent 95% CL upper limits on the visible BSM cross-section ($\sigma_{\mathrm{vis}}$), the visible number of signal events ($S^{95}_{\rm obs}$), the number of signal events ($S^{95}_{\rm exp}$) given the expected number of background events (and $\pm1\sigma$ variations of the expected background), and the discovery $p$-value ($p(s = 0)$), all calculated with pseudo-experiments, are also shown for each signal region.

Illustration of the best expected signal region per signal grid point for the $\tilde{t}_2 \rightarrow h\tilde{t}_1$ models with $\tilde{t}_1\to t\tilde{\chi}^0_1$. This mapping is used for the final combined exclusion limits 1 = A, 2 = B, 3 = C.

Illustration of the best expected signal region per signal grid point for the $\tilde{t}_2 \rightarrow h\tilde{t}_1$ models with $\tilde{t}_1\to t\tilde{\chi}^0_1$. This mapping is used for the final combined exclusion limits 1 = A, 2 = B, 3 = C.

Illustration of the best expected signal region per signal grid point for the $\tilde{t}_2 \rightarrow Z\tilde{t}_1$ models with $\tilde{t}_1\to t\tilde{\chi}^0_1$. This mapping is used for the final combined exclusion limits 1 = A, 2 = B, 3 = C.

Illustration of the best expected signal region per signal grid point for the $\tilde{t}_2 \rightarrow Z\tilde{t}_1$ models with $\tilde{t}_1\to t\tilde{\chi}^0_1$. This mapping is used for the final combined exclusion limits 1 = A, 2 = B, 3 = C.

Jet multiplicity distributions in VR$^{1\ell 4b}_C$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

Jet multiplicity distributions in VR$^{1\ell 4b}_C$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

Jet multiplicity distributions in VR$^{1\ell 4b}_B$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

Jet multiplicity distributions in VR$^{1\ell 4b}_B$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

Jet multiplicity distributions in VR$^{1\ell 4b}_A$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

Jet multiplicity distributions in VR$^{1\ell 4b}_A$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

E$^{T}_\text{miss}$ distributions in VR$^{1\ell 4b}_C$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

E$^{T}_\text{miss}$ distributions in VR$^{1\ell 4b}_C$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

E$^{T}_\text{miss}$ distributions in VR$^{1\ell 4b}_B$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

E$^{T}_\text{miss}$ distributions in VR$^{1\ell 4b}_B$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

$E^{T}_\text{miss}$ distributions in VR$^{1\ell 4b}_A$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

$E^{T}_\text{miss}$ distributions in VR$^{1\ell 4b}_A$ for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. The "Others" category contains the contributions from $t\bar{t} h$, $t\bar{t} WW$, $t\bar{t} t$, $t\bar{t} t\bar{t}$, $Wh$, and $Zh$ production.

Jet multiplicity for events with at least 3 jets, one $b$-tagged jets for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. In order to enhance the contribution from fake or non-prompt leptons from $t\bar{t}$ events, the events are required to have at least one different flavour lepton pair and no same flavour pair with opposite charge.

Jet multiplicity for events with at least 3 jets, one $b$-tagged jets for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. In order to enhance the contribution from fake or non-prompt leptons from $t\bar{t}$ events, the events are required to have at least one different flavour lepton pair and no same flavour pair with opposite charge.

$E^{T}_\text{miss}$ for events with at least 3 jets, one $b$-tagged jets for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. In order to enhance the contribution from fake or non-prompt leptons from $t\bar{t}$ events, the events are required to have at least one different flavour lepton pair and no same flavour pair with opposite charge.

$E^{T}_\text{miss}$ for events with at least 3 jets, one $b$-tagged jets for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. In order to enhance the contribution from fake or non-prompt leptons from $t\bar{t}$ events, the events are required to have at least one different flavour lepton pair and no same flavour pair with opposite charge.

$p_{\rm T}^{\ell\ell}$ for events with at least 3 jets, one $b$-tagged jets for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. In order to enhance the contribution from fake or non-prompt leptons from $t\bar{t}$ events, the events are required to have at least one different flavour lepton pair and no same flavour pair with opposite charge.

$p_{\rm T}^{\ell\ell}$ for events with at least 3 jets, one $b$-tagged jets for an integrated luminosity of 36.1 fb$^{-1}$. The contributions from all SM backgrounds are shown as a histogram stack; the bands represent the total uncertainty. In order to enhance the contribution from fake or non-prompt leptons from $t\bar{t}$ events, the events are required to have at least one different flavour lepton pair and no same flavour pair with opposite charge.

Distribution of $m_{bb}$ for events passing all the signal selection requirements, except that on $m_{bb}$, for SR$^{1\ell 4b}_A$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Distribution of $m_{bb}$ for events passing all the signal selection requirements, except that on $m_{bb}$, for SR$^{1\ell 4b}_A$ after the background fit described in Section 5. The contributions from all SM backgrounds are shown; the bands represent the total uncertainty. The last bin in each figure contains the overflow.

Upper limits on cross-sections (in fb) at 95% CL for $\tilde{t}_1$ pair production with $\tilde{t}_1 \to t \tilde{\chi}^0_2$ and $\tilde{\chi}^0_2 \to \tilde{\chi}^0_1 h$ with 50% BR and $\tilde{\chi}^0_2 \to \tilde{\chi}^0_1 Z$ with 50% BR

Upper limits on cross-sections (in fb) at 95% CL for $\tilde{t}_1$ pair production with $\tilde{t}_1 \to t \tilde{\chi}^0_2$ and $\tilde{\chi}^0_2 \to \tilde{\chi}^0_1 h$ with 50% BR and $\tilde{\chi}^0_2 \to \tilde{\chi}^0_1 Z$ with 50% BR

Upper limits on cross-sections (in fb) at 95% CL for $\tilde{t}_2$ pair production with $\tilde{t}_2 \to \tilde{t}_1 h$ with $\tilde{t}_1 \to t\tilde{\chi}^0_1$

Upper limits on cross-sections (in fb) at 95% CL for $\tilde{t}_2$ pair production with $\tilde{t}_2 \to \tilde{t}_1 h$ with $\tilde{t}_1 \to t\tilde{\chi}^0_1$

Upper limits on cross-sections (in fb) at 95% CL for $\tilde{t}_2$ pair production with $\tilde{t}_2 \to \tilde{t}_1 Z$ with $\tilde{t}_1 \to t\tilde{\chi}^0_1$

Upper limits on cross-sections (in fb) at 95% CL for $\tilde{t}_2$ pair production with $\tilde{t}_2 \to \tilde{t}_1 Z$ with $\tilde{t}_1 \to t\tilde{\chi}^0_1$

SR$^{3\ell 1b}_A$ acceptance for each signal model.

SR$^{3\ell 1b}_A$ acceptance for each signal model.

SR$^{3\ell 1b}_B$ acceptance for each signal model.

SR$^{3\ell 1b}_B$ acceptance for each signal model.

SR$^{3\ell 1b}_C$ acceptance for each signal model.

SR$^{3\ell 1b}_C$ acceptance for each signal model.

SR$^{1\ell 4b}_A$ acceptance for each signal model

SR$^{1\ell 4b}_A$ acceptance for each signal model

SR$^{1\ell 4b}_B$ acceptance for each signal model

SR$^{1\ell 4b}_B$ acceptance for each signal model

SR$^{1\ell 4b}_C$ acceptance for each signal model

SR$^{1\ell 4b}_C$ acceptance for each signal model

SR$^{3\ell 1b}_A$ efficiency for each signal model

SR$^{3\ell 1b}_A$ efficiency for each signal model

SR$^{3\ell 1b}_B$ efficiency for each signal model

SR$^{3\ell 1b}_B$ efficiency for each signal model

SR$^{3\ell 1b}_C$ efficiency for each signal model

SR$^{3\ell 1b}_C$ efficiency for each signal model

SR$^{1\ell 4b}_A$ efficiency for each signal model

SR$^{1\ell 4b}_A$ efficiency for each signal model

SR$^{1\ell 4b}_B$ efficiency for each signal model

SR$^{1\ell 4b}_B$ efficiency for each signal model

SR$^{1\ell 4b}_C$ efficiency for each signal model

SR$^{1\ell 4b}_C$ efficiency for each signal model

Number of signal events selected at different stages for some scenarios in the $\tilde{t}_2 \rightarrow h\tilde{t}_1$ with $\tilde{t}_1\to t\tilde{\chi}^0_1$ model.

Number of signal events selected at different stages for some scenarios in the $\tilde{t}_2 \rightarrow h\tilde{t}_1$ with $\tilde{t}_1\to t\tilde{\chi}^0_1$ model.

Number of signal events selected at different stages for some scenarios in the $\tilde{t}_2 \rightarrow Z\tilde{t}_1$ with $\tilde{t}_1\to t\tilde{\chi}^0_1$ model.

Number of signal events selected at different stages for some scenarios in the $\tilde{t}_2 \rightarrow Z\tilde{t}_1$ with $\tilde{t}_1\to t\tilde{\chi}^0_1$ model.

Cutflow table for a pair produced coloron of 1500 GeV decaying into two quarks.

The observed number of data, background and top squark signal events in each of the signal regions of the inclusive selection

The observed number of data, background and coloron signal events in each of the signal regions of the inclusive selection

The observed number of data, background and top squark signal events in each of the signal regions of the b-tagged selection

Signal acceptance and efficiency (in %) as a function of M(STOP), before mass windows

Signal acceptance (in %) and efficiency as a function of M(STOP), after mass windows

Signal acceptance and efficiency (in %) as a function of M(RHO), before mass windows

Signal acceptance and efficiency (in %) as a function of M(RHO), after mass windows

Signal acceptance (in %) and efficiency as a function of M(STOP), before mass windows

Signal acceptance (in %) and efficiency as a function of M(STOP), after mass windows

Cross section excluded at 95% CL as a function of the top squark mass, for a pair produced top squark with decays into a pair of light-quarks.

Cross section excluded at 95% CL as a function of the cooron mass, for a pair produced coloron with decays into a pair of light-quarks.

Cross section excluded at 95% CL as a function of the top squark mass, for a pair produced top squark with decays into a b- and an s-quark.

Upper 95% CL limits on the Z' production cross-section times branching ratio to two electrons as a function of Z' pole mass.

Upper 95% CL limits on the Z' production cross-section times branching ratio to two muons as a function of Z' pole mass.

Upper 95% CL limits on the Z' production cross-section times branching ratio to two leptons as a function of Z' pole mass.

Upper 95% CL limits on the acceptance times Z' production cross-section times branching ratio to two leptons in the dielectron channel as a function of Z' pole mass. Expected limits in the dielectron channel for different widths with an applied mass window of two times the true width of the signal around the pole mass.

Upper 95% CL limits on the acceptance times Z' production cross-section times branching ratio to two leptons in the dielectron channel as a function of Z' pole mass. Observed limits in the dielectron channel for different widths with an applied mass window of two times the true width of the signal around the pole mass.

Upper 95% CL limits on the acceptance times Z' production cross-section times branching ratio to two leptons in the dimuon channel as a function of Z' pole mass. Expected limits in the dimuon channel for different widths with an applied mass window of two times the true width of the signal around the pole mass.

Upper 95% CL limits on the acceptance times Z' production cross-section times branching ratio to two leptons in the dimuon channel as a function of Z' pole mass. Observed limits in the dimuon channel for different widths with an applied mass window of two times the true width of the signal around the pole mass.

Upper 95% CL limits on the acceptance times Z' production cross-section times branching ratio to two leptons in the combined dilepton channel as a function of Z' pole mass. Expected limits in the dilepton channel for different widths with an applied mass window of two times the true width of the signal around the pole mass.

Upper 95% CL limits on the acceptance times Z' production cross-section times branching ratio to two leptons in the dilepton channel as a function of Z' pole mass. Observed limits in the dilepton channel for different widths with an applied mass window of two times the true width of the signal around the pole mass.

The number of events as a function of the dijet invariant mass, compared to background prediction from fit and corresponding uncertainties, in the region defined by |y*|<1.2 optimized for the W* search.

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [3.4-3.7] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [3.4-3.7] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [3.7-4.0] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [3.7-4.0] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.0-4.3] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.0-4.3] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.3-4.6] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.3-4.6] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.6-4.9] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.6-4.9] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.9-5.4] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in [4.9-5.4] TeV dijet invariant mass region

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in dijet invariant mass region above 5.4 TeV

The number of events normalized to bin width as a function of the chi angular separation between the two jets, compared to background prediction from Monte Carlo simulation and corresponding uncertainties, in dijet invariant mass region above 5.4 TeV