Measured charged jet differential cross section ratios for INEL proton-proton collisions at $\sqrt{s}$ = 7 TeV for $15<p_{T}^{ch jet}<20$ GeV/$c$.

Invariant mass distribution of the selected $\mathrm{B}^+\mathrm{K}^-$ candidates in data

Invariant mass distribution of the selected $\mathrm{B}^0 \mathrm{K}^{0}_{\mathrm{S}}$ candidates in data

The observed signal yields ($N$), natural widths ($\Gamma$), and mass differences from the fits to the $m_{\mathrm{BK}}$ distributions in data, for the two channels: $\mathrm{B}^+\mathrm{K}^-$ and $\mathrm{B}^0 \mathrm{K}^{0}_{\mathrm{S}}$. The uncertainties are statistical only.

The measured ratios of branching fractions

The measured ratios of cross sections times branching fractions

The measured mass differences $M(\mathrm{B}^{(*)0}_{\mathrm{s1,2}})-M^{\mathrm{PDG}}_{\mathrm{B}}-M^{\mathrm{PDG}}_{\mathrm{K}}$

The measured masses of $\mathrm{B}^{*}_{\mathrm{s2}}(5840)^0$ and $\mathrm{B}_{\mathrm{s1}}(5830)^0$ mesons

The measured mass differences between neutral and charged B mesons

The measured $\mathrm{B}^{*}_{\mathrm{s2}}(5840)^0$ natural width

The nuclear modification factor of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The nuclear modification factor of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points. Bins where no data point has been reported are denoted as 'empty'.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The RXePb of charged particles having |eta|<1 in XeXe collisions at sqrt(s_NN)=5.44 TeV and PbPb collisions at sqrt(s_NN)=5.02 TeV. The first systematic uncertainty describes uncertainties that are not fully correlated across points, while the second systematic uncertainty is a normalization uncertainty that is fully correlated across all points.

The average N_part, N_coll, and TAA for various centrality classes of XeXe collisions at 5.44 TeV.

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.

Distribution of $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Distribution of $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from charged particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{0}$ (N) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0}^{2}$ ($p_{T}^{d,*})$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{0.5}^{1}$ (LHA) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{1}^{1}$ (width) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\lambda_{2}^{1}$ (thrust) reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\varepsilon$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $z_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\Delta R_{g}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $n_{SD}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{21}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{32}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $\tau_{43}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{1}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{2}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(0.5)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(1.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $C_{3}^{(2.0)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(1)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $M_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{2}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

Covariance matrix for $N_{3}^{(2)}$ reconstructed from all particles with pt > 1 GeV, unfolded to the particle level.

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.