Showing 10 of 509 results
The results of a search for the direct pair production of top squarks, the supersymmetric partner of the top quark, in final states with one isolated electron or muon, several energetic jets, and missing transverse momentum are reported. The analysis also targets spin-0 mediator models, where the mediator decays into a pair of dark-matter particles and is produced in association with a pair of top quarks. The search uses data from proton-proton collisions delivered by the Large Hadron Collider in 2015 and 2016 at a centre-of-mass energy of $\sqrt{s}=13$ TeV and recorded by the ATLAS detector, corresponding to an integrated luminosity of 36 fb$^{-1}$. A wide range of signal scenarios with different mass-splittings between the top squark, the lightest neutralino and possible intermediate supersymmetric particles are considered, including cases where the W bosons or the top quarks produced in the decay chain are off-shell. No significant excess over the Standard Model prediction is observed. The null results are used to set exclusion limits at 95% confidence level in several supersymmetry benchmark models. For pair-produced top-squarks decaying into top quarks, top-squark masses up to 940 GeV are excluded. Stringent exclusion limits are also derived for all other considered top-squark decay scenarios. For the spin-0 mediator models, upper limits are set on the visible cross-section.
$\textbf{Distribution 1 } -$ Kinematic distribution of $m_{\rm top}^{\rm reclustered}$ in tN_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 1 } -$ Kinematic distribution of $m_{\rm top}^{\rm reclustered}$ in tN_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 1 } -$ Kinematic distribution of $m_{\rm top}^{\rm reclustered}$ in tN_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 1 } -$ Kinematic distribution of $m_{\rm top}^{\rm reclustered}$ in tN_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 2 } -$ Kinematic distribution of amT2 in bC2x_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 2 } -$ Kinematic distribution of amT2 in bC2x_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 2 } -$ Kinematic distribution of amT2 in bC2x_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 2 } -$ Kinematic distribution of amT2 in bC2x_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 3 } -$ Kinematic distribution of mT in bC2x_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 3 } -$ Kinematic distribution of mT in bC2x_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 3 } -$ Kinematic distribution of mT in bC2x_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 3 } -$ Kinematic distribution of mT in bC2x_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 4 } -$ Kinematic distribution of ETmiss in bCbv. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 4 } -$ Kinematic distribution of ETmiss in bCbv. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 4 } -$ Kinematic distribution of ETmiss in bCbv. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 4 } -$ Kinematic distribution of ETmiss in bCbv. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 5 } -$ Kinematic distribution of mT in DM_low. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 5 } -$ Kinematic distribution of mT in DM_low. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 5 } -$ Kinematic distribution of mT in DM_low. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 5 } -$ Kinematic distribution of mT in DM_low. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 6 } -$ Kinematic distribution of ETmiss in DM_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 6 } -$ Kinematic distribution of ETmiss in DM_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 6 } -$ Kinematic distribution of ETmiss in DM_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 6 } -$ Kinematic distribution of ETmiss in DM_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 7 } -$ Distributions of BDT score for the tN_diag_low region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 7 } -$ Distributions of BDT score for the tN_diag_low region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 7 } -$ Distributions of BDT score for the tN_diag_low region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 7 } -$ Distributions of BDT score for the tN_diag_low region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 8 } -$ Distributions of BDT score for the tN_diag_med region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 8 } -$ Distributions of BDT score for the tN_diag_med region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 8 } -$ Distributions of BDT score for the tN_diag_med region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 8 } -$ Distributions of BDT score for the tN_diag_med region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 9 } -$ Distributions of BDT score for the tN_diag_high region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 9 } -$ Distributions of BDT score for the tN_diag_high region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 9 } -$ Distributions of BDT score for the tN_diag_high region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 9 } -$ Distributions of BDT score for the tN_diag_high region. The SM background predictions are obtained using the background-only fit configuration.
$\textbf{Distribution 10 } -$ Kinematic distribution of ETmiss in tN_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 10 } -$ Kinematic distribution of ETmiss in tN_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 10 } -$ Kinematic distribution of ETmiss in tN_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 10 } -$ Kinematic distribution of ETmiss in tN_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 11 } -$ Kinematic distribution of amT2 in bWN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 11 } -$ Kinematic distribution of amT2 in bWN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 11 } -$ Kinematic distribution of amT2 in bWN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 11 } -$ Kinematic distribution of amT2 in bWN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 12 } -$ Kinematic distribution of pT(l)/ETmiss in bffN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 12 } -$ Kinematic distribution of pT(l)/ETmiss in bffN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 12 } -$ Kinematic distribution of pT(l)/ETmiss in bffN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 12 } -$ Kinematic distribution of pT(l)/ETmiss in bffN. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 13 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 13 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 13 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 13 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_diag. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 14 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 14 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 14 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 14 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_med. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 15 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 15 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 15 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Distribution 15 } -$ Kinematic distribution of pT(l)/ETmiss in bCsoft_high. The full event selection in the corresponding signal region is applied, except for the requirement that is imposed on the variable being plotted. The predicted SM backgrounds are scaled with the normalisation factors obtained from the corresponding control regions. The last bin contains overflows.
$\textbf{Exclusion contour 1 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 1 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 1 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 1 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 1 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 1 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 1 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 1 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Selected SR 1 } -$ Selected signal regions for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{Selected SR 1 } -$ Selected signal regions for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{Selected SR 1 } -$ Selected signal regions for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{Selected SR 1 } -$ Selected signal regions for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{Exclusion contour 2 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 2 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 2 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 2 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 2 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 2 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 2 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Exclusion contour 2 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(STOP)-m(NEUTRALINO) for the direct stop pair production assuming either stop -> t N1, stop -> b W C1 or stop -> b f f' N1 decay with a branching ratio of 100%.
$\textbf{Selected SR 2 } -$ Selected signal regions for the bino LSP model in the m(STOP) versus m(STOP)-m(NEUTRALINO) plane.
$\textbf{Selected SR 2 } -$ Selected signal regions for the bino LSP model in the m(STOP) versus m(STOP)-m(NEUTRALINO) plane.
$\textbf{Selected SR 2 } -$ Selected signal regions for the bino LSP model in the m(STOP) versus m(STOP)-m(NEUTRALINO) plane.
$\textbf{Selected SR 2 } -$ Selected signal regions for the bino LSP model in the m(STOP) versus m(STOP)-m(NEUTRALINO) plane.
$\textbf{Exclusion contour 3 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 3 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 3 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 3 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 3 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 3 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 3 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 3 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 3 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 3 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 3 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 3 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu < 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 4 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 4 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 4 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 4 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Selected SR 4 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for the direct stop/sbottom pair production in the wino NLSP model under the hypothesis of mq3L < mtR and mu > 0, where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, sbottom -> t C1, sbottom -> b N1, and sbottom -> b N2) are considered with different branching ratios for each signal point. N2 decays to N1 predominantly via either Z boson or Higgs boson depending on the sign of the μ parameter.
$\textbf{Exclusion contour 5 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 5 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 5 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 5 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 5 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 5 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 5 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 5 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production assuming b C1 decay with a branching ratio of 100%. The chargino mass is assumed to be close to the stop mass, m(C1) = m(STOP) - 10 GeV.
$\textbf{Exclusion contour 6 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 6 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 6 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 6 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 6 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 6 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 6 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 6 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 6 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 6 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 6 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 6 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 7 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 7 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 7 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 7 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 7 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 8 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 8 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 8 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 8 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 8 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 9 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 10 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 10 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 10 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 10 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 10 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly left-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 11 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 11 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 11 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 11 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 11 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for a mostly right-handed stop. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (exp.) } -$ Expected 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 12 (obs.) } -$ Observed 95% excluded regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 12 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 12 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 12 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Selected SR 12 } -$ Selected signal regions in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model for large $\tan\beta$. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{Exclusion contour 13 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 13 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 13 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 13 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 13 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 13 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 13 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 13 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Selected SR 13 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Selected SR 13 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Selected SR 13 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Selected SR 13 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} < m_{t_{R}}$ hypothesis. Both stop/sbottom pair productions are considered.
$\textbf{Exclusion contour 14 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{Exclusion contour 14 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{Exclusion contour 14 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{Exclusion contour 14 (exp.) } -$ Expected 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{Exclusion contour 14 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.<br><b>Note:</b> As no observed exclusion is found for this model, the contour is empty.
$\textbf{Exclusion contour 14 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.<br><b>Note:</b> As no observed exclusion is found for this model, the contour is empty.
$\textbf{Exclusion contour 14 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.<br><b>Note:</b> As no observed exclusion is found for this model, the contour is empty.
$\textbf{Exclusion contour 14 (obs.) } -$ Observed 95% excluded regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.<br><b>Note:</b> As no observed exclusion is found for this model, the contour is empty.
$\textbf{Selected SR 14 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{Selected SR 14 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{Selected SR 14 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{Selected SR 14 } -$ Selected signal regions in the plane of mm(STOP) versus m(NEUTRALINO) or the direct stop/sbottom pair production in the well-tempered neutralino model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2, b1 -> t C1, b1 -> b N1, and b1 -> b N2) are considered with different branching ratio for each signal point for the $m_{q_{3L}} > m_{t_{R}}$. Only stop pair production is considered.
$\textbf{DM Upper Limit 1 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 1 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 1 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 1 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 2 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a pseudoscalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 2 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a pseudoscalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 2 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a pseudoscalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 2 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a pseudoscalar mediator. The limit is shown as a function of the mediator mass for a fixed mass of the DM candidate of 1 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 3 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 3 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 3 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 3 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis of a scalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 4 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis a pseudoscalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 4 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis a pseudoscalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 4 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis a pseudoscalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{DM Upper Limit 4 } -$ Upper limit on the ratio of the DM production cross-section to the simplified model expectation under the hypothesis a pseudoscalar mediator. The limit is shown as a function of the DM candidate mass for a fixed mediator mass of 10 GeV. The coupling of the mediator to SM and DM particles is assumed to be g=1.
$\textbf{X-section U.L. 1 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{X-section U.L. 1 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{X-section U.L. 1 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{X-section U.L. 1 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(NEUTRALINO) plane.
$\textbf{X-section U.L. 2 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(STOP)-m(NEUTRALINO) plane.
$\textbf{X-section U.L. 2 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(STOP)-m(NEUTRALINO) plane.
$\textbf{X-section U.L. 2 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(STOP)-m(NEUTRALINO) plane.
$\textbf{X-section U.L. 2 } -$ Observed upper limit on the signal cross section for the bino LSP model in the m(STOP) vs m(STOP)-m(NEUTRALINO) plane.
$\textbf{X-section U.L. 3 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu < 0
$\textbf{X-section U.L. 3 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu < 0
$\textbf{X-section U.L. 3 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu < 0
$\textbf{X-section U.L. 3 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu < 0
$\textbf{X-section U.L. 4 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu > 0
$\textbf{X-section U.L. 4 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu > 0
$\textbf{X-section U.L. 4 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu > 0
$\textbf{X-section U.L. 4 } -$ Observed upper limit on the signal cross section for the wino NLSP model with mu > 0
$\textbf{X-section U.L. 5 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 5 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 5 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 5 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 6 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 6 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 6 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 6 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 7 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 7 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 7 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 7 } -$ Observed upper limit on the signal cross section for the higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 8 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 8 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 8 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 8 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with left-handed stop squarks.
$\textbf{X-section U.L. 9 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 9 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 9 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 9 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with right-handed stop squarks.
$\textbf{X-section U.L. 10 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 10 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 10 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 10 } -$ Observed upper limit on the signal cross section for the variable m(CHARGINO) - m(NEUTRALINO) higgsino LSP model with large tan beta.
$\textbf{X-section U.L. 11 } -$ Observed upper limit on the signal cross section for the simplified model with m(STOP) - m(CHARGINO) = 10 GeV.
$\textbf{X-section U.L. 11 } -$ Observed upper limit on the signal cross section for the simplified model with m(STOP) - m(CHARGINO) = 10 GeV.
$\textbf{X-section U.L. 11 } -$ Observed upper limit on the signal cross section for the simplified model with m(STOP) - m(CHARGINO) = 10 GeV.
$\textbf{X-section U.L. 11 } -$ Observed upper limit on the signal cross section for the simplified model with m(STOP) - m(CHARGINO) = 10 GeV.
$\textbf{X-section U.L. 12 } -$ Observed 95% upper cross-section limit in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{X-section U.L. 12 } -$ Observed 95% upper cross-section limit in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{X-section U.L. 12 } -$ Observed 95% upper cross-section limit in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{X-section U.L. 12 } -$ Observed 95% upper cross-section limit in the plane of m(STOP) versus m(NEUTRALINO) for direct stop pair production in the higgsino LSP model where various decay modes (stop -> b C1, stop -> t N1, stop -> t N2) are considered with different branching ratios depending on the hypothesis being considered. In this model, dm(C1,N1) =5 GeV and dm(N2,N1)=10 GeV are assumed.
$\textbf{X-section U.L. 13 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with left-handed stop squarks.
$\textbf{X-section U.L. 13 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with left-handed stop squarks.
$\textbf{X-section U.L. 13 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with left-handed stop squarks.
$\textbf{X-section U.L. 13 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with left-handed stop squarks.
$\textbf{X-section U.L. 14 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with right-handed stop squarks.
$\textbf{X-section U.L. 14 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with right-handed stop squarks.
$\textbf{X-section U.L. 14 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with right-handed stop squarks.
$\textbf{X-section U.L. 14 } -$ Observed upper limit on the signal cross section for the well-tempered neutralino model with right-handed stop squarks.
$\textbf{Cutflow 1 } -$ Cutflow for tN_med for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 1 } -$ Cutflow for tN_med for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 1 } -$ Cutflow for tN_med for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 1 } -$ Cutflow for tN_med for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 2 } -$ Cutflow for tN_high for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (1000, 1) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 2 } -$ Cutflow for tN_high for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (1000, 1) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 2 } -$ Cutflow for tN_high for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (1000, 1) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 2 } -$ Cutflow for tN_high for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (1000, 1) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 3 } -$ Cutflow for bWN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 230) GeV in bWN. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 3 } -$ Cutflow for bWN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 230) GeV in bWN. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 3 } -$ Cutflow for bWN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 230) GeV in bWN. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 3 } -$ Cutflow for bWN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 230) GeV in bWN. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 4 } -$ Cutflow for bffN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 4 } -$ Cutflow for bffN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 4 } -$ Cutflow for bffN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 4 } -$ Cutflow for bffN for the pure bino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{0}_{1} )$ = (350, 300) GeV. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 5 } -$ Cutflow for bC2x_diag for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (737, 500, 250) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 5 } -$ Cutflow for bC2x_diag for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (737, 500, 250) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 5 } -$ Cutflow for bC2x_diag for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (737, 500, 250) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 5 } -$ Cutflow for bC2x_diag for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (737, 500, 250) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 6 } -$ Cutflow for bC2x_med for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (842, 300, 150) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 6 } -$ Cutflow for bC2x_med for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (842, 300, 150) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 6 } -$ Cutflow for bC2x_med for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (842, 300, 150) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 6 } -$ Cutflow for bC2x_med for the wino NLSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (842, 300, 150) GeV. Only stop pair production is considered in the cutflow. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 7 } -$ Cutflow for the simplified signal model with $\Delta m( \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = 10 GeV, considering $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (700, 690, 1). The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 7 } -$ Cutflow for the simplified signal model with $\Delta m( \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = 10 GeV, considering $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (700, 690, 1). The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 7 } -$ Cutflow for the simplified signal model with $\Delta m( \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = 10 GeV, considering $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (700, 690, 1). The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 7 } -$ Cutflow for the simplified signal model with $\Delta m( \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = 10 GeV, considering $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (700, 690, 1). The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 8 } -$ Cutflow for bCsoft_diag for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (400, 355, 350) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 8 } -$ Cutflow for bCsoft_diag for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (400, 355, 350) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 8 } -$ Cutflow for bCsoft_diag for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (400, 355, 350) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 8 } -$ Cutflow for bCsoft_diag for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (400, 355, 350) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 9 } -$ Cutflow for bCsoft_med for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 205, 200) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 9 } -$ Cutflow for bCsoft_med for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 205, 200) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 9 } -$ Cutflow for bCsoft_med for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 205, 200) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 9 } -$ Cutflow for bCsoft_med for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (600, 205, 200) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 10 } -$ Cutflow for bCsoft_high for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (800, 155, 150) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 10 } -$ Cutflow for bCsoft_high for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (800, 155, 150) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 10 } -$ Cutflow for bCsoft_high for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (800, 155, 150) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 10 } -$ Cutflow for bCsoft_high for the higgsino LSP signal model with $m(\tilde{t}_{1} , \tilde{\chi}^{\pm}_{1} , \tilde{\chi}^{0}_{1} )$ = (800, 155, 150) GeV, assuming $\tilde{t}_{1} \sim \tilde{t}_{\mathrm{L}}$ and large $\tan\beta$. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV. Numbers are provided for the discovery SR, even if a shape fit is used for placing exclusion limits.
$\textbf{Cutflow 11 } -$ Cutflow for DM_high for the spin-0 mediator model with $m(\phi, \chi)$ = (300, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 11 } -$ Cutflow for DM_high for the spin-0 mediator model with $m(\phi, \chi)$ = (300, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 11 } -$ Cutflow for DM_high for the spin-0 mediator model with $m(\phi, \chi)$ = (300, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 11 } -$ Cutflow for DM_high for the spin-0 mediator model with $m(\phi, \chi)$ = (300, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 12 } -$ Cutflow for DM_low for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 12 } -$ Cutflow for DM_low for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 12 } -$ Cutflow for DM_low for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 12 } -$ Cutflow for DM_low for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 13 } -$ Cutflow for DM_low_loose for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 13 } -$ Cutflow for DM_low_loose for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 13 } -$ Cutflow for DM_low_loose for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Cutflow 13 } -$ Cutflow for DM_low_loose for the spin-0 mediator model with $m(\phi, \chi)$ = (20, 1) GeV, assuming g=1 and a scalar mediator. The DxAOD skimming step requires at least one of the following criteria to be fullfilled: one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ triggers has fired and there is at least one loose muon (electron) with $p_{\mathrm{T}}$ > 3.5 (4.5) GeV; or one of the $E_{\mathrm{T}}^{\mathrm{miss}}$ or lepton triggers has fired and there is at least one loose lepton with $p_{\mathrm{T}}$ > 25 GeV.
$\textbf{Acceptance 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 1 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $m_{\tilde{\chi}^{0}_{1}}$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 2 } -$ Acceptance and efficiency for the bino LSP model in the $m_{\tilde{t}_{1}}$ vs $\Delta m(\tilde{t}_{1},\tilde{\chi}^{0}_{1})$ plane. Efficiencies larger than 100% are observed in the bWN SR due differences in $am_{\mathrm{T2}}$ between truth and reconstruction level, in the absence of $b$-tagging inefficiencies. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Acceptance 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Acceptance 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Acceptance 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Efficiency 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Efficiency 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Efficiency 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Efficiency 3 } -$ Acceptance and efficiency for the wino NLSP model with $\mu > 0$.
$\textbf{Acceptance 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 4 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV. The model assumes large $\tan\beta$ and the $\tilde{t}_{1}$ to be mostly $\tilde{t}_{L}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 5 } -$ Acceptance and efficiency for the higgsino LSP model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) = 5$ GeV, in the region where $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{0}_{1}) < m_{\textrm{top}}$. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Acceptance 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Acceptance 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Acceptance 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Efficiency 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Efficiency 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Efficiency 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Efficiency 6 } -$ Acceptance and efficiency for the simplified model with $\Delta m (\tilde{\chi}^{\pm}_{1}, \tilde{\chi}^{\pm}_{1}) = 10$ GeV.
$\textbf{Acceptance 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Acceptance 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
$\textbf{Efficiency 7 } -$ Acceptance and efficiency for the spin-0 mediator model, assuming a scalar mediator. Acceptance and efficiency numbers are provided for discovery SRs even if shape fits are used for placing exclusion limits.
Jet substructure observables have significantly extended the search program for physics beyond the Standard Model at the Large Hadron Collider. The state-of-the-art tools have been motivated by theoretical calculations, but there has never been a direct comparison between data and calculations of jet substructure observables that are accurate beyond leading-logarithm approximation. Such observables are significant not only for probing the collinear regime of QCD that is largely unexplored at a hadron collider, but also for improving the understanding of jet substructure properties that are used in many studies at the Large Hadron Collider. This Letter documents a measurement of the first jet substructure quantity at a hadron collider to be calculated at next-to-next-to-leading-logarithm accuracy. The normalized, differential cross-section is measured as a function of log$_{10}\rho^2$, where $\rho$ is the ratio of the soft-drop mass to the ungroomed jet transverse momentum. This quantity is measured in dijet events from 32.9 fb$^{-1}$ of $\sqrt{s} = 13$ TeV proton-proton collisions recorded by the ATLAS detector. The data are unfolded to correct for detector effects and compared to precise QCD calculations and leading-logarithm particle-level Monte Carlo simulations.
Data from Fig 3a. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for $\beta$ = 0, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, $\sigma$(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$.
Data from Fig 3a. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for $\beta$ = 0, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, $\sigma$(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$.
Data from Fig 3b. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for $\beta$ = 1, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, $\sigma$(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$.
Data from Fig 3b. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for $\beta$ = 1, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, $\sigma$(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$.
Data from Fig 3c. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for $\beta$ = 2, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, $\sigma$(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$. The uncertainties are applied symmetrically, though the cross section cannot go below zero in the first bin.
Data from Fig 4 and Fig 8a-16a. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for beta = 0, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, sigma(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$. Each set of 10 bins corresponds to one $p_T$ bin in {600, 650, 700, 750, 800, 850, 900, 950, 1000, ∞ } and 10 evenly spaced bins in $log_{10}(\rho^2)$ from -4.5 to -0.5.
Data from Fig 4 and Fig 8b-16b. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for $\beta$ = 1, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, sigma(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$. Each set of 10 bins corresponds to one $p_T$ bin in {600, 650, 700, 750, 800, 850, 900, 950, 1000, ∞ } and 10 evenly spaced bins in $log_{10}(\rho^2)$ from -4.5 to -0.5.
Data from Fig 8c-16c. The unfolded $log_{10}(\rho^2)$ distribution for anti-kt R=0.8 jets with $p_T$(lead) > 600 GeV, after the soft drop algorithm is applied for $\beta$ = 2, in data. All uncertainties described in the text are shown on the data; the uncertainties from the calculations are shown on each one. The distributions are normalized to the integrated cross section, sigma(resum), measured in the resummation region, $-3.7 < log_{10}(\rho^2) < -1.7$. Each set of 10 bins corresponds to one $p_T$ bin in {600, 650, 700, 750, 800, 850, 900, 950, 1000, ∞ } and 10 evenly spaced bins in $log_{10}(\rho^2)$ from -4.5 to -0.5.
Data from Fig 6a. The summed covariance matrices of the systematic and statistical uncertainties for the combined $p_T$ and $log_{10}(\rho^2)$ bins for $\beta$ = 0. Each group of 10 bins corresponds to a bin of $p_T$ in {600, 650, 700, 750, 800, 850, 900, 950, 1000, ∞ }; each bin within the $p_T$ bin corresponds to 10 evenly spaced bins in $log_{10}(\rho^2)$ from -4.5 to -0.5.
Data from Fig 6b. The summed covariance matrices of the systematic and statistical uncertainties for the combined $p_T$ and $log_{10}(\rho^2)$ bins for $\beta$ = 1. Each group of 10 bins corresponds to a bin of $p_T$ in {600, 650, 700, 750, 800, 850, 900, 950, 1000, ∞ }; each bin within the $p_T$ bin corresponds to 10 evenly spaced bins in $log_{10}(\rho^2)$ from -4.5 to -0.5.
Data from Fig 6c. The summed covariance matrices of the systematic and statistical uncertainties for the combined $p_T$ and $log_{10}(\rho^2)$ bins for $\beta$ = 2. Each group of 10 bins corresponds to a bin of $p_T$ in {600, 650, 700, 750, 800, 850, 900, 950, 1000, ∞ }; each bin within the $p_T$ bin corresponds to 10 evenly spaced bins in $log_{10}(\rho^2)$ from -4.5 to -0.5.
Data from Fig 7a. The summed covariance matrices of the systematic and statistical uncertainties for the $log_{10}(\rho^2)$ bins for $\beta$ = 0, inclusive in $p_T$.
Data from Fig 7b. The summed covariance matrices of the systematic and statistical uncertainties for the $log_{10}(\rho^2)$ bins for $\beta$ = 1, inclusive in $p_T$.
Data from Fig 7c. The summed covariance matrices of the systematic and statistical uncertainties for the $log_{10}(\rho^2)$ bins for $\beta$ = 2, inclusive in $p_T$.
Results of a search for new phenomena in final states with an energetic jet and large missing transverse momentum are reported. The search uses proton--proton collision data corresponding to an integrated luminosity of 36.1 fb${}^{-1}$ at a centre-of-mass energy of 13 TeV collected in 2015 and 2016 with the ATLAS detector at the Large Hadron Collider. Events are required to have at least one jet with a transverse momentum above 250 GeV and no leptons ($e$ or $\mu$). Several signal regions are considered with increasing requirements on the missing transverse momentum above 250 GeV. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in models with pair-produced weakly interacting dark-matter candidates, large extra spatial dimensions, and supersymmetric particles in several compressed scenarios.
The measured leading jet $p_{T}$ distribution in the W($\rightarrow \mu \nu$)+jets control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
The measured $E_{T}^{miss}$ distribution in the W($\rightarrow e \nu$)+jets control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
The measured leading jet $p_{T}$ distribution in the W($\rightarrow e \nu$)+jets control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
The measured $E_{T}^{miss}$ distribution in the Z/$\gamma ^{*}$($\rightarrow \mu \mu$)+jets control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
The measured leading jet $p_{T}$ distribution in the Z/$\gamma ^{*}$($\rightarrow \mu \mu$)+jets control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
The measured $E_{T}^{miss}$ distribution in the top control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
The measured leading jet $p_{T}$ distribution in the top control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
Measured distribution of the $E_{T}^{miss}$ for the $E_{T}^{miss}$ > 250GeV selection compared to the SM predictions. The latter are normalized with normalization factors as determined by the global fit that considers exclusive $E_{T}^{miss}$ regions. The last bin of the distribution contains overflows.
Measured distribution of the leading jet $p_{T}$ for the $E_{T}^{miss}$ > 250GeV selection compared to the SM predictions. The latter are normalized with normalization factors as determined by the global fit that considers exclusive $E_{T}^{miss}$ regions. The last bin of the distribution contains overflows.
Measured distribution of the leading jet $|\eta|$ for the $E_{T}^{miss}$ > 250GeV selection compared to the SM predictions. The latter are normalized with normalization factors as determined by the global fit that considers exclusive $E_{T}^{miss}$ regions. The last bin of the distribution contains overflows.
Measured distribution of the jet multiplicity for the $E_{T}^{miss}$ > 250GeV selection compared to the SM predictions. The latter are normalized with normalization factors as determined by the global fit that considers exclusive $E_{T}^{miss}$ regions. The last bin of the distribution contains overflows.
The expected $95\%$ 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 assumed mediator mass m$_{Z_{A}}$ and the dark matter mass m$_{\chi}$.
The measured $E_{T}^{miss}$ distribution in the W($\rightarrow \mu \nu$)+jets control region, for the $E_{T}^{miss}$ > 250GeV inclusive selection, compared to the background predictions. The latter include the global normalization factors extracted from the fit. The last bin of the distribution contains overflows.
The observed $95\%$ 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 assumed mediator mass m$_{Z_{A}}$ and the dark matter mass m$_{\chi}$.
The observed $90\%$ CL exclusion limit on the spin-dependent WIMP–proton scattering cross section in the context of the simplified model with axial-vector couplings, assuming minimal mediator width and the coupling values $g_{q} = 0.25$ and $g_{\chi} = 1$.
The expected $95\%$ CL exclusion limit for a simplified model of dark matter production involving a vector operator, Dirac DM and couplings $g_{q} = 0.25$ and $g_{\chi} = 1$ as a function of the assumed mediator mass m$_{Z_{V}}$ and the dark matter mass m$_{\chi}$.
The observed $95\%$ CL exclusion limit for a simplified model of dark matter production involving a vector operator, Dirac DM and couplings $g_{q} = 0.25$ and $g_{\chi} = 1$ as a function of the assumed mediator mass m$_{Z_{V}}$ and the dark matter mass m$_{\chi}$.
The expected and observed $95\%$ CL limits on the signal strength $\mu = \sigma^{95\% CL}/\sigma$ as a function of the mediator mass for a very light WIMP, in a model with spin-0 pseudoscalar mediator and $g_{q}=g_{\chi}=1.0$.
The expected and observed $95\%$ CL limits on the signal strength $\mu = \sigma^{95\% CL}/\sigma$ as a function of the WIMP mass for $m_{Z_{P}}=10$ GeV, in a model with spin-0 pseudoscalar mediator and $g_{q}=g_{\chi}=1.0$.
The expected exclusion contour at $95\%$ CL in the m$_{\eta}$–m$_{\chi}$ parameter plane for the coloured scalar mediator model, with minimal width and coupling set to $g=1$.
The observed exclusion contour at $95\%$ CL in the m$_{\eta}$–m$_{\chi}$ parameter plane for the coloured scalar mediator model, with minimal width and coupling set to $g=1$.
The expected excluded region at the $95\%$ CL in the ($\tilde{t}_{1}$,$\chi^{0}_{1}$) mass plane for the decay channel $\tilde{t}_{1} \rightarrow c + \chi^{0}_{1}$ (B = $100\%$).
The observed excluded region at the $95\%$ CL in the ($\tilde{t}_{1}$,$\chi^{0}_{1}$) mass plane for the decay channel $\tilde{t}_{1} \rightarrow c + \chi^{0}_{1}$ (B = $100\%$).
The expected excluded region at the $95\%$ CL in the ($\tilde{t}_{1}$,$\chi^{0}_{1}$) mass plane for the decay channel $\tilde{t}_{1} \rightarrow b + ff' + \chi^{0}_{1}$ (B = $100\%$).
The observed excluded region at the $95\%$ CL in the ($\tilde{t}_{1}$,$\chi^{0}_{1}$) mass plane for the decay channel $\tilde{t}_{1} \rightarrow b + ff' + \chi^{0}_{1}$ (B = $100\%$).
The expected exclusion plane at $95\%$ CL as a function of sbottom and neutralino masses for the decay channel $\tilde{b}_{1} \rightarrow b + \chi^{0}_{1}$ (B = $100\%$).
The observed exclusion plane at $95\%$ CL as a function of sbottom and neutralino masses for the decay channel $\tilde{b}_{1} \rightarrow b + \chi^{0}_{1}$ (B = $100\%$).
The expected exclusion region at $95\%$ CL as a function of squark mass and the squark-neutralino mass difference for $\tilde{q}_{1} → q + \chi^{0}_{1}$ (q =u,d,c,s).
The observed exclusion region at $95\%$ CL as a function of squark mass and the squark-neutralino mass difference for $\tilde{q}_{1} → q + \chi^{0}_{1}$ (q =u,d,c,s).
Expected and observed $95\%$ CL lower limits on the fundamental Planck scale in 4+n dimensions, M$_D$, as a function of the number of extra dimensions.
Expected and observed $95\%$ CL upper limit on the signal strength $\mu$ in the hypothesis of an axial-vector mediator, g$_{q}=0.25$, g$_{\chi}=1.0$ and minimal mediator width, as a function of the assumed mediator and DM masses.
Observed $90\%$ CL exclusion limit on the spin-dependent WIMP–neutron scattering cross section in the context of the simplified model with axial-vector couplings, assuming minimal mediator width and the coupling values $g_{q}=0.25$ and $g_{\chi}=1$.
Expected and observed $95\%$ CL upper limit on the signal strength $\mu$ in the hypothesis of a pseudoscalar mediator, $g_{q}=g_{\chi}=1.0$ and minimal mediator width, as a function of the assumed mediator and DM masses.
This paper presents a measurement of the $W$ boson production cross section and the $W^{+}/W^{-}$ cross-section ratio, both in association with jets, in proton--proton collisions at $\sqrt{s}=8$ TeV with the ATLAS experiment at the Large Hadron Collider. The measurement is performed in final states containing one electron and missing transverse momentum using data corresponding to an integrated luminosity of 20.2 fb$^{-1}$. Differential cross sections for events with one or two jets are presented for a range of observables, including jet transverse momenta and rapidities, the scalar sum of transverse momenta of the visible particles and the missing transverse momentum in the event, and the transverse momentum of the $W$ boson. For a subset of the observables, the differential cross sections of positively and negatively charged $W$ bosons are measured separately. In the cross-section ratio of $W^{+}/W^{-}$ the dominant systematic uncertainties cancel out, improving the measurement precision by up to a factor of nine. The observables and ratios selected for this paper provide valuable input for the up quark, down quark, and gluon parton distribution functions of the proton.
Cross section for the production of W bosons for different inclusive jet multiplicities.
Statistical correlation between bins in data for the cross section for the production of W bosons for different inclusive jet multiplicities.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the inclusive jet multiplicity.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the inclusive jet multiplicity.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the inclusive jet multiplicity.
Differential cross section for the production of W bosons as a function of H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1.
Differential cross section for the production of W bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Differential cross section for the production of W bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Differential cross section for the production of W bosons as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1.
Differential cross section for the production of W bosons as a function of second leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of second leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross section for the production of W bosons as a function of second leading jet rapidity for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of second leading jet rapidity for events with N<sub> jets</sub> ≥ 2.
Differential cross section for the production of W bosons as a function of Δ R<sub>jet1,jet2</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of Δ R<sub>jet1,jet2</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross section for the production of W bosons as a function of dijet invariant mass for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of dijet invariant mass for events with N<sub> jets</sub> ≥ 2.
Cross section for the production of W bosons as a function of exclusive jet multiplicity.
Statistical correlation between bins in data for the cross section for the production of W bosons as a function of exclusive jet multiplicity.
Differential cross section for the production of W bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross section for the production of W bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross section for the production of W bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Differential cross section for the production of W bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 0.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 0.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the electron η for events with N<sub> jets</sub> ≥ 0.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 0.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 0.
Differential cross section for the production of W bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross section for the production of W bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 1.
Differential cross sections for the production of W<sup>+</sup> bosons, W<sup>-</sup> bosons and the W<sup>+</sup>/W<sup>-</sup> cross section ratio as a function of the electron η for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>+</sup> bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 1.
Statistical correlation between bins in data for the differential cross sections for the production of W<sup>-</sup> bosons as a function of the electron η for events with N<sub> jets</sub> ≥ 1.
List of experimentally considered systematic uncertainties for the W+jets cross section measurement
Non-perturbative corrections for the cross section for the production of W bosons for different inclusive jet multiplicities.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the inclusive jet multiplicity.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of second leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of second leading jet rapidity for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of Δ R<sub>jet1,jet2</sub> for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of dijet invariant mass for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the cross section for the production of W bosons as a function of exclusive jet multiplicity.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross section for the production of W bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
Non-perturbative corrections for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 2.
NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the H<sub> T</sub> for events with N<sub> jets</sub> ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].
NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the W p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].
NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the leading jet p<sub>T</sub> for events with N<sub> jets</sub> ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].
NNLO/NLO k-factors determined with NNLO Njetti for the differential cross sections for the production of W<sup>+</sup> bosons and W<sup>-</sup> bosons as a function of the leading jet rapidity for events with N<sub> jets</sub> ≥ 1. These numbers were obtained with code described in Phys. Rev. Lett. 115 (2015) 062002 [arXiv:1504.02131].
Inclusive jet and dijet cross-sections are measured in proton-proton collisions at a centre-of-mass energy of 13 TeV. The measurement uses a dataset with an integrated luminosity of 3.2 fb$^{-1}$ recorded in 2015 with the ATLAS detector at the Large Hadron Collider. Jets are identified using the anti-${k_t}$ algorithm with a radius parameter value of $R=0.4$. The inclusive jet cross-sections are measured double-differentially as a function of the jet transverse momentum, covering the range from 100 GeV to 3.5 TeV, and the absolute jet rapidity up to $|y|=3$. The double-differential dijet production cross-sections are presented as a function of the dijet mass, covering the range from 300 GeV to 9 TeV, and the half absolute rapidity separation between the two leading jets within $|y|<3$, $y*$, up to $y*=3$. Next-to-leading-order, and next-to-next-to-leading-order for the inclusive jet measurement, perturbative QCD calculations corrected for non-perturbative and electroweak effects are compared to the measured cross-sections.
rapidity bin 0 < |Y| < 0.5 anti-kt R=0.4
rapidity bin 0.5 < |Y| < 1.0 anti-kt R=0.4
rapidity bin 1.0 < |Y| < 1.5 anti-kt R=0.4
rapidity bin 1.5 < |Y| < 2.0 anti-kt R=0.4
rapidity bin 2.0 < |Y| < 2.5 anti-kt R=0.4
rapidity bin 2.5 < |Y| < 3.0 anti-kt R=0.4
rapidity bin 0 < y* < 0.5 anti-kt R=0.4
rapidity bin 0.5 < y* < 1.0 anti-kt R=0.4
rapidity bin 1.0 < y* < 1.5 anti-kt R=0.4
rapidity bin 1.5 < y* < 2.0 anti-kt R=0.4
rapidity bin 2.0 < y* < 2.5 anti-kt R=0.4
rapidity bin 2.5 < y* < 3.0 anti-kt R=0.4
A search for supersymmetry involving the pair production of gluinos decaying via third-generation squarks into the lightest neutralino ($\displaystyle\tilde\chi^0_1$) is reported. It uses LHC proton--proton collision data at a centre-of-mass energy $\sqrt{s} = 13$ TeV with an integrated luminosity of 36.1 fb$^{-1}$ collected with the ATLAS detector in 2015 and 2016. The search is performed in events containing large missing transverse momentum and several energetic jets, at least three of which must be identified as originating from $b$-quarks. To increase the sensitivity, the sample is divided into subsamples based on the presence or absence of electrons or muons. No excess is found above the predicted background. For $\displaystyle\tilde\chi^0_1$ masses below approximately 300 GeV, gluino masses of less than 1.97 (1.92) TeV are excluded at 95% confidence level in simplified models involving the pair production of gluinos that decay via top (bottom) squarks. An interpretation of the limits in terms of the branching ratios of the gluinos into third-generation squarks is also provided. These results improve upon the exclusion limits obtained with the 3.2 fb$^{-1}$ of data collected in 2015.
Observed 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Expected 95% CL exclusion contour for Gtt model.
Observed 95% CL exclusion contour for Gbb model.
Observed 95% CL exclusion contour for Gbb model.
Observed 95% CL exclusion contour for Gbb model.
Observed 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gbb model.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.8 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 2.0 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 600 GeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Expected 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Observed 95% CL exclusion contour for Gluino mass = 1.9 TeV, Neutralino mass = 1 TeV.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gbb-VC.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-Gtt-1l-B.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-1L-II.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HI.
Distribution of ETMISS for SR-0L-HH.
Distribution of ETMISS for SR-0L-HH.
Distribution of ETMISS for SR-0L-HH.
Distribution of ETMISS for SR-0L-HH.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-B.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-M.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-C.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gbb model in SR-Gbb-VC.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-B.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-M.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-0l-C.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-B.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-M.
Acceptances for Gtt model in SR-Gtt-1l-C.
Acceptances for Gtt model in SR-Gtt-1l-C.
Acceptances for Gtt model in SR-Gtt-1l-C.
Acceptances for Gtt model in SR-Gtt-1l-C.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-B.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-M.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-C.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gbb model in SR-Gbb-VC.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-B.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-B.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-1l-M.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
Experimental efficiencies for Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gbb model in SR-Gbb-VC.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-0l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-B.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-M.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
95% CL upper limit on the cross-section times branching ratio (in fb) for the Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-B.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-M.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-C.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Expected 95% CL exclusion contour for Gbb model in SR-Gbb-VC.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-0l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-B.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-M.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Observed 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected 95% CL exclusion contour for Gtt model in SR-Gtt-1l-C.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-B selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-M selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-C selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gbb-0L-VC selection for a Gbb signal point (MGLUON,MNEUTRALINO) = (1900,1400) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-1L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-B selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-M selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
Expected number of signal events after each step of the Gtt-0L-C selection for a Gtt signal point (MGLUON,MNEUTRALINO) = (1900,1) GeV.
A search for weakly interacting massive particle dark matter produced in association with bottom or top quarks is presented. Final states containing third-generation quarks and missing transverse momentum are considered. The analysis uses 36.1 $fb^{-1}$ of proton-proton collision data recorded by the ATLAS experiment at $\sqrt{s}$ = 13 TeV in 2015 and 2016. No significant excess of events above the estimated backgrounds is observed. The results are interpreted in the framework of simplified models of spin-0 dark-matter mediators. For colour-neutral spin-0 mediators produced in association with top quarks and decaying into a pair of dark-matter particles, mediator masses below 50 GeV are excluded assuming a dark-matter candidate mass of 1 GeV and unitary couplings. For scalar and pseudoscalar mediators produced in association with bottom quarks, the search sets limits on the production cross-section of 300 times the predicted rate for mediators with masses between 10 and 50 GeV and assuming a dark-matter mass of 1 GeV and unitary coupling. Constraints on colour-charged scalar simplified models are also presented. Assuming a dark-matter particle mass of 35 GeV, mediator particles with mass below 1.1 TeV are excluded for couplings yielding a dark-matter relic density consistent with measurements.
- - - - - - - - Overview of HEPData Record - - - - - - - - <br/><br/> <b>Systematic uncertainties:</b> <a href="80080?version=1&table=Table2">table</a><br/><br/> <b>Fit results:</b> <a href="80080?version=1&table=Table3">SRb1 and SRb2</a> <a href="80080?version=1&table=Table4">SRt1, SRt2 and SRt3</a><br/><br/> <b>Upper limits:</b> <a href="80080?version=1&table=Table5">table</a><br/><br/> <b>SR distributions:</b> <ul> <li><a href="80080?version=1&table=Table6">SRb1: $E_{\mathrm T}^{\mathrm{miss}}$</a> <li><a href="80080?version=1&table=Table7">SRb2: $\cos{\theta}^*_{bb}$</a> <li><a href="80080?version=1&table=Table8">SRt1: $m_{\mathrm T}^{\mathrm{b,min}}$</a> <li><a href="80080?version=1&table=Table9">SRt2: $E_{\mathrm T}^{\mathrm{miss,sig}}$</a> <li><a href="80080?version=1&table=Table10">SRt3: $\xi^{+}_{\ell\ell}$</a> <li><a href="80080?version=1&table=Table34">SRb1: jet $p_{T}$</a> <li><a href="80080?version=1&table=Table35">SRb2: $H_{\mathrm T}^{ratio}$</a> <li><a href="80080?version=1&table=Table36">SRt1: $\Delta R_{bb}$</a> <li><a href="80080?version=1&table=Table37">SRt2: $M_{\mathrm T}^{b,min}$</a> <li><a href="80080?version=1&table=Table38">SRt3: $\Delta \phi_{boost}$</a> </ul> <b>Exclusion limits:</b> <ul> <li>Scalar SRb2 <a href="80080?version=1&table=Table11">expected</a> <a href="80080?version=1&table=Table12">observed</a> <li>Scalar SRt1/SRt2 <a href="80080?version=1&table=Table13">expected</a> <a href="80080?version=1&table=Table14">observed</a> <li>Scalar SRt3 <a href="80080?version=1&table=Table15">expected</a> <a href="80080?version=1&table=Table16">observed</a> <li>Pseudo-scalar SRb2 <a href="80080?version=1&table=Table17">expected</a> <a href="80080?version=1&table=Table18">observed</a> <li>Pseudo-scalar SRt1/SRt2 <a href="80080?version=1&table=Table19">expected</a> <a href="80080?version=1&table=Table20">observed</a> <li>Pseudo-scalar SRt3 <a href="80080?version=1&table=Table21">expected</a> <a href="80080?version=1&table=Table22">observed</a> <li>Scalar, SRt1/SRt2 vs DM mass <a href="80080?version=1&table=Table23">expected</a> <a href="80080?version=1&table=Table24">observed</a> <li>Scalar, SRt3 vs DM mass <a href="80080?version=1&table=Table25">expected</a> <a href="80080?version=1&table=Table26">observed</a> <li>Pseudo-scalar, SRt1/SRt2 vs DM mass <a href="80080?version=1&table=Table27">expected</a> <a href="80080?version=1&table=Table28">observed</a> <li>Pseudo-scalar, SRt3 vs DM mass <a href="80080?version=1&table=Table29">expected</a> <a href="80080?version=1&table=Table30">observed</a> <li>Colour-charged scalar mediators ($b-$FDM) <a href="80080?version=1&table=Table32">expected</a> <a href="80080?version=1&table=Table33">observed</a> </ul> <b>Direct detection plot:</b> <a href="80080?version=1&table=Table31">table</a><br/><br/> <b>Acceptances:</b> <ul> <li><a href="80080?version=1&table=Table39">SRb1</a> <li><a href="80080?version=1&table=Table41">SRb2 scalar</a> <li><a href="80080?version=1&table=Table44">SRb2 pseudo-scalar</a> <li><a href="80080?version=1&table=Table45">SRt2 scalar</a> <li><a href="80080?version=1&table=Table46">SRt1 scalar</a> <li><a href="80080?version=1&table=Table49">SRt2 pseudo-scalar</a> <li><a href="80080?version=1&table=Table50">SRt1 pseudo-scalar</a> <li><a href="80080?version=1&table=Table53">SRt3 scalar</a> <li><a href="80080?version=1&table=Table55">SRt3 pseudo-scalar</a> </ul> <b>Efficiencies:</b> <ul> <li><a href="80080?version=1&table=Table40">SRb1</a> <li><a href="80080?version=1&table=Table42">SRb2 scalar</a> <li><a href="80080?version=1&table=Table43">SRb2 pseudo-scalar</a> <li><a href="80080?version=1&table=Table47">SRt2 scalar</a> <li><a href="80080?version=1&table=Table48">SRt1 scalar</a> <li><a href="80080?version=1&table=Table51">SRt2 pseudo-scalar</a> <li><a href="80080?version=1&table=Table52">SRt1 pseudo-scalar</a> <li><a href="80080?version=1&table=Table54">SRt3 scalar</a> <li><a href="80080?version=1&table=Table56">SRt3 pseudo-scalar</a> </ul> <b>Cutflows:</b> <ul> <li><a href="80080?version=1&table=Table57">SRb1</a> <li><a href="80080?version=1&table=Table58">SRb2</a> <li><a href="80080?version=1&table=Table59">SRt1 scalar</a> <li><a href="80080?version=1&table=Table60">SRt2 scalar</a> <li><a href="80080?version=1&table=Table61">SRt1 pseudo-scalar</a> <li><a href="80080?version=1&table=Table62">SRt2 pseudo-scalar</a> <li><a href="80080?version=1&table=Table63">SRt3</a> </ul> <b>Truth Code snippets</b> are available under "Resources" (purple button on the left)
Summary of the main systematic uncertainties and their impact on the total SM background prediction in each of the signal regions studied. A range is shown for the four bins composing SRb2 . The total systematic uncertainty can be different from the sum in quadrature of individual sources due to the correlations between them resulting from the fit to the data. The quoted theoretical uncertainties include modelling and cross-section uncertainties.
Fit results in SRb1 and SRb2 for an integrated luminosity of $36.1 fb^{-1}$. The background normalisation parameters are obtained from the background-only fit in the CRs and are applied to the SRs. Small backgrounds are indicated as Others. The dominant component of these smaller background sources in SRb1 is di-boson processes. Benchmark signal models yields are given for each SR. The uncertainties on the yields include all systematic uncertainties.
Fit results in SRt1, SRt2 and SRt3 for an integrated luminosity of $36.1 fb^{-1}$. The background normalisation parameters are obtained from the background-only fit in the CRs and are applied to the SRs. Small backgrounds are indicated as Others. Benchmark signal models yields are given for each SR. The uncertainties on the yields include all systematic uncertainties.
95% CL upper limits on the visible cross-section ($\langle\epsilon\mathcal{A}\sigma\rangle^{\rm obs}_{95}$) and on the number of BSM events ($S^{\rm obs}_{95}$ ). The third column ($S^{\rm exp}_{95}$) shows the 95% CL upper limit on the number of signal events, given the expected number (and $\pm 1\sigma$ excursions on the expectation) of background events. The last column indicates the discovery $p$-value ($p(s = 0)$) and Z (the number of equivalent Gaussian standard deviations).
Comparison of the data with the post-fit SM prediction of the $E_{\mathrm T}^{\mathrm{miss}}$ distribution in SRb1. The last bins include overflows, where applicable. All signal region requirements except the one on the distribution shown are applied. The signal region requirement on the distribution shown is indicated by an arrow. The bottom panel shows the ratio of the data over the prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit SM prediction of the $\cos{\theta}^*_{bb}$ distribution in SRb2. The last bins include overflows, where applicable. All signal region requirements except the one on the distribution shown are applied. The signal region requirement on the distribution shown is indicated by an arrow. The bottom panel shows the ratio of the data over the prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit SM prediction of the $m_{\mathrm T}^{\mathrm{b,min}}$ distribution in SRt1. The last bins include overflows, where applicable. All signal region requirements except the one on the distribution shown are applied. The signal region requirement on the distribution shown is indicated by an arrow. The bottom panel shows the ratio of the data over the prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit SM prediction of the $E_{\mathrm T}^{\mathrm{miss,sig}}$ distribution in SRt2. The last bins include overflows, where applicable. All signal region requirements except the one on the distribution shown are applied. The signal region requirement on the distribution shown is indicated by an arrow. The bottom panel shows the ratio of the data over the prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit SM prediction of the $\xi^{+}_{\ell\ell}$ distribution in SRt3. The last bins include overflows, where applicable. All signal region requirements except the one on the distribution shown are applied. The signal region requirement on the distribution shown is indicated by an arrow. The bottom panel shows the ratio of the data over the prediction. The band includes all systematic uncertainties.
Expected exclusion limits for colour-neutral scalar model in the SRb2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Observed exclusion limits for colour-neutral scalar model in SRb2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Expected exclusion limits for colour-neutral scalar model in the SRt1/SRt2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Observed exclusion limits for colour-neutral scalar model in SRt1/SRt2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Expected exclusion limits for colour-neutral scalar model in SRt3 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Observed exclusion limits for colour-neutral scalar model in SRt3 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Expected exclusion limits for colour-neutral pseudo-scalar model in SRb2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Observed exclusion limits for colour-neutral pseudo-scalar model in SRb2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Expected exclusion limits for colour-neutral pseudo-scalar model in SRt1/SRt2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Observed exclusion limits for colour-neutral pseudo-scalar model in SRt1/SRt2 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Expected limits for colour-neutral pseudo-scalar model in SRt3 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Observed exclusion limits for colour-neutral pseudo-scalar model in SRt3 as a function of the mediator mass for a DM mass of 1 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Expected exclusion limits for colour-neutral scalar model in SRt1/SRt2 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Observed exclusion limits for colour-neutral scalar model in SRt1/SRt2 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Expected exclusion limits for colour-neutral scalar model in SRt3 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Observed exclusion limits for colour-neutral scalar model in SRt3 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Expected exclusion limits for colour-neutral pseudo-scalar model in SRt1/SRt2 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Observed exclusion limits for colour-neutral pseudo-scalar model in SRt1/SRt2 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$. To derive the results for the fully hadronic $t\bar{t}$ final state the region among SRt1 and SRt2 providing the best expected sensitivity is used.
Expected exclusion limits for colour-neutral pseudo-scalar model in SRt3 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Observed xclusion limits for colour-neutral pseudo-scalar model in SRt3 as a function of the DM mass for a mediator mass of 10 GeV. The limits are calculated at 95% C.L. and are expressed in terms of the ratio of the excluded cross-section over the nominal cross-section for a coupling assumption of $g = g_\chi = g_\nu = 1$.
Comparison of the 90% CL limits on the spin-independent DM–nucleon cross-section versus mediator mass between these results and the direct-detection experiments, in the context of the colour-neutral simplified model with scalar mediator. The black line indicates the exclusion contour derived from the observed limits of SRt3. Values inside the contour are excluded.
Expected exclusion limits for colour-charged scalar mediators ($b$-FDM) as a function of the mediator and DM masses for $36.1fb^{-1}$ of data. The limits are calculated at 95% C.L for a coupling assumption $\lambda_b$ yielding the measured relic density.
Exclusion observed limits for colour-charged scalar mediators ($b-$FDM) as a function of the mediator and DM masses for $36.1fb^{-1}$ of data. The limits are calculated at 95% C.L for a coupling assumption $\lambda_b$ yielding the measured relic density.
Comparison of the data with the post-fit Monte Carlo prediction of sub leading jet $p_{T}$ in SRb1. The last bin includes overflows. The bottom panel shows the ratio of the data over the Monte Carlo prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit Monte Carlo prediction of $H_{\mathrm T}^{ratio}$ distribution in SRb2. The last bin includes overflows. The bottom panel shows the ratio of the data over the Monte Carlo prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit Monte Carlo prediction of $\Delta R_{bb}$ in SRt1. The last bin includes overflows. The bottom panel shows the ratio of the data over the Monte Carlo prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit Monte Carlo prediction of $M_{\mathrm T}^{b,min}$ in SRt2. The last bin includes overflows. The bottom panel shows the ratio of the data over the Monte Carlo prediction. The band includes all systematic uncertainties.
Comparison of the data with the post-fit Monte Carlo prediction of $\Delta \phi_{boost}$ in SRt3. The last bin includes overflows. The bottom panel shows the ratio of the data over the Monte Carlo prediction. The band includes all systematic uncertainties.
Acceptance of the SRb1 selection of the $b$-FDM model signal samples
Efficiency of the SRb1 selection of the $b$-FDM model signal samples
Acceptance of the SRb2 selection of the colour-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with bottom-quark pairs.
Efficiency of the SRb2 selection to the colour-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with bottom-quark pairs
Efficiency of the SRb2 selection to the colour-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with bottom-quark pairs
Acceptance of SRb2 selection to the colour-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with bottom-quark pairs
Acceptance of the SRt2 selections to the color-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with top quarks.
Acceptance of the SRt1 selections to the color-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with top quarks.
Efficiency of the SRt2 selections to the color-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with top quarks.
Efficiency of the SRt1 selections to the color-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with top quarks.
Acceptance of the SRt2 selections to the color-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with top quarks.
Acceptance of the SRt1 selections to the color-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with top quarks.
Efficiency of the SRt2 selections to the color-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with top quarks.
Efficiency of the SRt1 selections to the color-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with top quarks.
Acceptance of the SRt3 selections to the color-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with top quarks.
Efficiency of the SRt3 selections to the color-neutral simplified model samples with scalar mediator decaying into dark matter pairs produced in association with top quarks.
Acceptance of the SRt3 selections to the color-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with top quarks.
Efficiency of the SRt3 selections to the color-neutral simplified model samples with pseudo-scalar mediator decaying into dark matter pairs produced in association with top quarks.
Number of signal events selected at different stages of the SRb1 selections for the $b$-FDM benchmark model $m(\phi_b,\chi)=(1000,35)$GeV
Number of signal events selected at different stages of the SRb2 selections for the $b\bar{b} +\phi$ benchmark model $m(\phi,\chi)=(20,1)$GeV, $g=1$.
Number of signal events selected at different stages of the SRt1 selections for the $t \bar{t} +\phi$ benchmark model $m(\phi,\chi)=(20,1)$GeV, $g=1$.
Number of signal events selected at different stages of the SRt2 selections for the $t \bar{t} +\phi$ benchmark model $m(\phi,\chi)=(20,1)$GeV, $g=1$.
Number of signal events selected at different stages of the SRt1 selections for the $t \bar{t} +a$ benchmark model $m(a,\chi)=(20,1)$GeV, $g=1$.
Number of signal events selected at different stages of the SRt2 selections for the $t \bar{t} +a$ benchmark model $m(\phi,\chi)=(20,1)$GeV, $g=1$.
Number of signal events selected at different stages of the SRt3 selections for the $t \bar{t} +\phi$ benchmark model $m(\phi,\chi)=(20,1)$GeV, $g=1$.
A search for doubly charged Higgs bosons with pairs of prompt, isolated, highly energetic leptons with the same electric charge is presented. The search uses a proton-proton collision data sample at a centre-of-mass energy of 13 TeV corresponding to 36.1 $\mathrm{fb}^{-1}$ of integrated luminosity recorded in 2015 and 2016 by the ATLAS detector at the LHC. This analysis focuses on the decays $H^{\pm\pm}\rightarrow e^{\pm}e^{\pm}$, $H^{\pm\pm}\rightarrow e^{\pm}\mu^{\pm}$ and $H^{\pm\pm}\rightarrow \mu^{\pm}\mu^{\pm}$, fitting the dilepton mass spectra in several exclusive signal regions. No significant evidence of a signal is observed and corresponding limits on the production cross-section are derived at 95% confidence level. The observed lower limit on the mass of a doubly charged Higgs boson only coupling to left-handed leptons ($e$,$\mu$) varies from 770 GeV to 870 GeV (850 GeV expected) for $B(H^{\pm\pm}\rightarrow \ell^{\pm}\ell^{\pm})$ = 100% and both the expected and observed mass limits are above 450 GeV for $B(H^{\pm\pm}\rightarrow \ell^{\pm}\ell^{\pm})$ = 10% and any combination of partial branching ratios.
Observed and expected upper limit on the cross-section for $pp \to H^{++}H^{--}$ for a combination of partial branching ratios of $B(ee) = 100\%$, $B(e \mu ) = 0\%$, and $B( \mu \mu ) = 0\%$.
Observed and expected upper limit on the cross-section for $pp \to H^{++}H^{--}$ for a combination of partial branching ratios of $B(ee) = 0\%$, $B(e \mu ) = 0\%$, and $B( \mu \mu ) = 100\%$.
Observed and expected upper limit on the cross-section for $pp \to H^{++}H^{--}$ for a combination of partial branching ratios of $B(ee) = 0\%$, $B(e \mu ) = 100\%$, and $B( \mu \mu ) = 0\%$.
Observed and expected upper limit on the cross-section for $pp \to H^{++}H^{--}$ for a combination of partial branching ratios of $B(ee) = 30\%$, $B(e \mu ) = 40\%$, and $B( \mu \mu ) = 30\%$.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{L}^{\pm\pm} \to e^{\pm}e^{\pm})$ where $B(H_{L}^{\pm\pm} \to X) = 1 - B(H_{L}^{\pm\pm} \to e^{\pm}e^{\pm})$, with "$X$" not entering any of the signal regions.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{L}^{\pm\pm} \to \mu^{\pm}\mu^{\pm})$ where $B(H_{L}^{\pm\pm} \to X) = 1 - B(H_{L}^{\pm\pm} \to \mu^{\pm}\mu^{\pm})$, with "$X$" not entering any of the signal regions.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{L}^{\pm\pm} \to e^{\pm}\mu^{\pm})$ where $B(H_{L}^{\pm\pm} \to X) = 1 - B(H_{L}^{\pm\pm} \to e^{\pm}\mu^{\pm})$, with "$X$" not entering any of the signal regions.
Minimum observed and expected lower limit (among all partial branching ratio combinations) on the $H_{L}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{L}^{\pm\pm} \to \ell^{\pm}\ell^{\pm})$ where $B(H_{L}^{\pm\pm} \to X) = 1 - B(H_{L}^{\pm\pm} \to \ell^{\pm}\ell^{\pm})$, with "$X$" not entering any of the signal regions.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{R}^{\pm\pm} \to e^{\pm}e^{\pm})$ where $B(H_{R}^{\pm\pm} \to X) = 1 - B(H_{R}^{\pm\pm} \to e^{\pm}e^{\pm})$, with "$X$" not entering any of the signal regions.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{R}^{\pm\pm} \to \mu^{\pm}\mu^{\pm})$ where $B(H_{R}^{\pm\pm} \to X) = 1 - B(H_{R}^{\pm\pm} \to \mu^{\pm}\mu^{\pm})$, with "$X$" not entering any of the signal regions.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{R}^{\pm\pm} \to e^{\pm}\mu^{\pm})$ where $B(H_{R}^{\pm\pm} \to X) = 1 - B(H_{R}^{\pm\pm} \to e^{\pm}\mu^{\pm})$, with "$X$" not entering any of the signal regions.
Minimum observed and expected lower limit (among all partial branching ratio combinations) on the $H_{R}^{\pm\pm}$ boson mass as a function of the branching ratio $B(H_{R}^{\pm\pm} \to \ell^{\pm}\ell^{\pm})$ where $B(H_{R}^{\pm\pm} \to X) = 1 - B(H_{R}^{\pm\pm} \to \ell^{\pm}\ell^{\pm})$, with "$X$" not entering any of the signal regions.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 100%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 100%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 90%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 90%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 80%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 80%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 70%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 70%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 60%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 60%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 50%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 50%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 40%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 40%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 30%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 30%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 20%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 20%.
Observed and expected lower limit on the $H_{L}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 10%.
Observed and expected lower limit on the $H_{R}^{\pm\pm}$ boson mass for all branching ratio combinations ($B(ee)$,$B(e\mu)$,$B(\mu\mu)$) that sum to 10%.
This Letter presents the measurement of differential cross sections of isolated prompt photons produced in association with a b-jet or a c-jet. These final states provide sensitivity to the heavy-flavour content of the proton and aspects related to the modelling of heavy-flavour quarks in perturbative QCD. The measurement uses proton-proton collision data at a centre-of-mass energy of 8 TeV recorded by the ATLAS detector at the LHC in 2012 corresponding to an integrated luminosity of up to 20.2 fb$^{-1}$. The differential cross sections are measured for each jet flavour with respect to the transverse energy of the leading photon in two photon pseudorapidity regions: $|\eta^\gamma|<1.37$ and $1.56<|\eta^\gamma|<2.37$. The measurement covers photon transverse energies $25 < E_\textrm{T}^\gamma<400$ GeV and $25 < E_\textrm{T}^\gamma<350$ GeV respectively for the two $|\eta^\gamma|$ regions. For each jet flavour, the ratio of the cross sections in the two $|\eta^\gamma|$ regions is also measured. The measurement is corrected for detector effects and compared to leading-order and next-to-leading-order perturbative QCD calculations, based on various treatments and assumptions about the heavy-flavour content of the proton. Overall, the predictions agree well with the measurement, but some deviations are observed at high photon transverse energies. The total uncertainty in the measurement ranges between 13% and 66%, while the central $\gamma+b$ measurement exhibits the smallest uncertainty, ranging from 13% to 27%, which is comparable to the precision of the theoretical predictions.
Measured fiducial integrated $\gamma+b$ and $\gamma+c$ cross sections for $|\eta^\gamma|<1.37$ and $1.56<|\eta^\gamma|<2.37$.
Measured $\gamma+b$ fiducial differential cross section as a function of $E_\text{T}^\gamma$ for $|\eta^\gamma|<1.37$.
Measured $\gamma+b$ fiducial differential cross section as a function of $E_\text{T}^\gamma$ for $1.56<|\eta^\gamma|<2.37$.
Measured $\gamma+c$ fiducial differential cross section as a function of $E_\text{T}^\gamma$ for $|\eta^\gamma|<1.37$.
Measured $\gamma+c$ fiducial differential cross section as a function of $E_\text{T}^\gamma$ for $1.56<|\eta^\gamma|<2.37$.
Measured ratio of the $\gamma+b$ fiducial differential cross section as a function of $E_\text{T}^\gamma$ for $|\eta^\gamma|<1.37$ to that for $1.56<|\eta^\gamma|<2.37$.
Measured ratio of the $\gamma+c$ fiducial differential cross section as a function of $E_\text{T}^\gamma$ for $|\eta^\gamma|<1.37$ to that for $1.56<|\eta^\gamma|<2.37$.
Statistical correlation between the $\gamma+b$ and the $\gamma+c$ cross sections in a given $E_\text{T}^\gamma$ bin and $|\eta^\gamma|$ region. The two cross sections are correlated as the heavy flavour fractions are extracted simultaneously from a template fit, performed in each $E_\text{T}^\gamma$ bin and separately for the two $|\eta^\gamma|$ regions.
Signed shifts of the individual systematic uncertainties on the $\gamma+b$ cross section for $|\eta^\gamma|<1.37$. The numbers after the name of the uncertainty source refer to the individual component in that uncertainty. Each bin of the MC statistical uncertainty is independent of any other bin. The first four components of the photon energy scale uncertainty are specific to this $|\eta^\gamma|$ region and are independent of the components in the other region. The region is indicated as part of their name to indicate the independence between the $|\eta^\gamma|$ regions. The uncertainties on the prompt photon modelling, non-perturbative QCD models and particle-level migration effects are only varied once and not up and down by their nature, but are symmetrised for the final results. Only uncertainties which have at least a 1% variation in at least one bin of the $\gamma+b$ and $\gamma+c$ cross section measurements, including the ratios, are listed. The others are summed in quadrature and listed as a single entry.
Signed shifts of the individual systematic uncertainties on the $\gamma+b$ cross section for $1.56<|\eta^\gamma|<2.37$. The numbers after the name of the uncertainty source refer to the individual component in that uncertainty. Each bin of the MC statistical uncertainty is independent of any other bin. The first four components of the photon energy scale uncertainty are specific to this $|\eta^\gamma|$ region and are independent of the components in the other region. The region is indicated as part of their name to indicate the independence between the $|\eta^\gamma|$ regions. The uncertainties on the prompt photon modelling, non-perturbative QCD models and particle-level migration effects are only varied once and not up and down by their nature, but are symmetrised for the final results. Only uncertainties which have at least a 1% variation in at least one bin of the $\gamma+b$ and $\gamma+c$ cross section measurements, including the ratios, are listed. The others are summed in quadrature and listed as a single entry.
Signed shifts of the individual systematic uncertainties on the $\gamma+c$ cross section for $|\eta^\gamma|<1.37$. The numbers after the name of the uncertainty source refer to the individual component in that uncertainty. Each bin of the MC statistical uncertainty is independent of any other bin. The first four components of the photon energy scale uncertainty are specific to this $|\eta^\gamma|$ region and are independent of the components in the other region. The region is indicated as part of their name to indicate the independence between the $|\eta^\gamma|$ regions. The uncertainties on the prompt photon modelling, non-perturbative QCD models and particle-level migration effects are only varied once and not up and down by their nature, but are symmetrised for the final results. Only uncertainties which have at least a 1% variation in at least one bin of the $\gamma+b$ and $\gamma+c$ cross section measurements, including the ratios, are listed. The others are summed in quadrature and listed as a single entry.
Signed shifts of the individual systematic uncertainties on the $\gamma+c$ cross section for $1.56<|\eta^\gamma|<2.37$. The numbers after the name of the uncertainty source refer to the individual component in that uncertainty. Each bin of the MC statistical uncertainty is independent of any other bin. The first four components of the photon energy scale uncertainty are specific to this $|\eta^\gamma|$ region and are independent of the components in the other region. The region is indicated as part of their name to indicate the independence between the $|\eta^\gamma|$ regions. The uncertainties on the prompt photon modelling, non-perturbative QCD models and particle-level migration effects are only varied once and not up and down by their nature, but are symmetrised for the final results. Only uncertainties which have at least a 1% variation in at least one bin of the $\gamma+b$ and $\gamma+c$ cross section measurements, including the ratios, are listed. The others are summed in quadrature and listed as a single entry.
A search for massive coloured resonances which are pair-produced and decay into two jets is presented. The analysis uses 36.7 fb$^{-1}$ of $\sqrt{s}=$ 13 TeV pp collision data recorded by the ATLAS experiment at the LHC in 2015 and 2016. No significant deviation from the background prediction is observed. Results are interpreted in a SUSY simplified model where the lightest supersymmetric particle is the top squark, $\tilde{t}$, which decays promptly into two quarks through $R$-parity-violating couplings. Top squarks with masses in the range 100 GeV < $m_{\tilde{t}}$ < 410 GeV are excluded at 95% confidence level. If the decay is into a $b$-quark and a light quark, a dedicated selection requiring two $b$-tags is used to exclude masses in the ranges 100 GeV < $m_{\tilde{t}}$ < 470 GeV and 480 GeV < $m_{\tilde{t}}$ < 610 GeV. Additional limits are set on the pair-production of massive colour-octet resonances.
- - - - - - - - - - - - - - - - - - - - <p><b>Cutflows:</b><br> <a href="79059?version=1&table=CutflowTable1">Stop 100GeV</a><br> <a href="79059?version=1&table=CutflowTable2">Stop 500GeV</a><br> <a href="79059?version=1&table=CutflowTable3">Coloron 1500GeV</a><br> </p> <p><b>Event Yields:</b><br> <a href="79059?version=1&table=SRdistribution1">Inclusive stop SR</a><br> <a href="79059?version=1&table=SRdistribution2">Inclusive coloron SR </a><br> <a href="79059?version=1&table=SRdistribution3">b-tagged stop SR</a><br> </p> <p><b>Acceptances and Efficiencies:</b><br> <a href="79059?version=1&table=Acceptance1">Inclusive stop SR, before mass window</a><br> <a href="79059?version=1&table=Acceptance2">Inclusive stop SR, after mass window</a><br> <a href="79059?version=1&table=Acceptance3">Inclusive coloron SR, before mass window</a><br> <a href="79059?version=1&table=Acceptance4">Inclusive coloron SR, after mass window</a><br> <a href="79059?version=1&table=Acceptance5">b-tagged stop SR, before mass window</a><br> <a href="79059?version=1&table=Acceptance6">b-tagged stop SR, after mass window</a><br> </p> <p><b>Cross section upper limits:</b><br> <a href="79059?version=1&table=Limitoncrosssection1">Inclusive stop SR</a><br> <a href="79059?version=1&table=Limitoncrosssection2">Inclusive coloron SR</a><br> <a href="79059?version=1&table=Limitoncrosssection3">b-tagged stop SR</a><br> </p> <p><b>Truth Code</b> and <b>SLHA Files</b> for the cutflows are available under "Resources" (purple button on the left) </p>
Cutflow table for a pair produced top squark of 100 GeV decaying into a b- and an s-quark.
Cutflow table for a pair produced top squark of 500 GeV decaying into a b- and an s-quark.
Cutflow table for a pair produced coloron of 1500 GeV decaying into two quarks.
The observed number of data, background and top squark signal events in each of the signal regions of the inclusive selection
The observed number of data, background and coloron signal events in each of the signal regions of the inclusive selection
The observed number of data, background and top squark signal events in each of the signal regions of the b-tagged selection
Signal acceptance and efficiency (in %) as a function of M(STOP), before mass windows
Signal acceptance (in %) and efficiency as a function of M(STOP), after mass windows
Signal acceptance and efficiency (in %) as a function of M(RHO), before mass windows
Signal acceptance and efficiency (in %) as a function of M(RHO), after mass windows
Signal acceptance (in %) and efficiency as a function of M(STOP), before mass windows
Signal acceptance (in %) and efficiency as a function of M(STOP), after mass windows
Cross section excluded at 95% CL as a function of the top squark mass, for a pair produced top squark with decays into a pair of light-quarks.
Cross section excluded at 95% CL as a function of the cooron mass, for a pair produced coloron with decays into a pair of light-quarks.
Cross section excluded at 95% CL as a function of the top squark mass, for a pair produced top squark with decays into a b- and an s-quark.
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