The expected upper limits on the production cross-section times the product of branching ratios for the benchmark signal scenario involving a scalar particle $X$ with narrow width decaying via $X\rightarrow aa\rightarrow 4\gamma$, $\sigma_X\times B(X\rightarrow aa)\times B(a\rightarrow\gamma\gamma)^2$. The limits for $m_{a}$ = 5 GeV and 10 GeV do not cover as large a range as the other mass points, since the region of interest is limited to $ m_{a} < 0.01 \times m_{X}$. Additionally, the expected limits are not provided for a small number of points, indicated with a hyphen, because of a technical failure with the computation.

The observed upper limits on the production cross-section times the product of branching ratios for the benchmark signal scenario involving a scalar particle $X$ with narrow width decaying via $X\rightarrow aa\rightarrow 6\pi^0$, $\sigma_X\times B(X\rightarrow aa)\times B(a\rightarrow 3\pi^0)^2$. The limits for $m_{a}$ = 5 GeV and 10 GeV do not cover as large a range as the other mass points, since the region of interest is limited to $ m_{a} < 0.01 \times m_{X}$.

The expected upper limits on the production cross-section times the product of branching ratios for the benchmark signal scenario involving a scalar particle $X$ with narrow width decaying via $X\rightarrow aa\rightarrow 6\pi^0$, $\sigma_X\times B(X\rightarrow aa)\times B(a\rightarrow 3\pi^0)^2$. The limits for $m_{a}$ = 5 GeV and 10 GeV do not cover as large a range as the other mass points, since the region of interest is limited to $ m_{a} < 0.01 \times m_{X}$. Additionally, the expected limits are not provided for a small number of points, indicated with a hyphen, because of a technical failure with the computation.

Observed 95% CL upper limits on the visible cross section as a function of $m_X$ and the fraction of events in the low-$\Delta E$ category.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.1 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.5 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.7 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 1 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 2 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 5 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 10 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 0.5 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 0.7 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 1 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 2 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 5 GeV.

Selection efficiency for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 10 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.1 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.5 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 0.7 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 1 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 2 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 5 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 2\gamma$ with $m_a$ = 10 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 0.5 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 0.7 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 1 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 2 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 5 GeV.

Fraction of reconstructed photons with a value of shower shape variable $\Delta E$ lower than the threshold, for reconstructed photons originating from the decay $a\rightarrow 3\pi^0\rightarrow 6\gamma$ with $m_a$ = 10 GeV.

Selection efficiency for photons originating from the BSM process $X\rightarrow\gamma\gamma$, where the $X$ particle is a high-mass narrow-width scalar particle originating from the gluon--gluon fusion process.

Fraction of photons with a value of shower shape variable $\Delta E$ lower than the threshold, for photons originating from the BSM process $X\rightarrow\gamma\gamma$, where the $X$ particle is a high-mass narrow-width scalar particle originating from the gluon--gluon fusion process.

1$\tau$ MediumMass SR eff.

2$\tau$ Compressed SR eff.

2$\tau$ Compressed SR eff.

2$\tau$ HighMass SR eff.

2$\tau$ HighMass SR eff.

2$\tau$ multibin SR eff.

2$\tau$ multibin SR eff.

2$\tau$ GMSB SR eff.

2$\tau$ GMSB SR eff.

1$\tau$ Compressed SR eff.

1$\tau$ Compressed SR eff.

1$\tau$ MediumMass SR eff.

1$\tau$ MediumMass SR eff.

2$\tau$ Compressed SR eff.

2$\tau$ Compressed SR eff.

2$\tau$ HighMass SR eff.

2$\tau$ HighMass SR eff.

2$\tau$ multibin SR eff.

2$\tau$ multibin SR eff.

2$\tau$ GMSB SR eff.

2$\tau$ GMSB SR eff.

1$\tau$ Compressed SR acceptance.

1$\tau$ Compressed SR acceptance.

1$\tau$ MediumMass SR acceptance.

1$\tau$ MediumMass SR acceptance.

2$\tau$ Compressed SR acceptance.

2$\tau$ Compressed SR acceptance.

2$\tau$ HighMass SR acceptance.

2$\tau$ HighMass SR acceptance.

2$\tau$ multibin SR acceptance.

2$\tau$ multibin SR acceptance.

2$\tau$ GMSB SR acceptance.

2$\tau$ GMSB SR acceptance.

1$\tau$ Compressed SR acceptance.

1$\tau$ Compressed SR acceptance.

1$\tau$ MediumMass SR acceptance.

1$\tau$ MediumMass SR acceptance.

2$\tau$ Compressed SR acceptance.

2$\tau$ Compressed SR acceptance.

2$\tau$ HighMass SR acceptance.

2$\tau$ HighMass SR acceptance.

2$\tau$ multibin SR acceptance.

2$\tau$ multibin SR acceptance.

2$\tau$ GMSB SR acceptance.

2$\tau$ GMSB SR acceptance.

Cutflow table of the $1\tau$ compressed SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $1\tau$ compressed SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $1\tau$ medium-mass SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $1\tau$ medium-mass SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ compressed SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ compressed SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ high-mass SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ high-mass SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ multibin SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ multibin SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ GMSB SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Cutflow table of the $2\tau$ GMSB SR for the four signal benchmark scenarios of low, medium, and high mass-splitting in the simplified model as well as the GMSB model.

Best performing fit setups entering the final combination as a function of the LSP mass and the gluino mass. 'S' marks the simultaneous fit of the four simplified model single-bin SRs, 'M' denotes the simultaneous fit of the two $1\tau$ SRs and the $2\tau$ multibin SR.

Best performing fit setups entering the final combination as a function of the LSP mass and the gluino mass. 'S' marks the simultaneous fit of the four simplified model single-bin SRs, 'M' denotes the simultaneous fit of the two $1\tau$ SRs and the $2\tau$ multibin SR.

Observed exclusion contour at 95% CL as a function of tanBeta and the SUSY-breaking mass scale Lambda.

Observed exclusion contour at 95% CL as a function of tanBeta and the SUSY-breaking mass scale Lambda.

Expected exclusion contour at 95% CL as a function of tanBeta and the SUSY-breaking mass scale Lambda.

Expected exclusion contour at 95% CL as a function of tanBeta and the SUSY-breaking mass scale Lambda.

Observed exclusion contour at 95% CL as a function of the LSP mass and the gluino mass.

Observed exclusion contour at 95% CL as a function of the LSP mass and the gluino mass.

Expected exclusion contour at 95% CL as a function of the LSP mass and the gluino mass.

Expected exclusion contour at 95% CL as a function of the LSP mass and the gluino mass.

Observed upper limits on the production cross section at 95% CL in pb as a function of tanBeta and SUSY breaking mass scale Lambda.

Observed upper limits on the production cross section at 95% CL in pb as a function of tanBeta and SUSY breaking mass scale Lambda.

Observed upper limits on the production cross section at 95% CL in pb as a function of the LSP mass and the gluino mass.

Observed upper limits on the production cross section at 95% CL in pb as a function of the LSP mass and the gluino mass.

Yields of the expected background from the SM in the bins of the multibin SR of the $2\tau$ channel with all bins being simultaneously used to constrain the background prediction. Expectation is given with the scalings computed in the combined fit applied. Uncertainties are statistial plus systematrics. Only the subsamples contributing the respective region are considered.

Yields of the expected background from the SM in the bins of the multibin SR of the $2\tau$ channel with all bins being simultaneously used to constrain the background prediction. Expectation is given with the scalings computed in the combined fit applied. Uncertainties are statistial plus systematrics. Only the subsamples contributing the respective region are considered.

$m_{\mathrm{T}}^{\tau}$ in the compressed $m_{\mathrm{T}}^{\tau}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau}$ in the compressed $m_{\mathrm{T}}^{\tau}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$E_{\mathrm{T}}^{\mathrm{miss}}$ in the compressed $E_{\mathrm{T}}^{\mathrm{miss}}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$E_{\mathrm{T}}^{\mathrm{miss}}$ in the compressed $E_{\mathrm{T}}^{\mathrm{miss}}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau}$ in the medium-mass $m_{\mathrm{T}}^{\tau}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau}$ in the medium-mass $m_{\mathrm{T}}^{\tau}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$E_{\mathrm{T}}^{\mathrm{miss}}$ in the medium-mass $E_{\mathrm{T}}^{\mathrm{miss}}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$E_{\mathrm{T}}^{\mathrm{miss}}$ in the medium-mass $E_{\mathrm{T}}^{\mathrm{miss}}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$H_{\mathrm{T}}$ in the medium-mass $H_{\mathrm{T}}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$H_{\mathrm{T}}$ in the medium-mass $H_{\mathrm{T}}$ VR of the $1\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau_1}$ + $m_{\mathrm{T}}^{\tau_2}$ in the top VR of the $2\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau_1}$ + $m_{\mathrm{T}}^{\tau_2}$ in the top VR of the $2\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$H_{\mathrm{T}}$ in the $W$ VR of the $2\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$H_{\mathrm{T}}$ in the $W$ VR of the $2\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau_1}$ + $m_{\mathrm{T}}^{\tau_2}$ in the $Z$ VR of the $2\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau_1}$ + $m_{\mathrm{T}}^{\tau_2}$ in the $Z$ VR of the $2\tau$ channel, illustrating the background modeling after the fit. The last bin includes overflow events.

$m_{\mathrm{T}}^{\tau}$ in the compressed SR of the $1\tau$ channel before application of the $m_{\mathrm{T}}^{\tau}$ > 80 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$m_{\mathrm{T}}^{\tau}$ in the compressed SR of the $1\tau$ channel before application of the $m_{\mathrm{T}}^{\tau}$ > 80 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$H_{\mathrm{T}}$ in the medium-mass SR of the $1\tau$ channel before application of the $H_{\mathrm{T}}$ > 1000 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$H_{\mathrm{T}}$ in the medium-mass SR of the $1\tau$ channel before application of the $H_{\mathrm{T}}$ > 1000 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$m_{\mathrm{T}}^{\mathrm{sum}}$ in the compressed SR of the $2\tau$ channel before application of the $m_{\mathrm{T}}^{\mathrm{sum}}$ > 1600 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$m_{\mathrm{T}}^{\mathrm{sum}}$ in the compressed SR of the $2\tau$ channel before application of the $m_{\mathrm{T}}^{\mathrm{sum}}$ > 1600 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$H_{\mathrm{T}}$ in the high-mass SR of the $2\tau$ channel before application of the $H_{\mathrm{T}}$ > 1100 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$H_{\mathrm{T}}$ in the high-mass SR of the $2\tau$ channel before application of the $H_{\mathrm{T}}$ > 1100 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

mT(tau_1) + mT(tau_2) in the multibin SR of the 2T channel. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

mT(tau_1) + mT(tau_2) in the multibin SR of the 2T channel. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$H_{\mathrm{T}}$ in the GMSB SR of the $2\tau$ channel before application of the $H_{\mathrm{T}}$ > 1900 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

$H_{\mathrm{T}}$ in the GMSB SR of the $2\tau$ channel before application of the $H_{\mathrm{T}}$ > 1900 GeV requirement. The last bin includes overflow events. Signal predictions corresponding to the simplified model scenarios of low (LM), medium (MM), and high mass-splitting (HM) as well as for the GMSB benchmark are given.

Expected and observed upper limits on $\tan\beta$ as a function of $m_{H^{+}}$ in the hMSSM scenario of the MSSM. Limits are shown for $\tan\beta$ values in the range of 0.5-60, where predictions are available from both scenarios. The bands surrounding the expected limits show the 68% and 95% confidence intervals. The limits are based on the combination of the $\ell+$jets and $\ell\ell$ final states. The production cross-section of $t\bar{t}H$ and $tH$, as well as the branching ratios of the $H$, are fixed to their SM values at each point in the plane. Uncertainties on the predicted $H^{+}$ cross-sections or branching ratios are not considered.

Expected and observed lower limits on $\tan\beta$ as a function of $m_{H^{+}}$ in the hMSSM scenario of the MSSM. Limits are shown for $\tan\beta$ values in the range of 0.5-60, where predictions are available from both scenarios. The bands surrounding the expected limits show the 68% and 95% confidence intervals. The limits are based on the combination of the $\ell+$jets and $\ell\ell$ final states. The production cross-section of $t\bar{t}H$ and $tH$, as well as the branching ratios of the $H$, are fixed to their SM values at each point in the plane. Uncertainties on the predicted $H^{+}$ cross-sections or branching ratios are not considered.

Expected and observed 95% CL lower limits on the mass of a vector-like $T$ quark in the branching-ratio plane.

Expected and observed 95% CL lower limits on the mass of a vector-like $B$ quark in the branching-ratio plane.

Expected and observed upper limits at the 95% CL on the $T\bar T$ cross section as a function of $T$ mass under the assumption BR($T\to Wb$)=1.

Expected and observed upper limits at the 95% CL on the $B\bar B$ cross section as a function of $B$ mass under the assumption BR($T\to Zt$)=1.

Expected and observed upper limits at the 95% CL on the $B\bar B$ cross section as a function of $B$ mass under the assumption BR($B\to Wt$)=1.

Expected and observed upper limits at the 95% CL on the $B\bar B$ cross section as a function of $B$ mass under the assumption BR($B\to Zb$)=1.

Expected and observed limits on vector-like T-quark pair production as a function of mass, assuming the branching ratios expected in the singlet model.

Mass hypotheses excluded at 95% CL as a function of the branching ratio, expected and observed limits for a vector-like B-quark.

Mass hypotheses excluded at 95% CL as a function of the branching ratio, expected and observed limits for a vector-like B-quark.

Mass hypotheses excluded at 95% CL as a function of the branching ratio, expected and observed limits for a vector-like T-quark.

Mass hypotheses excluded at 95% CL as a function of the branching ratio, expected and observed limits for a vector-like T-quark.

Expected and observed limits on vector-like T5/3 pair production as a function of mass, assuming a branching ratio B(T5/3 -> Wt) = 100%.

Expected and observed limits on vector-like T5/3 pair production as a function of mass, assuming a branching ratio B(T5/3 -> Wt) = 100%.

Expected and observed limits on vector-like T5/3 single- plus pair-production as a function of mass and T5/3tW coupling assuming a branching ratio B(T5/3 -> Wt) = 100%.

Expected and observed limits on vector-like T5/3 single- plus pair-production as a function of mass and T5/3tW coupling assuming a branching ratio B(T5/3 -> Wt) = 100%.

Expected and observed limits on photon KK excitation pair-production as a function of the KK excitation mass of the photon in the 2UED/RPP model assuming a branching ratio B(A(1,1)-> t tbar)) = 100%.

Expected and observed limits on photon KK excitation pair-production as a function of the KK excitation mass of the photon in the 2UED/RPP model assuming a branching ratio B(A(1,1)-> t tbar)) = 100%.

Expected and observed limits on the cross-section of the four-top-quark production through a heavy scalar Higgs boson times the branching ratio for the Higgs boson to decay into t tbar as a function of the heavy scalar Higgs mass.

Expected and observed limits on the cross-section of the four-top-quark production through a heavy scalar Higgs boson times the branching ratio for the Higgs boson to decay into t tbar as a function of the heavy scalar Higgs mass.

Expected and observed limits on the cross-section for prompt tt production as a function of the mass of the exotic FCNC mediator particle in a dark matter model.

Expected and observed limits on the cross-section for prompt tt production as a function of the mass of the exotic FCNC mediator particle in a dark matter model.

Expected and observed limits on the cross-section for on-shell mediator subprocesses of the same-sign top-quark pair production as a function of the mass of the exotic FCNC mediator particle in a dark matter model.

Expected and observed limits on the cross-section for on-shell mediator subprocesses of the same-sign top-quark pair production as a function of the mass of the exotic FCNC mediator particle in a dark matter model.

Expected and observed limits on the cross-section for off-shell mediator subprocesses of the same-sign top-quark pair production as a function of the mass of the exotic FCNC mediator particle in a dark matter model.

Expected and observed limits on the cross-section for off-shell mediator subprocesses of the same-sign top-quark pair production as a function of the mass of the exotic FCNC mediator particle in a dark matter model.

Expected and observed constraints in the (gSM, mV) plane for the combined visible same-sign top-quark pair production for gSM=0.1

Expected and observed constraints in the (gSM, mV) plane for the combined visible same-sign top-quark pair production for gSM=0.1

Expected and observed constraints in the (gSM, mV) plane for the combined visible same-sign top-quark pair production for gSM=0.5

Expected and observed constraints in the (gSM, mV) plane for the combined visible same-sign top-quark pair production for gSM=0.5

Expected and observed constraints in the (gSM, mV) plane for the combined visible same-sign top-quark pair production for gSM=1.0

Expected and observed constraints in the (gSM, mV) plane for the combined visible same-sign top-quark pair production for gSM=1.0

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-W/Z signal region with the merged event topology after the profile-likelihood fit. This is shown for the 0b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-W/Z signal region with the merged event topology after the profile-likelihood fit. This is shown for the 1b-tagged jet, high purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-W/Z signal region with the merged event topology after the profile-likelihood fit. This is shown for the 1b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-W/Z signal region with the merged event topology after the profile-likelihood fit. This is shown for the 2b-tagged jet event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-W/Z signal region with the resolved event topology after the profile-likelihood fit. This is shown for the 0b-tagged jet event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-W/Z signal region with the resolved event topology after the profile-likelihood fit. This is shown for the 1b-tagged jet event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-W/Z signal region with the resolved event topology after the profile-likelihood fit. This is shown for the 2b-tagged jet event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, high purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, high purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 350 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 350 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 90 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 350 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

Expected exclusion contours at 95% C.L. of the dark matter mediator particles (m_chi, m_Zp) for the combined mono-W and mono-Z search in the frame of the simplified model with the Dirac DM particles and couplings g_SM = 0.25 and g_DM = 1.

Observed exclusion contours at 95% C.L. of the dark matter mediator particles (m_chi, m_Zp) for the combined mono-W and mono-Z search in the frame of the simplified model with the Dirac DM particles and couplings g_SM = 0.25 and g_DM = 1.

Exclusion contours at 95% C.L. of the cross section as a function of Z' mass (mZp), for the mono-Z' dark fermion model, with the light dark sector scenario, with parameters g_SM = 0.1 and g_DM = 1.

Exclusion contours at 95% C.L. of the cross section as a function of Z' mass (mZp), for the mono-Z' dark fermion model, with the heavy dark sector scenario, with parameters g_SM = 0.1 and g_DM = 1.

Exclusion contours at 95% C.L. of the cross section as a function of Z' mass (mZp), for the mono-Z' dark Higgs model, with the light dark sector scenario, with parameters g_SM = 0.1 and g_DM = 1.

Exclusion contours at 95% C.L. of the cross section as a function of Z' mass (mZp), for the mono-Z' dark Higgs model, with the heavy dark sector scenario, with parameters g_SM = 0.1 and g_DM = 1.

Exclusion contours at 95% C.L. of the product of the couplings g_SM g_DM as a function of Z' mass (mZp), for the mono-Z' dark fermion model, with the light dark sector scenario, with parameter g_DM = 1.

Exclusion contours at 95% C.L. of the product of the couplings g_SM g_DM as a function of Z' mass (mZp), for the mono-Z' dark fermion model, with the heavy dark sector scenario, with parameter g_DM = 1.

Exclusion contours at 95% C.L. of the product of the couplings g_SM g_DM as a function of Z' mass (mZp), for the mono-Z' dark Higgs model, with the light dark sector scenario, with parameter g_DM = 1.

Exclusion contours at 95% C.L. of the product of the couplings g_SM g_DM as a function of Z' mass (mZp), for the mono-Z' dark Higgs model, with the heavy dark sector scenario, with parameter g_DM = 1.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, high purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, high purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 80 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, low purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, high purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, high purity, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the merged event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 100 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 110 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 110 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 110 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 120 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 120 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 120 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 130 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 130 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 130 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 140 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 140 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 140 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 150 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 150 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 150 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 160 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 160 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 160 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 170 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 170 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 170 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 180 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 180 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 180 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 190 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 190 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 190 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 200 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 200 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 200 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 250 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 250 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 250 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 300 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 300 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 300 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 400 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 400 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 400 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 450 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 450 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 450 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 500 GeV after the profile-likelihood fit. This is shown for the 0b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 500 GeV after the profile-likelihood fit. This is shown for the 1b-tagged jet, event category.

The observed and expected MET distributions with 36.1fb-1 of data with sqrt(s) = 13 TeV in the mono-Z' signal region with the resolved event topology for a Z' mass of 500 GeV after the profile-likelihood fit. This is shown for the 2b-tagged jet, event category.

Observed and expected 95% CL upper limits on the cross-section of gluon-fusion initialted resonant production of the mass of the resonance times the branch ratio of X to HH and the BR of HH to gammagamma WW, without assuming the BR of H to gammagamma and H to WW.

The systematic uncertainty on the unfolded distribution as a function of minimax-mbl, broken down by components.

The covariance matrix for the unfolded, normalized data in bins of minimax-mbl shown in Figure 2. Redundant entries are suppressed.

Leading lepton transverse momentum distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

Sub-leading lepton transverse momentum distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

Leading lepton pseudorapidity distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

Sub-leading lepton pseudorapidity distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

Leading b-jet transverse momentum distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

Sub-leading b-jet transverse momentum distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

Leading b-jet pseudorapidity distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

Sub-leading b-jet pseudorapidity distribution for events passing the signal selection in bins of minimax-mbl. The data here are not unfolded.

The detector-level minimax-m(bl) distribution for events entering the Z+jets control region.

The detector-level minimax-m(bl) distribution for events entering the same-sign lepton control region.

Exclusion limits on higgsino pair production divided by the theory cross-section.The results of the low-mass analysis are used below m(higgsino) = 300 GeV, while those of the high-mass analysis are used above. The figure shows the observed and expected 95% upper limits on the higgsino pair production cross-section as a function of m(higgsino).

Observed and expected 95% limits in the m(higgsino) vs BR(higgsino to higgs+gravitino) plane. The regions above the lines are excluded by the analyses.

The observed and expected 95% upper limits on the total pair production cross section for degenerate higgsinos as a function of m(higgsino) for the high-mass search. Only the high-mass analysis results are used in this figure.

The observed and expected 95% upper limits on the total pair production cross section for degenerate higgsinos as a function of m(higgsino) for the high-mass search, divided by the theory cross section. Only the high-mass analysis results are used in this figure.

The observed and expected 95% upper limits on the total pair production cross section for degenerate higgsinos as a function of m(higgsino) for the low-mass search. Only the low-mass analysis results are used in this figure.

The observed and expected 95% upper limits on the total pair production cross section for degenerate higgsinos as a function of m(higgsino) for the low-mass search, divided by the theory cross section. Only the low-mass analysis results are used in this figure.

Particle-level acceptance for the low-mass discovery signal regions low-SR-MET0-meff440 and low-SR-MET150-meff440, shown as a function of higgsino mass. The acceptance is defined as the fraction of signal events passing the particle-level event selection that emulates the detector-level selection. The acceptance calculation considers only those signal events where both higgsinos decay to Higgs bosons that subsequently both decay to b-quarks.

The experimental efficiency of the low-mass analysis, for the two discovery signal regions low-SR-MET0-meff440 and low-SR-MET150-meff440, as a function of higgsino mass. The experimental efficiency is defined as the number of events passing the detector-level event selection divided by the number of events passing the event selection for a perfect detector. The denominator is obtained by implementing particle-level event selection that emulate the detector-level selection. Such particle-level selection is not applied on the numerator.

Particle-level acceptance for the high-mass discovery signal regions SR-4b-meff1-A-disc and SR-3b-meff3-A, shown as a function of higgsino mass. The acceptance is defined as the fraction of signal events passing the particle-level event selection that emulates the detector-level selection. The acceptance calculation considers only those signal events where both higgsinos decay to Higgs bosons that subsequently both decay to b-quarks.

The experimental efficiency of the high-mass analysis, for the two discovery signal regions SR-4b-meff1-A-disc and SR-3b-meff3-A, as a function of higgsino mass. The experimental efficiency is defined as the number of events passing the detector-level event selection divided by the number of events passing the event selection for a perfect detector. The denominator is obtained by implementing particle-level event selection that emulate the detector-level selection. Such particle-level selection is not applied on the numerator.

Example cutflow for SR-3b-meff3-A.

Example cutflow for SR-4b-meff1-A-disc.

Cutflow for low-mass analysis for each signal mass point.

Distributions of kinematic variables in the signal regions for the $2\ell$ channels after applying all selection requirements. The histograms show the post-fit background predictions. The last bin includes the overflow. The distribution for $R_{\textrm{ISR}}$ in SR$2\ell$_ISR is plotted. The expected distribution for a benchmark signal model, normalized to the NLO+NLL cross-section times integrated luminosity, is also shown for comparison.

Distributions of kinematic variables in the signal regions for the $3\ell$ channels after applying all selection requirements. The histograms show the post-fit background predictions. The last bin includes the overflow. The distribution for $H_{3,1}^{\textrm{PP}}$ in SR$3\ell$_Low is plotted. The expected distribution for a benchmark signal model, normalized to the NLO+NLL cross-section times integrated luminosity, is also shown for comparison.

Distributions of kinematic variables in the signal regions for the $3\ell$ channels after applying all selection requirements. The histograms show the post-fit background predictions. The last bin includes the overflow. The distribution of $p_{\textrm{T}}^{\ell_{1}}$ in SR$3\ell$_Low is plotted. The expected distribution for a benchmark signal model, normalized to the NLO+NLL cross-section times integrated luminosity, is also shown for comparison.

Distributions of kinematic variables in the signal regions for the $3\ell$ channels after applying all selection requirements. The histograms show the post-fit background predictions. The last bin includes the overflow. The distribution of $p_{\mathrm{T\ ISR}}^{~\textrm{CM}}$ in SR$3\ell$_ISR is plotted. The expected distribution for a benchmark signal model, normalized to the NLO+NLL cross-section times integrated luminosity, is also shown for comparison.

Distributions of kinematic variables in the signal regions for the $3\ell$ channels after applying all selection requirements. The histograms show the post-fit background predictions. The last bin includes the overflow. The distribution of $R_{\textrm{ISR}}$ in SR$3\ell$_ISR is plotted. The expected distribution for a benchmark signal model, normalized to the NLO+NLL cross-section times integrated luminosity, is also shown for comparison.

Expected exclusion limits at 95% CL on the masses of C1/N2 and N1 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the 2$\ell$ search, assuming 100\% branching ratio of the sparticles to decay to SM $W/Z$ bosons and LSP.

Observed exclusion limits at 95% CL on the masses of C1/N2 and N1 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the 2$\ell$ search, assuming 100% branching ratio of the sparticles to decay to SM $W/Z$ bosons and LSP.

Expected exclusion limits at 95% CL on the masses of C1/N2 and N1 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the the $3\ell$ search, assuming 100% branching ratio of the sparticles to decay to SM $W/Z$ bosons and LSP.

Observed exclusion limits at 95% CL on the masses of C1/N2 and N1 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the the $3\ell$ search, assuming 100% branching ratio of the sparticles to decay to SM $W/Z$ bosons and LSP.

Expected exclusion limits at 95% CL on the masses of C1/N2 and N1 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the statistical combination of the $2\ell$ and 3$\ell$ search channels, assuming 100\% branching ratio of the sparticles to decay to SM $W/Z$ bosons and LSP.

Observed exclusion limits at 95% CL on the masses of C1/N2 and N1 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the statistical combination of the $2\ell$ and 3$\ell$ search channels, assuming 100% branching ratio of the sparticles to decay to SM $W/Z$ bosons and LSP.

Signal region acceptance for chargino-neutralino production in SR2L_High. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR2L_High.

Signal region acceptanceXefficiency for chargino-neutralino production in SR2L_High.

Signal region acceptance for chargino-neutralino production in SR2L_Int. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR2L_Int.

Signal region acceptanceXefficiency for chargino-neutralino production in SR2L_Int.

Signal region acceptance for chargino-neutralino production in SR2L_Low. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR2L_Low.

Signal region acceptanceXefficiency for chargino-neutralino production in SR2L_Low.

Signal region acceptance for chargino-neutralino production in SR2L_ISR. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR2L_ISR.

Signal region acceptanceXefficiency for chargino-neutralino production in SR2L_ISR.

Signal region acceptance for chargino-neutralino production in SR3L_High. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR3L_High.

Signal region acceptanceXefficiency for chargino-neutralino production in SR3L_High.

Signal region acceptance for chargino-neutralino production in SR3L_Int. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR3L_Int.

Signal region acceptanceXefficiency for chargino-neutralino production in SR3L_Int.

Signal region acceptance for chargino-neutralino production in SR3L_Low. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR3L_Low.

Signal region acceptanceXefficiency for chargino-neutralino production in SR3L_Low.

Signal region acceptance for chargino-neutralino production in SR3L_ISR. The acceptance is with respect to all possible $W/Z$ decays.

Signal region efficiency for chargino-neutralino production in SR3L_ISR.

Signal region acceptanceXefficiency for chargino-neutralino production in SR3L_ISR.

Observed 95% CL upper limit on the production cross-section of C1/N2 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the 2$\ell$ search, assuming 100% branching ratio of the sparticles to decay to SM $W/Z$ bosons and N1.

Observed 95% CL upper limit on the production cross-section of C1/N2 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the 3$\ell$ search, assuming 100% branching ratio of the sparticles to decay to SM $W/Z$ bosons and N1.

Observed 95% CL upper limit on the production cross-section of C1/N2 from the analysis of 36.1fb$^{-1}$ of 13 TeV $pp$ collision data obtained from the statistical combination of 2 and 3$\ell$ searches, assuming 100% branching ratio of the sparticles to decay to SM $W/Z$ bosons and N1.

Signal cutflow for SR2L_High and m[C1/N2,N1] = [500,0] GeV. 5000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.

Signal cutflow for SR2L_Int and m[C1/N2,N1] = [400,200] GeV. 10000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.

Signal cutflow for SR2L_Low and m[C1/N2,N1] = [200,100] GeV. 20000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.

Signal cutflow for SR2L_ISR and m[C1/N2,N1] = [200,100] GeV. 20000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.

Signal cutflow for SR3L_High and m[C1/N2,N1] = [500,0] GeV. 5000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.

Signal cutflow for SR3L_Int and m[C1/N2,N1] = [400,200] GeV. 10000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.

Signal cutflow for SR3L_Low and m[C1/N2,N1] = [200,100] GeV. 20000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.

Signal cutflow for SR3L_ISR and m[C1/N2,N1] = [200,100] GeV. 20000 events were generated for this point. The unweighted number of events correspond to the number of selected MC events in the produced sample, while the weighted yield is normalized to the luminosity of the data.