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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Distribution of missing transverse momentum in the data and for the background in the PhJetCR. The total background expectation is normali zed to the post-fit result. The errors include both statistical and systematic uncertainties determined by a bin-by-bin fit.

Distribution of missing transverse momentum in the signal region for data and for the background predicted from the fit in the CRs. Overflows are included in the final bin. The errors include both statistical and systematic components. The expected yield of events from the simplified model with $m_\chi$ = 150 GeV and $m_{med}$ = 500 GeV is also shown.

Distribution of photon transverse momentum in the signal region for data and for the background predicted from the fit in the CRs. Overflows are included in the final bin. The errors include both statistical and systematic components. The expected yield of events from the simplified model with $m_\chi$ = 150 GeV and $m_{med}$ = 500 GeV is also shown.

The observed and 95% CL exclusion limit for a simplified model of dark matter production involving an axial-vector operator, Dirac DM and couplings $g_q$ = 0.25 and $g_\chi$ = 1 as a function of the dark matter mass $m_\chi$ and the axial-mediator mass $m_{med}$.

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

The observed 95% CL lower limits on $M_\ast$ for a dimension-7 operator EFT model with a contact interaction of type $\gamma\gamma\chi\chi$ as a function of dark matter mass $m_\chi$.

The observed 95% CL lower limits on the mass scale $M_D$ in the ADD models of large extra dimensions, for several values of the number of extra dimensions.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 640 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 720 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 800 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 880 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 960 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1040 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1120 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1200 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1280 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1360 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1440 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1520 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1600 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1680 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1760 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1840 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1920 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 2000 GeV and Neutralino mass 50 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 400 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 480 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 560 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 640 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 720 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 800 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 880 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 960 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1040 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1120 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1200 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1280 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1360 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1440 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1520 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1600 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1680 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1760 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1840 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1920 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 2000 GeV and Neutralino mass 150 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 400 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 480 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 560 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 640 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 720 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 800 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 880 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 960 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1040 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1120 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1200 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1280 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1360 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1440 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1520 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1600 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1680 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1760 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1840 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 1920 GeV and Neutralino mass 500 GeV.

95 PCT CL upper limits to cross section and the GGM acceptance as a function of Gluino mass for Squark mass 2000 GeV and Neutralino mass 500 GeV.

Lower 95 PCT exclusion limits on the squark and gluino masses for a neutralino mass of 50 GeV.

Lower 95 PCT exclusion limits on the squark and gluino masses for a neutralino mass of 150 GeV.

Lower 95 PCT exclusion limits on the squark and gluino masses for a neutralino mass of 500 GeV.

Ratio of the Z'NU to Z'SSM acceptance times efficiency (ACC*EFF) in the lep-had channel as a function of sin^2phi and the Z' mass.

Z' SSM acceptance (ACC) and product of acceptance and efficiency (ACC*EFF) for the had-had and lep-had selections as a function of the Z' mass.

Number of expected Z'SSM signal (NS), background (NB) and observed (N) events passing the total transverse mass ($m_{\rm T}^{\rm tot}$) threshold in the had-had and lep-had channels.

Median expected and observed 95% CL upper limits on the cross-section times branching fraction to tau+tau- for Z'SSM production for the exclusive had-had and lep-had channels, and for both channels combined.

Observed 95% CL upper limits on the cross-section times branching fraction to tau+tau- for Z'L and Z'R production for the combination of the had-had and lep-had channels.

Observed 95% CL lower limit on the Z'NU mass as a function of sin^2(phi).

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. This table is for the observed limit for BR=75% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. This table is for the expected limit for BR=75% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Observed limit for BR=50% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Expected limit for BR=50% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Observed limit for BR=25% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Expected limit for BR=25% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Observed limit for BR=0% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Combined exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow t + \tilde{\chi}_1^0 $ with branching ratio x and through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm $ with branching ratio 1-x. Expected limit for BR=0% - Observed limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d63 - Expected limit x=BR=100% See Fig 24. hepdata.cedar.ac.uk/view/ins1380183/d64.

Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%. Limits for the b0L and t1L soft-lepton analyses in two scenarios Delta M = 5 GeV in light green and Delta M = 20 GeV in dark green), for a total of four limits - dM=5 GeV, b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d19 - dM=5 GeV, b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d22 - dM=5 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d40 - dM=5 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d41 - dM=20 GeV, b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d25 - dM=20 GeV, b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d28 - dM=20 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d43 - dM=20 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d44.

Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%.Limits for the b0L, t1L and t2L analyses in scenarios with a fixed chargino mass of 106 GeV (dark green) and 150 GeV (light green) - M(ch1)=150 GeV, b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d13 - M(ch1)=150 GeV, b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d16 - M(ch1)=150 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d34 - M(ch1)=150 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d35 - M(ch1)=106 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d37 - M(ch1)=106 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d38 - M(ch1)=106 GeV, t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d25 - M(ch1)=106 GeV, t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d26.

Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%.Limits for the t1L and t2L analyses in scenarios with the mass of the chargino set to twice the mass of the neutralino - M(ch1)=2M(chi0), t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d31 - M(ch1)=2M(chi0), t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d32 - M(ch1)=2M(chi0), t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d16 - M(ch1)=2M(chi0), t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d17.

Summary of the ATLAS Run 1 searches for direct stop pair production in models where the decay mode $\tilde{t}_1 \rightarrow b \tilde{\chi}^{\pm}$ with $ \tilde{\chi}_1^{\pm} \rightarrow W \tilde{\chi_1^0}$ is assumed with a branching ratio of 100%.Limits for the t1L and t2L and WW analyses in scenarios with the mass difference between chargino and neutralino is 10 GeV - dM=10 GeV, t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d46 - dM=10 GeV, t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d47 - dM=10 GeV, t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d10 - dM=10 GeV, t2L expected limit hepdata.cedar.ac.uk/view/ins1286444/d11 - dM=10 GeV, WW observed limit hepdata.cedar.ac.uk/view/ins1380183/d45 - dM=10 GeV, WW expected limit hepdata.cedar.ac.uk/view/ins1380183/d46.

Exclusion limits assuming that the stop decays through $\tilde{t}_1 \rightarrow b + \tilde{\chi}_1^\pm + W^{(*)} + \tilde{\chi}_1^0$ with branching ratio of 100% assuming a fixed stop mass of 300 GeV. - t1L observed limit hepdata.cedar.ac.uk/view/ins1304456/d49 - t1L expected limit hepdata.cedar.ac.uk/view/ins1304456/d50 - b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d7 - b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d10.

Exclusion limits at 95% CL in the scenario where $\tilde{t}_2$ pair production is assumed, followed by the decay $\tilde{t}_2 \rightarrow Z \tilde{t}_1$ or $\tilde{t}_2 \rightarrow \tilde{t}_1 h$ and then by $\tilde{t}_1 \rightarrow t \tilde{\chi}_1^0$ with a branching ratio of 100%, as a function of the $\tilde{t}_2$ and $\tilde{\chi}_1^0$ mass. The $\tilde{t}_1$ mass is 180 GeV larger than the neutralino mass. This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d11 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d8.

Exclusion limits at 95% CL in the scenario where $\tilde{t}_2$ pair production is assumed, followed by the decay $\tilde{t}_2 \rightarrow Z \tilde{t}_1$ or $\tilde{t}_2 \rightarrow \tilde{t}_1 h$ and then by $\tilde{t}_1 \rightarrow t \tilde{\chi}_1^0$ with a branching ratio of 100%, as a function of the $\tilde{t}_2$ and $\tilde{\chi}_1^0$ mass. The $\tilde{t}_1$ mass is 180 GeV larger than the neutralino mass. This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d11 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d8.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t1L/t0L observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=350 GeV and m(chi1)=20 GeV (top plot). This table is for the t1L/t0L expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d14 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d15.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t1L/t0L observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=20 GeV (top plot). This table is for the t1Lt0L expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d16 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d17.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t2t1H observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t2t1H expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t1L/t0L observed limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.

Exclusion limits as a function of the stop2 branching ratio for decays into Z, Higgs and neutralino. m(t2)=500 GeV and m(chi1)=120 GeV (top plot). This table is for the t1Lt0L expected limit. - t2t1Z observed limit hepdata.cedar.ac.uk/view/ins1286622/d18 - t2t1Z expected limit hepdata.cedar.ac.uk/view/ins1286622/d19.

Observed and expected 95% CL limits on sbottom pair production where the sbottom is assumed to decay as b1->b chi10 with a branching ratio of 100%. - b0L observed limit hepdata.cedar.ac.uk/view/ins1247462/d1 - b0L expected limit hepdata.cedar.ac.uk/view/ins1247462/d4 - tc observed limit hepdata.cedar.ac.uk/view/ins1304459 (root macro) - tc expected limit hepdata.cedar.ac.uk/view/ins1304459 (root macro).

Exclusion limits at 95% CL for a scenario where sbottoms are pair produced and decay as b1 -> t chi1+ with a BR of 100% - SS3L observed limit (mchi+=60 GeV): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoN60_observed.C - SS3L expected limit (mchi+=60 GeV): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoN60_expected.C - SS3L observed limit (mchi+=2 mchi0): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoNhalfC_observed.C - SS3L expected limit (mchi+=2 mchi0): hepdata.cedar.ac.uk/resource/6164/finalExclusionGraphs/SBottomTopCharginoNhalfC_expected.C.

Exclusion limits at 95% CL for a scenario where sbottoms are pair produced and decay as b1 -> b chi2 with a BR of 100% - g3b observed limit hepdata.cedar.ac.uk/view/ins1304457/d10 - g3b expected limit hepdata.cedar.ac.uk/view/ins1304457/d11.

Observed 95% CL exclusion limits for the naturalness-inspired set of pMSSM models from the combination t0L, t1L and tb analyses using the signal region yielding the smallest CLs value for the signal- plus-background hypothesis. This table is for the observed limit.

Expected 95% CL exclusion limits for the naturalness-inspired set of pMSSM models from the combination t0L, t1L and tb analyses using the signal region yielding the smallest CLs value for the signal- plus-background hypothesis. This table is for the expected limit.

Observed 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mqL3. The limit is obtained as the combination of the t0L, t1L, tb and SS3L analyses, This table is for the observed limit.

Expected 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mqL3. The limit is obtained as the combination of the t0L, t1L, tb and SS3L analyses, This table is for the expected limit.

Observed 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mtR. The limit is obtained using the t0L analysis. This table is for the observed limit.

Expected 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mtR. The limit is obtained using the t0L analysis. This table is for the expected limit.

Observed 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(qL3). The limit of is obtained as the combination of the t0L, g3b, t2t1Z and SS3L analyses, This table is for the observed limit.

Expected 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(qL3). The limit of is obtained as the combination of the t0L, g3b, t2t1Z and SS3L analyses, This table is for the expected limit.

Observed 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(bR). The limit of is obtained as the combination of thet0L, t2t1Z and tb analyses, This table is for the observed limit.

Expected 95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(bR). The limit of is obtained as the combination of thet0L, t2t1Z and tb analyses, This table is for the expected limit.

Expected and observed 95% CL limits on the signal strength mu (defined as the ratio of the obtained stop cross section to the theoretical prediction) for the production of stop pairs as a function of m(stop). The stop is assumed to decay as t1->t chi0 or through its three-body decay depending on its mass. The neutralino is assumed to have a mass of 1 GeV.

Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via $\tilde{t}_1 \rightarrow b \chi^\pm_1$ followed by $\chi^\pm_1 \rightarrow W \chi_1^0$ with $\Delta m(t_1, \chi_1^0)$ = 10 GeV. This table is for the observed limit.

Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via $\tilde{t}_1 \rightarrow b \chi^\pm_1$ followed by $\chi^\pm_1 \rightarrow W \chi_1^0$ with $\Delta m(t_1, \chi_1^0)$ = 10 GeV. This table is for the expected limit.

Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via three-body or four-body decay (depending on the neutralino and stop mass). This table is for the observed limit. - t1L observed limit (3-body) hepdata.cedar.ac.uk/view/ins1304456/d25 - t1L observed limit (4-body) hepdata.cedar.ac.uk/view/ins1304456/d28 - t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d23.

Exclusion limits at 95% CL in the scenario where both pair-produced stop decay exclusively via three-body or four-body decay (depending on the neutralino and stop mass). This table is for the expected limit. - t1L observed limit (3-body) hepdata.cedar.ac.uk/view/ins1304456/d25 - t1L observed limit (4-body) hepdata.cedar.ac.uk/view/ins1304456/d28 - t2L observed limit hepdata.cedar.ac.uk/view/ins1286444/d23.

Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=5GeV. This table is for the Observed limit.

Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=5GeV. This table is for the Expected limit.

Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=20 GeV. This table is for the Observed limit.

Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 25% and DM=20 GeV. This table is for the Expected limit.

Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=5GeV. This table is for the Observed limit.

Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=5 GeV. This table is for the Expected limit.

Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=20GeV. This table is for the Observed limit.

Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 50% and DM=20 GeV. This table is for the Expected limit.

Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=5GeV. This table is for the Observed limit.

Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=5 GeV. This table is for the Expected limit.

Observed exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=20GeV. This table is for the Observed limit.

Expected exclusion limits at 95% CL from the tb signal regions for simplified models with stop decays into both stop1->t chi10 and stop1-> b ch1 for BR(stop1->t chi10) = 75% and DM=20 GeV. This table is for the Expected limit.

Observed exclusion limits at 95% CL from the tb signal regions in the natural pMSSM model. This table is for the Observed limit.

Expected exclusion limits at 95% CL from the tb signal regions in the natural pMSSM model. This table is for the Expected limit.

Combined exclusion limits at 95% CL in the scenario where both stops decay exclusively via $\tilde t_1 \rightarrow t \tilde \chi_1^0 $. Observed limit contour line for the t0L/t1L combination.

Combined exclusion limits at 95% CL in the scenario where both stops decay exclusively via $\tilde t_1 \rightarrow t \tilde \chi_1^0 $. Expected limit contour line for the t0L/t1L combination.

Best expected SR for the WW analysis and the three- and four-body decays.

Cross-section upper limit for the WW analysis and the three- and four-body decays.

Expected CLs for the WW analysis and the 3- and 4-body decays.

Observed CLs for the WW analysis and the 3- and 4-body decays.

Best expected SR for the WW analysis and the stop1->chargino1 decay.

Cross section upper limit for the WW analysis and the stop1->chargino1 decay.

Expected CLs for the WW analysis and the stop1->chargino1 decay.

Observed CLs for the WW analysis and the stop1->chargino1 decay.

Cross section upper limit for the t2t1h analysis.

Expected CLs for the t2t1h analysis.

Observed CLs for the t2t1h analysis.

Best expected SR for the tb analysis in the pMSSM model.

Cross section upper limit for the tb analysis in the pMSSM model.

Efficiency for the SRinA signal region for the pMSSM model.

Efficiency for the SRinB signal region for the pMSSM model.

Efficiency for the SRinC signal region for the pMSSM model.

Efficiency for the SRexA signal region for the pMSSM model.

Best expected SR for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=50%.

Cross section upper limit for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=50%.

Best expected SR for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=50%.

Cross section upper limit for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=50%.

Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=25%.

Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=25%.

Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 5 GeV and BR=75%.

Best expected SR and cross section upper limit for the tb analysis in the simplified model with Delta(m) = 20 GeV and BR=75%.

Exclusion limits for the naturalness-inspired set of pMSSM models from the combination t0L, t1L and tb analyses using the signal region yielding the smallest CLs value for the signal- plus-background hypothesis. This table is for the best expected signal region.

95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mqL3. The limit is obtained as the combination of the t0L, t1L, tb and SS3L analyses, This table is for the best expected signal region.

Expected 95% CL exclusion limits for the pMSSM model with well-tempered neutralinos as a function of M1 and mtR. The limit is obtained using the t0L analysis. This table is for the best expected signal region.

95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(qL3). The limit of is obtained as the combination of the t0L, g3b, t2t1Z and SS3L analyses, This table is for the best expected signal region.

95% CL exclusion limits for the set of h/Z-enriched pMSSM models as a function of $\mu$ and m(bR). The limit of is obtained as the combination of the t0L, t2t1Z and tb analyses, This table is for the best expected signal region.

Expected exclusion limits in the gluino-neutralino mass plane, for the higgsino-bino GGM model with $\mu < 0$, using the merged $\rm{SR}^{\gamma b}_{L}$ and $\rm{SR}^{\gamma b}_{H}$ analyses.

Observed exclusion limits in the $M_3$-$\mu$ plane, for the higgsino-bino GGM model with $\mu > 0$, using the merged $\rm{SR}^{\gamma j}_{L}$ and $\rm{SR}^{\gamma j}_{H}$ analyses.

Expected exclusion limits in the $M_3$-$\mu$ plane, for the higgsino-bino GGM model with $\mu > 0$, using the merged $\rm{SR}^{\gamma j}_{L}$ and $\rm{SR}^{\gamma j}_{H}$ analyses.

Contour of exclusion in wino production cross section from the photon+$\ell$ analysis, as a function of the wino mass parameter $m_{\tilde{W}}$. The expected limit is shown along with its $\pm 1$ and $\pm 2$ standard deviation values.

Numbers of selected data events at progressive stages of the selection, for each SR for the diphoton, photon+j and photon+$\ell$ analyses. Where no number is shown the cut was not applied.

Expected number of signal events at progressive stages of the selection, shown for points in the parameter space that typify the region for which each selection of the diphoton, photon+j and photon+$\ell$ analyses is optimized, and scaled to an integrated luminosity of $20.3\,\mathrm{fb}^{-1}$. Where no number is shown the cut was not applied.

Expected number of signal events at progressive stages of the $\rm{SR}^{\gamma b}_{H}$ selection, shown for data and signal Monte Carlo datasets.

Expected number of signal events at progressive stages of the $\rm{SR}^{\gamma b}_{L}$ selection, shown for data and signal Monte Carlo datasets.

$\rm{SR}^{\gamma\gamma}_{S-H}$ and $\rm{SR}^{\gamma\gamma}_{S-L}$ signal acceptance*efficiency across the strong-production parameter space, for $m_{\tilde{g}}$ between 1550 and 1600 GeV.

$\rm{SR}^{\gamma\gamma}_{S-H}$ and $\rm{SR}^{\gamma\gamma}_{S-L}$ signal acceptance*efficiency across the strong-production parameter space, for $m_{\tilde{g}} = 1500$ GeV.

$\rm{SR}^{\gamma\gamma}_{S-H}$ and $\rm{SR}^{\gamma\gamma}_{S-L}$ signal acceptance*efficiency across the strong-production parameter space, for $m_{\tilde{g}}$ between 1350 and 1450 GeV.

$\rm{SR}^{\gamma\gamma}_{S-H}$ and $\rm{SR}^{\gamma\gamma}_{S-L}$ signal acceptance*efficiency across the strong-production parameter space, for $m_{\tilde{g}}$ between 1250 and 1300 GeV.

$\rm{SR}^{\gamma\gamma}_{S-H}$ and $\rm{SR}^{\gamma\gamma}_{S-L}$ signal acceptance*efficiency across the strong-production parameter space, for $m_{\tilde{g}}$ between 1150 and 1200 GeV.

$\rm{SR}^{\gamma\gamma}_{S-H}$ and $\rm{SR}^{\gamma\gamma}_{S-L}$ signal acceptance*efficiency across the strong-production parameter space, for $m_{\tilde{g}}$ between 1000 and 1100 GeV.

$\rm{SR}^{\gamma\gamma}_{W-H}$ and $\rm{SR}^{\gamma\gamma}_{W-L}$ signal acceptance*efficiency for $m_{\tilde{W}}$ between 650 and 800 GeV.

$\rm{SR}^{\gamma\gamma}_{W-H}$ and $\rm{SR}^{\gamma\gamma}_{W-L}$ signal acceptance*efficiency for $m_{\tilde{W}}$ between 400 and 600 GeV.

$\rm{SR}^{\gamma\gamma}_{W-H}$ and $\rm{SR}^{\gamma\gamma}_{W-L}$ signal acceptance*efficiency for $m_{\tilde{W}}$ between 100 and 400 GeV.

$\rm{SR}^{\gamma b}_{H}$ signal acceptance*efficiency for combined strong and weak production across the $\mu<0$ higgsino-bino parameter space.

$\rm{SR}^{\gamma b}_{L}$ signal acceptance*efficiency for combined strong and weak production across the $\mu<0$ higgsino-bino parameter space.

$\rm{SR}^{\gamma j}_{H}$ signal acceptance*efficiency for combined strong and weak production across the $\mu>0$ higgsino-bino parameter space.

$\rm{SR}^{\gamma j}_{L}$ signal acceptance*efficiency for combined strong and weak production across the $\mu>0$ higgsino-bino parameter space.

Acceptance-times-efficiency (a*e) for the photon+$\ell$ analysis SRs.

The total NLO+NLL strong production cross sections with uncertainties for GGM gluino-neutralino signal points for the diphoton and photon+b analyses. In the variant of the grid used in the diphoton analysis, the electroweak production cross section is negligible.

The total NLO cross sections with uncertainties for GGM wino-bino signal points, for all final states, for the diphoton analysis. The direct bino production cross section is negligible.

The NLO gaugino pair production cross sections with relative uncertainties for GGM gluino-neutralino signal points for the photon+b analysis.

The best signal region used for each signal point in the photon+b analysis.

The total NLO+NLL cross sections with uncertainties for the strong production GGM signal grid for the photon+j analysis.

The total NLO cross sections with uncertainties for the electroweak production GGM signal grid for the photon+j analysis.

The best signal region used for each signal point in the photon+j analysis.

Measured jet multiplicity distribution in the $W\mu\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured dilepton invariant mass distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured $E_{T}^{miss}$ distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured leading jet $p_{T}$ distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured jet multiplicity distribution in the $Z\mu\mu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows. P P --> Z0 JET(S) X.

Measured transverse mass distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured $E_{T}^{miss}$ distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured leading jet $p_{T}$ distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured jet multiplicity distribution in the $We\nu$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured dilepton invariant mass distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured $E_{T}^{miss}$ distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured leading jet $p_{T}$ distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured jet multiplicity distribution in the $Zee$+jets control region for the inclusive SR1 selection, compared to the background expectations. The latter include the global normalization factors extracted from the data. Where appropriate, the last bin of the distribution includes overflows.

Measured distribution of the jet multiplicity for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of $E_{T}^{miss}$ for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of leading jet $p_{T}$ for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_{T}$ to $E_{T}^{miss}$ ratio for the SR1 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the jet multiplicity for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the jet multiplicity for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ for SR9 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ to $E_{T}^{miss}$ ratio for SR7 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Measured distribution of the leading jet $p_T$ to $E_{T}^{miss}$ ratio for SR9 selection compared to the SM expectations. The $Z\nu\nu$+jets contribution is shown as constrained by the $W\mu\nu$+jets control sample. Where appropriate, the last bin of the distribution includes overflows. The distribution of different ADD, WIMP and GMSB scenarios are included.

Observed and expected 95$\%$ CL limit on the fundamental Planck scale in $4+n$ dimensions, $M_D$, as a function of the number of extra dimensions. In the figure the two results overlap. The shaded areas around the expected limit indicate the expected $\pm 1\sigma$ and $\pm 2\sigma$ ranges of limits in the absence of a signal. The 95$\%$ CL observed limits after the suppression of the events with $\hat{s} > M_D^2$ is applied (truncated) are also given.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the scalar operator D1. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the vector operator D5. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the axial vector operator D8. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the tensor operator D9. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the gluon operator D11. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the gluon operator C5. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

Observed 95% CL limits on the suppression scale M* as a function of the mediator mass Mmed, assuming a Z'-like boson in a simplified model and a DM mass of 50 GeV and 400 GeV. The width of the mediator is varied between Mmed/3 and Mmed/8pi.

Observed 95% CL upper limits on the product of couplings of the simplified model vertex in the plane of mediator and WIMP mass (Mmed versus m_chi).

Upper limits at 90% C.L. on the WIMP-nucleon scattering cross section as a function of m_chi for spin-independent interactions, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

Upper limits at 90% C.L. on the WIMP-nucleon scattering cross section as a function of m_chi for spin-dependent interactions, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

Upper limits at 90% C.L. on the WIMP-nucleon annihilation cross section as a function of m_chi, for a coupling strength of unity or the maximum value that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for degenerate squark/gluino masses.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 1/2 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 1/4 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 2 \times m_{\tilde{q}}$.

95$\%$ CL lower limits on the gravitino mass $m_{\tilde{G}}$ as a function of the squark mass $m_{\tilde{q}}$ for non-degenerate squark/gluino masses: $ m_{\tilde{g}} = 4 \times m_{\tilde{q}}$.

Observed and expected 95$\%$ CL upper limit on $\sigma \times {\rm{BR}}(H \to {\rm{invisible}})$ as a function of the Higgs boson mass.

Limits at 95% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the scalar operator C1. Results where EFT truncation is applied are also shown for couplings of 1 and the perturbative limit.

95% C.L. observed exclusion contour for all regions combined.

Best expected signal region for signal points.

95% CLs observed upper limit on model cross-section for signal points in the signal region with $m_{CT}>150$ GeV.

95% C.L. expected exclusion contour for the $m_{CT}>150 $ GeV region.

95% C.L. observed exclusion contour for the $m_{CT}>150 $ GeV region.

95% CLs observed upper limit on model cross-section for signal points in the signal region with $m_{CT}>200$ GeV.

95% C.L. expected exclusion contour for the $m_{CT}>200 $ GeV region.

95% C.L. observed exclusion contour for the $m_{CT}>200 $ GeV region.

95% CLs observed upper limit on model cross-section for signal points in the signal region with $m_{CT}>250$ GeV.

95% C.L. expected exclusion contour for the $m_{CT}>250 $ GeV region.

95% C.L. observed exclusion contour for the $m_{CT}>250 $ GeV region.

95% CLs upper limit on model cross-section for signal points in C1.

95% CLs upper limit on model cross-section for signal points in C2.

Acceptance times Efficiency for signal points in the signal region with $m_{CT}>150$ GeV.

Acceptance times Efficiency for signal points in the signal region with $m_{CT}>200$ GeV.

Acceptance times Efficiency for signal points in the signal region with $m_{CT}>250$ GeV.

Acceptance (flavour-blind) for signal points in the signal region with $m_{CT}>150$ GeV.

Acceptance (flavour-blind) for signal points in the signal region with $m_{CT}>200$ GeV.

Acceptance (flavour-blind) for signal points in the signal region with $m_{CT}>250$ GeV.

Signal cross-sections and uncertainties.

Distribution of ETmiss in the signal region for data and for the background predicted from the fit in the CRs. Overflows are included in the final bin.

Limits at 90% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the vector operator D5. Results where EFT truncation is applied are also shown, assuming coupling values sqrt(g_f g_chi)= 1, 4pi.

Limits at 90% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the axial-vector operator D8. Results where EFT truncation is applied are also shown, assuming coupling values sqrt(g_f g_chi)= 1, 4pi.

Limits at 90% C.L. on the EFT suppression scale M* as a function of the WIMP mass m_chi, for the tensor operator D9. Results where EFT truncation is applied are also shown, assuming coupling values sqrt(g_f g_chi)= 1, 4pi.

Upper limits at 90% C.L. on the WIMP-nucleon scattering cross section as a function of m_chi for spin-independent and spin-dependent interactions, for a coupling strength g = sqrt(g_f g_chi) of unity or the maximum value (4 pi) that keeps the model within its perturbative regime. The truncation procedure is applied for both cases.

Upper limits at 95% C.L. on the WIMP simplified model coupling parameter, sqrt(g_f g_chi), with vector coupling and mediator width Gamma=m_V/3, as a function of WIMP (m_chi) and the mediator particle (m_V) masses.

Observed lower limits at 95% C.L. on the EFT suppression scale M* as a function of the mediator mass mV, for a Z'-like mediator with vector interactions. For a dark-matter mass m_chi of 50 or 400 GeV, results are shown for different values of the mediator total decay width Gamma.

Observed lower limits at 95% C.L. on the EFT suppression scale M* as a function of the mediator mass mV, for a Z'-like mediator with axial-vector interactions. For a dark-matter mass m_chi of 50 or 400 GeV, results are shown for different values of the mediator total decay width Gamma.

Limits at 95% C.L. on the effective mass scale M* in the (k2, k1) parameter plane for the s-channel EFT model inspired by Fermi-LAT gamma-ray line, for m_chi = 130 GeV. The upper part of the plane is excluded.

Lower limits at 95% C.L. on the mass scale M_D in the ADD models of large extra dimensions, for several values of the number of extra dimensions.

Upper limits at 95% C.L. on the cross section for the compressed squark model, as a function of the squark mass, m_squark, and of the difference between the squark mass and the mass of the neutralino, m_squark-m_neutralino, in the compressed region of m_squark-m_neutralino < 50 GeV.

Transverse-momentum distributions of (K*(892)0 + anti-K*(892)0)/2 in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 60.0-80.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 0.0-5.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 5.0-10.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 0.0-10.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 10.0-20.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 20.0-30.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 30.0-40.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 40.0-50.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 50.0-60.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 60.0-70.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 70.0-80.0%.

Transverse-momentum distributions of phi(1020) mesons in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 80.0-90.0%.

Mass of K*(892)0 mesons (combined with the antiparticle) as a function of pT for central (0-20%, first y column) and peripheral (60-80%, second y column) Pb-Pb collisions at sqrt(sNN)=2.76 TeV.

Width of K*(892)0 mesons (combined with the antiparticle) as a function of pT for central (0-20%, first y column) and peripheral (60-80%, second y column) Pb-Pb collisions at sqrt(sNN)=2.76 TeV.

Mass of phi(2010) mesons as a function of pT for central (0-10%, first y column) and peripheral (70-80%, second y column) Pb-Pb collisions at sqrt(sNN)=2.76 TeV. UPDATE (27 JAN 2015): replaced with the final published values.

Width of phi(1020) mesons as a function of pT for central (0-10%, first y column) and peripheral (70-80%, second y column) Pb-Pb collisions at sqrt(sNN)=2.76 TeV.

Yield (dN/dy) of (K*(892)0 + anti-K*(892)0)/2 for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. In the table, the first systematic uncertainty is uncorrelated between centrality intervals, the second is the normalization uncertainty.

Yield (dN/dy) of phi(1020) mesons for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. In the table, the first systematic uncertainty is uncorrelated between centrality intervals and the second is the normalization uncertainty.

Ratio of pT-integrated yields (K*(892)0 + anti-K*(892)0)/(2K-) for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. The K- yields are taken from PRC 88, 044910 (2013). In the paper this ratio is plotted as a function of the cube root of the mid-rapidity charged-particle multiplicity density (dNch/deta)^1/3 values taken from PRL 106, 032301 (2011).

Ratio of pT-integrated yields phi(1020)/K- for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. The K- yields are taken from PRC 88, 044910 (2013). In the paper this ratio is plotted as a function of the cube root of the mid-rapidity charged-particle multiplicity density (dNch/deta)^1/3 values taken from PRL 106, 032301 (2011).

Mean transverse momentum of K*(892)0 mesons (combined with the antiparticle) for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. In the paper this ratio is plotted as a function of the <Npart> values (the mean number of participant nucleons per collision) taken from PRC 88, 044909 (2013).

Mean transverse momentum of phi(1020) mesons for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. In the paper this ratio is plotted as a function of the <Npart> values (the mean number of participant nucleons per collision) taken from PRC 88, 044909 (2013).

pT-dependent ratio (Omega- + anti-Omega+)/phi(1020) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 0.0-10.0%. The Omega pT distributions are taken from PLB 728, 216 (2013).

pT-dependent ratio (p + anti-p)/phi(1020) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 0.0-10.0%.

pT-dependent ratio (p + anti-p)/phi(1020) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 10.0-20.0%.

pT-dependent ratio (p + anti-p)/phi(1020) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 20.0-40.0%.

pT-dependent ratio (p + anti-p)/phi(1020) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 40.0-60.0%.

pT-dependent ratio (p + anti-p)/phi(1020) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 60.0-80.0%.

pT-dependent ratio (p + anti-p)/phi(1020) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 80.0-90.0%.

pT-dependent ratio phi(1020)/(pi+ + pi-) in Pb-Pb collisions at sqrt(sNN)=2.76 TeV, centrality 0.0-10.0%.

Enhancement ratio of phi(1020) for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. The enhancement ratio is the ratio of the yield of a particle in A-A collisions to the yield of the particle in pp collisions, scaled by the average number of participant nucleons: Enhancement=[Yield(A-A)/<Npart(A-A)>]/[Yield(pp)/2]. The phi(1020) yield for pp collisions at sqrt(s)=2.76 TeV is interpolated between the measured yields at sqrt(s)=900 GeV and sqrt(s)=7 TeV. In the tables, the first systematic uncertainty is the uncorrelated uncertainty from the Pb-Pb data, the second is the normalization uncertainty from the Pb-Pb data, and the third is from the uncertainty in <Npart>. In the paper this ratio is plotted as a function of the <Npart> values taken from PRC 88, 044909 (2013).

Enhancement ratio of Lambda for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. The enhancement ratio is the ratio of the yield of a particle in A-A collisions to the yield of the particle in pp collisions, scaled by the average number of participant nucleons: Enhancement=[Yield(A-A)/<Npart(A-A)>]/[Yield(pp)/2]. The Lambda yield for pp collisions at sqrt(s)=2.76 TeV is extrapolated from the measured yield at sqrt(s)=7 TeV. In the tables, the first systematic uncertainty is the uncertainty from the Pb-Pb data and the second is from the uncertainty in <Npart>. In the paper this ratio is plotted as a function of the <Npart> values taken from PRC 88, 044909 (2013).

Ratio of pT-integrated yields phi(1020)/(pi+ + pi-) for different centrality intervals in Pb-Pb collisions at sqrt(sNN)=2.76 TeV. The charged pion yields are taken from PRC 88, 044910 (2013). In the paper this ratio is plotted as a function of the <Npart> values taken from PRC 88, 044909 (2013).

Reconstructed $\cos\theta^*$ distributions for data and the SM background estimate in the dimuon channel.

Reconstructed $A_{\rm FB}$ distributions for data and the SM background estimate as a function of dielectron mass.

Reconstructed $A_{\rm FB}$ distributions for data and the SM background estimate as a function of dimuon mass.

Summary of 95% C.L. lower exclusion limits on $\Lambda$ for the combined dilepton contact interaction search, using a uniform positive prior in 1/$\Lambda^2$.

Summary of 95% C.L. lower exclusion limits on $M_{\rm S}$ for the combined dilepton ADD large extra dimensions search, using a uniform positive prior in 1/$M_{\rm S}^8$.

Reconstructed $\cos\theta^*$ distributions for data and the SM background estimate in the electron channel.

Reconstructed $\cos\theta^*$ distributions for data and the SM background estimate in the muon channel.

Spectrum of ETmiss for the muon channel after the event selection. The spectrum is shown with the requirement MT > 252 GeV.

Spectrum of MT for the electron channel after the event selection.

Spectrum of MT for the muon channel after the event selection.

Observed and expected limits on SIGMA*B for WPRIME at 95% CL in the electron channel.

Observed and expected limits on SIGMA*B for W* at 95% CL in the electron channel.

Observed and expected limits on SIGMA*B for WPRIME at 95% CL in the muon channel.

Observed and expected limits on SIGMA*B for W* at 95% CL in the muon channel.

Observed and expected limits on SIGMA*B for WPRIME at 95% CL for the combination of the electron and muon channels.

Observed and expected limits on SIGMA*B for W* at 95% CL for the combination of the electron and muon channels.

Observed limits on M* as a function of the DM particle mass M(chi) at 90% CL for the combination of the electron and muon channel for various operators in the EFT.

Observed limits on the DM-nucleon scattering cross-section as a function of M(chi) at 90% CL for various operators in the EFT.

Observed limits on M* as a function of the DM particle mass M(chi) at 90% CL in the electron for various operators in the EFT.

Observed limits on M* as a function of the DM particle mass M(chi) at 90% CL in the muon for various operators in the EFT.

Observed limits on M* as a function of the DM particle mass M(chi) at 95% CL in the electron for various operators in the EFT.

Observed limits on M* as a function of the DM particle mass M(chi) at 95% CL in the muon for various operators in the EFT.

Observed limits on M* as a function of the DM particle mass M(chi) at 95% CL for the combination of the electron and muon channel for various operators in the EFT.

The effective mass distribution in 3-jet signal region.

The effective mass distribution in 4-jet (W) signal region.

The effective mass distribution in 4-jet very-loose and loose signal regions.

The effective mass distribution in 4-jet medium signal region.

The effective mass distribution in 4-jet tight signal region.

The effective mass distribution in 5-jet signal region.

The effective mass distribution in 6-jet loose and medium signal regions.

The effective mass distribution in 6-jet tight signal region.

The effective mass distribution in 6-jet very-tight signal region.

Observed limit 95% CL.

Expected limit 95% CL.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Expected limit 95% CL -1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Expected limit 95% CL -1 sigma.

Observed limit 95% CL (m_chi^0_1=0GeV).

Expected limit 95% CL (m_chi^0_1=0GeV).

Observed limit 95% CL +1 sigma (m_chi^0_1=0GeV).

Observed limit 95% CL -1 sigma (m_chi^0_1=0GeV).

Expected limit 95% CL +1 sigma (m_chi^0_1=0GeV).

Expected limit 95% CL -1 sigma (m_chi^0_1=0GeV).

Observed limit 95% CL (m_chi^0_1=395GeV).

Expected limit 95% CL (m_chi^0_1=395GeV).

Observed limit 95% CL (m_chi^0_1=695GeV).

Expected limit 95% CL (m_chi^0_1=695GeV).

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Observed CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with minus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Expected CLs contour with minus 1-sigma experimental uncertainty for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

First of two expected CLs contours with minus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Second of two expected CLs contours with minus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with plus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Observed CLs contour with minus 1-sigma signal cross-section uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour with plus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected CLs contour with minus 1-sigma experimental uncertainty for the pair-produced squarks each decaying via an intermediate chargino1 to a quark, a W boson and a neutralino1.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL.

Expected limit 95% CL -1 sigma.

Expected limit 95% CL +1 sigma.

Observed limit 95% CL -1 sigma.

Observed limit 95% CL +1 sigma.

Observed limit 95% CL.

Signal region for points.

Signal region for points.

Signal region for points (m_chi^0_1=0GeV).

Signal region for points (m_chi^0_1=395GeV).

Signal region for points (m_chi^0_1=695GeV).

Observed 95% CL cross-section upper limit for pair-produced gluinos decaying directly.

Observed 95% CL cross-section upper limit for associated gluino-squark production.

Observed 95% CL cross-section upper limit for pair-produced squarks decaying directly.

Observed 95% CL cross-section upper limit for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed 95% CL cross-section upper limit for the pair-produced gluinos each decaying via an intermediate chargino1 to two quarks, a W boson and a neutralino1.

Observed 95% CL cross-section upper limit for the pair-produced squarks each decaying via an intermediate chargino1 to quark, a W boson and a neutralino1.

Observed 95% CL cross-section upper limit for the pair-produced squarks each decaying via an intermediate chargino1 to quark, a W boson and a neutralino1.

Signal region for points.

Observed 95% CL cross-section upper limit for pair-produced gluinos decaying via stops into top+charm+neutralino1.

Production cross-section in PB.

Signal acceptance in PCT for SR2jl.

Signal acceptance times reconstruction efficiency in PCT for SR2jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jl.

Signal acceptance in PCT for SR2jm.

Signal acceptance times reconstruction efficiency in PCT for SR2jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jm.

Signal acceptance in PCT for SR2jt.

Signal acceptance times reconstruction efficiency in PCT for SR2jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jt.

Signal acceptance in PCT for SR2jW.

Signal acceptance times reconstruction efficiency in PCT for SR2jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jW.

Signal acceptance in PCT for SR3j.

Signal acceptance times reconstruction efficiency in PCT for SR3j.

Uncertainty on signal acceptance times reconstruction efficiency for SR3j.

Signal acceptance in PCT for SR4jW.

Signal acceptance times reconstruction efficiency in PCT for SR4jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jW.

Signal acceptance in PCT for SR4jl-.

Signal acceptance times reconstruction efficiency in PCT for SR4jl-.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl-.

Signal acceptance in PCT for SR4jl.

Signal acceptance times reconstruction efficiency in PCT for SR4jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl.

Signal acceptance in PCT for SR4jm.

Signal acceptance times reconstruction efficiency in PCT for SR4jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jm.

Signal acceptance in PCT for SR4jt.

Signal acceptance times reconstruction efficiency in PCT for SR4jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jt.

Signal acceptance in PCT for SR5j.

Signal acceptance times reconstruction efficiency in PCT for SR5j.

Uncertainty on signal acceptance times reconstruction efficiency for SR5j.

Signal acceptance in PCT for SR6jl.

Signal acceptance times reconstruction efficiency in PCT for SR6jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jl.

Signal acceptance in PCT for SR6jm.

Signal acceptance times reconstruction efficiency in PCT for SR6jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jm.

Signal acceptance in PCT for SR6jt.

Signal acceptance times reconstruction efficiency in PCT for SR6jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt.

Signal acceptance in PCT for SR6jt+.

Signal acceptance times reconstruction efficiency in PCT for SR6jt+.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt+.

Production cross-section in PB.

Signal acceptance in PCT for SR2jl.

Signal acceptance times reconstruction efficiency in PCT for SR2jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jl.

Signal acceptance in PCT for SR2jm.

Signal acceptance times reconstruction efficiency in PCT for SR2jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jm.

Signal acceptance in PCT for SR2jt.

Signal acceptance times reconstruction efficiency in PCT for SR2jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jt.

Signal acceptance in PCT for SR2jW.

Signal acceptance times reconstruction efficiency in PCT for SR2jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR2jW.

Signal acceptance in PCT for SR3j.

Signal acceptance times reconstruction efficiency in PCT for SR3j.

Uncertainty on signal acceptance times reconstruction efficiency for SR3j.

Signal acceptance in PCT for SR4jW.

Signal acceptance times reconstruction efficiency in PCT for SR4jW.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jW.

Signal acceptance in PCT for SR4jl-.

Signal acceptance times reconstruction efficiency in PCT for SR4jl-.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl-.

Signal acceptance in PCT for SR4jl.

Signal acceptance times reconstruction efficiency in PCT for SR4jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jl.

Signal acceptance in PCT for SR4jm.

Signal acceptance times reconstruction efficiency in PCT for SR4jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jm.

Signal acceptance in PCT for SR4jt.

Signal acceptance times reconstruction efficiency in PCT for SR4jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR4jt.

Signal acceptance in PCT for SR5j.

Signal acceptance times reconstruction efficiency in PCT for SR5j.

Uncertainty on signal acceptance times reconstruction efficiency for SR5j.

Signal acceptance in PCT for SR6jl.

Signal acceptance times reconstruction efficiency in PCT for SR6jl.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jl.

Signal acceptance in PCT for SR6jm.

Signal acceptance times reconstruction efficiency in PCT for SR6jm.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jm.

Signal acceptance in PCT for SR6jt.

Signal acceptance times reconstruction efficiency in PCT for SR6jt.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt.

Signal acceptance in PCT for SR6jt+.

Signal acceptance times reconstruction efficiency in PCT for SR6jt+.

Uncertainty on signal acceptance times reconstruction efficiency for SR6jt+.

The fully corrected measurement of ASYM(FB) as a function of the muon-pair invariant mass.

M(jj) in Top CR for SR-Zjets.

SF - M(ll) in SR-WWa w/o M(ll) and ET(miss,rel).

DF - M(ll) in SR-WWa w/o M(ll) and ET(miss,rel).

SF - ET(miss,rel) in SR-WWa w/o M(ll) and ET(miss,rel).

DF - ET(miss,rel) in SR-WWa w/o M(ll) and ET(miss,rel).

SF - MT2 in SR-MT2 w/o MT2.

DF - MT2 in SR-MT2 w/o MT2.

SF - ET(miss,rel) in SR-Zjets w/o ET(miss,rel).

Observed 95% CL exclusion contour for chargino pair production via sleptons.

Expected 95% CL exclusion contour for chargino pair production via sleptons.

Observed 95% CL exclusion contour for chargino pair production via WW.

Observed 95% CL limit on signal strength for chargino pair production via WW for mN1 = 0 GeV.

Expected 95% CL limit on signal strength for chargino pair production via WW for mN1 = 0 GeV.

Observed 95% CL exclusion contour for chargino neutralino production via WZ.

Expected 95% CL exclusion contour for chargino neutralino production via WZ.

Observed 95% CL exclusion contour for chargino neutralino production via WZ (2+3L combination).

Expected 95% CL exclusion contour for chargino neutralino production via WZ (2+3L combination).

Observed 95% CL exclusion contour for slepton pair production (right-handed).

Expected 95% CL exclusion contour for slepton pair production (right-handed).

Observed 95% CL exclusion contour for slepton pair production (left-handed).

Expected 95% CL exclusion contour for slepton pair production (left-handed).

Observed 95% CL exclusion contour for slepton pair production (right- plus left-handed).

Expected 95% CL exclusion contour for slepton pair production (right- plus left-handed).

Expected 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=100 GeV.

Observed 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=100 GeV.

Expected 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=140 GeV.

Observed 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=140 GeV.

Expected 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=250 GeV.

Observed 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=250 GeV.

Observed 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=250 GeV (2+3L combination).

Expected 95% CL exclusion contour for pMSSM w/ right-handed sleptons, M1=250 GeV (2+3L combination).

Expected 95% CL exclusion contour for pMSSM w/o sleptons, M1=50 GeV.

Observed 95% CL exclusion contour for pMSSM w/o sleptons, M1=50 GeV.

Expected 95% CL exclusion contour for pMSSM w/o sleptons, M1=50 GeV (2+3L combination).

Observed 95% CL exclusion contour for pMSSM w/o sleptons, M1=50 GeV (2+3L combination).

Observed 95% CL exclusion contour for selectron pair production (right-handed).

Expected 95% CL exclusion contour for selectron pair production (right-handed).

Observed 95% CL exclusion contour for selectron pair production (left-handed).

Expected 95% CL exclusion contour for selectron pair production (left-handed).

Observed 95% CL exclusion contour for selectron pair production (right- plus left-handed).

Expected 95% CL exclusion contour for selectron pair production (right- plus left-handed).

Observed 95% CL exclusion contour for smuon pair production (right-handed).

Expected 95% CL exclusion contour for smuon pair production (right-handed).

Observed 95% CL exclusion contour for smuon pair production (left-handed).

Expected 95% CL exclusion contour for smuon pair production (left-handed).

Observed 95% CL exclusion contour for smuon pair production (right- plus left-handed).

Expected 95% CL exclusion contour for smuon pair production (right- plus left-handed).

Observed 95% CL exclusion contour for chargino pair production via sleptons.

Expected 95% CL exclusion contour for chargino pair production via sleptons.

Signal regions contributing to Fig. 06a.

Signal regions contributing to Fig. 05.

Signal regions contributing to Fig. 08a.

Signal regions contributing to Fig. 08b.

Signal regions contributing to Fig. 08c.

Signal regions contributing to Fig. 09a.

Signal regions contributing to Fig. 09b.

Signal regions contributing to Fig. 09c.

Signal regions contributing to Fig. 10a.

Observed cross-section limits for Fig. 06a.

Observed cross-section limits for Fig. 05.

Observed cross-section limits for Fig. 07a.

Observed cross-section limits for Fig. 08a.

Observed cross-section limits for Fig. 08b.

Observed cross-section limits for Fig. 08c.

Observed CLs values for Fig. 06a.

Observed CLs values for Fig. 05.

Observed CLs values for Fig. 07a.

Observed CLs values for Fig. 08a.

Observed CLs values for Fig. 08b.

Observed CLs values for Fig. 08c.

Observed CLs values for Fig. 09a.

Observed CLs values for Fig. 09b.

Observed CLs values for Fig. 09c.

Observed CLs values for Fig. 10a.

ET(miss,rel) in WW CR for SR-MT2 and SR-WWb/c.

ET(miss,rel) in Top CR for SR-WWa.

Central light jets multiplicity in Top CR for SR-Zjets.

ET(miss,rel) in ZV CR for SR-WWa.

SF - ET(miss,rel) in SR-MT2 w/o MT2.

DF - ET(miss,rel) in SR-MT2 w/o MT2.

Number of generated events for Fig. 06a.

Number of generated events for Fig. 05.

Number of generated events for Fig. 07a.

Number of generated events for Fig. 08a.

Number of events generated for Fig. 08b.

Number of events generated for Fig. 08c.

Production cross-sections in Fig. 06a.

Production cross-sections in Fig. 05.

Production cross-sections in Fig. 07a.

Production cross-sections in Fig. 08a.

Production cross-sections in Fig. 08b.

Production cross-sections in Fig. 08c.

Acceptance IN PCT in Fig. 06a.

Acceptance IN PCT in Fig. 05.

Acceptance IN PCT in Fig. 07a.

Acceptance IN PCT in Fig. 08a.

Acceptance IN PCT in Fig. 08b.

Acceptance IN PCT in Fig. 08c.

Efficiency IN PCT in Fig. 06a.

Efficiency IN PCT in Fig. 05.

Efficiency IN PCT in Fig. 07a.

Efficiency IN PCT in Fig. 08a.

Efficiency IN PCT in Fig. 08b.

Efficiency IN PCT in Fig. 08c.

Total systematic uncertainty IN PCT on signal yields in Fig. 06a.

Total systematic uncertainty IN PCT on signal yields in Fig. 05.

Total systematic uncertainty IN PCT on signal yields in Fig. 07a.

Total systematic uncertainty IN PCT on signal yields in Fig. 08a.

Total systematic uncertainty IN PCT on signal yields in Fig. 08b.

Total systematic uncertainty IN PCT on signal yields in Fig. 08c.

Observed 95% CL exclusion contour for chargino neutralino production via WZ (2+3L combination).

Expected 95% CL exclusion contour for chargino neutralino production via WZ (2+3L combination).

The product of the electronic width of the PHI(1020) and its branching fraction to KS KL.

Cross section measurement for PHI(1680).

Mass measurement for PHI(1680).

Measurement of the PHI(1680) width.

The product of the electronic width of the PHI(1680) and its branching fraction to KS KL.

The measured E+ E- --> KS KL cross section as a function of the centre-of-mass energy.

The measured E+ E- --> KS KL PI+ PI- cross section as a function of the centre-of-mass energy.

The measured E+ E- --> KS KS PI+ PI- cross section as a function of the centre-of-mass energy.

The measured E+ E- --> KS KS K+ K- cross section as a function of the centre-of-mass energy.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KL PI+ PI-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KS PI+ PI-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KS K+ K-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K*(892) KS PI) * BR(K*(892) --> KS PI) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K2*(1430) KS PI) * BR(K2*(1430) --> KS PI) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K*(892)+ K*(892)-) * (BR(K*(892) --> KS PI))**2 and the 90% C.L. J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> K2*(1430) K*(892)) * BR(K2*(1430) --> KS PI) * BR(K*(892) --> KS PI) and the 90% C.L. J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> KS KS PHI(1020)) * BR(PHI --> K+ K-) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> F2PRIME(1525) PHI(1020)) * BR(PHI --> K+ K-} * BR(F2PRIME(1525) --> KS KS) and the J/PSI branching fraction.

The product WIDTH(E+ E- --> J/PSI) * BR(J/PSI --> F2PRIME(1525) K+ K-) * BR(F2PRIME(1525) --> KS KS) and the J/PSI branching fraction.

Effective mass distribution in the multi-jet CR DS-lowMass.

Distribution of Met in the W+jets control region with 20.3/fb.

Distribution of Meff in the W+jets control region with 20.3/fb.

Distribution of Mt2 in the W+jets control region with 20.3/fb.

Distribution of Mt(tau1)+Mt(tau2) in the W+jets control region with 20.3/fb.

Distribution of Meff in the W+jets control region with 20.3/fb.

Distribution of Meff in the Z+jets control region with 20.3/fb.

The stransverse mass distribution in the WW-C1N2 validation region.

Mt(tau1)+Mt(tau2) distribution in Top-VR.

The stransverse mass distribution in SR-C1N2.

Mt(tau1)+Mt(tau2) distribution in SR-C1C1.

Effective mass distribution in SRDS-highMass.

Effective mass distribution in SRDS-lowMass.

Expected 95% CL exclusion limits for simplified models with a combination of chargino-neutralino and chargino-chargino production.

Observed 95% CL exclusion limits for simplified models with a combination of chargino-neutralino and chargino-chargino production.

Expected 95% CL exclusion limits for simplified models with chargino-chargino production.

Observed 95% CL exclusion limits for simplified models with chargino-chargino production.

Upper limits on the cross section for production of only right-handed stau pairs.

Upper limits on the cross section for production of only left-handed stau pairs.

Upper limits on the signal strength for the associated production of right-handed and left-handed stau pairs.

Expected 95% CL exclusion limits for the pMSSM models with fixed stau mass, M1=50 GeV.

Observed 95% CL exclusion limits for the pMSSM models with fixed stau mass, M1=50 GeV.

Expected 95% CL exclusion limits for the pMSSM models with variable stau mass, M1=75 GeV.

Observed 95% CL exclusion limits for the pMSSM models with variable stau mass, M1=75 GeV.

Numbers give 95% CL excluded model cross sections for the simplified models with chargino-chargino production.

Numbers give 95% CL excluded model cross sections for the simplified models with chargino-neutralino production.

SR with best expected p0-value for each point for the simplified models with chargino-neutralino and chargino-chargino production. SR-C1N2 (SR-C1C1) is indicated with 1 (2) and SR-DS-highMass (SR-DS-lowMass) is indicated with 3 (4).

SR with best expected p0-value for each point for the simplified models with chargino-chargino production. SR-C1N2 (SR-C1C1) is indicated with 1 (2) and SR-DS-highMass (SR-DS-lowMass) is indicated with 3 (4).

SR with best expected p0-value for each point for direct stau pair production. SR-C1N2 (SR-C1C1) is indicated with 1 (2) and SR-DS-highMass (SR-DS-lowMass) is indicated with 3 (4).

SR with best expected p0-value for each point for direct stau pair production (left-handed). SR-C1N2 (SR-C1C1) is indicated with 1 (2) and SR-DS-highMass (SR-DS-lowMass) is indicated with 3 (4).

SR with best expected p0-value for each point for direct stau pair production (right-handed). SR-C1N2 (SR-C1C1) is indicated with 1 (2) and SR-DS-highMass (SR-DS-lowMass) is indicated with 3 (4).

SR with best expected p0-value for each point for the pMSSM models with fixed stau mass, M1=50 GeV. SR-C1N2 (SR-C1C1) is indicated with 1 (2) and SR-DS-highMass (SR-DS-lowMass) is indicated with 3 (4).

SR with best expected p0-value for each point for the pMSSM models with variable stau mass, M1=75 GeV. SR-C1N2 (SR-C1C1) is indicated with 1 (2) and SR-DS-highMass (SR-DS-lowMass) is indicated with 3 (4).

Cutflows for the three SUSY reference points. The event yields have been normalised to 20.3/fb.

Cutflows for data and the SM backgrounds estimated from MC.

Detailed information for the three SUSY benchmark grid points (from left to right): the reference point(1: (chargino1(neutralino2),neutralino1)=(250,100)GeV, 2: (chargino1,neutralino1)=(250,50) GeV, 3: (stauR (stauL), neutralino1)=(127(129),0) GeV), production process(1:chargino1-neutralino2, 2:chargino1-chargino1, 3:stauL-stauL, 4:stauR-stauR), cross section, number of generated MC events, considered signal region(1:C1N2, 2:C1C1, 3:DS-highMass,4:DS-lowMass), event yield after normalization to 20.3 fb-1, acceptance (Acc.), efficiency (Eff.) on the signal selection, absolute systematic uncertainty on signal yields, 95% CL observed and expected limits on the number of events.

Number of generated events for the simplified models with chargino-neutralino production.

Number of generated events for the simplified models with chargino-chargino production.

Number of generated events for direct left-handed stau pair production.

Number of generated events for direct right-handed stau pair production.

Production cross section for the simplified models with chargino-neutralino production.

Production cross section for the simplified models with chargino-chargino production.

Production cross section for direct left-handed stau pair production.

Production cross section for direct right-handed stau pair production.

Acceptance for the simplified models with chargino-neutralino production.

Acceptance for the simplified models with chargino-chargino production.

Acceptance for direct left-handed stau pair production.

Acceptance for direct right-handed stau pair production.

Efficiency for the simplified models with chargino-neutralino production.

Efficiency for the simplified models with chargino-chargino production.

Efficiency for direct stau (the left-handed) pair production.

Efficiency for direct stau (the right-handed) pair production.

Experimental systematics (in percentage) for the simplified models with chargino-neutralino production.

Experimental systematics (in percentage) for the simplified models with chargino-chargino production.

Experimental systematics (in percentage) for direct stau (the left-handed) pair production.

Experimental systematics (in percentage) for direct stau (the right-handed) pair production.

Observed CLs for the simplified models with chargino-neutralino production.

Observed CLs for the simplified models with chargino-chargino production.

Observed CLs for direct stau (the left-handed) pair production.

Observed CLs for direct stau (the right-handed) pair production.

Expected CLs for the simplified models with chargino-neutralino production.

Expected CLs for the simplified models with chargino-chargino production.

Expected CLs for direct stau (the left-handed) pair production.

Expected CLs for direct stau (the right-handed) pair production.

Observed and expected numbers of events with exactly three leptons with the scalar sum of jet transverse momentum values HT < 200 GeV. "On-Z" refers to events with at least one E+ E- or MU+ MU- (OSSF) pair with dilepton mass between 75 and 105 GeV, while "Off-Z" refers to events with one or two OSSF pairs, none of which fall in this mass range. The OSSFN designation refers to the number of E+ E- and MU+ MU- pairs in the event. Search channels binned in ET have been combined into coarse ET bins for the purposes of presentation.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z GRAVITINO) = 0.5 for strong plus electroweak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0 for strong plus electroweak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0 for strong plus electroweak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z0 GRAVITINO) = 0.5. The chargino-Higgsino mass is fixed at 150 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z0 GRAVITINO) = 0.5. The chargino-Higgsino mass is fixed at 350 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 150 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 350 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 150 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the natural Higgsino NLSP scenario with strong plus electroweak production for BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0. The chargino-Higgsino mass is fixed at 350 GeV.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 150 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 250 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0 and strong plus weak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limit on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 350 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z0 GRAVITINO) = 1.0 and strong plus weak production.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the slepton co-NLSP model in the gluino-chargino (wino-like chargino) mass plane.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the stau-NLSP and stau-NNLSP scenario in the degenerate smuon- and selectron- stau mass plane.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the T1tttt model in the gluino-neutralino mass plane.

The product of acceptance and efficiency for the calculation of the 95% C.L. limits for the T6ttWW model in the sbottom-chargino mass plane.

Observed 95% C.L. exclusion contour for the T1tttt scenario.

Observed - 1sig(theoretical) 95% C.L. exclusion contour for the T1tttt scenario.

Observed + 1sig(theoretical) 95% C.L. exclusion contour for the T1tttt scenario.

Expected 95% C.L. exclusion contour for the T1tttt scenario.

Expected - 1sig 95% C.L. exclusion contour for the T1tttt scenario.

Expected + 1sig 95% C.L. exclusion contour for the T1tttt scenario.

Observed 95% C.L. exclusion contour for the T6ttWW scenario.

Observed - 1sig(theoretical) 95% C.L. exclusion contour for the T6ttWW scenario.

Observed + 1sig(theoretical) 95% C.L. exclusion contour for the T6ttWW scenario.

Expected 95% C.L. exclusion contour for the T6ttWW scenario.

Expected - 1sig 95% C.L. exclusion contour for the T6ttWW scenario.

Expected + 1sig 95% C.L. exclusion contour for the T6ttWW scenario.

Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = BR(NEUTRALINO1 --> Z GRAVITINO) = 0.5 for strong plus electroweak production.

Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> HIGGS GRAVITINO) = 1.0 for strong plus electroweak production. Successive instances of SIG(OBS) = SIG(EXP) =0 have been rebinned over M(STOP) to reduce the size of the table.

Observed and expected 95% C.L. limits for the natural Higgsino NLSP scenario with BR(NEUTRALINO1 --> Z0 GLUINO) = 1.0 for strong plus electroweak production.

Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 150 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 250 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

Observed 95% C.L. limits on BR(NEUTRALINO1 --> HIGGS GRAVITINO) for the natural Higgsino NLSP scenario with fixed chargino-Higgsino mass of 350 GeV assuming BR(NEUTRALINO1 --> HIGGS GRAVITINO) + BR(NEUTRALINO1 --> Z GRAVITINO) = 1.0 and strong plus weak production.

Observed and expected 95% C.L. limits for the slepton co-NLSP model in the gluino-chargino (wino-like chargino) mass plane are shown.

Observed and expected 95% C.L. limits for the stau-NLSP and stau-NNLSP scenario in the degenerate smuon- and selectron- stau mass plane are shown. Successive instances of SIG(OBS) = SIG(EXP) =0 have been rebinned over M(SELECTRON) to reduce the size of the table.

Observed and expected 95% C.L. limits for the T1tttt model in the gluino-neutralino mass plane are shown.

Observed and expected 95% C.L. limits for the T6ttWW model in the sbottom-chargino mass plane are given.

Distribution of mT2 for events passing all the signal candidate selection requirements, except that on mT2 of the L100 selection, for DF events.

Distribution of mT2 for events passing all the signal candidate selection requirements, except that on mT2 of the L110 selection, for SF events.

Distribution of mT2 for events passing all the signal candidate selection requirements, except that on mT2 of the L110 selection, for DF events.

Observed 95% CL exclusion contour in the (STOP1, CHARGINO1) mass plane for a fixed value of m(NEUTRALINO1) = 1 GeV.

Expected 95% CL exclusion contour in the (STOP1, CHARGINO1) mass plane for a fixed value of m(NEUTRALINO1) = 1 GeV.

Observed 95% CL exclusion minus 1 sigma contour in the (STOP1, CHARGINO1) mass plane for a fixed value of m(NEUTRALINO1) = 1 GeV.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) - m(CHARGINO1) = 10 GeV.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) - m(CHARGINO1) = 10 GeV.

Observed 95% CL exclusion minus 1 sigma contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) - m(CHARGINO1) = 10 GeV.

Observed 95% CL exclusion contour in the (CHARGINO1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) = 300 GeV.

Expected 95% CL exclusion contour in the (CHARGINO1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) = 300 GeV.

Observed 95% CL exclusion minus one sigma contour in the (CHARGINO1, NEUTRALINO1) mass plane for a fixed value of m(STOP1) = 300 GeV.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane of m(CHARGINO1) = 2 m(NEUTRALINO1).

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for m(CHARGINO1) = 2 m(NEUTRALINO1).

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane for m(CHARGINO1) = 2 m(NEUTRALINO1).

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane.

Observed 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(CHARGINO1) = 106 GeV.

Expected 95% CL exclusion contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(CHARGINO1) = 106 GeV.

Observed 95% CL exclusion minus one sigma contour in the (STOP1, NEUTRALINO1) mass plane for a fixed value of m(CHARGINO1) = 106 GeV.

Expected CLs values for Fig. 14.

Observed CLs values for Fig. 14.

Observed cross-section limits for Fig. 14.

Expected CLs values for Fig. 15.

Observed CLs values for Fig. 15.

Observed cross-section limits for Fig. 15.

Expected CLs values for Fig. 16.

Observed CLs values for Fig. 16.

Observed cross-section limits for Fig. 14.

Expected CLs values for Fig. 17.

Observed CLs values for Fig. 17.

Observed cross-section limits for Fig. 17.

Expected CLs values for Fig. 19.

Observed CLs values for Fig. 19.

Observed cross-section limits for Fig. 19.

Number of generated events for Fig. 16.

Acceptance of S1 for Fig. 16.

Efficiency of S1 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S1 for Fig. 16.

Acceptance of S2 for Fig. 16.

Efficiency of S2 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S2 for Fig. 16.

Acceptance of S3 for Fig. 16.

Efficiency of S3 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S3 for Fig. 16.

Acceptance of S4 for Fig. 16.

Efficiency of S4 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S4 for Fig. 16.

Acceptance of S5 for Fig. 16.

Efficiency of S5 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S5 for Fig. 16.

Acceptance of S6 for Fig. 16.

Efficiency of S6 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S6 for Fig. 16.

Acceptance of S7 for Fig. 16.

Efficiency of S7 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in S7 for Fig. 16.

Acceptance of H160 for Fig. 16.

Efficiency of H160 for Fig. 16.

Total systematic uncertainty IN PCT on signal yields in H160 for Fig. 16.

Observed cross-section limits for Fig. 20.

Observed cross-section limits for Fig. 20.

Expected cross-section limits for Fig. 20.

Total number of generated MC events for each point of the grid.

Observed upper limit on the signal cross-section, in pb, for each point of the grid in the different flavour channel.

Observed upper limit on the signal cross-section, in pb, for each point of the grid in the same flavour channel.

The best expected signal region chosen for each point of the grid in the different flavour channel.

The best expected signal region chosen for each point of the grid in the same flavour channel.

Observed CLs for each point of the grid in the different flavour channel.

Observed CLs for each point of the grid in the same flavour channel.

Expected CLs for each point of the grid in the different flavour channel.

Expected CLs for each point of the grid in the same flavour channel.

Signal acceptance for all the analysis cuts, except the BDTG cut, for each point of the grid in the different flavour channel.

Signal acceptance for all the analysis cuts, except the BDTG cut, for each point of the grid in the same flavour channel.

Signal efficiency, including the acceptance of the BDTG cut, for each point of the grid in the different flavour channel.

Signal efficiency, including the acceptance of the BDTG cut, for each point of the grid in the same flavour channel.

Total signal experimental systematic uncertainty for each point of the grid in the different flavour channel.

Signal efficiency, including the acceptance of the BDTG cut, for each point of the grid in the same flavour channel.

Number of simulated events passing various stages of the selection in the hadronic mT2 analysis for a signal sample with m(STOP1)=300 GeV, m(CHARGINO1) = 150 GeV and m(NEUTRALINO1) = 50 GeV, and with the top squark decaying as STOP1 --> CHARGINO1+ BOTTOM -> W(*)+NEUTRALINO1+ BOTTOM with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the hadronic mT2 analysis for a signal sample with m(STOP1)=250 GeV, m(CHARGINO1) = 106 GeV and m(NEUTRALINO1) = 60 GeV, and with the top squark decaying as STOP1 --> CHARGINO1+ BOTTOM -> W(*)+NEUTRALINO1+ BOTTOM with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the leptonic mT2 analysis for two signal samples with the top squark decaying as STOP1 --> CHARGINO1+ BOTTOM -> W(*)+NEUTRALINO1+BOTTOM with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the leptonic mT2 analysis for a signal sample with m(STOP1)=180 GeV and m(NEUTRALINO1) = 60 GeV, and with the top squark decaying as STOP1 --> W + BOTTOM + NEUTRALINO1 with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise.

Number of simulated events passing various stages of the selection in the in the MVA analysis for all signal samples used to train the BDTG and with the top squark decaying as STOP1 --> TOP + NEUTRALINO1 with unit probability. Event weights are applied to correct simulated events to data. "Isolation" includes the effects of tight ID for electrons and the isolation selection for both electrons and muons. "Cleaning cuts" refer to cuts applied to remove non-collision backgrounds and detector noise. The index i in category (Ci) is the one reported in table 3 for each signal point, SF and DF.

The effective mass distribution in VR2Z.

The ETmiss distribution in SR0noZa.

The effective mass distribution in SR0noZa.

The ETmiss distribution in SR1noZa.

The effective mass distribution in SR1noZa.

The ETmiss distribution in SR2noZa.

The effective mass distribution in SR2noZa.

The ETmiss distribution in SR0noZb.

The effective mass distribution in SR0noZb.

The ETmiss distribution in SR1noZb.

The effective mass distribution in SR1noZb.

The ETmiss distribution in SR2noZb.

The effective mass distribution in SR2noZb.

The ETmiss distribution in SR0Z.

The effective mass distribution in SR0Z.

The ETmiss distribution in SR1Z.

The effective mass distribution in SR1Z.

The ETmiss distribution in SR2Z.

The effective mass distribution in SR2Z.

Observed 95% CL exclusion contour for the RPV chargino NLSP model with lambda_121 != 0.

Expected 95% CL exclusion contour for the RPV chargino NLSP model with lambda_121 != 0.

Observed 95% CL exclusion contour for the RPV chargino NLSP model with lambda_122 != 0.

Expected 95% CL exclusion contour for the RPV chargino NLSP model with lambda_122 != 0.

Observed 95% CL exclusion contour for the RPV chargino NLSP model with lambda_133 != 0.

Expected 95% CL exclusion contour for the RPV chargino NLSP model with lambda_133 != 0.

Observed 95% CL exclusion contour for the RPV chargino NLSP model with lambda_233 != 0.

Expected 95% CL exclusion contour for the RPV chargino NLSP model with lambda_233 != 0.

Observed 95% CL exclusion contour for the RPV gluino NLSP model with lambda_121 != 0.

Expected 95% CL exclusion contour for the RPV gluino NLSP model with lambda_121 != 0.

Observed 95% CL exclusion contour for the RPV gluino NLSP model with lambda_122 != 0.

Expected 95% CL exclusion contour for the RPV gluino NLSP model with lambda_122 != 0.

Observed 95% CL exclusion contour for the RPV gluino NLSP model with lambda_133 != 0.

Expected 95% CL exclusion contour for the RPV gluino NLSP model with lambda_133 != 0.

Observed 95% CL exclusion contour for the RPV gluino NLSP model with lambda_233 != 0.

Expected 95% CL exclusion contour for the RPV gluino NLSP model with lambda_233 != 0.

Observed 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_121 != 0.

Expected 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_121 != 0.

Observed 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_122 != 0.

Expected 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_122 != 0.

Observed 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_133 != 0.

Expected 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_133 != 0.

Observed 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_233 != 0.

Expected 95% CL exclusion contour for the RPV Lslepton NLSP model with lambda_233 != 0.

Observed 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_121 != 0.

Expected 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_121 != 0.

Observed 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_122 != 0.

Expected 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_122 != 0.

Observed 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_133 != 0.

Expected 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_133 != 0.

Observed 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_233 != 0.

Expected 95% CL exclusion contour for the RPV Rslepton NLSP model with lambda_233 != 0.

Observed 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_121 != 0.

Expected 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_121 != 0.

Observed 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_122 != 0.

Expected 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_122 != 0.

Observed 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_133 != 0.

Expected 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_133 != 0.

Observed 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_233 != 0.

Expected 95% CL exclusion contour for the RPV sneutrino NLSP model with lambda_233 != 0.

Observed 95% CL exclusion contour for the R-slepton RPC model.

Expected 95% CL exclusion contour for the R-slepton RPC model.

Observed and expected 95% CL cross-section upper limits for the Stau RPC model, together with the theoretically predicted cross-section.

Observed and expected 95% CL cross-section upper limits for the Z RPC model, together with the theoretically predicted cross-section.

Observed 95% CL exclusion contour for the GGM tan beta = 1.5 model.

Expected 95% CL exclusion contour for the GGM tan beta = 1.5 model.

Observed 95% CL exclusion contour for the GGM tan beta = 30 model.

Expected 95% CL exclusion contour for the GGM tan beta = 30 model.

Observed 95% CL cross-section upper limit for the RPV chargino NLSP models with lambda_121 != 0 and lambda_122 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV chargino NLSP models with lambda_133 != 0 and lambda_233 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV gluino NLSP models with lambda_121 != 0 and lambda_122 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV gluino NLSP models with lambda_133 != 0 and lambda_233 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV Lslepton NLSP models with lambda_121 != 0 and lambda_122 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV Lslepton NLSP models with lambda_133 != 0 and lambda_233 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV Rslepton NLSP models with lambda_121 != 0 and lambda_122 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV Rslepton NLSP models with lambda_133 != 0 and lambda_233 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV sneutrino NLSP models with lambda_121 != 0 and lambda_122 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the RPV sneutrino NLSP models with lambda_133 != 0 and lambda_233 != 0, and the selection of Z-veto signal regions used to set limits in these models. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bba' means that the regions SR0noZb, SR1noZb and SR2noZa were used, in addition to the three Z-rich regions (SR0-2Z).

Observed 95% CL cross-section upper limit for the R-slepton RPC model, and the selection of Z-veto signal regions used to set limits in this model. The combination of regions used is ordered by the minimum number of hadronic taus required. For example, ``bbb' means that the regions SR0noZb, SR1noZb and SR2noZb were used, in addition to the three Z-rich regions (SR0-2Z). For the RPC stau and Z models, the ``aaa' combination of regions was used throughout.

Performance of the SR0noZa selection in the R-slepton RPC model: number of generated signal events; total signal cross-section; acceptance; efficiency; total experimental systematic uncertainty, not including Monte Carlo statistics; observed CL using this region alone; expected CL using this region alone.

Performance of the SR0noZb selection in the RPV chargino NLSP model with lambda_121 != 0: number of generated signal events; total signal cross-section; acceptance; efficiency; total experimental systematic uncertainty, not including Monte Carlo statistics; observed CL using this region alone; expected CL using this region alone.

Performance of the SR1noZa selection in the RPV sneutrino NLSP model with lambda_233 != 0: number of generated signal events; total signal cross-section; acceptance; efficiency; total experimental systematic uncertainty, not including Monte Carlo statistics; observed CL using this region alone; expected CL using this region alone.

Performance of the SR1noZb selection in the RPV gluino NLSP model with lambda_133 != 0: number of generated signal events; total signal cross-section; acceptance; efficiency; total experimental systematic uncertainty, not including Monte Carlo statistics; observed CL using this region alone; expected CL using this region alone.

Performance of the SR2noZa selection in the RPV sneutrino NLSP model with lambda_233 != 0: number of generated signal events; total signal cross-section; acceptance; efficiency; total experimental systematic uncertainty, not including Monte Carlo statistics; observed CL using this region alone; expected CL using this region alone.

Performance of the SR2noZb selection in the RPV gluino NLSP model with lambda_133 != 0: number of generated signal events; total signal cross-section; acceptance; efficiency; total experimental systematic uncertainty, not including Monte Carlo statistics; observed CL using this region alone; expected CL using this region alone.

Performance of the SR0Z selection in the GGM tan beta = 30 model: number of generated signal events; total signal cross-section; acceptance; efficiency; total experimental systematic uncertainty, not including Monte Carlo statistics; observed CL using this region alone; expected CL using this region alone.

Cut flows for a representative selection of SUSY signal points in the Z-veto signal regions. In each case, m2 and m1 refer to the axes of the plots in Sec. XI, where m2 is the larger of the two masses. The number of events expected for a luminosity of 20.3 fb-1 is quoted at each step of the selection. The preselection requires four baseline leptons, at least two of which are light leptons; the signal lepton selection is made at the ``Lepton Multiplicity' stage. ``Event Cleaning' refers to the selection criteria applied to remove non-collision backgrounds and detector noise.

Cut flows for a representative selection of SUSY signal points in the Z-rich signal regions. In each case, m2 and m1 refer to the axes of the plots in Sec. XI, where m2 is the larger of the two masses (or the value of mu in the case of GGM models). The number of events expected for a luminosity of 20.3 fb-1 is quoted at each step of the selection. The preselection requires four baseline leptons, at least two of which are light leptons; the signal lepton selection is made at the ``Lepton Multiplicity' stage. ``Event Cleaning' refers to the selection criteria applied to remove non-collision backgrounds and detector noise.

Cut flows by lepton channel for a representative selection of SUSY signal points in the SR0noZa signal region. In each case, m2 and m1 refer to the axes of the plots in Sec. XI, where m2 is the larger of the two masses. The number of events expected for a luminosity of 20.3 fb-1 is quoted at each step of the selection. The preselection requires four baseline leptons, at least two of which are light leptons; the signal lepton selection is made at the ``Lepton Multiplicity' stage. ``Event Cleaning' refers to the selection criteria applied to remove non-collision backgrounds and detector noise. The RPC R-slepton model is used, with (m2,m1) = (450,300) GeV.

Cut flows by lepton channel for a representative selection of SUSY signal points in the SR1noZb signal region. In each case, m2 and m1 refer to the axes of the plots in Sec. XI, where m2 is the larger of the two masses. The number of events expected for a luminosity of 20.3 fb-1 is quoted at each step of the selection. The preselection requires four baseline leptons, at least two of which are light leptons; the signal lepton selection is made at the ``Lepton Multiplicity' stage. ``Event Cleaning' refers to the selection criteria applied to remove non-collision backgrounds and detector noise. The RPV gluino NLSP model is used, with lambda_133 != 0 and (m2,m1) = (800,400) GeV.

Cut flows by lepton channel for a representative selection of SUSY signal points in the SR0Z signal region. In each case, m2 and m1 refer to the axes of the plots in Sec. XI, where m2 is the value of mu. The number of events expected for a luminosity of 20.3 fb-1 is quoted at each step of the selection. The preselection requires four baseline leptons, at least two of which are light leptons; the signal lepton selection is made at the ``Lepton Multiplicity' stage. ``Event Cleaning' refers to the selection criteria applied to remove non-collision backgrounds and detector noise. The GGM tan beta = 30 model is used, with (m2,m1) = (200,1000) GeV.