The covariance matrix containing the experimental uncertainties of Figure 2a is shown.

The covariance matrix containing the model uncertainties of Figure 2a is shown.

The covariance matrix containing the statistical uncertainties of Figure 2b is shown.

The covariance matrix containing the experimental uncertainties of Figure 2b is shown.

The covariance matrix containing the model uncertainties of Figure 2b is shown.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and a $\tilde{\chi}_1^\pm$ that decays to $W^\pm\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction to $q_i\bar{q}_j W\pm\tilde{\chi}_1^0$.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to bottom quarks ($\tilde{g}\to b\bar{b}\tilde{\chi}_1^0$). Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to top quarks ($\tilde{g}\to t\bar{t}\tilde{\chi}_1^0$). Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for light-flavor squark pair production, where the squarks decay to $q\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay and 1-fold degeneracy in the light-flavor squarks (corresponding to the inner set of curves in the limit plot). To get the theory cross section for other N-fold degeneracy assumptions (e.g. 8-fold for the outer curves in the limit plot), just multiply by N.

Exclusion limits at 95% CL for bottom squark pair production, where the squarks decay to $b\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay to $t\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay to $b\tilde{\chi}_1^\pm$ and the $\tilde{\chi}_1^0$ decay to $W^\pm\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay either to $b\tilde{\chi}_1^\pm\to bW^\pm\tilde{\chi}_1^0$ or to $t\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for top squark pair production, where the squarks decay to $c\tilde{\chi}_1^0$. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, assuming unity branching fraction for the given decay.

Exclusion limits at 95% CL for the mono-$\phi$ model, in which a resonantly-produced colored scalar decays to a massive Dirac fermion and a quark. Signal cross sections are calculated at leading order in $\alpha_S$, assuming unity branching fraction for the given decay.

Cross section limits for $\mathrm{LQ}\to\mathrm{q}\nu$, where $q=u,\,d,\,s,\,\mathrm{or}\,c$. Limits are at the 95% confidence level. Theory cross sections are LO for vector LQ, and NLO for scalar LQ. Branching ratio is assumed to be 100% to $\mathrm{q}\nu$.

Cross section limits for $\mathrm{LQ}\to\mathrm{b}\nu$. Limits are at the 95% confidence level. Theory cross sections are LO for vector LQ, and NLO for scalar LQ. Branching ratio is assumed to be 100% to $\mathrm{b}\nu$.

Cross section limits for $\mathrm{LQ}\to\mathrm{t}\nu$. Limits are at the 95% confidence level. Theory cross sections are LO for vector LQ, and NLO for scalar LQ. Branching ratios are assumed to be $\mathcal{B}(\mathrm{LQ}\to\mathrm{t}\nu)=1-\beta$, and $\mathcal{B}(\mathrm{LQ}\to\mathrm{b}\tau)=\beta$.

Predictions and observations for monojet signal regions

Predictions and observations for signal regions with $250 \leq H_\mathrm{T} < 450$ GeV

Predictions and observations for signal regions with $450 \leq H_\mathrm{T} < 575$ GeV and $N_\mathrm{j}<7$

Predictions and observations for signal regions with $450 \leq H_\mathrm{T} < 575$ GeV and $N_\mathrm{j}\geq7$

Predictions and observations for signal regions with $575 \leq H_\mathrm{T} < 1200$ GeV and $N_\mathrm{j}^\mathrm{hi}<4$

Predictions and observations for signal regions with $575 \leq H_\mathrm{T} < 1200$ GeV and $4\leq N_\mathrm{j}^\mathrm{hi}<7$

Predictions and observations for signal regions with $575 \leq H_\mathrm{T} < 1200$ GeV and $N_\mathrm{j}\geq7$

Predictions and observations for signal regions with $1200 \leq H_\mathrm{T} < 1500$ GeV and $N_\mathrm{j}^\mathrm{hi}<4$

Predictions and observations for signal regions with $1200 \leq H_\mathrm{T} < 1500$ GeV and $4\leq N_\mathrm{j}^\mathrm{hi}<7$

Predictions and observations for signal regions with $1200 \leq H_\mathrm{T} < 1500$ GeV and $N_\mathrm{j}\geq7$

Predictions and observations for signal regions with $H_\mathrm{T} \geq 1500$ GeV and $N_\mathrm{j}<7$

Predictions and observations for signal regions with $H_\mathrm{T} \geq 1500$ GeV and $N_\mathrm{j}\geq7$

Covariance matrix for the 282 signal regions of the inclusive $M_\mathrm{T2}$ search

Correlation matrix for the 282 signal regions of the inclusive $M_\mathrm{T2}$ search

Bin number definitions for the $M_\mathrm{T2}$ covariance and correlation matrices

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 10$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 50$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 200$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct light squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 10$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark.

Exclusion limits at 95% CL for direct light squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 50$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark.

Exclusion limits at 95% CL for direct light squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino is long-lived with $c\tau_0 = 200$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino is long-lived with $c\tau_0 = 10$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino is long-lived with $c\tau_0 = 50$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino is long-lived with $c\tau_0 = 200$ cm and mass O(100) MeV greater than the neutralino's mass. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

The maximum chargino mass excluded at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the gluino mass is fixed to 1900 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

The maximum chargino mass excluded at 95% CL for direct squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the squark mass is fixed to 900 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, for a single light squark. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

The maximum chargino mass excluded at 95% CL for direct squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the squark mass is fixed to 1500 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, and the eight light squarks' masses are assumed to be degenerate. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 1$ to 2000 cm while the stop mass is fixed to 1000 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$. If all kinematically allowed chargino masses are excluded, the curves, including 68 and 95% expected, tend to overlap. At short decay lengths, horizontal exclusion lines are obtained from the inclusive analysis, as this is not affected by track reconstruction inefficiencies, which may arise when the chargino decays before the CMS tracker, and therefore shows better sensitivity to scenarios with very small lifetime compared to the disappearing track search, based on median expected limits.

Exclusion limits at 95% CL for direct gluino pair production, where the gluinos decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 5$ to 1000 cm while the gluino mass is fixed to 1600 GeV and the neutralino's mass is fixed to 1575 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Exclusion limits at 95% CL for direct squark pair production, where the squarks decay to light-flavor quarks and either the lightest neutralino, or the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 5$ to 1000 cm while the squark mass is fixed to 2000 GeV and the neutralino's mass is fixed to 1000 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$, and the eight light squarks' masses are assumed to be degenerate.

Exclusion limits at 95% CL for direct stop pair production, where the stops decay to either a top and the lightest neutralino, or a bottom and the lightest chargino, and the chargino mass is O(100) MeV greater than the neutralino's mass. The chargino's lifetime is varied from $c\tau_{0} = 5$ to 1000 cm while the stop mass is fixed to 1100 GeV and the neutralino's mass is fixed to 1000 GeV. Signal cross sections are calculated at approximately NNLO+NNLL order in $\alpha_S$.

Predictions and observations for 2016 disappearing track signal regions

Predictions and observations for 2017-2018 pixel track signal regions

Predictions and observations for 2017-2018 medium (M) and long (L) length track signal regions

Covariance matrix for the 68 signal regions of the disappearing tracks $M_\mathrm{T2}$ search

Correlation matrix for the 68 signal regions of the disappearing tracks $M_\mathrm{T2}$ search

Integrated jet shape as a function of the radius r for the PT range 40-50 GeV.

Differential jet shape as a function of the radius r for the PT range 50-70 GeV.

Integrated jet shape as a function of the radius r for the PT range 50-70 GeV.

Differential jet shape as a function of the radius r for the PT range 70-100 GeV.

Integrated jet shape as a function of the radius r for the PT range 70-100 GeV.

Differential jet shape as a function of the radius r for the PT range 100-150 GeV.

Integrated jet shape as a function of the radius r for the PT range 100-150 GeV.

Observed 95 PCT exclusion limit in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Expected 95 PCT exclusion limit in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Observed 95 PCT exclusion limit in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Number of MC signal events in the M(stop), M(neutralino) plane in gaugino universality scenario.

Number of MC signal events in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Number of MC signal events in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Cross section in the M(stop), M(neutralino) plane in gaugino universality scenario.

Cross section in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Cross section in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Acceptance in the 1LSR signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Acceptance in the 1LSR signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Efficiency in the 1LSR signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Efficiency in the 1LSR signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Total PCT systematic uncertainty in the 1LSR region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Total PCT systematic uncertainty in the 1LSR region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Acceptance in the 2LSR1 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Acceptance in the 2LSR2 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Efficiency in the 2LSR1 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Efficiency in the 2LSR2 signal region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Total PCT systematic uncertainty in the 2LSR1 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Total PCT systematic uncertainty in the 2LSR2 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

Acceptance in the 2LSR1 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Acceptance in the 2LSR2 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Efficiency in the 2LSR1 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Efficiency in the 2LSR2 signal region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Total PCT systematic uncertainty in the 2LSR1 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Total PCT systematic uncertainty in the 2LSR2 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

Acceptance in the 2LSR1 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Acceptance in the 2LSR2 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Efficiency in the 2LSR1 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Efficiency in the 2LSR2 signal region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Total PCT systematic uncertainty in the 2LSR1 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

Total PCT systematic uncertainty in the 2LSR2 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

expected CLs values for the 1LSR region in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the 1LSR region in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values combining the 1LSR and 2LSR1 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values combining the 1LSR and 2LSR1 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values combining the 1LSR and 2LSR2 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values combining the 1LSR and 2LSR2 regions in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the best expected combination in the M(stop), M(neutralino) plane in gaugino universality scenario.

observed CLs values for the best expected combination in the M(stop), M(neutralino) plane in gaugino universality scenario.

expected CLs values for the 1LSR region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the 1LSR region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the 2LSR1 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the 2LSR1 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the 2LSR2 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the 2LSR2 region in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values combining the 1LSR and 2LSR1 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values combining the 1LSR and 2LSR1 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values combining the 1LSR and 2LSR2 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values combining the 1LSR and 2LSR2 regions in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the best expected combination in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

observed CLs values for the best expected combination in the M(chargino), M(neutralino) plane in the scenario where M(stop) = 180 GEV.

expected CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

observed CLs values for the 2LSR1 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

expected CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

observed CLs values for the 2LSR2 region in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

expected CLs values for the best expected combination in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

observed CLs values for the best expected combination in the M(stop), M(neutralino) plane in the scenario where M(chargino) = 106 GEV.

(1) Number of generated MC events for the spin 1/2 top partner signal grid (2) Relative Cross section uncertainties for the spin 1/2 top partner signal grid.

(1) Acceptance of the same flavour selection for the spin 1/2 top partner signal grid (2) Selection efficiency of the same flavour selection for the spin 1/2 top partner signal grid (3) Product of the acceptance and efficiency of the same flavour selection for the spin 1/2 top partner signal grid (4) Relative experimental uncertainties on the acceptance times efficiency of the same flavour selection for the spin 1/2 top partner signal grid.

(1) Acceptance of the different flavour selection for the spin 1/2 top partner signal grid (2) Selection efficiency of the different flavour selection for the spin 1/2 top partner signal grid (3) Product of the acceptance and efficiency of the different flavour selection for the spin 1/2 top partner signal grid (4) Relative experimental uncertainties on the acceptance times efficiency of the different flavour selection for the spin 1/2 top partner signal grid.

(1) Observed CLs values for the scalar top signal grid (2) Expected CLs values for the scalar top signal grid.

(1) Observed CLs values for the spin 1/2 top partner signal grid (2) Expected CLs values for the spin 1/2 top partner signal grid.

Cross section limits [pb] for the scalar top signal grid.

Cross section limits [pb] for the spin 1/2 top partner signal grid.

Observed 95% CL limit for stop grid as a function of the scalar top and neutralino masses.

Observed 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying signal cross section of +1sigma.

Observed 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying signal cross section of -1sigma.

Expected 95% CL limit for stop grid as a function of the scalar top and neutralino masses.

Expected 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying the uncertainty of +1sigma.

Expected 95% CL limit for stop grid as a function of the scalar top and neutralino masses, varying the uncertainty of -1sigma.

Observed 95% CL limit for top partner grid as a function of the top partner and neutralino masses.

Observed 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying signal cross section of +1sigma.

Observed 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying signal cross section of -1sigma.

Expected 95% CL limit for top partner grid as a function of the top partner and neutralino masses.

Expected 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying the uncertainty of +1sigma.

Expected 95% CL limit for top partner grid as a function of the top partner and neutralino masses, varying the uncertainty of -1sigma.

Distribution of the PT of the leading muon for E-MU events in the Signal Region, before the application of the leading lepton PT cut.

Distribution of the missing ET for all events in the Signal Region.

Distribution of MET-significnce, ie the missing ET/sqrt(scalar sum of PT of all leptons and jets), for all events in the Signal Region.

Distribution of the missing ET for E-E events in the Z Control Region.

Distribution of the missing ET for MU-MU events in the Z Control Region.

Distribution of the missing ET for E-E events in the Top Control Region.

Distribution of the missing ET for E-MU events in the Top Control Region.

Distribution of the missing ET for MU-MU events in the Top Control Region.

Distribution of the Jet Multiplicity for all events in the Top Control Region.

Distribution of the B-Jet Multiplicity for all events in the Top Control Region.

Distribution of the PT of the leading Jet for all events in the Top Control Region.

Distribution of the PT of the leading B-Jet for all events in the Top Control Region.

The stop pair production cross section and its uncertainty due to PDF, factorization and the renormalization scales.