Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{1})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}^{\mathrm{add.}}_{2})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{2})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{add.}})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\Delta\mathrm{R}_{\mathrm{b}\mathrm{b}}^{\mathrm{avg}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}_{3})|$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}_{3})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}_{3})$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}_{3})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}_{4})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}_{4})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{b}}_{\mathrm{T}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{b}}_{\mathrm{T}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $|\eta(\mathrm{b}^{\mathrm{extra}}_{1})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{1})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}^{\mathrm{extra}}_{2})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{2})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{extra}})|$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $H^{\mathrm{j}}_{\mathrm{T}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{j}}_{\mathrm{T}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $\mathrm{m}_{\mathrm{b}\mathrm{b}}^{\mathrm{max}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $H^{\mathrm{light}}_{\mathrm{T}}$ in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $H^{\mathrm{light}}_{\mathrm{T}}$ in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space.

Normalized differential cross section of $N_{\mathrm{jets}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Normalized differential cross section of $N_{\mathrm{jets}}$ in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space.

Normalized differential cross section of $N_{\mathrm{b}}$ in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space.

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{add.}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\Delta\mathrm{R}_{\mathrm{b}\mathrm{b}}^{\mathrm{avg}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}_{4})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}_{4})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{extra}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $\mathrm{m}_{\mathrm{b}\mathrm{b}}^{\mathrm{max}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Correlation of parameters of interest in fit of $N_{\mathrm{jets}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $N_{\mathrm{jets}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Correlation of parameters of interest in fit of $N_{\mathrm{b}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{add.}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{add.}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{add.}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{add.}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\Delta\mathrm{R}_{\mathrm{b}\mathrm{b}}^{\mathrm{avg}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}_{3})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}_{3})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}_{4})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}_{4})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{b}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $|\Delta\phi(\mathrm{lj}^{\mathrm{extra}}_{1},\mathrm{b}_{\mathrm{soft}})|$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{1})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}^{\mathrm{extra}}_{2})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}^{\mathrm{extra}}_{2})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $|\eta(\mathrm{b}\mathrm{b}^{\mathrm{extra}})|$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\Delta\mathrm{R}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\mathrm{m}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{b}\mathrm{b}^{\mathrm{extra}})$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $p_{\mathrm{T}}(\mathrm{lj}^{\mathrm{extra}}_{1})$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{j}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $\mathrm{m}_{\mathrm{b}\mathrm{b}}^{\mathrm{max}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 6$ jets: $\geq 3 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $H^{\mathrm{light}}_{\mathrm{T}}$ observable in $\geq 7$ jets: $\geq 4 \mathrm{b}$, $\geq 3$ light phase space

Covariances of all nuisance parameters and POIs in fit of $N_{\mathrm{jets}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $N_{\mathrm{jets}}$ observable in $\geq 6$ jets: $\geq 4 \mathrm{b}$ phase space

Covariances of all nuisance parameters and POIs in fit of $N_{\mathrm{b}}$ observable in $\geq 5$ jets: $\geq 3 \mathrm{b}$ phase space

Fiducial cross sections from the measurements of all observables, compared to predictions from different ttbb simulation approaches. For each of the normalized differential measurements the fiducial cross section in the respective phase space is also determined. In the paper only one representative observable is quoted for each fiducial phase space, while here the measured cross section with the uncertainties from the fit to the respective observable is summarized.

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 distrubution of second leading jet pT for SR1 for the combined EE and MUMU channels. Tabulated are the observed Data rates and the Standard Model predictions as well as the distributions expected for two signal scenarios, both with an STOP mass of 250 GeV, and NEUTRALINO1 masses of 100 GeV and 220 GeV respectively. The last pT bin includes the number of overflow events for both data abd SM expectation.

The observed exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The expected exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The +1sigma contour around the median of the expected exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The -1sigma contour around the median of the expected exclusion limits at 95% C.L. (using the CLs prescription) in the stop-neutralino1 mass plane, assuming direct stop pair production in the framework of GMSB models with light higgsinos.

The acceptance, using prompt leptons only, in the stop1-neutralino1 mass plane for SR1 and SR2.

The efficiancy in the stop1-neutralino1 mass plane for SR1 and SR2.

The total systematic uncertainty, including both theoretical and experimental uncertainties, in the stop1-neutralino1 mass plane for SR1 and SR2.

The CLs values in the stop1-neutralino1 mass plane for SR1 and SR2.

The number of generated MC events for each signal point in the stop1-neutralino1 mass plane before applying the dilepton filter efficiency. After that, 25K events per point are simulated.

The cross section of stop1-stop1 in the stop1-neutralino1 mass plane.

Figure 2-a. Expected limit +1sigma.

Figure 2-a. Expected limit.

Figure 2-a. Expected limit -1sigma.

Figure 2-b. Observed limit +1sigma-th.

Figure 2-b. Observed limit.

Figure 2-b. Observed limit -1sigma-th.

Figure 2-b. Expected limit +1sigma.

Figure 3a. Auxiliary material. Theoretical uncertainty for the Gbb model.

Figure 7b. Auxiliary material. Efficiency for the Gbb model in the signal region SR4-M.

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.

Parton-level normalized $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 8 TeV. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level normalized $t\bar t$ differential cross-sections for the $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 8 TeV. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level normalized $t\bar t$ differential cross-sections for the $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 8 TeV. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level absolute $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 7 TeV. The cross-sections in the last bins include events (if any) beyond of the bin edges. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level absolute $t\bar t$ differential cross-sections for the $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 7 TeV. The cross-sections in the last bins include events (if any) beyond of the bin edges. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level absolute $t\bar t$ differential cross-sections for the $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 7 TeV. The cross-sections in the last bins include events (if any) beyond of the bin edges. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level absolute $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 8 TeV. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level absolute $t\bar t$ differential cross-sections for the $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 8 TeV. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Parton-level absolute $t\bar t$ differential cross-sections for the $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 8 TeV. The uncertainties quoted in the second column represent the statistical and systematic uncertainties added in quadrature.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 7 TeV. The elements of the covariance matrix are in units of 10$^{-6}$ GeV$^{-2}$.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 7 TeV. The elements of the covariance matrix are in units of 10$^{-6}$ GeV$^{-2}$.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 7 TeV. The elements of the covariance matrix are unit-less.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 8 TeV. The elements of the covariance matrix are in units of 10$^{-6}$ GeV$^{-2}$.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 8 TeV. The elements of the covariance matrix are in units of 10$^{-6}$ GeV$^{-2}$.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 8 TeV. The elements of the covariance matrix are unit-less.

Full covariance matrix of the absolute $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 7 TeV. The elements of the covariance matrix are in units of pb$^2$ GeV$^{-2}$.

Full covariance matrix of the absolute $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 7 TeV. The elements of the covariance matrix are in units of pb$^2$ GeV$^{-2}$.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 7 TeV. The elements of the covariance matrix are pb$^2$.

Full covariance matrix of the absolute $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 8 TeV. The elements of the covariance matrix are in units of pb$^2$ GeV$^{-2}$.

Full covariance matrix of the absolute $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 8 TeV. The elements of the covariance matrix are in units of pb$^2$ GeV$^{-2}$.

Full covariance matrix of the normalized $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 8 TeV. The elements of the covariance matrix are pb$^2$.

Statistical bin-to-bin correlations in the normalized $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 7 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the normalized $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 7 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the normalized $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 7 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the normalized $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 8 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the normalized $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 8 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the normalized $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 8 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the absolute $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 7 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the absolute $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 7 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the absolute $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 7 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the absolute $t\bar t$ differential cross-sections for $t\bar t$ system mass $m_{t\bar t}$ at $\sqrt{s}$ = 8 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the absolute $t\bar t$ differential cross-sections for $t\bar t$ system transverse momentum $p_{T, t\bar t}$ at $\sqrt{s}$ = 8 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

Statistical bin-to-bin correlations in the absolute $t\bar t$ differential cross-sections for $t\bar t$ system absolute rapidity $|y_{t\bar t}|$ at $\sqrt{s}$ = 8 TeV. The off-diagonal correlations mainly due to bin migrations in unfolding and the normalization condition.

(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.

The leptonic asymmetry dependence on the invariant mass of top-antitop system ($m_{t\bar{t}}$) in the fiducial volume.

The leptonic asymmetry dependence on the longitudinal boost of the top-antitop system ($\beta_z^{t\bar{t}}$) in the fiducial volume.

The leptonic asymmetry dependence on the transverse momentum of the top-antitop system ($p_T^{t\bar{t}}$) in the fiducial volume.

The top-antitop inclusive asymmetry in the fiducial volume.

The top-antitop asymmetry dependence on the invariant mass of top-antitop system ($m_{t\bar{t}}$) in the fiducial volume.

The top-antitop asymmetry dependence on the longitudinal boost of the top-antitop system ($\beta_z^{t\bar{t}}$) in the fiducial volume.

The top-antitop asymmetry dependence on the transverse momentum of the top-antitop system ($p_T^{t\bar{t}}$) in the fiducial volume.