stop mass in the Tstop3 and Tstop10 simplified models, see their Figures 7 and 8. A combination of this search with the all-hadronic search is presented in Figure 9.

40 SIRUNYAN 18DN searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for direct electroweak production of charginos and for pair production of top squarks in events with two leptons (electrons or muons) of the opposite electric charge. No significant excess above the Standard Model expectations is observed. Limits are set on the chargino mass in the Tchiichi1C and TchiichiE simplified models, see their Figure 8. Limits are also set on the stop mass in the Tstop1 and Tstop2 simplified models, see their Figure 9.

41 AABOUD 17Aj searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 700 GeV are set on the top squark mass in Tstop11 simplified models, assuming $m_{\tilde{\chi}_1^0} = m_{\tilde{\tau}_1} - 275$ GeV and $m_{\tilde{\chi}_2^0} = m_{\tilde{\chi}_1^0} + 100$ GeV. See their Figure 4(e).

42 AABOUD 17AX searched in 36 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events containing two jets identified as originating from b-quarks and large missing transverse momentum, with or without leptons. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set on the masses of top squarks. Assuming 50% BR for Tstop1 and Tstop2 simplified models, a $\tilde{t}_1$ mass below 880 (860) GeV is excluded for $m_{\tilde{\chi}_1^0} = 0$ (<250) GeV. See their Fig. 7(b).

43 AABOUD 17AY searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with at least four jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits in the range 250–1000 GeV are set on the top squark mass in Tstop1 simplified models. For the first time, additional constraints are set for the region $m_{\tilde{\tau}_1} \sim m_t + m_{\tilde{\chi}_1^0}$, with exclusion of the $\tilde{t}_1$ mass range 235–590 GeV. See their Figure 8.

44 AABOUD 17AY searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with at least four jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits in the range 450–850 GeV are set on the top squark mass in a mixture of Tstop1 and Tstop2 simplified models with BR=50% and assuming $m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_0} = 1$ GeV and $m_{\tilde{\chi}_1^0} < 240$ GeV. Constraints are given for various values of the BR. See their Figure 9.

45 AABOUD 17BE searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two opposite-charge leptons (electrons and muons) and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 720 GeV are set on the top squark mass in Tstop1 simplified models, assuming massless neutralinos. See their Figure 9 (2-body area).

46 AABOUD 17BE searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two opposite-charge leptons (electrons and muons) and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 400 GeV are set on the top squark mass in Tstop3 simplified models, assuming $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0} = 40$ GeV. See their Figure 9 (4-body area).

47 AABOUD 17BE searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two opposite-charge leptons (electrons and muons) and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 430 GeV are set on the top squark mass in Tstop1 simplified models where top quarks are offshell, assuming $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ close to the W mass. See their Figure 9 (3-body area).

48 AABOUD 17BE searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two opposite-charge leptons (electrons and muons) and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 700 GeV are set on the top squark mass in Tstop2 simplified models, assuming $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^\pm} = 10$ GeV and massless neutralinos. See their Figure 10.

49 KHACHATRYAN 17 searched in 2.3 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events containing four or more jets, no more than one lepton, and missing transverse momentum, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the stop mass in the Tstop1 simplified model, see Fig. 17.
50 KHACHATRYAN 17AD searched in 2.3 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events containing at least four jets (including b-jets), missing transverse momentum and tagged top quarks. No evidence for an excess over the expected background is observed. Top squark masses in the range 250–740 GeV and neutralino masses up to 240 GeV are excluded at 95% C.L. See Fig. 12.

51 KHACHATRYAN 17AD searched in 2.3 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events containing at least four jets (including b-jets), missing transverse momentum and tagged top quarks. No evidence for an excess over the expected background is observed. Limits are derived on the $\tilde{\tau}$ mass in simplified models that are a mixture of Tstop1 and Tstop2 with branching fractions 50% for each of the two decay modes: top squark masses of up to 610 GeV and neutralino masses up to 190 GeV are excluded at 95% C.L. The $\tilde{\chi}_1^\pm$ and the $\tilde{\chi}_1^0$ are assumed to be nearly degenerate in mass, with a 5 GeV difference between their masses. See Fig. 12.

52 KHACHATRYAN 17P searched in 2.3 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with one or more jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A, Tglu3A, Tglu3B, Tglu3C and Tglu3D simplified models, see their Figures 7 and 8. Limits are also set on the squark mass in the Tsqk1 simplified model, see their Fig. 7, and on the bottom mass in the Tsbot1 simplified model, see Fig. 8. Finally, limits are set on the stop mass in the Tstop1, Tstop3, Tstop4, Tstop6 and Tstop7 simplified models, see Fig. 8.

53 KHACHATRYAN 17S searched in 18.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing multiple jets and missing transverse momentum, using the $\alpha_T$ variable to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the stop mass in the Tstop4 model: for $\Delta m = m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ equal to 10 and 80 GeV, masses of stop below 240 and 260 GeV are excluded, respectively. See their Fig. 3.

55 KHACHATRYAN 17S searched in 18.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing multiple jets and missing transverse momentum, using the $\alpha_T$ variable to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the stop mass in the Tstop2 model: assuming $m_{\tilde{\chi}_1^\pm} = 0.25 m_{\tilde{\tau}_1} + 0.75 m_{\tilde{\chi}_1^0}$, masses of stop up to 325 GeV and masses of the neutralino up to 225 GeV are excluded. See their Fig. 3.

56 KHACHATRYAN 17S searched in 18.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing multiple jets and missing transverse momentum, using the $\alpha_T$ variable to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the stop mass in the Tstop2 model: assuming $m_{\tilde{\chi}_1^\pm} = 0.75 m_{\tilde{\tau}_1} + 0.25 m_{\tilde{\chi}_1^0}$, masses of stop up to 400 GeV are excluded for low neutralino masses. See their Fig. 3.

57 KHACHATRYAN 17S searched in 18.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing multiple jets and missing transverse momentum, using the $\alpha_T$ variable to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the stop mass in the Tstop1 model: assuming masses of stop up to 500 GeV and masses of the neutralino up to 105 GeV are excluded. See their Fig. 3.

58 SIRUNYAN 17AS searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with a single lepton (electron or muon), jets, and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1, Tstop2 and Tstop8 simplified models, see their Figures 5, 6 and 7.

59 SIRUNYAN 17AT searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for direct production of top squarks in events with jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1, Tstop2, Tstop3, Tstop4, Tstop8 and Tstop10 simplified models, see their Figures 9 to 14.

60 SIRUNYAN 17AZ searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with one or more jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A, Tglu3A simplified models, see their Figures 6. Limits are also set on the squark mass in the Tsqk1 simplified model (for single light squark and for 8 degenerate light squarks), on the bottom mass in the Tstbot1 simplified model and on the stop mass in the Tstop1 simplified model, see their Fig. 7. Finally, limits are set on the stop mass in the Tstop2, Tstop4 and Tstop8 simplified models, see Fig. 8.

61 SIRUNYAN 17K searched in 2.3 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for direct production of stop or bottom pairs in events with multiple jets and significant $E_T$. A second search also requires an isolated lepton and is combined with the all-hadronic search. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1, Tstop8 and Tstop4 simplified models, see their Figures 7, 8 and 9 (for the Tstop4 limits, only the results of the all-hadronic search are used). Limits are also set on the bottom mass in the Tstbot1 simplified model, see Fig. 10 (also here, only the results of the all-hadronic search are used).

62 SIRUNYAN 17P searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with multiple jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu1C, Tglu2A, Tglu3A and Tglu3D simplified models, see their Fig. 12. Limits are also set on the squark mass in the Tsqk1 simplified model, on the stop mass in the Tstop1 simplified model, and on the bottom mass in the Tstbot1 simplified model, see Fig. 13.

63 AABOUD 16D searched in 3.2 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV in events with an energetic jet and large missing transverse momentum. The results are interpreted as 95% C.L. limits on mass of stop decaying into a charm-quark and the lightest neutralino in scenarios with $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ between 5 and 20 GeV. See their Fig. 5.

64 AABOUD 16J searched in 3.2 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV in final states with one isolated electron or muon, jets, and missing transverse momentum. For the direct stop pair production model where the stop decays via top and lightest neutralino, the results exclude at 95% C.L. stop masses between 745 GeV and 780 GeV for a massless $\tilde{\chi}_1^0$. See their Fig. 8.

65 AAD 16AY searched in 20 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with either two hadronically decaying tau leptons, one hadronically decaying via a light and one light lepton, or two light leptons. No significant excess over the Standard Model expectation is found. Exclusion limits at 95% C.L. on the mass of top squarks decaying via $\tilde{\tau}$ to a nearly massless gravitino are placed depending on $m_{\tilde{\tau}}$ which is ranging from the 87 GeV LEP limit to $m_{\tilde{\tau}_1}$. See their Figs. 9 and 10.

66 KHACHATRYAN 16AV searched in 19.7 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with one or two isolated leptons, hadronic jets, b-jets and $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1 and Tstop2 simplified models, see Fig. 11.

67 KHACHATRYAN 16BK searched in 18.9 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with hadronic jets and $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1 and Tstop2 simplified models, see Fig. 16.

68 KHACHATRYAN 16BS searched in 2.3 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with at least one energetic jet, no isolated leptons, and significant $E_T$, using the transverse mass variable $M_{T2}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1 simplified model, see Fig. 11 and Table 3.

69 KHACHATRYAN 16Y searched in 19.7 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with one or two soft isolated leptons, hadronic jets, and $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop3 simplified model, see Fig. 3.

70 AAD 15CJ searched in 20 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for evidence of third generation squarks by combining a large number of searches covering various final states. Stop decays with and without charginos in the decay chain are considered and summaries of all ATLAS Run 1 searches for direct stop production can be found in Fig. 4 (no intermediate charginos) and Fig. 7 (intermediate charginos). Limits are set on stop masses in compressed mass regions regions, with $B(\tilde{t} \to c\tilde{\chi}_1^0) + B(\tilde{t} \to bff'\tilde{\chi}_1^0) = 1$, see Fig. 5. Limits are also set on stop masses assuming that both the decay $t \to t\tilde{\chi}_1^0$ and $t \to b\tilde{\chi}_1^\pm$ are possible, with both their branching ratios summing up to 1, assuming $\tilde{\chi}_1^\pm \to W^*(\tilde{\chi}_1^0)$ and $m_{\tilde{\chi}_1^\pm} = 2 m_{\tilde{\chi}_1^0}$, see Fig. 6. Limits on the mass of the next-to-lightest stop $\tilde{t}_2$, decaying either to $Z\tilde{\tau}_1$, $h\tilde{\tau}_1$ or $t\tilde{\chi}_1^0$, are also presented, see Figs. 9 and 10. Interpretations in the pMSSM are also discussed, see Figs. 13–15.
71 AAD 15j interpreted the measurement of spin correlations in $t\bar{t}$ production using 20.3 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV in exclusion limits on the pair production of light $\tilde{t}_1$ squarks with masses similar to the top quark mass. The $\tilde{t}_1$ is assumed to decay through $\tilde{t}_1 \to t\tilde{\chi}_0^1$ with predominantly right-handed top and a 100% branching ratio. The data are found to be consistent with the Standard Model expectations and masses between the top quark mass and 191 GeV are excluded, see their Fig. 2.

72 KHACHATRYAN 15AF searched in 19.5 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events with at least two energetic jets and significant $E_T$, using the transverse mass variable $M_{T2}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in simplified models where the decay $\tilde{t} \to t\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, see Fig. 12. See also Table 5. Exclusions in the CMSSM, assuming $\tan\beta = 30$, $A_0 = -2 \max(m_0, m_{1/2})$ and $\mu > 0$, are also presented, see Fig. 15.

73 KHACHATRYAN 15AH searched in 19.4 or 19.7 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events containing either a fully reconstructed top quark, or events containing dijets requiring one or both jets to originate from b-quarks, or events containing a mono-jet. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in simplified models where the decay $\tilde{t} \to t\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, see Fig. 9. Limits are also set in simplified models where the decays $\tilde{t} \to t\tilde{\chi}_0^1$ and $\tilde{t} \to b\tilde{\chi}_1^-$, with $m_{\tilde{\chi}_1^-} - m_{\tilde{\chi}_1^0} = 5$ GeV, each take place with a branching ratio of 50%, see Fig. 10, or with other fractions, see Fig. 11. Finally, limits are set in a simplified model where the decay $\tilde{t} \to c\tilde{\chi}_1^0$ takes place with a branching ratio of 100%, see Figs. 9, 10 and 11.

74 KHACHATRYAN 15AH searched in 19.4 or 19.7 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events containing either a fully reconstructed top quark, or events containing dijets requiring one or both jets to originate from b-quarks, or events containing a mono-jet. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in simplified models where the decay $\tilde{t} \to t\tilde{\chi}_1^0$ takes place with a branching ratio of 100%, see Fig. 9. Limits are also set in simplified models where the decays $\tilde{t} \to t\tilde{\chi}_0^1$ and $\tilde{t} \to b\tilde{\chi}_1^+$, with $m_{\tilde{\chi}_1^-} - m_{\tilde{\chi}_1^0} = 5$ GeV, each take place with a branching ratio of 50%, see Fig. 10, or with other fractions, see Fig. 11. Finally, limits are set in a simplified model where the decay $\tilde{t} \to c\tilde{\chi}_1^0$ takes place with a branching ratio of 100%, see Figs. 9, 10, and 11.

75 KHACHATRYAN 15x searched in 19.3 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events with at least two energetic jets, at least one of which is required to originate from a b quark, possibly a lepton, and significant $E_T$, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in simplified models where the decay $\tilde{t} \to t\tilde{\chi}_1^0$ and the decay $\tilde{t} \to b\tilde{\chi}_1^+$, with $m_{\tilde{\chi}_1^+} - m_{\tilde{\chi}_1^0} = 5$ GeV, take place with branching ratios varying between 0 and 100%, see Figs. 15, 16 and 17.

76 AAD 14AJ searched in 20.1 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events containing four or more jets and large missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set on the masses of third-generation squarks in simplified models which either assume that the decay $\tilde{t}_1 \to t\tilde{\chi}_0^1$ takes place 100% of the time, see Fig. 8, or that this decay takes place 50% of the time, while the decay $\tilde{t}_1 \to b\tilde{\chi}_1^+$ takes place the other 50% of the time, see Fig. 9.

77 AAD 14BD searched in 20 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events containing one isolated lepton, jets and large missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set on the masses of third-generation squarks in simplified models which either assume that the decay $\tilde{t}_1 \to t\tilde{\chi}_0^1$ takes place 100% of the time, see Fig. 15, or the decay $\tilde{t}_1 \to b\tilde{\chi}_1^+$ takes place 100% of the time, see Fig. 16–22. For the mixed decay scenario, see Fig. 23.

78 AAD 14F searched in 20.3 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events containing two leptons (e or $\mu$), and possibly jets and missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set on the masses of third-generation squarks in simplified models which either assume that the decay $\tilde{t}_1 \to b\tilde{\chi}_1^+$ takes place 100% of the time, see Figs. 14–17 and 20, or that the decay $\tilde{t}_1 \to t\tilde{\chi}_0^1$ takes place 100% of the time, see Figs. 18 and 19.

79 AAD 14T searched in 20.3 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for monojet-like and c-tagged events. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set on the masses of third-generation squarks in simplified models which assume that the decay $\tilde{t}_1 \to c\tilde{\chi}_1^0$ takes place 100% of the time, see Fig. 9 and 10. The results of the monojet-like analysis are also interpreted in terms of stop pair production in the four-body decay $\tilde{t}_1 \to b\tilde{t}t'\tilde{\chi}_1^0$, see Fig. 11.

80 CHATRCHYAN 14AH searched in 4.7 fb$^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with at least two energetic jets and significant $E_T$, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. A second analysis requires at least one of the jets to be originating from a b-quark. No significant excess above the Standard Model expectations is observed. Limits are set on bottom masses in simplified models where the decay $\tilde{t} \to t\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, see Figs. 28 and 29. Exclusions in the CMSSM, assuming $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, are also presented, see Fig. 26.

81 CHATRCHYAN 14R searched in 19.5 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events with at least three leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in a natural higgsino NLSP simplified model (GMSB) where the decay $\tilde{t} \to b\tilde{\chi}_1^+$, with $\tilde{\chi}_1^+ \to (qq'/\ell\nu)H$, $Z\tilde{G}$, takes place with a branching ratio of 100% (the particles between brackets have a soft $p_T$ spectrum), see Figs. 4–6.

82 AABOUD 17AF searched in 36 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for evidence of top squarks in events containing 2 leptons, jets, b-jets and $E_T$. In Tstop6 model, assuming $m_{\tilde{\chi}_1^0} = 0$ GeV, $\tilde{t}_1$ masses up to 850 GeV are excluded for $m_{\tilde{\chi}_2^0} > 200$ GeV.

83 AABOUD 17AF searched in 36 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for evidence of $\tilde{t}_2$ in events containing 2 leptons, jets, b-jets and $E_T$. In Tstop7 model, assuming $m_{\tilde{\chi}_1^0} = 50$ GeV and 100% decays via Z boson, $\tilde{t}_2$ masses up to 800 GeV are excluded. Exclusion limits are also shown as a function of the $\tilde{t}_2$ branching ratios in their Figure 7.

84 AABOUD 17AF searched in 36 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for evidence of $\tilde{t}_2$ in events containing 2 leptons, jets, b-jets and $E_T$. In Tstop7 model, assuming $m_{\tilde{\chi}_1^0} = 50$ GeV and 100% decays via higgs boson, $\tilde{t}_2$ masses up to 880 GeV are excluded. Exclusion limits are also shown as a function of the $\tilde{t}_2$ branching ratios in their Figure 7.

85 AABOUD 17AY searched in 36.1 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for events with at least four jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the top quark mass assuming three pMSSM-inspired models. The first one, referred to as Higgsino LSP model, assumes $m_{\tilde{\chi}_1^-} - m_{\tilde{\chi}_1^0} = 5$ GeV and $m_{\tilde{\chi}_2^-} - m_{\tilde{\chi}_1^0} = 10$ GeV, with a mixture of decay modes as in Tstop1, Tstop2 and Tstop6. See their Figure 10. The second and third models are referred to as Wino NLSP and well-tempered pMSSM models, respectively. See their Figure 11 and Figure 12, and text for details on assumptions.

86 AAD 14B searched in 20.3 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events containing a Z boson, with or without additional leptons, plus jets originating from b-quarks and significant missing transverse momentum. No excess over the expected SM background is observed. Limits are derived in simplified models featuring $\tilde{t}_2$ production, with $\tilde{t}_2 \to Z\tilde{t}_1$, $\tilde{t}_1 \to t\tilde{\chi}_1^0$ with a 100% branching ratio, see Fig. 4, and in the framework of natural GMSB, see Fig. 6.

87 CHATRCHYAN 14U searched in 19.7 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for evidence of direct pair production of top squarks, with Higgs bosons in the decay chain. The search is performed using a selection of events containing two Higgs bosons, each decaying to a photon pair, missing transverse energy and possibly b-quark jets. No significant excesses over the expected SM backgrounds are observed. The results are interpreted in the context of a “natural SUSY” simplified model where the decays $\tilde{t}_1 \to b\tilde{\chi}_1^+$, with $\tilde{\chi}_1^+ \to f\ell'\tilde{\chi}_1^0$, and $\tilde{\chi}_1^0 \to H\tilde{G}$, all happen with 100% branching ratio, see Fig. 4.

88 KHACHATRYAN 14C searched in 19.5 fb$^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for evidence of direct pair production of top squarks, with Higgs or Z-bosons in the decay chain. The search is performed using a selection of events containing leptons and b-quark jets. No significant excesses over the expected SM backgrounds are observed. The results are interpreted in the context of a simplified model with pair production of a heavier top-quark mass eigenstate $\tilde{t}_2$ decaying to a lighter top-quark eigenstate $\tilde{t}_1$ via either $\tilde{t}_2 \to H\tilde{t}_1$ or $\tilde{t}_2 \to Z\tilde{t}_1$, followed in both cases by $\tilde{t}_1 \to t\tilde{\chi}_1^0$. The interpretation is performed in the region where the mass difference between the $\tilde{t}_1$ and $\tilde{\chi}_1^0$ is approximately equal to the top-quark mass, which is not probed by searches for direct $\tilde{t}_1$ pair production, see Figs. 5 and 6. The analysis excludes top squarks with masses $m_{\tilde{t}_2} < 575$ GeV and $m_{\tilde{t}_1} < 400$ GeV at 95% C.L.

## R-parity violating $\tilde{t}$ (Stop) mass limit

<table><thead><tr><th>VALUE (GeV)</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>none 500-520,<br>580-770</td><td>95</td><td>1 TUMASYAN</td><td>23L CMS</td><td>4 jets with dijet masses &gt; 350 GeV, Tstop1aRPV</td></tr><tr><td>&gt;1500</td><td>95</td><td>2 TUMASYAN</td><td>22AF CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to b\tilde{t}$, $\tau_c = 2$ cm</td></tr><tr><td>&gt;1500</td><td>95</td><td>2 TUMASYAN</td><td>22AF CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to d\tilde{t}$, $\tau_c = 2$ cm</td></tr><tr><td>&gt; 460</td><td>95</td><td>2 TUMASYAN</td><td>22AF CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to b\tilde{t}$, 0.01cm &lt; $\tau_c &lt; 1000$ cm</td></tr><tr><td>&gt; 460</td><td>95</td><td>2 TUMASYAN</td><td>22AF CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to d\tilde{t}$, 0.01cm &lt; $\tau_c &lt; 1000$ cm</td></tr><tr><td>&gt;1100</td><td>95</td><td>3 AAD</td><td>21BF ATLS</td><td>$\ell^\pm + b$-jets + many jets, Tstop14, $\lambda_{323}^3$ electroweakino decay, 500 GeV &lt; $m_{\tilde{\chi}_1^0} &lt; 800$ GeV</td></tr><tr><td>&gt;1150</td><td>95</td><td>3 AAD</td><td>21BF ATLS</td><td>$\ell^\pm + b$-jets + many jets, Tstop15, $\lambda_{323}^3$ electroweakino decay, 600 GeV &lt; $m_{\tilde{\chi}_1^0} &lt; 900$ GeV</td></tr><tr><td>&gt;1300</td><td>95</td><td>3 AAD</td><td>21BF ATLS</td><td>$\ell^\pm + b$-jets + many jets, Tstop1, $\lambda_{323}^3$, electroweakino decay, 500 GeV &lt; $m_{\tilde{\chi}_1^0} &lt; 1000$ GeV</td></tr><tr><td>&gt;1600</td><td>95</td><td>4 SIRUNYAN</td><td>21AF CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to d\tilde{d}$, $\lambda_{3i3}^2$ coupling, 0.4 mm &lt; $\tau_c &lt; 80$ mm</td></tr><tr><td>&gt;1600</td><td>95</td><td>5 SIRUNYAN</td><td>21U CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to b\tilde{t}$, 5 &lt; $\tau_c &lt; 240$ mm</td></tr><tr><td>&gt;1600</td><td>95</td><td>5 SIRUNYAN</td><td>21U CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to d\tilde{t}$, $\lambda_{3i1}^2$ coupling, 3 &lt; $\tau_c &lt; 360$ mm</td></tr><tr><td>&gt;1600</td><td>95</td><td>5 SIRUNYAN</td><td>21U CMS</td><td>long-lived $\tilde{t}$, $\tilde{t} \to d\tilde{d}$, $\lambda_{3ii1}^2$ coupling, 2 &lt; $\tau_c &lt; 1320$ mm</td></tr><tr><td>&gt; 670</td><td>95</td><td>6 SIRUNYAN</td><td>21V CMS</td><td>$\ell^\pm + \ge 7$ jets, Tstop1 with $\tilde{\chi}_1^0 \to q\bar{q}$, $\lambda_{abc}''^2$ coupling, a,b,c $\in 1,2$</td></tr><tr><td>&gt; 870</td><td>95</td><td>6 SIRUNYAN</td><td>21V CMS</td><td>$\ell^\pm + \ge 7$ jets, stealth SYY model</td></tr><tr><td>&gt;1700</td><td>95</td><td>7 AAD</td><td>20M ATLS</td><td>$\tilde{t} \to q\mu$, long-lived, Tstop3RPV, $\tau = 0.1$ ns</td></tr><tr><td>&gt;1150</td><td>95</td><td>8 SIRUNYAN</td><td>19BI ATLS</td><td>$\tilde{t} \to b\mu$, long-lived, Tstop2RPV, $\tau_c = 0.1$ cm</td></tr><tr><td>&gt;1100</td><td>95</td><td>9 SIRUNYAN</td><td>19BJ CMS</td><td>$\tilde{t} \to b\bar{e}$, Tstop2RPV, prompt $\tilde{t} \to d\bar{s}$, $\lambda_{3i1}^2$ coupling</td></tr><tr><td>none 100-410</td><td>95</td><td>10 AABOUD</td><td>18BB ATLS</td><td>4 jets, Tstop1RPV with $\tilde{t} \to d\bar{s}$, $\lambda_{3i1}^2$ coupling</td></tr></tbody></table>
<table><tbody><tr><td>none 100-470, 480-610</td><td>95</td><td>11 AABOUD</td><td>18BB ATLS</td><td>4 jets, Tstop1RPV, λ''<sub>323</sub> coupling</td></tr><tr><td>≥ 600-1500</td><td>95</td><td>12 AABOUD</td><td>18P ATLS</td><td>2ℓ + b-jets, Tstop2RPV, depending on λ''<sub>333</sub> coupling (i = 1, 2, 3)</td></tr><tr><td>>1130</td><td>95</td><td>13 SIRUNYAN</td><td>18AD CMS</td><td>˜t → bℓ, long-lived, cτ = 70-100 mm</td></tr><tr><td>> 550</td><td>95</td><td>13 SIRUNYAN</td><td>18AD CMS</td><td>˜t → bℓ, long-lived, cτ = 1-1000 mm</td></tr><tr><td>>1400</td><td>95</td><td>14 SIRUNYAN</td><td>18DV CMS</td><td>long-lived t, t → d<span style="text-decoration: overline">d</span>, 0.6 mm &lt; cτ &lt; 80 mm</td></tr><tr><td>none 80-520</td><td>95</td><td>15 SIRUNYAN</td><td>18DY CMS</td><td>2, 4 jets, Tstop3RPV, λ''<sub>312</sub> coupling</td></tr><tr><td>none 80-270, 285-340, 400-525</td><td>95</td><td>15 SIRUNYAN</td><td>18DY CMS</td><td>2, 4 jets, Tstop1RPV, λ''<sub>323</sub> coupling</td></tr><tr><td>>1200</td><td>95</td><td>16 AABOUD</td><td>17AI ATLS</td><td>≥ 1ℓ+ ≥ 8 jets, Tstop1 with λ''<sub>1</sub> → tbs, λ''<sub>323</sub> coupling, m<sub>1</sub><sup>0</sup> = 500 GeV<sup>323</sup></td></tr><tr><td>none, 100-315</td><td>95</td><td>17 AAD</td><td>16AM ATLS</td><td>2 large-radius jets, Tstop1RPV</td></tr><tr><td>none, 200-350</td><td>95</td><td>18 KHACHATRY...15L CMS</td><td>˜t → qq, λ''<sub>312</sub> ≠ 0</td><td>˜t → qb, λ''<sub>323</sub> ≠ 0</td></tr><tr><td>none, 200-385</td><td>95</td><td>18 KHACHATRY...15L CMS</td><td>˜t → qb, λ''<sub>323</sub> ≠ 0</td><td>τ + b-jets, Q<span style="text-decoration: overline">D</span>, λ''<sub>333</sub> ≠ 0, ˜t → τb simplified model</td></tr><tr><td>> 740</td><td>95</td><td>19 KHACHATRY...14T CMS</td><td>τ + b-jets, Q<span style="text-decoration: overline">D</span>, λ''<sub>3jk</sub> ≠ 0</td><td>τ + b-jets, Q<span style="text-decoration: overline">D</span>, λ''<sub>3jk</sub> ≠ 0</td></tr><tr><td>> 580</td><td>95</td><td>19 KHACHATRY...14T CMS</td><td>(j ≠ 3), ˜t → λ''<sub>±</sub> b, λ''<sub>±</sub> → qqτ<sup>±</sup> simplified model</td><td>(j ≠ 3), ˜t → λ''<sub>±</sub> b, λ''<sub>±</sub> → qqτ<sup>±</sup> simplified model</td></tr></tbody></table>

• • • We do not use the following data for averages, fits, limits, etc. • • •

<table><tbody><tr><td>> 770</td><td>95</td><td>20 AAD</td><td>21B ATLS</td><td>≥ 8 jets, ≥ 5 b-jets, Tstop4RPV</td></tr><tr><td>> 890</td><td>95</td><td>21 KHACHATRY...16AC CMS</td><td>e<sup>+</sup> e<sup>-</sup> + ≥ 5 jets; ˜t → bλ''<sub>1</sub>;<br>λ''<sub>1</sub> → ℓℓ'j, λ''<sub>ijk</sub></td><td>λ''<sub>1</sub> → ℓℓ'j, λ''<sub>ijk</sub></td></tr><tr><td>>1000</td><td>95</td><td>21 KHACHATRY...16AC CMS</td><td>μ<sup>+</sup> μ<sup>-</sup> + ≥ 5 jets; ˜t → bλ''<sub>1</sub>;<br>λ''<sub>1</sub> → ℓℓ'j, λ''<sub>ijk</sub></td><td>μ<sup>+</sup> μ<sup>-</sup> + ≥ 5 jets; ˜t → bλ''<sub>1</sub>;<br>λ''<sub>1</sub> → ℓℓ'ν, λ<sub>121</sub> or<br>λ<sub>122</sub> ≠ 0</td></tr><tr><td>> 950</td><td>95</td><td>22 KHACHATRY...16BX CMS</td><td>˜t → t<span style="text-decoration: overline">χ</span><sub>1</sub><sup>0</sup>, λ''<sub>323</sub> coupling and on the ˜t mass in an RPV model with top squark pair production and the RPV decay ˜t → d<span style="text-decoration: overline">d</span> with λ''<sub>3ij</sub> coupling, see their Figure 7.</td><td>˜t → t<span style="text-decoration: overline">χ</span><sub>1</sub><sup>0</sup>, λ''<sub>323</sub> coupling and on the ˜t mass in an RPV model with top squark pair production and the RPV decay ˜t → d<span style="text-decoration: overline">d</span> with λ''<sub>3ij</sub> coupling, see their Figure 7.</td></tr><tr><td>> 790</td><td>95</td><td>23 KHACHATRY...15E CMS</td><td>˜t<sub>1</sub> → bℓ, cτ = 2 cm</td><td>˜t<sub>1</sub> → bℓ, cτ = 2 cm</td></tr></tbody></table>

1 TUMASYAN 23L searched in 138 fb⁻¹ of pp collisions at √s = 13 TeV for pairs of dijet resonances with the same mass in final states with at least four jets, for the case where the four-jet production proceeds via an intermediate resonant state and for nonresonant production. No significant excess above the Standard Model expectations is observed. Limits are set in the nonresonant search on the top squark mass in the simplified model Tstop1aRPV with λ''312 coupling, assuming B(ds) = 1, see their figure 12. Limits are also set on resonant pair production of dijet resonances via high mass intermediate states and compared to a signal model of diquarks that decay into pairs of vector-like quarks, see their figures 10 and 11.

2 TUMASYAN 22AF searched for evidence of new long-lived particles decaying into leptons in pp collisions at √s = 13 TeV, corresponding to 118 (113) fb⁻¹ in the ee channel (eµ and µµ) channels. The leptons are required to have transverse impact parameter values between 0.01 and 10 cm and are not required to form a common vertex. No significant excess above the Standard Model expectations is observed. Limits are set on the mass of the top squark in RPV models with top squark pair production and ˜t → bτ and ˜t → d<span style="text-decoration: overline">d</span>, see their Figure 4, which contains a wider range of lifetime limits. Limits are also set on a gauge-mediated SUSY breaking model, where the next-to-lightest SUSY particle is a lepton and the lightest SUSY particle a gravitino G̃, see their Figure 5, which also contains a wider range of lifetime limits. Limits are also set in a model that produces BSM Higgs bosons (H) with a mass of 125 GeV through gluongluon fusion, where the H decays to two long-lived scalars S, each of which decays to two oppositely charged and same-flavor leptons.

3 AAD 21B searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for pair production of gluinos, stops, electroweakinos decaying RPV either directly or indirectly via the LSP. The final state in all cases is one or two leptons, many jets (up to fifteen) and b-jets. Different models with different branching fractions of the gluino or stop follow from the assumptions on the nature of the electroweakinos. No significant excess above the Standard Model predictions is observed. Limits are set on the gluino, t₁, electroweakino masses as a function of the λ''<sub>1</sub> mass in several scenarios of gluino, stop and electroweakino pair production.

4 SIRUNYAN 21AF searched in 140 fb⁻¹ of pp collisions at √s = 13 TeV for supersymmetry in events with two with displaced vertices from long-lived particles decaying into multijet or dijet final states. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the simplified model Tglu2RPV with λ''<sub>323</sub> coupling, on the λ''<sub>1</sub> mass in an RPV model with λ''<sub>1</sub> pair production and the RPV decay λ''<sub>1</sub> → tbs with λ''<sub>323</sub> coupling and on the ˜t mass in an RPV model with top squark pair production and the RPV decay ˜t → d<span style="text-decoration: overline">d</span> with λ''<sub>3ij</sub> coupling, see their Figure 7.

5 SIRUNYAN 21U searched in 132 fb⁻¹ of pp collisions at √s = 13 TeV for supersymmetry in events with displaced tracks and displaced vertices associated with a dijet system. No significant excess above the Standard Model expectations is observed. Limits are set on long-lived gluinos in an RPC GMSB SUSY model of gluino pair production, with g̃ → gG̃, see their Figure 9, in Tglu1A in a mini-split model, see their Figure 10, and in an RPV model of gluino pair production, with g̃ → tbs with coupling λ''<sub>323</sub>, see their Figure 11. Limits are also set on long-lived top squarks in Tstop2RPV, see their Figure 12, in an RPV model with ˜t → d<span style="text-decoration: overline">d</span> and λ''<sub>31</sub> coupling, see their Figure 13, and in a dynamical RPV model with ˜t → d<span style="text-decoration: overline">d</span> via a nonholomorphic RPV coupling λ''<sub>311</sub>, see their Figure 14. The best mass limit is achieved in all cases at cτ = 30 mm.

6 SIRUNYAN 21V searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for supersymmetry in events with one charged lepton (e<sup>+</sup> or µ<sup>+</sup>) and ≥ 7 jets. No significant excess above the Standard Model expectations is observed. Limits are set on an RPV SUSY model like Tstop1 with the additional decay λ''<sub>1</sub> → qqq with coupling λ''<sub>abc</sub>, with a,b,c ∈ 1,2, and

on a superlight SUSY model such as SYY, with one scalar particle S with even R-parity and its superpartner S̃, both singlets under all SM interactions, and with a portal mediated by loop interactions involving a new vectorlike messenger field (Y), where pair produced top squarks decay as ˜t → tg̃S̃, and S̃ → G̃S, and S → gg, see their Figure 6 and 7.

7 AAD 20M searched for long-lived particles decaying into hadrons and at least one muon in events containing a displaced muon track and a displaced vertex. The analysis uses a dataset of pp collisions at √s = 13 TeV corresponding to an integrated luminosity of 136 fb⁻¹. Using the Tstop3RPV simplified model, top squarks with masses up to 1.7 TeV are excluded for a lifetime of 0.1 ns, and masses below 1.3 TeV are excluded for lifetimes between 0.01 ns and 30 ns, see their Fig. 7. The dependence on the RPV coupling λ<sub>23k</sub> multiplied by cosθ<sub>t</sub>, with θ<sub>t</sub> the mixing angle between the left- and right-handed t squarks, is also shown, see their Fig. 7.

8 SIRUNYAN 19BI searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV in final states with two muons and two jets, or with one muon, two jets, and missing transverse momentum. Limits are set in a model of pair-produced, prompt or long-lived top squarks with R-parity violating decays to a b-quark and a lepton (Tstop2RPV), branching fraction of ˜t → bµ equal to 1/3 and cτ between 0.1 cm and 10 cm in the case of long-lived top squarks. See their Fig. 10.

9 SIRUNYAN 19BJ searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV in final states with two electrons and two jets, or with one electron, two jets, and missing transverse momentum. Limits are set in a model of pair-produced, prompt top squarks with R-parity violating decays to a b-quark and a lepton (Tstop2RPV), assuming branching fraction of ˜t → be equal to 1/3 and cτ = 0 cm. See their Fig.10.

10 AABOUD 18BB searched in 36.7 fb⁻¹ of pp collisions at √s = 13 TeV for massive coloured resonances which are pair-produced and decay into two jets. No significant deviation from the background prediction is observed. Results are interpreted in a SUSY simplified model as Tstop1RPV with ˜t → ds. Top squarks with masses in the range 100-410 GeV are excluded, see their Figure 9(a). The λ''<sub>312</sub> coupling is assumed to be sufficiently large for the decays to be prompt, but small enough to neglect the single-top squark resonant production through RPV couplings.

11 AABOUD 18BB searched in 36.7 fb⁻¹ of pp collisions at √s = 13 TeV for massive coloured resonances which are pair-produced and decay into two jets. No significant deviation from the background prediction is observed. Results are interpreted in Tstop1RPV. Top squarks with masses in the range 100-470 GeV or 480-610 GeV are excluded, see their Figure 9(b). The λ''<sub>323</sub> coupling is assumed to be sufficiently large for the decays to be prompt, but small enough to neglect the single-top squark resonant production through RPV couplings.

12 AABOUD 18P searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for pair-produced top squarks that decay through RPV λ''<sub>333</sub> (i = 1, 2, 3) couplings to a final state with two leptons and two jets, at least one of which is identified as a b-jet. No significant excess is observed over the SM background. In the Tstop2RPV model, lower limits on the top squark masses between 600 and 1500 GeV are set depending on the branching fraction to be, bµ, and bτ final states. See their Figs 6 and 7.

13 SIRUNYAN 18AD searched in 2.6 fb⁻¹ of pp collisions at √s = 13 TeV for long-lived particles by exploiting the multiplicity of displaced jets to search for the presence of signal decays occurring at distances between 1 and 1000 mm. Limits are set in a model of pair-produced, long-lived top squarks with R-parity violating decays to a b-quark and a lepton, see their Figure 3.

14 SIRUNYAN 18DV searched in 38.5 fb⁻¹ of pp collisions at √s = 13 TeV for long-lived particles in events with multiple jets and two displaced vertices composed of many tracks. No events with two well-separated high-track-multiplicity vertices were observed. Limits are set on the stop and the gluino mass in RPV models of supersymmetry where the stop (gluino) is decaying solely into dijet (multijet) final states, see their Figures 6 and 7.

15 SIRUNYAN 18DV searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for the pair production of resonances, each decaying to two quarks. The search is conducted separately in a boosted (two-jet) and resolved (four-jet) jet topology. The mass spectra are found to be consistent with the Standard Model expectations. Limits are set on the stop mass in the Tstop3RPV and Tstop1RPV simplified models, see their Figure 11.

16 AABOUD 17AI searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with one or more isolated lepton, at least eight jets, either zero or many b-jets, for evidence of R-parity violating decays of the top squark. No significant excess above the Standard Model expectations is observed. Limits up to 1.25 (1.10) TeV are set on the top squark mass in R-parity-violating supersymmetry models where ˜t₁ decays for a bino LSP as: ˜t → t<span style="text-decoration: overline">χ</span><sub>1</sub><sup>0</sup> and for a higgsino LSP as ˜t → t<span style="text-decoration: overline">χ</span><sub>1,2</sub><sup>0</sup>/b<span style="text-decoration: overline">χ</span><sub>1</sub><sup>+</sup>. These are followed by the decays through the non-zero λ''<sub>323</sub> coupling λ''<sub>1,2</sub><sup>0</sup> → tbs, λ''<sub>1</sub><sup>+</sup> → bbs. See their Figure 10 and text for details on model assumptions.

17 AAD 16AM searched in 17.4 fb⁻¹ of pp collisions at √s = 8 TeV for events containing two large-radius hadronic jets. No deviation from the background prediction is observed. Top squarks with masses between 100 and 315 GeV are excluded at 95% C.L. in the hypothesis that they both decay via R-parity violating coupling λ''<sub>323</sub> to b- and s-quarks. See their Fig. 10.

18 KHACHATRY 15L searched in 19.4 fb⁻¹ of pp collisions at √s = 8 TeV for pair production of heavy resonances decaying to pairs of jets in four jet events. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in R-parity-violating supersymmetry models where ˜t → qq (λ''<sub>312</sub> ≠ 0), see Fig. 6 (top) and ˜t → qtb (λ''<sub>323</sub> ≠ 0), see Fig. 6 (bottom).

19 KHACHATRY 14T searched in 19.7 fb⁻¹ of pp collisions at √s = 8 TeV for events with τ-leptons and b-quark jets, possibly with extra light-flavour jets. No excess above the Standard Model expectations is observed. Limits are set on stop masses in RPV SUSY models with Q<span style="text-decoration: overline">D</span> couplings, in two simplified models. In the first model, the decay ˜t → τb is considered, with λ''<sub>333</sub> ≠ 0, see Fig. 3. In the second model, the decay ˜t → λ''<sub>31</sub> b, with the subsequent decay λ''<sub>323</sub> → qqτ<sup>±</sup> is considered, with λ''<sub>3jk</sub> ≠ 0 and the mass splitting between the top squark and the charging chosen to be 100 GeV, see Fig. 4.

20 AAD 21B searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least eight jets and at least 5 b-jets, for evidence of R-parity violating decays of the top squark. No significant excess above the Standard Model expectations is observed. Limits up to 950 GeV are set on the top squark mass in Tstop4RPV simplified model. See their Figure 7 for more detailed mass bounds.

21 KHACHATRY 16AC searched in 19.7 fb⁻¹ of pp collisions at √s = 8 TeV for events with low missing transverse momentum, two oppositely charged electrons or muons, and at least five jets, at least one of which is a b-jet, for evidence of R-parity violating,
charging-mediated decays of the top squark. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in R-parity-violating supersymmetry models where $\bar{t} \to b\tilde{\chi}_1^\pm$ with $\tilde{\chi}_1^\pm \to \ell^\pm jj$, $\tilde{\chi}_{ijk}^\pm \neq 0$ ($i,j,k \le 2$), and with $m_{\tilde{t}} - m_{\tilde{\chi}_1^\pm} = 100$ GeV, see Fig. 3.

22 KHACHATRYAN 16Bx searched in 19.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing 4 leptons coming from R-parity-violating decays of $\tilde{\chi}_1^0 \to \ell\ell\nu$ with $\lambda_{121} \neq 0$ or $\lambda_{122} \neq 0$. No excess over the expected background is observed. Limits are derived on the gluino, squark and stop masses, see Fig. 23.

23 KHACHATRYAN 15E searched for long-lived particles decaying to leptons in 19.7 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV. Events were selected with an electron and muon with opposite charges and each with transverse impact parameter values between 0.02 and 2 cm. Limits are set on SUSY benchmark models with pair production of top squarks decaying into an $e\mu$ final state via RPV interactions. See their Fig. 2

Heavy $\tilde{g}$ (Gluino) mass limit

For $m_{\tilde{g}} > 60-70$ GeV, it is expected that gluinos would undergo a cascade decay via a number of neutralinos and/or charginos rather than undergo a direct decay to photinos as assumed by some papers. Limits obtained when direct decay is assumed are usually higher than limits when cascade decays are included.

Some earlier papers are now obsolete and have been omitted. They were last listed in our PDG 14 edition: K. Olive, et al. (Particle Data Group), Chinese Physics C38 070001 (2014) (http://pdg.lbl.gov).

R-parity conserving heavy $\tilde{g}$ (Gluino) mass limit

<table><thead><tr><th>VALUE (GeV)</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th><th></th></tr></thead><tbody><tr><td>&gt;2200</td><td>95</td><td>1 AAD</td><td>23AB ATLS</td><td>≥ 1 γ + jets + E<sub>T</sub>, GGM-like, Tglu4D, χ<sub>1</sub><sup>0</sup> NLSP, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &gt; 300 GeV</td><td></td></tr><tr><td>&gt;2200</td><td>95</td><td>1 AAD</td><td>23AB ATLS</td><td>≥ 1 γ + jets + E<sub>T</sub>, GGM-like, Tglu4G, χ<sub>1</sub><sup>0</sup> NLSP, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &gt; 350 GeV</td><td></td></tr><tr><td>&gt;2250</td><td>95</td><td>2 AAD</td><td>23AE ATLS</td><td>2 SFOS ℓ, jets, E<sub>T</sub>, Tglu1G, m<sub>χ̃<sub>0</sub></sub><sup>0</sup> = 100 GeV</td><td></td></tr><tr><td>&gt;1950</td><td>95</td><td>3 AAD</td><td>23AE ATLS</td><td>2 SFOS ℓ, jets, E<sub>T</sub>, Tglu1H, m<sub>χ̃<sub>2</sub></sub><sup>0</sup> = (m<sub>g̃</sub> + m<sub>χ̃<sub>0</sub></sub>)/2, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 100 GeV</td><td></td></tr><tr><td>&gt;2440</td><td>95</td><td>4 AAD</td><td>23AL ATLS</td><td>At least 3 b-tagged jets, 0 or 1 lepton, Tglu3B, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1 GeV</td><td></td></tr><tr><td>&gt;2350</td><td>95</td><td>4 AAD</td><td>23AL ATLS</td><td>At least 3 b-tagged jets, 0 or 1 lepton, Tglu2A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1 GeV</td><td></td></tr><tr><td>&gt;2050</td><td>95</td><td>5 AAD</td><td>23AL ATLS</td><td>At least 3 b-tagged jets, 0 or 1 lepton, Tglu3E, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> - m<sub>χ̃<sub>0</sub></sub><sup>0</sup> = 2 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1 GeV</td><td></td></tr><tr><td>&gt;2320</td><td>95</td><td>6 HAYRAPETY...23E</td><td>CMS</td><td>γ + jets + E<sub>T</sub>, Tglu4E, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1700 GeV</td><td></td></tr><tr><td>&gt;2375</td><td>95</td><td>6 HAYRAPETY...23E</td><td>CMS</td><td>γ + jets + E<sub>T</sub>, Tglu4D, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1700 GeV</td><td></td></tr><tr><td>&gt;2260</td><td>95</td><td>6 HAYRAPETY...23E</td><td>CMS</td><td>γ + jets + E<sub>T</sub>, Tglu4F, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1700 GeV</td><td></td></tr><tr><td>&gt;2120</td><td>95</td><td>7 TUMASYAN</td><td>23AY CMS</td><td>ℓ<sup>±</sup> + ≥ 6 jets + ≥ 1 b-jet, Tglu3A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td><td></td></tr><tr><td>&gt;2050</td><td>95</td><td>7 TUMASYAN</td><td>23AY CMS</td><td>ℓ<sup>±</sup> + ≥ 5 jets, 0 b-jets, Tglu1B, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = 0.5(m<sub>g̃</sub> + m<sub>χ̃<sub>0</sub></sub>)</td><td></td></tr><tr><td>&gt;2200</td><td>95</td><td>8 AAD</td><td>22U ATLS</td><td>g̃ → qqχ̃<sub>0</sub><sup>±</sup>, qqχ̃<sub>1</sub><sup>±</sup>, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = 1000 GeV, τ(χ̃<sup>±</sup>) = 1 ns</td><td></td></tr><tr><td>&gt;2330</td><td>95</td><td>9 TUMASYAN</td><td>22V CMS</td><td>3 or 4 b-tagged jets or 2 large-radius jets, E<sub>T</sub>; Tglu1I; m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1 GeV</td><td></td></tr><tr><td>&gt;2200</td><td>95</td><td>10 AAD</td><td>21AK ATLS</td><td>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tglu1B, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = (m<sub>g̃</sub> + m<sub>χ̃<sub>0</sub></sub>)/2, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 400 GeV</td><td></td></tr><tr><td>none<br>1300-2050</td><td>95</td><td>10 AAD</td><td>21AK ATLS</td><td>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tglu1B, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = (m<sub>g̃</sub> + m<sub>χ̃<sub>0</sub></sub>)/2, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 1000 GeV</td><td></td></tr><tr><td>&gt;2300</td><td>95</td><td>11 AAD</td><td>21L ATLS</td><td>jets + E<sub>T</sub>, Tglu1A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 200 GeV</td><td></td></tr><tr><td>&gt;3000</td><td>95</td><td>11 AAD</td><td>21L ATLS</td><td>jets + E<sub>T</sub>, combined g̃g̃, g̃, q̃, q̃q̃ production, g̃ → qq'χ̃<sub>1</sub><sup>0</sup>, q̃ → qχ̃<sub>1</sub><sup>0</sup>, m̃q̃ = m̃g̃, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td><td></td></tr><tr><td>&gt;2200</td><td>95</td><td>11 AAD</td><td>21L ATLS</td><td>jets + E<sub>T</sub>, Tglu1B, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td><td></td></tr><tr><td>&gt;1400</td><td>95</td><td>12 AAD</td><td>21X ATLS</td><td>jets in empty bunch crossings, Tglu1A, long-lived R-hadron, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 100 GeV, 10<sup>-5</sup> s &lt; τR-hadron &lt; 10<sup>3</sup> s</td><td></td></tr></tbody></table>

<table><tbody><tr><td>&gt;870</td><td>95</td><td>12 AAD</td><td>21X ATLS</td><td>jets in empty bunch crossings, Tglu1A, long-lived R-hadron, m<sub>g̃</sub> - m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 100 GeV, 10<sup>-5</sup> s &lt; τR-hadron &lt; 10<sup>3</sup> s</td></tr><tr><td>&gt;2260</td><td>95</td><td>13 SIRUNYAN</td><td>21AD CMS</td><td>jets + E<sub>T</sub>, Tglu3A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 1050 GeV</td></tr><tr><td>&gt;2150</td><td>95</td><td>13 SIRUNYAN</td><td>21AD CMS</td><td>jets + E<sub>T</sub>, Tglu3C, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 600 GeV, m<sub>ℓ̃</sub> - m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 20 GeV</td></tr><tr><td>&gt;2250</td><td>95</td><td>13 SIRUNYAN</td><td>21AD CMS</td><td>jets + E<sub>T</sub>, Tglu3D, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 700 GeV, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> - m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 5 GeV</td></tr><tr><td>&gt;1870</td><td>95</td><td>14 SIRUNYAN</td><td>21M CMS</td><td>ℓ<sup>±</sup>ℓ<sup>∓</sup> + E<sub>T</sub>, Tglu4C, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1100 GeV</td></tr><tr><td>&gt;1980</td><td>95</td><td>15 AAD</td><td>20AL ATLS</td><td>8 or more jets + E<sub>T</sub>, Tglu1E, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 100 GeV</td></tr><tr><td>&gt;1820</td><td>95</td><td>15 AAD</td><td>20AL ATLS</td><td>8 or more jets + E<sub>T</sub>, Tglu3A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 100 GeV</td></tr><tr><td>&gt;1600</td><td>95</td><td>16 AAD</td><td>20V ATLS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> + jets, Tglu1E, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 100 GeV</td></tr><tr><td>&gt;1975</td><td>95</td><td>17 SIRUNYAN</td><td>20B CMS</td><td>≥ 1γ + E<sub>T</sub>, Tglu4A, BR(g̃ → qqχ̃<sub>1</sub><sup>±</sup>) = 0.5, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> ≈ m<sub>g̃</sub></td></tr><tr><td>&gt;1920</td><td>95</td><td>18 SIRUNYAN</td><td>20BJ CMS</td><td>jets + E<sub>T</sub>, Tglu1H, m<sub>g̃</sub> - m<sub>χ̃<sub>2</sub></sub><sup>0</sup> = 50 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1 GeV</td></tr><tr><td>&gt;2150</td><td>95</td><td>19 SIRUNYAN</td><td>20E CMS</td><td>1ℓ+jets, Tglu3A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 700 GeV</td></tr><tr><td>&gt;2050</td><td>95</td><td>19 SIRUNYAN</td><td>20E CMS</td><td>1ℓ+jets, Tglu3A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 1100 GeV</td></tr><tr><td>&gt;1650</td><td>95</td><td>19 SIRUNYAN</td><td>20E CMS</td><td>1ℓ+jets, Tglu3C, m<sub>ℓ̃</sub> - m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 175 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 1150 GeV</td></tr><tr><td>&gt;1700</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu3A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1610</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu3B, m<sub>ℓ̃</sub> - m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 175 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1300</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu3C, m<sub>ℓ̃</sub> - m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 20 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1500</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu3D, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = m<sub>χ̃<sub>1</sub></sub><sup>0</sup> + 5 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1350</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu1C, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = (m<sub>g̃</sub> + m<sub>χ̃<sub>0</sub></sub>)/2, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1250</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu1C, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = m<sub>χ̃<sub>1</sub></sub><sup>0</sup> + 20 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1425</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu1B, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = (m<sub>g̃</sub> + m<sub>χ̃<sub>0</sub></sub>)/2, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1425</td><td>95</td><td>20 SIRUNYAN</td><td>20T CMS</td><td>same-sign ℓ<sup>±</sup>ℓ<sup>±</sup> or ≥ 3ℓ<sup>±</sup> + jets, Tglu1B, m<sub>χ̃<sub>1</sub></sub><sup>±</sup> = m<sub>χ̃<sub>1</sub></sub><sup>0</sup> + 20 GeV, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;2000</td><td>95</td><td>21 AABOUD</td><td>19I ATL</td><td>≥ 2 jets + 1 or 2 + E<sub>T</sub>, Tglu1F, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 100 GeV</td></tr><tr><td>&gt;1860</td><td>95</td><td>22 SIRUNYAN</td><td>19AG CMS</td><td>2γ + E<sub>T</sub>, Tglu4B, 500 GeV &lt;m<sub>χ̃<sub>1</sub></sub><sup>0</sup> &lt; 1500 GeV</td></tr><tr><td>&gt;1920</td><td>95</td><td>23 SIRUNYAN</td><td>19AU CMS</td><td>γ + jets + b-jets + E<sub>T</sub>, Tglu4D, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 127 GeV</td></tr><tr><td>&gt;1950</td><td>95</td><td>23 SIRUNYAN</td><td>19AU CMS</td><td>γ + jets + b-jets + E<sub>T</sub>, Tglu4E, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1 GeV</td></tr><tr><td>&gt;1800</td><td>95</td><td>23 SIRUNYAN</td><td>19AU CMS</td><td>γ + jets + b-jets + E<sub>T</sub>, Tglu4F, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1 GeV</td></tr><tr><td>&gt;2090</td><td>95</td><td>23 SIRUNYAN</td><td>19AU CMS</td><td>γ + jets + b-jets + E<sub>T</sub>, Tglu4D, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1200 GeV</td></tr><tr><td>&gt;2120</td><td>95</td><td>23 SIRUNYAN</td><td>19AU CMS</td><td>γ + jets + b-jets + E<sub>T</sub>, Tglu4E, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1200 GeV</td></tr><tr><td>&gt;1970</td><td>95</td><td>23 SIRUNYAN</td><td>19AU CMS</td><td>γ + jets + b-jets + E<sub>T</sub>, Tglu4F, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 1200 GeV</td></tr><tr><td>&gt;1700</td><td>95</td><td>24 SIRUNYAN</td><td>19CE CMS</td><td>2 jets, Stealth SUSY, Tglu1A and χ̃<sub>1</sub><sup>0</sup> → Sγ (S → S G̃), m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 200 GeV</td></tr><tr><td>&gt;2000</td><td>95</td><td>25 SIRUNYAN</td><td>19CH CMS</td><td>jets + E<sub>T</sub>, Tglu1A, m<sub>χ̃<sub>1</sub></sub><sup>0</sup> = 0 GeV</td></tr></tbody></table>
<table>
  <tbody>
    <tr>
      <td>&gt;2030</td>
      <td>95</td>
      <td>25 SIRUNYAN</td>
      <td>19CH CMS jets+&epsilon;<sub>T</sub>, Tglu1C, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>=m<sub>&chi;</sub><sup>0</sup>=0.5(m<sub>&chi;</sub><sup>0</sup>+m<sub>&chi;</sub><sup>0</sup>), m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1860</td>
      <td>95</td>
      <td>47 AABOUD</td>
      <td>17AJ ATLS same-sign &ell; &pm; &ell;<sup>0</sup>/3 &ell; + jets + &epsilon;<sub>T</sub>, Tglu1G, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=200 GeV</td>
    </tr>
    <tr>
      <td>&gt;2270</td>
      <td>95</td>
      <td>25 SIRUNYAN</td>
      <td>19CH CMS jets+&epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;2100</td>
      <td>95</td>
      <td>48 AABOUD</td>
      <td>17AR ATLS 1&ell;+jets+&epsilon;<sub>T</sub>, Tglu1B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0</td>
    </tr>
    <tr>
      <td>&gt;2180</td>
      <td>95</td>
      <td>25 SIRUNYAN</td>
      <td>19CH CMS jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1740</td>
      <td>95</td>
      <td>49 AABOUD</td>
      <td>17AR ATLS 1&ell;+jets+&epsilon;<sub>T</sub>, Tglu1E, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0</td>
    </tr>
    <tr>
      <td>&gt;1750</td>
      <td>95</td>
      <td>26 SIRUNYAN</td>
      <td>19K CMS &gamma;+&ell;+&epsilon;<sub>T</sub>, Tglu4A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=1500 GeV</td>
      <td>&gt;1800</td>
      <td>95</td>
      <td>50 AABOUD</td>
      <td>17AY ATLS jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=m<sub>&chi;</sub><sup>0</sup><sub>1</sub></td>
    </tr>
    <tr>
      <td>&gt;2000</td>
      <td>95</td>
      <td>27 SIRUNYAN</td>
      <td>19S CMS 1 or 2 &ell; + jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 700 GeV</td>
      <td>&gt;1800</td>
      <td>95</td>
      <td>51 AABOUD</td>
      <td>17AZ ATLS &ge; 7 jets+&epsilon;<sub>T</sub>, large R-jets and/or b-jets, Tglu1E, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
    </tr>
    <tr>
      <td>&gt;1900</td>
      <td>95</td>
      <td>27 SIRUNYAN</td>
      <td>19S CMS 1 or 2 &ell; + jets + &epsilon;<sub>T</sub>, Tglu3C, 150 GeV &lt; m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 950 GeV</td>
      <td>&gt;1540</td>
      <td>95</td>
      <td>52 AABOUD</td>
      <td>17AZ ATLS &ge; 7 jets+&epsilon;<sub>T</sub>, large R-jets and/or b-jets, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1970</td>
      <td>95</td>
      <td>28 AABOUD</td>
      <td>18AR ATLS jets+&ge; 3b-jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 300 GeV</td>
      <td>&gt;1340</td>
      <td>95</td>
      <td>53 AABOUD</td>
      <td>17N ATLS 2 same-flavor, opposite-sign &ell; + jets + &epsilon;<sub>T</sub>, Tglu1H, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0</td>
    </tr>
    <tr>
      <td>&gt;1920</td>
      <td>95</td>
      <td>29 AABOUD</td>
      <td>18AR ATLS jets+&ge; 3b-jets+&epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 600 GeV</td>
      <td>&gt;1340</td>
      <td>95</td>
      <td>54 AABOUD</td>
      <td>17N ATLS 2 same-flavor, opposite-sign &ell; + jets + &epsilon;<sub>T</sub>, Tglu1H, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0</td>
    </tr>
    <tr>
      <td>&gt;1650</td>
      <td>95</td>
      <td>30 AABOUD</td>
      <td>18AS ATLS &ge; 4 jets and disappearing tracks from &chi;<sup>&pm;</sup> &rarr; &chi;<sub>1</sub><sup>0</sup>&pi;<sup>&pm;</sup>, modified Tglu1A or Tglu1B, &chi;<sup>&pm;</sup> lifetime 0.2 ns, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>=460 GeV</td>
      <td>&gt;1310</td>
      <td>95</td>
      <td>55 AABOUD</td>
      <td>17N ATLS 2 same-flavor, opposite-sign &ell; + jets + &epsilon;<sub>T</sub>, Tglu1H, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0</td>
    </tr>
    <tr>
      <td>&gt;1850</td>
      <td>95</td>
      <td>31 AABOUD</td>
      <td>18BJ ATLS &ell; &pm; &ell;<sup>0</sup> + jets + &epsilon;<sub>T</sub>, Tglu1G, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
      <td>&gt;1700</td>
      <td>95</td>
      <td>56 KHACHATRY...17 CMS jets+&epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=200 GeV</td>
    </tr>
    <tr>
      <td>&gt;1650</td>
      <td>95</td>
      <td>32 AABOUD</td>
      <td>18BJ ATLS &ell; &pm; &ell;<sup>0</sup> + jets + &epsilon;<sub>T</sub>, Tglu1H, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
      <td>&gt;1400</td>
      <td>95</td>
      <td>56 KHACHATRY...17 CMS jets+&epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=200 GeV</td>
    </tr>
    <tr>
      <td>&gt;2150</td>
      <td>95</td>
      <td>33 AABOUD</td>
      <td>18U ATLS 2 &gamma; + &epsilon;<sub>T</sub>, GGM, Tglu4B, any NLSP mass</td>
      <td>&gt;1650</td>
      <td>95</td>
      <td>56 KHACHATRY...17 CMS jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=200 GeV</td>
    </tr>
    <tr>
      <td>&gt;1600</td>
      <td>95</td>
      <td>34 AABOUD</td>
      <td>18U ATLS &gamma; + jets + &epsilon;<sub>T</sub>, GGM higgsino-bino, mix of Tglu4B and Tglu4C, any NLSP mass</td>
      <td>&gt;1600</td>
      <td>95</td>
      <td>57 KHACHATRY...17AD CMS jets+b-jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;2030</td>
      <td>95</td>
      <td>35 AABOUD</td>
      <td>18V ATLS jets+&epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1550</td>
      <td>95</td>
      <td>58 KHACHATRY...17AD CMS jets+b-jets+&epsilon;<sub>T</sub>, Tglu3C, 200 &lt; m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 400 GeV</td>
    </tr>
    <tr>
      <td>&gt;1980</td>
      <td>95</td>
      <td>36 AABOUD</td>
      <td>18V ATLS jets+&epsilon;<sub>T</sub>, Tglu1B, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>=0.5(m<sub>&chi;</sub><sup>0</sup>+m<sub>&chi;</sub><sup>0</sup>), m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1450</td>
      <td>95</td>
      <td>59 KHACHATRY...17AS CMS 1&ell;, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 600 GeV</td>
    </tr>
    <tr>
      <td>&gt;1750</td>
      <td>95</td>
      <td>37 AABOUD</td>
      <td>18V ATLS jets+&epsilon;<sub>T</sub>, Tglu1C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=1 GeV, any m<sub>&chi;</sub><sup>0</sup><sub>2</sub> &gt; 100 GeV</td>
      <td>&gt;1570</td>
      <td>95</td>
      <td>59 KHACHATRY...17AS CMS 1&ell;, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 775 GeV</td>
    </tr>
    <tr>
      <td>&gt;2000</td>
      <td>95</td>
      <td>38 SIRUNYAN</td>
      <td>18AA CMS &ge; 1&gamma; + &epsilon;<sub>T</sub>, Tglu4A</td>
      <td>&gt;1570</td>
      <td>95</td>
      <td>59 KHACHATRY...17AS CMS 1&ell;, Tglu1B, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= (m<sub>&chi;</sub><sup>0</sup> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 725 GeV</td>
    </tr>
    <tr>
      <td>&gt;2100</td>
      <td>95</td>
      <td>38 SIRUNYAN</td>
      <td>18AA CMS &ge; 1&gamma; + &epsilon;<sub>T</sub>, Tglu4B</td>
      <td>&gt;1570</td>
      <td>95</td>
      <td>59 KHACHATRY...17AS CMS 1&ell;, Tglu1B, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= (m<sub>&chi;</sub><sup>0</sup> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 850 GeV</td>
    </tr>
    <tr>
      <td>&gt;1800</td>
      <td>95</td>
      <td>39 SIRUNYAN</td>
      <td>18AC CMS 1&ell;+jets, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 650 GeV</td>
      <td>none</td>
      <td>95</td>
      <td>60 KHACHATRY...17AW CMS &ge; 3&ell;<sup>0</sup>, 2 jets, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1700</td>
      <td>95</td>
      <td>39 SIRUNYAN</td>
      <td>18AC CMS 1&ell;+jets, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 1040 GeV</td>
      <td>&gt;1175</td>
      <td>95</td>
      <td>60 KHACHATRY...17AW CMS &ge; 3&ell;<sup>0</sup>, 2 jets, Tglu1C, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= (m<sub>&chi;</sub><sup>0</sup> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 400 GeV</td>
    </tr>
    <tr>
      <td>&gt;1900</td>
      <td>95</td>
      <td>39 SIRUNYAN</td>
      <td>18AC CMS 1&ell; + jets, Tglu1B, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= (m<sub>&chi;</sub><sup>0</sup> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 300 GeV</td>
      <td>&gt; 825</td>
      <td>95</td>
      <td>61 KHACHATRY...17P CMS 1 or more jets+&epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1250</td>
      <td>95</td>
      <td>39 SIRUNYAN</td>
      <td>18AC CMS 1&ell; + jets, Tglu1B, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= (m<sub>&chi;</sub><sup>0</sup> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 950 GeV</td>
      <td>&gt;1350</td>
      <td>95</td>
      <td>61 KHACHATRY...17P CMS 1 or more jets+&epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1610</td>
      <td>95</td>
      <td>40 SIRUNYAN</td>
      <td>18AL CMS &ge; 3&ell;<sup>0</sup> + jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 0 GeV</td>
      <td>&gt;1545</td>
      <td>95</td>
      <td>61 KHACHATRY...17P CMS 1 or more jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1160</td>
      <td>95</td>
      <td>40 SIRUNYAN</td>
      <td>18AL CMS &ge; 3&ell;<sup>0</sup> + jets + &epsilon;<sub>T</sub>, Tglu1C, m<sub>&chi;</sub><sup>0</sup><sub>2</sub>= m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= (m<sub>&chi;</sub><sup>0</sup> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub><0 0 GeV</td>
      <td>&gt;1120</td>
      <td>95</td>
      <td>61 KHACHATRY...17P CMS 1 or more jets+&epsilon;<sub>T</sub>, Tglu3D, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= m<sub>&chi;</sub><sup>0</sup><sub>1</sub> + 5 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
    </tr>
    <tr>
      <td>&gt;1500</td>
      <td>95</td>
      <td>41 SIRUNYAN</td>
      <td>18AR CMS &ell; &pm; &ell;<sup>0</sup> + jets + &epsilon;<sub>T</sub>, GMSB, Tglu4C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
      <td>&gt;1300</td>
      <td>95</td>
      <td>61 KHACHATRY...17P CMS 1 or more jets+&epsilon;<sub>T</sub>, Tglu3B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>= m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 175 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=50 GeV</td>
    </tr>
    <tr>
      <td>&gt;1770</td>
      <td>95</td>
      <td>41 SIRUNYAN</td>
      <td>18AR CMS &ell; &pm; &ell;<sup>0</sup> + jets + &epsilon;<sub>T</sub>, GMSB, Tglu4C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=1400 GeV</td>
      <td>&gt; 780</td>
      <td>95</td>
      <td>61 KHACHATRY...17P CMS 1 or more jets+&epsilon;<sub>T</sub>, Tglu3C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>= m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1625</td>
      <td>95</td>
      <td>42 SIRUNYAN</td>
      <td>18AY CMS jets+&epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1650</td>
      <td>95</td>
      <td>62 KHACHATRY...17V CMS 2 &gamma; + &epsilon;<sub>T</sub>, GGM, Tglu4B, any NLSP mass</td>
    </tr>
    <tr>
      <td>&gt;1825</td>
      <td>95</td>
      <td>42 SIRUNYAN</td>
      <td>18AY CMS jets+&epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1900</td>
      <td>95</td>
      <td>63 SIRUNYAN 17AF CMS 1&ell;+jets+b-jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1625</td>
      <td>95</td>
      <td>42 SIRUNYAN</td>
      <td>18AY CMS jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1600</td>
      <td>95</td>
      <td>63 SIRUNYAN 17AF CMS 1&ell;+jets+b-jets+&epsilon;<sub>T</sub>, Tglu3B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 175 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=50 GeV</td>
    </tr>
    <tr>
      <td>&gt;2040</td>
      <td>95</td>
      <td>43 SIRUNYAN</td>
      <td>18D CMS top quark (hadronically decaying) + jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1600</td>
      <td>95</td>
      <td>64 SIRUNYAN 17AY CMS &gamma; + jets+&epsilon;<sub>T</sub>, Tglu4B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1930</td>
      <td>95</td>
      <td>43 SIRUNYAN</td>
      <td>18D CMS top quark (hadronically decaying) + jets + &epsilon;<sub>T</sub>, Tglu3B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 175 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=200 GeV</td>
      <td>&gt;1800</td>
      <td>95</td>
      <td>64 SIRUNYAN 17AY CMS &gamma; + jets+&epsilon;<sub>T</sub>, Tglu4A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1690</td>
      <td>95</td>
      <td>43 SIRUNYAN</td>
      <td>18D CMS top quark (hadronically decaying) + jets + &epsilon;<sub>T</sub>, Tglu3C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
      <td>&gt;1600</td>
      <td>95</td>
      <td>65 SIRUNYAN 17AZ CMS &ge; 1 jets+&epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1990</td>
      <td>95</td>
      <td>43 SIRUNYAN</td>
      <td>18D CMS top quark (hadronically decaying) + jets + &epsilon;<sub>T</sub>, Tglu3E, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub>= m<sub>&chi;</sub><sup>0</sup><sub>1</sub> + 5 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
      <td>&gt;1860</td>
      <td>95</td>
      <td>65 SIRUNYAN 17AZ CMS &ge; 1 jets+&epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;2010</td>
      <td>95</td>
      <td>44 SIRUNYAN</td>
      <td>18M CMS &ge; 1 H (-> bb) + &epsilon;<sub>T</sub>, Tglu1l</td>
      <td>&gt;2025</td>
      <td>95</td>
      <td>65 SIRUNYAN 17AZ CMS &ge; 1 jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1825</td>
      <td>95</td>
      <td>44 SIRUNYAN</td>
      <td>18M CMS &ge; 1 H (-> bb) + &epsilon;<sub>T</sub>, Tglu1l</td>
      <td>&gt;1900</td>
      <td>95</td>
      <td>66 SIRUNYAN 17P CMS jets+&epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1750</td>
      <td>95</td>
      <td>45 AABOUD</td>
      <td>17AJ ATLS same-sign &ell;<sup>0</sup> &pm; &ell;/3 &ell; + jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
      <td>&gt;1825</td>
      <td>95</td>
      <td>66 SIRUNYAN 17P CMS jets+&epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1570</td>
      <td>95</td>
      <td>46 AABOUD</td>
      <td>17AJ ATLS same-sign &ell;<sup>0</sup> &pm; &ell;/3 &ell; + jets + &epsilon;<sub>T</sub>, Tglu1E, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
      <td>&gt;1950</td>
      <td>95</td>
      <td>66 SIRUNYAN 17P CMS jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1570</td>
      <td>95</td>
      <td>46 AABOUD</td>
      <td>17AJ ATLS same-sign &ell;<sup>0</sup> &pm; &ell;/3 &ell; + jets + &epsilon;<sub>T</sub>, Tglu1E, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=100 GeV</td>
      <td>&gt;1960</td>
      <td>95</td>
      <td>66 SIRUNYAN 17P CMS jets+&epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub>=0 GeV</td>
    </tr>
  </tbody>
</table>
# Searches Particle Listings
## Supersymmetric Particle Searches

<table>
  <tbody>
    <tr>
      <td>&gt;1800</td>
      <td>95</td>
      <td>66 SIRUNYAN</td>
      <td>17P</td>
      <td>CMS jets+&epsilon;<sub>T</sub>, Tglu1C, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub> = m<sub>&chi;</sub><sup>0</sup><sub>2</sub> = (m<sub>&tilde;g</sub>+m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
      <td>&gt;1050</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> &chi;<sub>1</sub><sup>0</sup> = m<sub>t</sub>, m<sub>t</sub><sup>0</sup> &lt; 800 GeV</td>
    </tr>
    <tr>
      <td>&gt;1870</td>
      <td>95</td>
      <td>66 SIRUNYAN</td>
      <td>17P</td>
      <td>CMS jets+&epsilon;<sub>T</sub>, Tglu3D, m<sub>&chi;</sub><sup>&pm;</sup><sub>1</sub> = m<sub>&chi;</sub><sup>0</sup><sub>1</sub> + 5 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 1000 GeV</td>
      <td>&gt;1725</td>
      <td>95</td>
      <td>80 KHACHATRY...16BS CMS jets + &epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1520</td>
      <td>95</td>
      <td>67 SIRUNYAN</td>
      <td>17S</td>
      <td>CMS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup> + jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
      <td>&gt;1750</td>
      <td>95</td>
      <td>80 KHACHATRY...16BS CMS jets + &epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1200</td>
      <td>95</td>
      <td>67 SIRUNYAN</td>
      <td>17S</td>
      <td>CMS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup> + jets + &epsilon;<sub>T</sub>, Tglu3D, m<sub>t</sub><sup>-</sup> &chi;<sub>1</sub><sup>0</sup> = m<sub>&chi;</sub><sup>0</sup><sub>1</sub> + 5 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td>
      <td>&gt;1550</td>
      <td>95</td>
      <td>80 KHACHATRY...16BS CMS jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1370</td>
      <td>95</td>
      <td>67 SIRUNYAN</td>
      <td>17S</td>
      <td>CMS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup> + jets + &epsilon;<sub>T</sub>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 175 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 50 GeV</td>
      <td>&gt;1440</td>
      <td>95</td>
      <td>81 KHACHATRY...16BY CMS opposite-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu4C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 1000 GeV</td>
    </tr>
    <tr>
      <td>&gt;1180</td>
      <td>95</td>
      <td>67 SIRUNYAN</td>
      <td>17S</td>
      <td>CMS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup> + jets + &epsilon;<sub>T</sub>, Tglu3C, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
      <td>&gt;1030</td>
      <td>95</td>
      <td>81 KHACHATRY...16BY CMS opposite-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu4C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
    </tr>
    <tr>
      <td>&gt;1280</td>
      <td>95</td>
      <td>67 SIRUNYAN</td>
      <td>17S</td>
      <td>CMS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup> + jets + &epsilon;<sub>T</sub>, Tglu1B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = (m<sub>&tilde;g</sub> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
      <td>&gt;1440</td>
      <td>95</td>
      <td>82 KHACHATRY...16V CMS jets + &epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1300</td>
      <td>95</td>
      <td>67 SIRUNYAN</td>
      <td>17S</td>
      <td>CMS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup> + jets + &epsilon;<sub>T</sub>, Tglu1B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td>
      <td>&gt;1600</td>
      <td>95</td>
      <td>82 KHACHATRY...16V CMS jets + &epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1570</td>
      <td>95</td>
      <td>68 AABOUD</td>
      <td>16AC</td>
      <td>ATLS &ge; 2 jets + 1 or 2 &tau; + &epsilon;<sub>T</sub>, Tglu1F, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td>
      <td>&gt;1550</td>
      <td>95</td>
      <td>82 KHACHATRY...16V CMS jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1460</td>
      <td>95</td>
      <td>69 AABOUD</td>
      <td>16J</td>
      <td>ATLS 1 &ell;<sup>&pm;</sup> + &ge; 4 jets + &epsilon;<sub>T</sub>, Tglu3C, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 5 GeV</td>
      <td>&gt;1450</td>
      <td>95</td>
      <td>82 KHACHATRY...16V CMS jets + &epsilon;<sub>T</sub>, Tglu1C, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1650</td>
      <td>95</td>
      <td>70 AABOUD</td>
      <td>16M</td>
      <td>ATLS 2 &gamma; + &epsilon;<sub>T</sub>, Tglu1D, any NLSP mass</td>
      <td>&gt;820</td>
      <td>95</td>
      <td>83 AAD 15BG ATLS GGM, &tilde;g &rarr; q&tilde;gZ&tilde;G, tan&beta; = 30, &mu; &gt; 600 GeV</td>
    </tr>
    <tr>
      <td>&gt;1510</td>
      <td>95</td>
      <td>71 AABOUD</td>
      <td>16N</td>
      <td>ATLS &ge; 4 jets + &epsilon;<sub>T</sub>, Tglu1A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
      <td>&gt;850</td>
      <td>95</td>
      <td>83 AAD 15BG ATLS GGM, &tilde;g &rarr; q&tilde;gZ&tilde;G, tan&beta; = 1.5, &mu; &gt; 450 GeV</td>
    </tr>
    <tr>
      <td>&gt;1500</td>
      <td>95</td>
      <td>72 AABOUD</td>
      <td>16N</td>
      <td>ATLS &ge; 4 jets + &epsilon;<sub>T</sub>, Tglu1B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = (m<sub>&tilde;g</sub>+m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 200 GeV</td>
      <td>&gt;1150</td>
      <td>95</td>
      <td>84 AAD 15BV ATLS general RPC &tilde;g decays, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 100 GeV</td>
    </tr>
    <tr>
      <td>&gt;1780</td>
      <td>95</td>
      <td>73 AAD</td>
      <td>16AD</td>
      <td>ATLS 0&ell;, &ge; 3 b-jets + &epsilon;<sub>T</sub>, Tglu2A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 800 GeV</td>
      <td>&gt;700</td>
      <td>95</td>
      <td>85 AAD 15BX ATLS &tilde;g &rarr; X&chi;<sub>1</sub><sup>0</sup>, independent of m<sub>&chi;</sub><sup>0</sup><sub>1</sub></td>
    </tr>
    <tr>
      <td>&gt;1760</td>
      <td>95</td>
      <td>74 AAD</td>
      <td>16AD</td>
      <td>ATLS 1&ell;, &ge; 3 b-jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 700 GeV</td>
      <td>&gt;1280</td>
      <td>95</td>
      <td>86 AAD 15CA ATLS &ge; 2 &gamma; + &epsilon;<sub>T</sub>, GGM, bino-like NLSP, any NLSP mass</td>
    </tr>
    <tr>
      <td>&gt;1300</td>
      <td>95</td>
      <td>75 AAD</td>
      <td>16BB</td>
      <td>ATLS 2 same-sign/3&ell; + jets + &epsilon;<sub>T</sub>, Tglu1D, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 600 GeV</td>
      <td>&gt;1290</td>
      <td>95</td>
      <td>86 AAD 15CA ATLS &ge; 1 &gamma; + b-jets + &epsilon;<sub>T</sub>, GGM, higgsino-bino admix. NLSP and &mu; &lt; 0, m(NLSP)&gt;450 GeV</td>
    </tr>
    <tr>
      <td>&gt;1100</td>
      <td>95</td>
      <td>75 AAD</td>
      <td>16BB</td>
      <td>ATLS 2 same-sign/3&ell; + jets + &epsilon;<sub>T</sub>, Tglu1E, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 300 GeV</td>
      <td>&gt;1260</td>
      <td>95</td>
      <td>86 AAD 15CA ATLS &ge; 1 &gamma; + jets + &epsilon;<sub>T</sub>, GGM, higgsino-bino admixture NLSP, all &mu; &gt; 0</td>
    </tr>
    <tr>
      <td>&gt;1200</td>
      <td>95</td>
      <td>75 AAD</td>
      <td>16BB</td>
      <td>ATLS 2 same-sign/3&ell; + jets + &epsilon;<sub>T</sub>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 600 GeV</td>
      <td>&gt;1140</td>
      <td>95</td>
      <td>87 KHACHATRY...15AF CMS &tilde;g &rarr; q&tilde;g&chi;<sub>1</sub><sup>0</sup>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1600</td>
      <td>95</td>
      <td>76 AAD</td>
      <td>16BG</td>
      <td>ATLS 1&ell;, &ge; 4 jets, &epsilon;<sub>T</sub>, Tglu1B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = (m<sub>&tilde;g</sub> + m<sub>&chi;</sub><sup>0</sup>)/2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td>
      <td>&gt;1150</td>
      <td>95</td>
      <td>87 KHACHATRY...15AF CMS &tilde;g &rarr; b&tilde;g&chi;<sub>1</sub><sup>0</sup>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1400</td>
      <td>95</td>
      <td>77 AAD</td>
      <td>16V</td>
      <td>ATLS &ge; 7 to &ge; 10 jets + &epsilon;<sub>T</sub>, Tglu1E, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 200 GeV</td>
      <td>&gt;1225</td>
      <td>95</td>
      <td>87 KHACHATRY...15AF CMS &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1400</td>
      <td>95</td>
      <td>77 AAD</td>
      <td>16V</td>
      <td>ATLS &ge; 7 to &ge; 10 jets + &epsilon;<sub>T</sub>, pMSSM M<sub>1</sub> = 60 GeV, M<sub>2</sub> = 3 TeV, tan&beta;=10, &mu; &lt; 0</td>
      <td>&gt;1300</td>
      <td>95</td>
      <td>87 KHACHATRY...15AF CMS CMSSM, tan&beta;=30, m<sub>&tilde;g</sub>=m<sub>&tilde;g</sub>, A<sub>0</sub>=-2max(m<sub>0</sub>,m<sub>1</sub>/2), &mu; &gt;0</td>
    </tr>
    <tr>
      <td>&gt;1100</td>
      <td>95</td>
      <td>78 KHACHATRY...16AM CMS</td>
      <td>16M</td>
      <td>ATLS boosted W+b, Tglu3C, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 80GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 400GeV</td>
      <td>&gt;1225</td>
      <td>95</td>
      <td>87 KHACHATRY...15AF CMS CMSSM, tan&beta;=30, m<sub>&tilde;g</sub>=m<sub>&tilde;g</sub>, A<sub>0</sub>=-2max(m<sub>0</sub>,m<sub>1</sub>/2), &mu; &gt;0</td>
    </tr>
    <tr>
      <td>&gt; 700</td>
      <td>95</td>
      <td>78 KHACHATRY...16AM CMS</td>
      <td>16M</td>
      <td>ATLS boosted W+b, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 175 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
      <td>&gt;1310</td>
      <td>95</td>
      <td>88 KHACHATRY...15I CMS &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
    </tr>
    <tr>
      <td>&gt;1050</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 800 GeV</td>
      <td>&gt;1175</td>
      <td>95</td>
      <td>89 KHACHATRY...15X CMS &tilde;g &rarr; b&tilde;g&chi;<sub>1</sub><sup>0</sup>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td>
    </tr>
    <tr>
      <td>&gt;1300</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1330</td>
      <td>95</td>
      <td>89 KHACHATRY...15X CMS &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td>
    </tr>
    <tr>
      <td>&gt;1140</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1700</td>
      <td>95</td>
      <td>90 AAD 14AE ATLS jets + &epsilon;<sub>T</sub>, &tilde;g &rarr; q&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 700 GeV</td>
      <td>&gt;1090</td>
      <td>95</td>
      <td>90 AAD 14AE ATLS jets + &epsilon;<sub>T</sub>, mSUGRA/CMSSM, m<sub>&tilde;g</sub> = m<sub>&tilde;g</sub></td>
    </tr>
    <tr>
      <td>&gt; 950</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3D, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = m<sub>&chi;</sub><sup>0</sup><sub>1</sub> + 5 GeV</td>
      <td>&gt;1600</td>
      <td>95</td>
      <td>91 AAD 14AG ATLS &tau; + jets + &epsilon;<sub>T</sub>, natural Gauge Mediation</td>
    </tr>
    <tr>
      <td>&gt;1100</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1350</td>
      <td>95</td>
      <td>91 AAD 14AG ATLS &tau; + jets + &epsilon;<sub>T</sub>, mGMSB, M<sub>mss</sub> = 250 GeV, N<sub>5</sub> = 3, &mu; &gt; 0, C<sub>grav</sub> = 1</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1000</td>
      <td>95</td>
      <td>92 AAD 14X ATLS &ge; 4&ell;<sup>&pm;</sup>, &tilde;g &rarr; q&tilde;g&chi;<sub>1</sub><sup>0</sup>, &chi;<sub>1</sub><sup>0</sup> &rarr; &ell;<sup>&pm;</sup> &ell;<sup>&mp;</sup> &tan&beta; = 30, GGM</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3D, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 100 GeV</td>
      <td>&gt;1000</td>
      <td>95</td>
      <td>93 CHATRCHYAN 14AH CMS jets + &epsilon;<sub>T</sub>, &tilde;g &rarr; q&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 50 GeV</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu1B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1350</td>
      <td>95</td>
      <td>93 CHATRCHYAN 14AH CMS jets + &epsilon;<sub>T</sub>, CMSSM, m<sub>&tilde;g</sub> = m<sub>&tilde;g</sub></td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1000</td>
      <td>95</td>
      <td>94 CHATRCHYAN 14AH CMS jets + &epsilon;<sub>T</sub>, &tilde;g &rarr; b&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 50 GeV</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1000</td>
      <td>95</td>
      <td>95 CHATRCHYAN 14AH CMS jets + &epsilon;<sub>T</sub>, &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 50 GeV</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3D, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 100 GeV</td>
      <td>&gt;1160</td>
      <td>95</td>
      <td>96 CHATRCHYAN 14I CMS jets + &epsilon;<sub>T</sub>, &tilde;g &rarr; q&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 100 GeV</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3D, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1260</td>
      <td>95</td>
      <td>96 CHATRCHYAN 14I CMS multijets + &epsilon;<sub>T</sub>, &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 100 GeV</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu1B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1130</td>
      <td>95</td>
      <td>96 CHATRCHYAN 14I CMS multijets + &epsilon;<sub>T</sub>, &tilde;g &rarr; q&tilde;gW/Z&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 100 GeV</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1210</td>
      <td>95</td>
      <td>97 CHATRCHYAN 14N CMS 1&ell;<sup>&pm;</sup> + jets + &ge; 2b-jets, &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV, m<sub>t</sub><sup>-</sup> &gt; m<sub>&tilde;g</sub></td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1260</td>
      <td>95</td>
      <td>98 CHATRCHYAN 14R CMS &ge; 3&ell;<sup>&pm;</sup>, (&tilde;g/&qtilde;) &rarr; q&ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup>&tilde;G simplified model, GMSB, slep-ton co-NLSP scenario</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1260</td>
      <td>95</td>
      <td>99 CHATRCHYAN 14R CMS &ge; 3&ell;<sup>&pm;</sup>, &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1260</td>
      <td>95</td>
      <td>99 CHATRCHYAN 14R CMS &ge; 3&ell;<sup>&pm;</sup>, &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model</td>
    </tr>
    <tr>
      <td>&gt; 850</td>
      <td>95</td>
      <td>79 KHACHATRY...16BJ CMS</td>
      <td>16M</td>
      <td>ATLS same-sign &ell;<sup>&pm;</sup> &ell;<sup>&pm;</sup>, Tglu3B, m<sub>t</sub><sup>-</sup> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 20 GeV, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td>
      <td>&gt;1260</td>
      <td>95</td>
      <td>99 CHATRCHYAN 14R CMS &ge; 3&ell;<sup>&pm;</sup>, &tilde;g &rarr; t&tilde;g&chi;<sub>1</sub><sup>0</sup> simplified model</td>
    </tr>
  </tbody>
</table>
⁶ HAYRAPETYAN 23E searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for evidence of gluino, top squark and electroweak pair production in events with at least one photon, multiple jets, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set in models for strong production, Tglu4D, Tglu4E, Tglu4F and TStop13, see their figure 9. They also interpret the results in the models for electroweak production, shown in their figure 10. Tchi1n1A assumes wino-like $\tilde{\chi}_1^\pm\tilde{\chi}_1^0$ production, while Tchi1ch1A assumes higgsino-like cross sections and includes $\tilde{\chi}_1^\pm\tilde{\chi}_1^0$, $\tilde{\chi}_1^0\tilde{\chi}_2$ and $\tilde{\chi}_1^0\tilde{\chi}_2^\pm$ production. For $\tilde{\chi}_1^0\tilde{\chi}_2$ alone no mass point can be excluded in the model Tchi1ch1A, but in another model for $\tilde{\chi}_1^0\tilde{\chi}_2^0$ production, Tn1n2A.

⁷ TUMASYAN 23AY searched in 138 fb⁻¹ of pp collisions at √s = 13 TeV for evidence of gluino pair production in events with a single electron or muon and multiple hadronic jets. No significant excess above the Standard Model expectations is observed. Limits are set in the models Tglu3A and Tglu1B, see their figure 11. For Tglu1B, the chargino mass is set to $m_{\tilde{\chi}_1^+} = 0.5 (m_{\tilde{g}} + m_{\tilde{\chi}_1^0})$.

⁸ AAD 22u searched for the signature of disappearing track from a long-lived chargino in 139 fb⁻¹ of pp collisions at √s = 13 TeV. Long-lived charginos decay into quasi-degenerate neutralino emitting a low-momentum particle whose identification is not attempted. The signal is identified by requiring short tracklets in the four pixel layers with no continuation in the SCT (strip) detector. The main background from fake tracklets is estimated directly with the data. No significant excess above the background prediction is found. The results are interpreted in an AMSB scenario (win LSP), on $pp \to \tilde{\chi}^\pm\tilde{\chi}^\pm$ and $pp \to \tilde{\chi}^\pm\tilde{\chi}_1^0$, assuming $B(\tilde{\chi}^\pm \to \tilde{\chi}_1^0\pi^\pm) = 100\%$, see their figure 7. Results are also interpreted in a higgsino-LSP model, with $pp \to \tilde{\chi}^\pm\tilde{\chi}^\mp$, and $pp \to \tilde{\chi}^\pm\tilde{\chi}_1^0\tilde{\chi}_2^0$, assuming $B(\tilde{\chi}^\pm \to \tilde{\chi}_1^0\pi^\pm) = 95.5\%$, $B(\tilde{\chi}^\pm \to \tilde{\chi}_1^0e^\pm) = 3\%$, $B(\tilde{\chi}^\pm \to \tilde{\chi}_1^0\mu^\pm) = 1.5\%$, see their figure 8. Finally, results are interpreted in a simplified model of gluino pair production, with $pp \to \tilde{g}\tilde{g}$ and $B(\tilde{g} \to qq\tilde{\chi}_1^0) = B(\tilde{g} \to qq\tilde{\chi}^+) = B(\tilde{g} \to qq\tilde{\chi}^-) = 1/3$, see their figure 9.

⁹ TUMASYAN 22v searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for evidence of electroweak pair production with decay to two Higgs bosons H, with H → bD, resulting either in 4 resolved b-jets or two large-radius jets, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the mass of $\tilde{\chi}_2^0$ and $\tilde{\chi}_1^\pm$ in the models Tn1n1A, see their Figures 11 and 12, or in a model where higgsino-like nearly mass degenerate $\tilde{\chi}_2^0$ and $\tilde{\chi}_1^0$ are pair produced and each decay to H and a bino-like $\tilde{\chi}_1^0$, see their Figure 13. Limits are also set on the gluino mass in the model Tglu1I, see their Figure 14.

¹⁰ AAD 21AK searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for pair production of gluinos and squarks in events with a single isolated electron or muon, originating from the decay of a W boson, multiple jets and significant E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1B simplified model and on the squark mass in the Tsqk3 simplified model, see their Figure 8.

¹¹ AAD 21l searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for pair production of gluinos and squarks in events with jets, large missing transverse momentum but no electrons or muons. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A and Tglu1B simplified models, on the squark mass in the Tsqk1 and Tsqk3 simplified models and in a simplified model for gluino-squark production, see their Figures 13-17.

¹² AAD 21x searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for the decay of long-lived R-hadrons stopped by the calorimeter, producing high-momentum jets resulting in large out-of-time energy deposits in the calorimeters. These decays are detected using data collected during periods in the LHC bunch structure when collisions are absent. No significant excess above the predicted background is observed. Limits are set on the R-hadron mass in the Tglu1A simplified model ad a function of the R-hadron lifetime, for different $m_{\tilde{\chi}_1^0}$. See Figures 9, 10.

¹³ SIRUNYAN 21AD searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for supersymmetry in events with multiple jets, no leptons, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the top squark mass in the simplified models Tstop1, Tstop2 with $m_{\tilde{\chi}_1^\pm} = (m_{\tilde{t}} + m_{\tilde{\chi}_1^0})/2$, and a 50:50 mixture of these with $m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_1^0} = 5$ GeV, see their Figure 8. Limits are also set on the top squark mass for 10 GeV $< m_{\tilde{t}} - m_{\tilde{\chi}_1^\pm} < 80$ GeV in the simplified models Tstop2, Tstop 3, and Tstop4, see their Figure 9. For indirect top squark production, limits are set on the gluino mass in the simplified models Tglu3A, Tglu3C with $m_{\tilde{t}} - m_{\tilde{\chi}_1^0} = 20$ GeV, and Tglu3D with $m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_1^0} = 5$ GeV, see their Figure 10.

¹⁴ SIRUNYAN 21M searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for supersymmetry in events with two opposite-sign same-flavor leptons (electrons, muons) and E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the simplified model Tglu4C, see their Figure 10, on the $\tilde{\chi}_1^0\tilde{\chi}_2^0$ and $\tilde{\chi}_1^0$ mass in Tchi1n2Fa, see their Figure 11, on the $\tilde{\chi}_1^0$ mass in Tn1n1C and Tn1n1B for $m_{\tilde{\chi}_1^0} = m_{\tilde{\chi}_1^0} = m_{\tilde{\chi}_1^0}$, see their Figure 12. Limits are also set on the light squark mass for the simplified model Tsqk2A, on the bottom mass in Tstbot3, see their Figure 13, and on the slepton mass in direct electroweak pair production of mass-degenerate left- and right-handed sleptons (electrons and muons), see Figure 14.

¹⁵ AAD 20AL searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for events with 8 or more jets and moderate missing transverse momentum. The selection makes requirements according to the number of b-tagged jets and the scalar sum of masses of large-radius jets. No significant excess above the Standard Model expectations is observed. Limits up to about 2 TeV are set on the gluino mass in Tglu1E simplified model. Limits up to about 1.8 TeV are set on the gluino mass in Tglu3A simplified model. See their Fig. 10(a).

¹⁶ AAD 20v searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV in final states with same-sign charged leptons (electrons or muons) and jets. No significant excess above the Standard Model expectation is observed. In the Tglu1E model, considering off-shell intermediate W and Z bosons in the decay chains, gluino masses are excluded at 95% C.L. up to 1600 GeV for neutralino masses of 100 GeV or above (up to 1000 GeV). See their Fig. 7(a).

¹⁷ SIRUNYAN 20b searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one photon and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on chargino masses in a general gauge-mediated SUSY breaking (GGM) scenario Tchi1n12-GGM, see Figure 4. Limits are also set on the NLSP mass in the Tchi1ch1F and Tchi1ch1G simplified models, see their Figure 5. Finally, limits are set on the gluino mass in the Tglu4A simplified model, see Figure 6.

¹⁸ SIRUNYAN 20BJ searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for events containing two hadronically decaying, highly energetic Z bosons and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1H simplified model, see their Figure 9.

¹⁹ SIRUNYAN 20E searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for events with a single electron or muon and multiple jets, including at least one identified as originating from a b-quark, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A simplified model, see their Fig. 10, and the Tglu3C simplified model, see their Fig. 11.

²⁰ SIRUNYAN 20T searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least two jets, and two isolated same-sign or three or more charged leptons (electrons or muons). No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A, Tglu3B, Tglu3C and Tglu3D simplified models, see their Figure 7, and in the Tglu1C and Tglu1B simplified models, see their Figures 8 and 9. Limits are also set on the bottom mass in the Tstbot2 simplified model, see their Figure 10, and on the stop mass in the Tstop7 simplified model, see their Figure 11. Finally, limits are set on the gluino mass in RPV simplified models where the gluino decays either via $\tilde{g} \to q\bar{q}\bar{q} + e/\mu/\tau$ or via $\tilde{g} \to t\bar{s}$, see Figure 12.

²¹ AABOUD 19I searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in final states with hadronic jets, 1 or two hadronically decaying $\tau$ and E<sub>T</sub>. In Tglu1F, gluino masses are excluded at 95% C.L. up to 2000 GeV for neutralino masses of 100 GeV or below. Neutralino masses up to 1000 GeV are excluded for all gluino masses below 1400 GeV. See their Fig. 9. Limits are also presented in the context of Gauge-Mediated Symmetry Breaking models: in this case, values of $\Lambda$ below 110 TeV are excluded at the 95% CL for all values of $\tan\beta$ in the range $2 < \tan\beta < 60$, see their Fig. 10.

²² SIRUNYAN 19AG searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with two photons and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu4B simplified model and on the squark mass in the Tsqk4B simplified model, see their Figure 3.

²³ SIRUNYAN 19AU searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one photon, jets, some of which are identified as originating from b-quarks, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. In the framework of GMSB, limits are set on the gluino mass in the Tglu4C, Tglu4D and Tglu4E simplified models, and on the top squark mass in the Tstop13 simplified model, see their Figure 5.

²⁴ SIRUNYAN 19CE searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for new particles decaying to a photon and two gluons in events with at least three large-radius jets of which two have substructure and are composed of a photon and two gluons. No statistically significant excess is observed above the SM background expectation. Upper limits at 95% confidence level on the cross section for gluino pair production are set, using a simplified Tglu1A-like stealth SUSY model. Gluino masses up to 1500-1700 GeV are excluded, depending on the neutralino mass, with the highest exclusion set for $m_{\tilde{\chi}_1^0} = 200$ GeV. See their Fig. 4.

²⁵ SIRUNYAN 19CH searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for events containing multiple jets and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu1C, Tglu2A and Tglu3A simplified models, see their Figure 13. Limits are also set on squark, bottom and stop masses in the Tsqk1, Tstbot1, Tstop1 simplified models, see their Figure 14.

²⁶ SIRUNYAN 19K searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with a photon, an electron or muon, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. In the framework of GMSB, limits are set on the chargino and neutralino mass in the Tchi1n1A simplified model, see their Figure 6. Limits are also set on the gluino mass in the Tglu4A simplified model, and on the squark mass in the Tsqk4A simplified model, see their Figure 7.

²⁷ SIRUNYAN 19S searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with zero or one charged leptons, jets and E<sub>T</sub>. The razor variables $(M_R$ and $R^2$) are used to categorize the events. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu3C simplified models, see Figures 22 and 23, and on the stop mass in the Tstop1 simplified model, see their Figure 24.

²⁸ AABOUD 18AR searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for gluino pair production in events containing large missing transverse momentum and several energetic jets, at least three of which must be identified as originating from b-quarks. No excess is found above the predicted background. In Tglu3A models, gluino masses of less than 1.97 TeV are excluded for $m_{\tilde{\chi}_1^0}$ below 300 GeV, see their Fig. 10(a). Interpretations are also provided for scenarios where Tglu3A modes mix with Tglu2A and Tglu3D, see their Fig. 11.

²⁹ AABOUD 18AR searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for gluino pair production in events containing large missing transverse momentum and several energetic jets, at least three of which must be identified as originating from b-quarks. No excess is found above the predicted background. In Tglu2A models, gluino masses of less than 1.92 TeV are excluded for $m_{\tilde{\chi}_1^0}$ below 600 GeV, see their Fig. 10(b). Interpretations are also provided for scenarios where Tglu2A modes mix with Tglu3A and Tglu3D, see their Fig. 11.

³⁰ AABOUD 18AS searched for in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for gluino pair production in the context of AMSB or phenomenological MSSM scenarios with wino-like LSP and long-lived charginos. Events with a disappearing track due to a low-momentum pion accompanied by at least four jets are considered. No significant excess above the Standard Model expectations is observed. Exclusion limits are set at 95% confidence level on the mass of gluinos for different chargino lifetimes. Gluino masses up to 1.65 TeV are excluded assuming a chargino mass of 460 GeV and lifetime of 0.2 ns, corresponding to a mass-splitting between the charged and neutral wino of around 160 MeV. See their Fig. 9.

³¹ AABOUD 18BJ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with two opposite-sign charged leptons (electrons and muons), jets and missing transverse momentum, with various requirements to be sensitive to signals with different kinematic endpoint values in the dilepton invariant mass distribution. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1G model: gluino masses below 1850 GeV are excluded for $m_{\tilde{\chi}_1^0} = 100$ GeV, see their Fig. 12(a).
<footnote n="32">32 AABOUD 18BJ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with two opposite-sign charged leptons (electrons and muons), jets and missing transverse momentum, with various requirements to be sensitive to signals with different kinematic endpoint values in the dilepton invariant mass distribution. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1H model: gluino masses below 1650 GeV are excluded for m<sub>χ̃0</sub> = 100 GeV, see their Fig. 13(a).</footnote>

<footnote n="33">33 AABOUD 18U searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with at least one isolated photon, possibly jets and significant transverse momentum targeting generalised models of gauge-mediated SUSY breaking. No significant excess of events is observed above the SM prediction. Results for the di-photon channel are interpreted in terms of lower limits on the masses of gluinos in Tglu4B models, which reach as high as 2.3 TeV. Gluinos with masses below 2.15 TeV are excluded for any NLSP mass, see their Fig. 8.</footnote>

<footnote n="34">34 AABOUD 18U searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with at least one isolated photon, possibly jets and significant transverse momentum targeting generalised models of gauge-mediated SUSY breaking. No significant excess of events is observed above the SM prediction. Results of the γ + jets + E<sub>T</sub> channel are interpreted in terms of lower limits on the masses of gluinos in GGM higgsino-bino models (mix of Tglu4B and Tglu4C), which reach as high as 2050 GeV. Gluino masses below 1600 GeV are excluded for any NLSP mass provided that m<sub>g̃</sub> - m<sub>χ̃0</sub> > 50 GeV. See their Fig. 11.</footnote>

<footnote n="35">35 AABOUD 18V searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with no charged leptons, jets and missing transverse momentum. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1A model: gluino masses below 2030 GeV are excluded for massless LSP, see their Fig. 13(b).</footnote>

<footnote n="36">36 AABOUD 18V searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with no charged leptons, jets and missing transverse momentum. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1B model. Assuming that m<sub>χ̃±</sub> = 0.5 (m<sub>g̃</sub> + m<sub>χ̃0</sub>), gluino masses below 1980 GeV are excluded for massless LSP, see their Fig. 14(c). Exclusions are also shown assuming m<sub>χ̃0</sub> = 60 GeV, see their Fig. 14(d).</footnote>

<footnote n="37">37 AABOUD 18V searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with no charged leptons, jets and missing transverse momentum. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1E model: gluino masses below 1750 GeV are excluded for m<sub>χ̃0</sub> = 1 GeV and any m<sub>χ̃2</sub> above 100 GeV, see their Fig. 15. Gluino mass exclusion up to 2 TeV is found for m<sub>χ̃0</sub> = 1 TeV.</footnote>

<footnote n="38">38 SIRUNYAN 18AA searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one photon and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on gluino masses in a general gauge-mediated SUSY breaking (GGM) scenario with bino-like χ̃<sub>1</sub> and wino-like χ̃<sub>1</sub> ± χ̃<sub>2</sub>, see Figure 7. Limits are also set on the NLSP mass in the Tchi1n1A and Tchi1ch1A simplified models, see their Figure 8. Finally, limits are set on the gluino mass in the Tglu4A and Tglu4B simplified models, see their Figure 9, and on the squark mass in the Tsqk4A and Tsqk4B simplified models, see their Figure 10.</footnote>

<footnote n="39">39 SIRUNYAN 18AC searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with a single electron or muon and multiple jets. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu1B simplified models, see their Figure 5.</footnote>

<footnote n="40">40 SIRUNYAN 18AL searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least three charged leptons, in any combination of electrons and muons, jets and significant E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu1C simplified models, see their Figure 5. Limits are also set on the bottom mass in the Tsbot2 simplified model, see their Figure 6, and on the stop mass in the Tstop7 simplified model, see their Figure 7.</footnote>

<footnote n="41">41 SIRUNYAN 18AR searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events containing two opposite-charge, same-flavour leptons (electrons or muons), jets and E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu4C simplified model, see their Figure 7. Limits are also set on the chargino/neutralino mass in the Tchi1n2F simplified models, see their Figure 8, and on the higgsino mass in the Tn1n1B and Tn1n1C simplified models, see their Figure 9. Finally, limits are set on the bottom mass in the Tsbot3 simplified model, see their Figure 10.</footnote>

<footnote n="42">42 SIRUNYAN 18AY searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events containing one or more jets and significant E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A and Tglu3A simplified models, see their Figure 3. Limits are also set on squark, squark and stop masses in the Tsqk1, Tsbot1, Tstop1 and Tstop4 simplified models, see their Figure 3. Finally, limits are set on long-lived gluino masses in a Tglu1A simplified model where the gluino is metastable or long-lived with proper decay lengths in the range 10⁻³ mm < cτ < 10⁵ mm, see their Figure 4.</footnote>

<footnote n="43">43 SIRUNYAN 18D searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events containing identified hadronically decaying top quarks, no leptons, and E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1 simplified model, see their Figure 8, and on the gluino mass in the Tglu3A, Tglu3B, Tglu3C and Tglu3E simplified models, see their Figure 9.</footnote>

<footnote n="44">44 SIRUNYAN 18M searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with one or more high-momentum Higgs bosons, decaying to pairs of b-quarks, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1l and Tglu1J simplified models, see their Figure 3.</footnote>

<footnote n="45">45 AABOUD 17AJ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.75 TeV are set on the gluino mass in Tglu3A simplified models in case of off-shell top squarks and for m<sub>χ̃0</sub> = 100 GeV. See their Figure 4(a).</footnote>

<footnote n="46">46 AABOUD 17AJ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.57 TeV are set on the gluino mass in Tglu1E simplified models (2-step models) for m<sub>χ̃0</sub> = 100 GeV. See their Figure 4(b).</footnote>

<footnote n="47">47 AABOUD 17AJ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.86 TeV are set on the gluino mass in Tglu1G simplified models for m<sub>χ̃0</sub> = 200 GeV. See their Figure 4(c).</footnote>

<footnote n="48">48 AABOUD 17AR searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with one isolated lepton, at least two jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 2.1 TeV are set on the gluino mass in Tglu1B simplified models, with x = (m<sub>χ̃±</sub> - m<sub>χ̃0</sub>) / (m<sub>g̃</sub> - m<sub>χ̃0</sub>) = 1/2. Similar limits are obtained for variable x and fixed neutralino mass, m<sub>χ̃0</sub> = 60 GeV. See their Figure 13.</footnote>

<footnote n="49">49 AABOUD 17AR searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with one isolated lepton, at least two jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.74 TeV are set on the gluino mass in Tglu1E simplified model. Limits up to 1.7 TeV are also set on pMSSM models leading to similar signal event topologies. See their Figure 13.</footnote>

<footnote n="50">50 AABOUD 17AY searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least four jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.8 TeV are set on the gluino mass in Tglu3A simplified models assuming m<sub>χ̃1</sub> - m<sub>χ̃0</sub> = 5 GeV. See their Figure 13.</footnote>

<footnote n="51">51 AABOUD 17AZ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least seven jets and large missing transverse momentum. Selected events are further classified based on the presence of large R-jets or b-jets and no leptons. No significant excess above the Standard Model expectations is observed. Limits up to 1.8 TeV are set on the gluino mass in Tglu1E simplified models. See their Figure 6b.</footnote>

<footnote n="52">52 AABOUD 17AZ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least seven jets and large missing transverse momentum. Selected events are further classified based on the presence of large R-jets or b-jets and no leptons. No significant excess above the Standard Model expectations is observed. Limits up to 1.54 TeV are set on the gluino mass in Tglu3A simplified models. See their Figure 7a.</footnote>

<footnote n="53">53 AABOUD 17N searched in 14.7 fb⁻¹ of pp collisions at √s = 13 TeV in final states with 2 same-flavor, opposite-sign leptons (electrons or muons), jets and large missing transverse momentum. In Tglu1J models, gluino masses are excluded at 95% C.L. up to 1300 GeV for m<sub>χ̃0</sub> = 0 GeV and m<sub>χ̃0</sub> = 1100 GeV. See their Fig. 12 for exclusion limits as a function of m<sub>χ̃0</sub>. Limits are also presented assuming m<sub>χ̃0</sub> = m<sub>χ̃1</sub> + 100 GeV, see their Fig. 13.</footnote>

<footnote n="54">54 AABOUD 17N searched in 14.7 fb⁻¹ of pp collisions at √s = 13 TeV in final states with 2 same-flavor, opposite-sign leptons (electrons or muons), jets and large missing transverse momentum. In Tglu1H models, gluino masses are excluded at 95% C.L. up to 1310 GeV for m<sub>χ̃0</sub> < 400 GeV and assuming m<sub>χ̃0</sub> = (m<sub>g̃</sub> + m<sub>χ̃1</sub>)/2. See their Fig. 15.</footnote>

<footnote n="55">55 AABOUD 17N searched in 14.7 fb⁻¹ of pp collisions at √s = 13 TeV in final states with 2 same-flavor, opposite-sign leptons (electrons or muons), jets and large missing transverse momentum. In Tglu1G models, gluino masses are excluded at 95% C.L. up to 1700 GeV for small m<sub>χ̃0</sub>. The results probe kinematic endpoints as small as m<sub>χ̃2</sub> - m<sub>χ̃0</sub> = (m<sub>g̃</sub> - m<sub>χ̃0</sub>)/2 = 50 GeV. See their Fig. 14.</footnote>

<footnote n="56">56 KHACHATRYAN 17I searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events containing four or more jets, no more than one lepton, and missing transverse momentum, using the razors variables (M<sub>R</sub> and R<sup>2</sup>) to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the gluino mass in the Tglu1A, Tglu2A and Tglu3A simplified models, see Figs. 16 and 17. Also, assuming gluinos decay only via three-body processes involving third-generation quarks plus a neutralino/chargino, and assuming m<sub>χ̃1</sub> = m<sub>χ̃0</sub> + 5 GeV, a branching ratio-independent limit on the gluino mass is given, see Fig. 16.</footnote>

<footnote n="57">57 KHACHATRYAN 17AD searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events containing at least four jets (including b-jets), missing transverse momentum and tagged top quarks. No evidence for an excess over the expected background is observed. Gluino masses up to 1550 GeV and neutralino masses up to 900 GeV are excluded at 95% C.L. See Fig. 13.</footnote>

<footnote n="58">58 KHACHATRYAN 17AD searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events containing at least four jets (including b-jets), missing transverse momentum and tagged top quarks. No evidence for an excess over the expected background is observed. Gluino masses up to 1450 GeV and neutralino masses up to 820 GeV are excluded at 95% C.L. See Fig. 13.</footnote>

<footnote n="59">59 KHACHATRYAN 17AS searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with a single electron or muon and multiple jets. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu1B simplified models, see their Fig. 7.</footnote>

<footnote n="60">60 KHACHATRYAN 17AW searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least three charged leptons, in any combination of electrons and muons, and significant E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu1C simplified models, and on the bottom mass in the Tsbot2 simplified model, see their Figure 4.</footnote>

<footnote n="61">61 KHACHATRYAN 17P searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with one or more jets and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A, Tglu3A, Tglu3B, Tglu3C and Tglu3D simplified models, see their Figures 7 and 8. Limits are also set on the squark mass in the Tsqk1 simplified model, see their Fig. 7, and on the bottom mass in the Tsbot1 simplified model, see Fig. 8. Finally, limits are set on the stop mass in the Tstop1, Tstop3, Tstop4, Tstop6 and Tstop7 simplified models, see Fig. 8.</footnote>

<footnote n="62">62 KHACHATRYAN 17V searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with two photons and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino and squark mass in the context of general gauge mediation models Tglu4B and Tsqk4, see their Fig. 4.</footnote>

<footnote n="63">63 SIRUNYAN 17AF searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with a single lepton (electron or muon), jets, including at least one jet originating from a b-quark, and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu3B simplified models, see their Figure 2.</footnote>

<footnote n="64">64 SIRUNYAN 17AY searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one photon, jets and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu4A and Tglu4B simplified models, see their Figure 2.</footnote>
simplified models, and on the squark mass in the Tskq4A and Tskq4B simplified models,
see their Figure 6.

65 SIRUNYAN 17A2 searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with one or more jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A, Tglu3A simplified models, see their Figures 6. Limits are also set on the squark mass in the Tskq1 simplified model (for single light squark and for 8 degenerate light squarks), on the bottom mass in the Tsgt01 simplified model and on the stop mass in the Tstop1 simplified model, see their Fig. 7. Finally, limits are set on the stop mass in the Tstop2, Tstop4 and Tstop8 simplified models, see Fig. 8.

66 SIRUNYAN 17P searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with multiple jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu1C, Tglu2A, Tglu3A and Tglu3D simplified models, see their Fig. 12. Limits are also set on the squark mass in the Tskq1 simplified model, on the stop mass in the Tstop1 simplified model, and on the bottom mass in the Tsgt01 simplified model, see Fig. 13.

67 SIRUNYAN 17S searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with two isolated same-sign leptons, jets, and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the mass of the gluino mass in the Tglu3A, Tglu3B, Tglu3C, Tglu3D and Tglu3B simplified models, see their Figures 5 and 6, and on the bottom mass in the Tsgt02 simplified model, see their Figure 6.

68 AABOUD 16AC searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV in final states with hadronic jets, 1 or two hadronically decaying τ and $E_T$. In Tglu1F, gluino masses are excluded at 95% C.L. up to 1570 GeV for neutralino masses of 100 GeV or below. Neutralino masses up to 700 GeV are excluded for all gluino masses between 800 GeV and 1500 GeV, while the strongest neutralino-mass exclusion of 750 GeV is achieved for gluino masses around 1400 GeV. See their Fig. 8. Limits are also presented in the context of Gauge-Mediated Symmetry Breaking models: in this case, values of A below 92 TeV are excluded at the 95% CL, corresponding to gluino masses below 2000 GeV. See their Fig. 9.

69 AABOUD 16J searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV in final states with one isolated electron or muon, hadronic jets, and $E_T$. Gluino-mediated pair production of stops with a nearly mass-degenerate stop and neutralino are targeted and gluino masses are excluded at 95% C.L. up to 1460 GeV. A 100% of stops decaying via charm + neutralino is assumed. The results are also valid in case of 4-body decays $t\bar{t} \to f'f'\chi_1^0\chi_1^0$. See their Fig. 8.

70 AABOUD 16M searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events with two photons, hadronic jets and $E_T$. No significant excess above the Standard Model expectations is observed. Exclusion limits at 95% C.L. are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for bino-like NLSP. See their Fig. 3.

71 AABOUD 16N searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events containing hadronic jets, large $E_T$, and no electrons or muons. No significant excess above the Standard Model expectations is observed. Gluino masses below 1510 GeV are excluded at the 95% C.L. in a simplified model with only gluinos and the lightest neutralino. See their Fig. 7b.

72 AABOUD 16N searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events containing hadronic jets, large $E_T$, and no electrons or muons. No significant excess above the Standard Model expectations is observed. Gluino masses below 1500 GeV are excluded at the 95% C.L. in a simplified model with gluinos decaying via an intermediate $\tilde{\chi}_1^\pm$ to two quarks, a W boson and a $\tilde{\chi}_1^0$, for $m_{\tilde{\chi}_1^0} = 200$ GeV. See their Fig. 8.

73 AAD 16AD searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events containing several energetic jets, of which at least three must be identified as b-jets, large $E_T$ and no electrons or muons. No significant excess above the Standard Model expectations is observed. For $\tilde{\chi}_1^0$ below 800 GeV, gluino masses below 1780 GeV are excluded at 95% C.L. for gluinos decaying via bottom squarks. See their Fig. 7a.

74 AAD 16AD searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events containing several energetic jets, of which at least three must be identified as b-jets, large $E_T$ and one electron or muon. Large-radius jets with a high mass are also used to identify highly boosted top squarks. No significant excess above the Standard Model expectations is observed. For $\tilde{\chi}_1^0$ below 700 GeV, gluino masses below 1760 GeV are excluded at 95% C.L. for gluinos decaying via top squarks. See their Fig. 7b.

75 AAD 16BB searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events with exactly two same-sign leptons or at least three leptons, multiple hadronic jets, b-jets, and $E_T$. No significant excess over the Standard Model expectation is found. Exclusion limits at 95% C.L. are set on the gluino mass in various simplified models (Tglu1D, Tglu1E, Tglu3A). See their Figs. 4a, 4b, and 4d.

76 AAD 16BG searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV in final states with one isolated electron or muon, hadronic jets, and $E_T$. The data agree with the SM background expectation in the six signal selections defined in the search, and the largest deviation is a 2.1 standard deviation excess. Gluinos are excluded at 95% C.L. up to 1600 GeV assuming they decay via the lightest chargino to the lightest neutralino as in the model Tglu1B for $m_{\tilde{\chi}_1^0} = 100$ GeV, assuming $m_{\tilde{\chi}_1^\pm} = (m_{\tilde{\tilde{g}}} + m_{\tilde{\chi}_1^0})/2$. See their Fig. 6.

77 AAD 16V searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events with $E_T$ various hadronic jet multiplicities from $\ge 7$ to $\ge 10$ and with various b-jet multiplicities. No significant excess over the Standard Model expectation is found. Exclusion limits at 95% C.L. are set on the gluino mass in one simplified model (Tglu1E) and a pMSSM-inspired model. See their Fig. 5.

78 KHACHATRYAN 16AM searched in 19.7 fb⁻¹ of pp collisions at √s = 8 TeV for events with highly boosted W-bosons and b-jets, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3C and Tglu3B simplified models, see Fig. 12.

79 KHACHATRYAN 16BJ searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with two isolated same-sign leptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the following simplified models: Tglu3A and Tglu3D, see Fig. 4, Tglu3B and Tglu3C, see Fig. 5, and Tglu1B, see Fig. 7.

80 KHACHATRYAN 16BS searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one energetic jet, no isolated leptons, and significant $E_T$, using the transverse mass variable $M_T$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A and Tglu3A simplified models, see Fig. 10 and Table 3.

81 KHACHATRYAN 16BY searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with two opposite-sign, same-flavour leptons, jets, and missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3C simplified model, see Fig. 4, and on bottom masses in the Tsgt03 simplified model, see Fig. 5.

82 KHACHATRYAN 16V searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least four energetic jets and significant $E_T$, no identified isolated electron or muon or charged track. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu1C, Tglu2A, and Tglu3A simplified models, see Fig. 8.

83 AAD 15BG searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for events with jets, missing $E_T$, and two opposite-sign same flavor isolated leptons featuring either a kinematic edge, or a peak at the Z-boson mass, in the invariant mass spectrum. No evidence for a statistically significant excess over the expected SM backgrounds are observed and 95% C.L. exclusion limits are derived in a GGM simplified model of gluino pair production where the gluino decays into quarks, a Z-boson, and a massless gravitino LSP, see Fig. 12. Also, limits are set in simplified models with slepton/neutrino intermediate states, see Fig. 13.

84 AAD 15BV summarized and extended ATLAS searches for gluinos and first- and second-generation squarks in final states containing jets and missing transverse momentum, with or without leptons or b-jets in the √s = 8 TeV data set collected in 2012. The paper reports the results of new interpretations and statistical combinations of previously published analyses, as well as new analyses. Exclusion limits at 95% C.L. are set on the gluino mass in several R-parity conserving models, leading to a generalized constraint on gluino masses exceeding 1150 GeV for lightest supersymmetric particle masses below 100 GeV. See their Figs. 10, 19, 20, 21, 23, 25, 26, 29-37.

85 AAD 15BX interpreted the results of a wide range of ATLAS direct searches for supersymmetry, during the first run of the LHC using the $\sqrt{s} = 7$ TeV and $\sqrt{s} = 8$ TeV data set collected in 2012, within the wider framework of the phenomenological MSSM (pMSSM). The integrated luminosity was up to 20.3 fb⁻¹. From an initial random sampling of 500 million pMSSM points, generated from the 19-parameter pMSSM, a total of 310,327 model points with $\tilde{\chi}_1^0$ LSP were selected each of which satisfies constraints from previous collider searches, precision measurements, cold dark matter energy density measurements and direct dark matter searches. The impact of the ATLAS Run 1 searches on this space was presented, considering the fraction of model points surviving, after projection into two-dimensional spaces of sparticle masses. Good complementarity is observed between different ATLAS analyses, with almost all showing regions of unique sensitivity. ATLAS searches have good sensitivity at LSP mass below 800 GeV.

86 AAD 15CA searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for events with one or more photons, hadronic jets or b-jets and $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for bino-like or higgsino-bino admixtures NLSP, see Fig. 8, 10, 11.

87 KHACHATRYAN 15AF searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events with at least two energetic jets and significant $E_T$, using the transverse mass variable $M_{T2}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay $\tilde{g} \to q\bar{q}\chi_1^0$ takes place with a branching ratio of 100%, see Fig. 13(a), or where the decay $\tilde{g} \to b\bar{b}\chi_1^0$ takes place with a branching ratio of 100%, see Fig. 13(b), or where the decay $\tilde{g} \to t\bar{t}\chi_1^0$ takes place with a branching ratio of 100%, see Fig. 13(c). See also Table 5. Exclusions in the CMSSM, assuming $\tan\beta = 30$, $A_0 = -2 \max(m_0, m_1/2)$ and $\mu > 0$, are also presented, see Fig. 15.

88 KHACHATRYAN 15I searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events in which b-jets and four W-bosons are produced. Five individual search channels are combined (fully hadronic, single lepton, same-sign dilepton, opposite-sign dilepton, multilepton). No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a simplified model where the decay $\tilde{g} \to t\bar{t}\chi_1^0$ takes place with a branching ratio of 100%, see Fig. 5. Also a simplified model with gluinos decaying into on-shell top squarks is considered, see Fig. 6.

89 KHACHATRYAN 15X searched in 19.3fb⁻¹ of pp collisions at √s = 8 TeV for events with at least two energetic jets, at least one of which is required to originate from a b quark, and significant $E_T$, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay $\tilde{g} \to b\bar{b}\chi_1^0$ and the decay $\tilde{g} \to t\bar{t}\chi_1^0$ takes place with branching ratios varying between 0, 50 and 100%, see Figs. 13 and 14.

90 AAD 14AE searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for strongly produced supersymmetric particles in events containing jets and large missing transverse momentum, and no electrons or muons. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set in several SUSY scenarios. For an interpretation in the minimal GMSB model, see their Fig. 8. For an interpretation in the mSUGRA/CMSSM with parameters $\tan\beta = 30$, $A_0 = -2 m_0$ and $\mu > 0$, see their Fig. 9.

91 AAD 14AG searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for events containing one hadronically decaying τ-lepton, zero or one additional light leptons (electrons or muons), jets and large missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set in several SUSY scenarios. For an interpretation in the minimal GMSB model, see their Fig. 8. For an interpretation in the mSUGRA/CMSSM with parameters $\tan\beta = 30$, $A_0 = -2 m_0$ and $\mu > 0$, see their Fig. 9. For an interpretation in the framework of natural Gauge Mediation, see Fig. 10. For an interpretation in the bRPV scenario, see their Fig. 11.

92 AAD 14X searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for events with at least four leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a general gauge-mediation model (GGM) where the decay $\tilde{g} \to q\bar{q}\chi_1^0$, with $\tilde{\chi}_1^0 \to t\bar{t}\ell^+\ell^-$, takes place with a branching ratio of 100%, for two choices of $\tan\beta = 1.5$ and 30, see Fig. 11. Also some constraints on the higgsino mass parameter $\mu$ are discussed.

93 CHATCHRYAN 14AH searched in 4.7 fb⁻¹ of pp collisions at √s = 7 TeV for events with at least two energetic jets and significant $E_T$, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on bottom masses in simplified models where the decay $\tilde{g} \to q\bar{q}\chi_1^0$ takes place with a branching ratio of 100%, see Fig. 28. Exclusions in the CMSSM, assuming $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, are also presented, see Fig. 26.
94 CHATRYCHYAN 14AH searched in 4.7 fb⁻¹ of pp collisions at √s = 7 TeV for events with at least two energetic jets and significant $E_T$, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. A second analysis requires at least one of the jets to be originating from a b-quark. No significant excess above the Standard Model expectations is observed. Limits are set on bottom masses in simplified models where the decay $\tilde{g} \to b\bar{b}\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, see Figs. 28 and 29. Exclusions in the CMSSM, assuming $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, are also presented, see Fig. 26.

95 CHATRYCHYAN 14AH searched in 4.7 fb⁻¹ of pp collisions at √s = 7 TeV for events with at least two energetic jets and significant $E_T$, using the razor variables ($M_R$ and $R^2$) to discriminate between signal and background processes. A second analysis requires at least one of the jets to be originating from a b-quark. No significant excess above the Standard Model expectations is observed. Limits are set on bottom masses in simplified models where the decay $\tilde{g} \to t\bar{t}\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, see Figs. 28 and 29. Exclusions in the CMSSM, assuming $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, are also presented, see Fig. 26.

96 CHATRYCHYAN 14I searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events containing multijets and large $E_T$. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing gluinos that decay via $\tilde{g} \to q\bar{q}\tilde{\chi}_0^1$ with a 100% branching ratio, see Fig. 7b, or via $\tilde{g} \to t\bar{t}\tilde{\chi}_0^1$ with a 100% branching ratio, see Fig. 7c, or via $\tilde{g} \to q\bar{q}W/Z\tilde{\chi}_0^1$, see Fig. 7d.

97 CHATRYCHYAN 14N searched in 19.3 fb⁻¹ of pp collisions at √s = 8 TeV for events containing a single isolated electron or muon and multiple jets, at least two of which are identified as originating from a b-quark. No significant excess over the expected SM backgrounds are observed. The results are interpreted in three simplified models of gluino pair production with subsequent decay into virtual or on-shell top squarks, where each of the top squarks decays in turn into a top quark and a $\tilde{\chi}_0^1$, see Fig. 4. The models differ in which masses are allowed to vary.

98 CHATRYCHYAN 14R searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events with at least three leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a slepton co-NLSP simplified model (GMSB) where the decay $\tilde{g} \to q\ell^\pm\ell^\mp\tilde{g}$ takes place with a branching ratio of 100%, see Fig. 8.

99 CHATRYCHYAN 14R searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events with at least three leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a simplified model where the decay $\tilde{g} \to t\bar{t}\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, see Fig. 11.

100 AABOUD 18BJ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with two opposite-sign charged leptons (electrons and muons), jets and missing transverse momentum, with various requirements to be sensitive to signals with different kinematic endpoint values in the dilepton invariant mass distribution. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1H model in case of $m_{\tilde{\chi}_0^1} = 1$ GeV: for any $m_{\tilde{\chi}_0^1}$, gluino masses below 1500 GeV are excluded, see their Fig. 14(a).

101 AABOUD 18V searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV in events with no charged leptons, jets and missing transverse momentum. The data are found to be consistent with the SM expectation. Results are interpreted in a Tglu1C-like model, assuming 50% BR for each gluino decay mode. Gluino masses below 1770 GeV are excluded for any $m_{\tilde{\chi}_0^1} - m_{\tilde{\chi}_0^1}$ and $m_{\tilde{\chi}_0^1} = 60$ GeV, see their Fig. 16(b).

102 AABOUD 17AZ searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least seven jets and large missing transverse momentum. Selected events are further classified based on the presence of large J-jets or b-jets and no leptons. No significant excess above the Standard Model expectations is observed. Limits are set for pMSSM models with $M_1 = 60$ GeV, $\tan(\beta) = 10$, $\mu < 0$ varying the soft-breaking parameters $M_3$ and $\mu$. Gluino masses up to 1600 GeV are excluded for $m_{\tilde{\chi}_1^\pm} = 200$ GeV. See their Figure 6a and text for details on the model.

103 KHACHATRYAN 16AY searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with one isolated high transverse momentum lepton (e or μ), hadronic jets of which at least one is identified as coming from a b-quark, and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A simplified model, see Fig. 10, and in the Tglu3B model, see Fig. 11.

104 CHACHATRYAN 16BT performed a global Bayesian analysis of a wide range of CMS results obtained with data samples corresponding to 5.0 fb⁻¹ of pp collisions at √s = 7 TeV and in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV. The set of searches considered, both individually and in combination, includes those with all-hadronic final states, same-sign and opposite-sign dileptons, and multi-lepton final states. An interpretation was given in a scan of the 19-parameter pMSSM. No scan points with a gluino mass less than 500 GeV survived and 98% of models with a squark mass less than 300 GeV were excluded.

105 AAD 15AB searched for the decay of neutral, weakly interacting, long-lived particles in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV. Signal events require at least two reconstructed vertices possibly originating from long-lived particles decaying to jets in the inner tracking detector and muon spectrometer. No significant excess of events over the expected background was found. Results were interpreted in Stealth SUSY benchmark models where a pair of gluinos decay to long-lived singlinos, $\tilde{s}$, which in turn each decay to a low-mass gravitino and a pair of jets. The 95% confidence-level limits are set on the cross section × branching ratio for the decay $\tilde{g} \to Sg$, as a function of the singlino proper lifetime ($\tau_c$). See their Fig. 10(f).

106 AAD 15AI searched in 20 fb⁻¹ of pp collisions at √s = 8 TeV for events containing at least one isolated lepton (electron or muon), jets, and large missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95% C.L. are set on the gluino mass in the CMSSM/mSUGRA, see Fig. 15, in the NUHMG, see Fig. 16, and in various simplified models, see Figs. 18–22.

107 AAD 15CB searched for events containing at least one long-lived particle that decays at a significant distance from its production point (displaced vertex, DV) into two leptons or into five or more charged particles in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV. The dilepton signature is characterised by DV formed from at least two lepton candidates. Four different final states were considered for the multilactus signature, in which the DV must be accompanied by a high-transverse momentum muon or electron candidate that originates from the DV, jets or missing transverse momentum. No events were observed

in any of the signal regions. Results were interpreted in SUSY scenarios involving R-parity violation, split supersymmetry, and gauge mediation. See their Fig. 12–20.

108 KHACHATRYAN 15AD searched in 19.4 fb⁻¹ of pp collisions at √s = 8 TeV for events with two opposite-sign same flavor isolated leptons featuring either a kinematic edge, or a peak at the Z-boson mass, in the invariant mass spectrum. No evidence for a statistically significant excess over the expected SM backgrounds is observed and 95% C.L. exclusion limits are derived in a simplified model of gluino pair production where the gluino decays into quarks, a Z-boson, and a massless gravitino LSP, see Fig. 9.

109 KHACHATRYAN 15AZ searched in 19.7 fb⁻¹ of pp collisions at √s = 8 TeV for events with either at least one photon, hadronic jets and $E_T$ (single photon channel) or with at least two photons and at least one jet and using the razor variables. No significant excess above the Standard Model expectations is observed. Limits are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for both a bino-like and wino-like neutralino NLSP scenario, see Fig. 8 and 9.

110 AAD 14AX searched in 20.1 fb⁻¹ of pp collisions at √s = 8 TeV for the strong production of supersymmetric particles in events containing either zero or at last one high-$p_T$ lepton, large missing transverse momentum, high jet multiplicity and at least three jets identified as originating from b-quarks. No excess over the expected SM background is observed. Limits are derived in mSUGRA/CMSSM models with $\tan\beta = 30$, $A_0 = -2m_0$ and $\mu > 0$, see their Fig. 14. Also, exclusion limits in simplified models containing gluinos and scalar top and bottom quarks are set, see their Figures 12, 13.

111 AAD 14E searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for strongly produced supersymmetric particles in events containing jets and two same-sign leptons or three leptons. The search also utilises jets originating from b-quarks, missing transverse momentum and other variables. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing gluinos and squarks, see Figures 5 and 6. In the $\tilde{g} \to q\bar{q}'\tilde{\chi}_0^1$, $\tilde{\chi}_0^1 \to W^*(\ell^\pm)\tilde{\chi}_0^2$, $\tilde{\chi}_0^2 \to Z^*(\ell^\pm)\tilde{\chi}_0^1$ simplified model, the following assumptions have been made: $m_{\tilde{\chi}_0^1} = 0.5$, $m_{\tilde{\chi}_0^1} + m_{\tilde{g}} = m_{\tilde{\chi}_0^2} = 0.5$ ($m_{\tilde{\chi}_0^1} + m_{\tilde{\chi}_0^2} < 520$ GeV. In the $\tilde{g} \to q\bar{q}'\tilde{\chi}_0^1$, $\tilde{\chi}_0^1 \to \ell^\pm\ell^\mp(\nu\nu)\tilde{\chi}_0^1$ simplified model, the following assumptions have been made: $m_{\tilde{\chi}_0^1} = m_{\tilde{\chi}_0^2} = 0.5$ ($m_{\tilde{\chi}_0^1} + m_{\tilde{g}} = m_{\tilde{\chi}_0^2} < 660$ GeV. Limits are also derived in the mSUGRA/CMSSM, DRPV and GMSB models, see their Fig. 8.

112 CHATRYCHYAN 14H searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay $\tilde{g} \to t\bar{t}\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, or where the decay $\tilde{g} \to \tilde{t}t$, $\tilde{t} \to t\bar{t}\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, with varying mass of the $\tilde{\chi}_0^1$, or where the decay $\tilde{g} \to b\bar{b}$, $b \to t\bar{t}\tilde{\chi}_0^1$, $\tilde{\chi}_0^1 \to W^\pm\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, with varying mass of the $\tilde{\chi}_0^1$, see Fig. 5.

113 CHATRYCHYAN 14H searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay $\tilde{g} \to q\bar{q}'\tilde{\chi}_0^1$, $\tilde{\chi}_0^1 \to W^\pm\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, with varying mass of the $\tilde{\chi}_0^1$ and $\tilde{\chi}_0^2$, see Fig. 7.

114 CHATRYCHYAN 14H searched in 19.5 fb⁻¹ of pp collisions at √s = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay $\tilde{g} \to b\bar{t}\tilde{\chi}_0^1$, $\tilde{\chi}_0^1 \to W^\pm\tilde{\chi}_0^1$ takes place with a branching ratio of 100%, for two choices of $m_{\tilde{\chi}_0^1}$ and fixed $m_{\tilde{\chi}_0^2}$, see Fig. 6.

R-parity violating heavy $\tilde{g}$ (Gluino) mass limit

<table><thead><tr><th>VALUE (GeV)</th><th>CL<sub>95</sub></th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&gt;2200</td><td>95</td><td>1 AAD</td><td>21BF ATLS</td><td>l<sup>±</sup> + b-jets + many jets, Tglu3F, λ<sup>0</sup><sub>11</sub> electroweakino decay, 500 GeV &lt; m<sub>χ<sub>0</sub><sup>1</sup></sub> &lt;</td></tr><tr><td>&gt;2250</td><td>95</td><td>1 AAD</td><td>21BF ATLS</td><td>l<sup>±</sup> + b-jets + many jets, Tglu3G, λ<sup>0</sup><sub>11</sub> electroweakino decay, 600 GeV &lt; m<sub>χ<sub>0</sub><sup>1</sup></sub> &lt;</td></tr><tr><td>&gt;2200</td><td>95</td><td>1 AAD</td><td>21BF ATLS</td><td>l<sup>±</sup> + b-jets + many jets, Tglu3B, λ<sup>0</sup><sub>11</sub> electroweakino decay, 600 GeV &lt; m<sub>χ<sub>0</sub><sup>1</sup></sub> &lt;</td></tr><tr><td>&gt;1800</td><td>95</td><td>1 AAD</td><td>21BF ATLS</td><td>l<sup>±</sup> + b-jets + many jets, Tglu3B, λ<sup>0</sup><sub>11</sub> 323, t decay, m<sub>t</sub> &lt;</td></tr><tr><td>&gt;2200</td><td>95</td><td>1 AAD</td><td>21BF ATLS</td><td>l<sup>±</sup> + b-jets + many jets, Tglu1A, λ', χ<sup>0</sup><sub>1</sub> decay with equal probability into e, μ, ν<sub>e</sub>, ν'μ, 400 GeV &lt; m<sub>χ<sub>0</sub><sup>1</sup></sub> &lt; 1700 GeV</td></tr><tr><td>&gt;2500</td><td>95</td><td>2 AAD</td><td>21Y ATLS</td><td>≥ 4ℓ, Tglu1A with χ<sup>0</sup><sub>1</sub> → l<sup>±</sup>l<sup>±</sup>ν, λ<sub>12k</sub> ≠ 0, m<sub>χ<sub>0</sub><sup>1</sup></sub> = 2200 GeV</td></tr><tr><td>&gt;1900</td><td>95</td><td>2 AAD</td><td>21Y ATLS</td><td>≥ 4ℓ, Tglu1A with χ<sup>0</sup><sub>1</sub> → l<sup>±</sup>l<sup>±</sup>ν, λ<sub>133</sub> ≠ 0, m<sub>χ<sub>0</sub><sup>1</sup></sub> = 1550 GeV</td></tr><tr><td>&gt;1600</td><td>95</td><td>3 AAD</td><td>20AL ATLS</td><td>8 or more jets + $E_T$, Tglu2RPV</td></tr><tr><td>&gt;1600</td><td>95</td><td>4 AAD</td><td>20V ATLS</td><td>same-sign l<sup>±</sup>l<sup>±</sup> + jets, g̃ → t b d simplified model</td></tr><tr><td>&gt;2150</td><td>95</td><td>5 SIRUNYAN</td><td>20T CMS</td><td>same-sign l<sup>±</sup>l<sup>±</sup> or ≥ 3l<sup>±</sup> + jets, g̃ → qqg̃q̃ + e/μ/τ simplified model</td></tr></tbody></table>
# Searches Particle Listings

## Supersymmetric Particle Searches

>1725 95 5 SIRUNYAN 20T CMS same-sign $\ell^\pm\ell^\pm$ or $\ge 3\ell^\pm$+jets, $\tilde{g} \to t\bar{b}s$ simplified model

>1500 95 6 SIRUNYAN 19F CMS $\tilde{g} \to jjj$ $\ge 4\ell, \lambda_{12k} \neq 0, m_{\tilde{\chi}_1^0} > 1000$ GeV

>2260 95 7 AABOUD 18Z ATLS $\tilde{g} \to jjj$ $\ge 4\ell, \lambda_{133} \neq 0, m_{\tilde{\chi}_1^0} > 500$ GeV

>1650 95 8 SIRUNYAN 18AK CMS $\tilde{g} \to t\bar{b}s, \lambda_{332}^{\prime\prime}$ coupling

>1690 95 9 SIRUNYAN 18D CMS top quark (hadronically decaying) + jets + $E_T$, Tglu3C, $m_{\tilde{\chi}_1^0} - m_{\tilde{\chi}_1^0} = 20$ GeV, $m_{\tilde{\chi}_1^0} = 0$ GeV

none 100-1410 95 10 SIRUNYAN 18EA CMS 2 large jets with four-parton substructure, $\tilde{g} \to 5q$

>2100 95 11 AABOUD 17AI ATLS $\ge 1\ell^+ \ge 8$ jets, Tglu3A and $\tilde{\chi}_1^0 \to uds, \lambda_{112}^{\prime\prime}$ coupling, $m_{\tilde{\chi}_1^0} = 1000$ GeV

>1650 95 12 AABOUD 17AI ATLS $\ge 1\ell^+ \ge 8$ jets, $\tilde{g} \to t\bar{t}, \tilde{t} \to b\bar{b}, \lambda_{323}^{\prime\prime}$ coupling, $m_{\tilde{\chi}_1^0} = 1000$ GeV

>1800 95 13 AABOUD 17AI ATLS $\ge 1\ell^+ \ge 8$ jets, Tglu1A and $\tilde{\chi}_1^0 \to q\bar{q}l, \lambda^{\prime\prime}$ coupling, $m_{\tilde{\chi}_1^0} = 1000$ GeV

>1800 95 14 AABOUD 17AJ ATLS same-sign $\ell^\pm\ell^\pm / 3\ell^+ + jets + E_T$, Tglu3A, $\lambda_{112}^{\prime\prime}$ coupling, $m_{\tilde{\chi}_1^0} = 50$ GeV

>1750 95 15 AABOUD 17AJ ATLS same-sign $\ell^\pm\ell^\pm / 3\ell^+ + jets + E_T$, Tglu1A and $\tilde{\chi}_1^0 \to q\bar{q}l, \lambda^{\prime\prime}$ coupling

>1450 95 16 AABOUD 17AJ ATLS same-sign $\ell^\pm\ell^\pm / 3\ell^+ + jets + E_T$, $\tilde{g} \to t\bar{t}_1$ and $\tilde{t}_1 \to sd, \lambda_{321}^{\prime\prime}$ coupling

>1450 95 17 AABOUD 17AJ ATLS same-sign $\ell^\pm\ell^\pm / 3\ell^+ + jets + E_T$, $\tilde{g} \to t\bar{t}_1$ and $\tilde{t}_1 \to bd, \lambda_{313}^{\prime\prime}$ coupling

>400 95 18 AABOUD 17AJ ATLS same-sign $\ell^\pm\ell^\pm / 3\ell^+ + jets + E_T$, $d_R \to tb(ts), \lambda_{313}^{\prime\prime}$ coupling ($\lambda_{321}^{\prime\prime}$) coupling

none 625-1375 95 19 AABOUD 17AZ ATLS $\ge 7$ jets+$E_T$, large R-jets and/or b-jets, $\tilde{g} \to t\bar{t}_1$ and $\tilde{t}_1 \to b\bar{b}, \lambda_{323}^{\prime\prime}$ coupling

none 600-650 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 100$ GeV

none 600-1030 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 900$ GeV

none 600-650 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 100$ GeV

none 600-1080 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 900$ GeV

none 600-680 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 900$ GeV

none 600-1080 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 900$ GeV

none 600-650 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 100$ GeV

none 600-1100 95 20 KHACHATRY..17Y CMS $\tilde{g} \to qqqqq, \lambda_{212}^{\prime\prime}$ coupling, $m_{\tilde{q}} = 900$ GeV

>1050 95 21 KHACHATRY..16BJ CMS same-sign $\ell^\pm\ell^\pm$, Tglu3A, $m_{\tilde{\chi}_1^0} < 800$ GeV

>1140 95 21 KHACHATRY..16BJ CMS same-sign $\ell^\pm\ell^\pm$, Tglu3B, $m_{\tilde{\chi}_1^0} = 20$ GeV, $m_{\tilde{\chi}_1^0} = 0$

>1030 95 22 KHACHATRY..16BX CMS $\tilde{g} \to t\bar{b}s, \lambda_{332}^{\prime\prime}$ coupling

>1150 95 23 AAD 15BV ATLS general RPC $\tilde{g}$ decays, $m_{\tilde{\chi}_1^0} < 100$ GeV

>1350 95 24 AAD 14X ATLS $\ge 4\ell^\pm, \tilde{g} \to q\bar{q}\tilde{\chi}_1^0, \tilde{\chi}_1^0 \to \ell^\pm\ell^\mp\nu$

>650 95 25 CHATRCHYAN14P CMS $\tilde{g} \to jjj$

none 200-835 95 25 CHATRCHYAN14P CMS $\tilde{g} \to jjj$

• • • We do not use the following data for averages, fits, limits, etc. • • •

>1875 95 26 AABOUD 18CF ATLS jets and large R-jets, Tglu2RPV and $\tilde{\chi}_1^0 \to q\bar{q}q, \lambda^{\prime\prime}$ coupling, $m_{\tilde{\chi}_1^0} = 1000$ GeV

>1400 95 27 KHACHATRY..16BX CMS $\tilde{g} \to q\bar{q}\tilde{\chi}_1^0, \tilde{\chi}_1^0 \to \ell^\ell\nu, \lambda_{121}$ or $\lambda_{122} \neq 0, m_{\tilde{\chi}_1^0} > 400$ GeV

>1600 95 23 AAD 15BV ATLS pMSSM, $M_1 = 60$ GeV, $m_{\tilde{q}} < 1500$ GeV

>1280 95 23 AAD 15BV ATLS mSUGRA, $m_0 > 2$ TeV

>1100 95 23 AAD 15BV ATLS via $\tilde{\tau}$, natural GMSB, all $m_{\tilde{\tau}} < 1000$ GeV

>1220 95 23 AAD 15BV ATLS $b$-jets, $\tilde{g} \to \tilde{t}_1 t$ and $\tilde{t}_1 \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0} < 1000$ GeV

>1180 95 23 AAD 15BV ATLS $b$-jets, $\tilde{g} \to \tilde{t}_1 t$ and $\tilde{t}_1 \to b\tilde{\chi}_1^\pm, m_{\tilde{\chi}_1^0} < 1000$ GeV, $m_{\tilde{\chi}_1^0} = 60$ GeV

>880 95 23 AAD 15BV ATLS jets, $\tilde{g} \to \tilde{t}_1 t$ and $\tilde{t}_1 \to sb, 400 < m_{\tilde{t}_1} < 1000$ GeV

>880 95 28 AAD 15CB ATLS $\ell, \tilde{g} \to (e/\mu)q\bar{q}$, benchmark gluino, neutralino masses

>600 95 28 AAD 15CB ATLS $\ell\ell/Z, \tilde{g} \to (e e/\mu\mu/\epsilon\mu)q\bar{q}, m_{\tilde{\chi}_1^0} = 400$ GeV and $0.7 < c\tau_{\tilde{\chi}_1^0} < 3 \times 10^5$ mm

>1000 95 29 AAD 15X ATLS $\ge 10$ jets, $\tilde{g} \to q\bar{q}\tilde{\chi}_1^0, \tilde{\chi}_1^0 \to q\bar{q}q, m_{\tilde{\chi}_1^0} = 500$ GeV

>917 95 29 AAD 15X ATLS $\ge 6,7$ jets, $\tilde{g} \to q\bar{q}q$ (light-quark, $\lambda^{\prime\prime}$ couplings)

>929 95 29 AAD 15X ATLS $\ge 6,7$ jets, $\tilde{g} \to q\bar{q}q$ (b-quark, $\lambda^{\prime\prime}$ couplings)

>1180 95 30 AAD 14AX ATLS $\ge 3$ b-jets + $E_T$, $\tilde{g} \to \tilde{t}_1 t\tilde{\chi}_1^0$, simplified model, $\tilde{t}_1 \to b\tilde{\chi}_1^\pm, m_{\tilde{\chi}_1^0} = 2m_{\tilde{\chi}_1^0}, m_{\tilde{\chi}_1^0} = 60$ GeV, $m_{\tilde{\chi}_1^0} < 1000$ GeV

>850 95 31 AAD 14E ATLS $\ell^\pm\ell^\pm(\ell^\mp) + jets, \tilde{g} \to t\tilde{t}_1$ with $\tilde{t}_1 \to b\bar{b}$ simplified model

>900 95 32 CHATRCHYAN14H CMS same-sign $\ell^\pm\ell^\pm, \tilde{g} \to t\bar{b}s$ simplified model

1 AAD 21BF searched in 139 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for pair production of gluinos, stops, electroweakinos decaying RPV either directly or indirectly via the LSP. The final state in all cases is one or two leptons, many jets (up to fifteen) and b-jets. Different models with different branching fractions of the gluino or stop follow from the assumptions on the nature of the electroweakinos. No significant excess above the Standard Model predictions is observed. Limits are set on the gluino, $\tilde{t}_1$, electroweakino masses as a function of the $\tilde{\chi}_1^0$ mass in several scenarios of gluino, stop and electroweakino pair production.

2 AAD 21Y searched in 139 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for supersymmetry in events with four or more leptons (electrons, muons and tau-leptons). No significant excess above the Standard Model expectations is observed. Limits are set on Tchi1n12-GGM, and RPV models similar to Tchi1n2l, Tglu1A (with $q = u, d, s, c, b$, with equal branching fractions), and $\ell_L/\bar{\nu} \to \ell/\nu\tilde{\chi}_1^0$ (mass-degenerate $\ell_L$ and $\bar{\nu}$ of all 3 generations), all with $\tilde{\chi}_1^0 \to \ell^\pm\ell^\mp\nu$ via $\lambda_{12k}$ or $\lambda_{133}$ (where $k \in 1,2$), see their Figure 11.

3 AAD 20AL searched in 139 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for events with 8 or more jets and moderate missing transverse momentum. The selection makes requirements according to the number of b-tagged jets and the scalar sum of masses of large-radius jets. No significant excess above the Standard Model expectations is observed. Exclusion limits at 95% C.L. are set on the gluino mass in RPV simplified models where the gluino decays via $\tilde{g} \to t\bar{b}g$ or $\tilde{g} \to t\bar{b}s$. They extend up to almost 1.6 TeV for a $\tilde{t}_1$ mass of 900 GeV. See their Fig. 10(c).

4 AAD 20V searched in 139 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for events with two same-sign charged leptons (electrons or muons) and jets. No significant excess above the Standard Model expectations is observed. Exclusion limits at 95% C.L. are set on the gluino mass in RPV simplified models where the gluino decays via $\tilde{g} \to t\bar{b}d$, see Figure 7(b).

5 SIRUNYAN 20T searched in 137 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for events with at least two jets, and two isolated same-sign or three or more charged leptons (electrons or muons). No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A, Tglu3B, Tglu3C and Tglu3D simplified models, see their Figure 7, and in the Tglu1C and Tglu1B simplified models, see their Figures 8 and 9. Limits are also set on the bottom mass in the Tsbot2 simplified model, see their Figure 10, and on the stop mass in the Tstop7 simplified model, see their Figure 11. Finally, limits are set on the gluino mass in RPV simplified models where the gluino decays either via $\tilde{g} \to q\bar{q}\tilde{q} + e/\mu/\tau$ or via $\tilde{g} \to t\bar{b}s$, see Figure 12.

6 SIRUNYAN 19F searched in 35.9 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for three-jet resonances produced in the decay of a gluino in R-parity violating supersymmetric models. The mass range from 200 to 2000GeV is explored in four separate mass regions. The observations show agreement with standard model expectations. The results are interpreted within the framework of R-parity violating SUSY, where pair-produced gluinos decay to a six quark final state. Gluino masses below 1500GeV are excluded at 95% C.L. See their Fig.5.

7 AABOUD 18Z searched in 36.1 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for events containing four or more charged leptons (electrons, muons and up to two hadronically decaying taus). No significant deviation from the expected SM background is observed. Limits are set on the Higgsing mass in simplified models of general gauge mediated supersymmetry $Tn1n1A/Tn1n1B/Tn1n1C$, see their Figure 9. Limits are also set on the wino, slepton, sneutrino and gluino mass in a simplified model of NLSP pair production with R-parity violating decays of the LSP via $\lambda_{12k}$ or $\lambda_{133}$ to charged leptons, see their Figures 7, 8.

8 SIRUNYAN 18AK searched in 35.9 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for events containing a single lepton, large jet and b-quark jet multiplicities, coming from R-parity-violating decays of gluinos. No excess over the expected background is observed. Limits are derived on the gluino mass, assuming the RPV $\tilde{g} \to t\bar{b}s$ decay, see their Figure 9.

9 SIRUNYAN 18D searched in 35.9 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for events containing identified hadronically decaying top quarks, no leptons, and $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1 simplified model, see their Figure 8, and on the gluino mass in the Tglu3A, Tglu3B, Tglu3C and Tglu3E simplified models, see their Figure 9.

10 SIRUNYAN 18EA searched in 38.2 fb$^{-1}$ of pp collisions at $\sqrt{s} = 13$ TeV for the pair production of resonances, each decaying to at least four quarks. Reconstructed particles are clustered into two large jets of similar mass, each consistent with four-parton
substructure. No statistically significant excess over the Standard Model expectation is observed. Limits are set on the squark and gluino mass in RPV supersymmetry models where squarks (gluinos) decay, through intermediate higgsinos, to four (five) quarks, see their Figure 4.

11 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with one or more isolated lepton, at least eight jets, either zero or many b-jets, for evidence of R-parity violating decays of the gluino. No significant excess above the Standard Model expectations is observed. Limits up to 2.1 TeV are set on the gluino mass in R-parity-violating supersymmetry models as Tglu3A with LSP decay through the non-zero $\lambda_{112}''$ coupling as $\tilde{\chi}_1^0 \to uds$. See their Figure 9.

12 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with one or more isolated lepton, at least eight jets, either zero or many b-jets, for evidence of R-parity violating decays of the gluino. No significant excess above the Standard Model expectations is observed. Limits up to 1.65 TeV are set on the gluino mass in R-parity-violating supersymmetry models with $\tilde{g} \to tt, t\bar{t} \to bss$ through the non-zero $\lambda_{323}''$ coupling. See their Figure 9.

13 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with one or more isolated lepton, at least eight jets, either zero or many b-jets, for evidence of R-parity violating decays of the gluino. No significant excess above the Standard Model expectations is observed. Limits up to 1.8 TeV are set on the gluino mass in R-parity-violating supersymmetry models as Tglu1A with the LSP decay through the non-zero $\lambda'$ coupling as $\tilde{\chi}_1^0 \to qq\ell$. See their Figure 9.

14 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.8 TeV are set on the gluino mass in R-parity-violating supersymmetry models as Tglu3A with LSP decaying through the non-zero $\lambda_{112}''$ coupling as $\tilde{\chi}_1^0 \to uds$. See their Figure 5(d).

15 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.75 TeV are set on the gluino mass in R-parity-violating supersymmetry models as Tglu1A with LSP decaying through the non-zero $\lambda'$ coupling as $\tilde{\chi}_1^0 \to qq\ell$. See their Figure 5(c).

16 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.45 TeV are set on the gluino mass in R-parity-violating supersymmetry models where $\tilde{g} \to t\bar{t}_1$ and $\tilde{t}_1 \to sd$ through the non-zero $\lambda_{321}''$ coupling. See their Figure 5(b).

17 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.45 TeV are set on the gluino mass in R-parity-violating supersymmetry models where $\tilde{g} \to t\bar{t}_1$ and $\tilde{t}_1 \to bd$ through the non-zero $\lambda_{313}''$ coupling. See their Figure 5(a).

18 AABOUD 17A1 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 400 GeV are set on the down type squark ($d_R$ mass in R-parity-violating supersymmetry models where $\tilde{d}_R \to tb$ through the non-zero $\lambda_{313}''$ coupling or $\tilde{d}_R \to ts$ through the non-zero $\lambda_{321}''$ coupling). See their Figure 5(e) and 5(f).

19 AABOUD 17A2 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with at least seven jets and large missing transverse momentum. Selected events are further classified based on the presence of large R-jets or b-jets and no leptons. No significant excess above the Standard Model expectations is observed. Limits are set for R-parity violating decays of the gluino assuming $\tilde{g} \to t\bar{t}_1$ and $\tilde{t}_1 \to bss$ through the non-zero $\lambda_{321}''$ couplings. The range 625-1375 GeV is excluded for $m_{\tilde{t}_1} = 400$ GeV. See their Figure 7b.

20 KHACHATRYAN 17γ searched in 19.7 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing at least 8 or 10 jets, possibly b-tagged, coming from R-parity-violating decays of supersymmetric particles. No excess over the expected background is observed. Limits are derived on the gluino mass, assuming various RPV decay modes, see Fig. 7.

21 KHACHATRYAN 16Bγ searched in 2.3 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the following simplified models: Tglu3A and Tglu3D, see Fig. 4, Tglu3B and Tglu3C, see Fig. 5, and Tglu1B, see Fig. 7.

22 KHACHATRYAN 16Bγ searched in 19.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing 0 or 1 leptons and b-tagged jets, coming from R-parity-violating decays of supersymmetric particles. No excess over the expected background is observed. Limits are derived on the gluino mass, assuming the RPV $\tilde{g} \to t\bar{t}_1$ and $\tilde{t}_1 \to bss$ decay, see Fig. 7 and 10.

23 AAD 15Bγ summarized and extended ATLAS searches for gluinos and first- and second-generation squarks in final states containing jets and missing transverse momentum, with or without leptons or b-jets in the $\sqrt{s} = 8$ TeV data set collected in 2012. The paper reports the results of new interpretations and statistical combinations of previously published analyses, as well as new analyses. Exclusion limits at 95% C.L. are set on the gluino mass in several R-parity conserving models, leading to a generalized constraint on gluino masses exceeding 1150 GeV for lightest supersymmetric particle masses below 100 GeV. See their Figs. 10, 19, 20, 21, 23, 25, 26, 29-37.

24 AAD 14x searched in 20.3 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with at least four leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in an R-parity violating simplified model where the decay $\tilde{g} \to q\bar{q}\chi_1^0$, with $\tilde{\chi}_1^0 \to \ell^\pm\ell\mp\nu$, takes place with a branching ratio of 100%, see Fig. 8.

25 CHATRCHYAN 14P searched in 19.4 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for three-jet resonances produced in the decay of a gluino in R-parity violating supersymmetric models. No excess over the expected SM background is observed. Assuming a 100% branching ratio for the gluino decay into three light-flavour jets, limits are set on the cross section of gluino pair production, see Fig. 7, and gluino masses below 650 GeV are excluded at 95% C.L. Assuming a 100% branching ratio for the gluino decaying to one b-quark jet and two light-flavour jets, gluino masses between 200 GeV and 835 GeV are excluded at 95% C.L.

26 AABOUD 18CF searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with several jets, possibly b-jets, and large-radius jets for evidence of R-parity violating decays of the gluino. No significant excess above the Standard Model expectations is

observed. Limits between 1000 and 1875 GeV are set on the gluino mass in R-parity-violating supersymmetry models as Tglu2RPV with the LSP decay through the non-zero $\lambda'$ coupling as $\tilde{\chi}_1^0 \to qq\ell$. The most stringent limit is obtained for $m_{\tilde{\chi}_1^0} = 1000$ GeV, the weakest for $m_{\tilde{\chi}_1^0} = 50$ GeV. See their Figure 7(b). Figure 7(a) presents results for gluinos directly decaying into 3 quarks, Tglu1RPV.

27 KHACHATRYAN 16Bγ searched in 19.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing 4 leptons coming from R-parity-violating decays of $\tilde{\chi}_1^0 \to \ell\ell\nu$ with $\lambda_{121} \neq 0$ or $\lambda_{122} \neq 0$. No excess over the expected background is observed. Limits are derived on the gluino, squark and stop masses, see Fig. 23.

28 AAD 15CB searched for events containing at least one long-lived particle that decays at a significant distance from its production point (displaced vertex, DV) into two leptons or into five or more charged particles in 20.3 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV. The dilepton signature is characterised by DV formed from at least two lepton candidates. Four different final states were considered for the multitakr signature, in which the DV must be accompanied by a high-transverse momentum muon or electron candidate that originates from the DV, jets or missing transverse momentum. No events were observed in any of the signal regions. Results were interpreted in SUSY scenarios involving R-parity violation, split supersymmetry, and gauge mediation. See their Fig. 12-20.

29 AAD 15X searched in 20.3 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events containing large number of jets, no requirements on missing transverse momentum and no isolated electrons or muons. The sensitivity of the search is enhanced by considering the number of b-tagged jets and the scalar sum of masses of large-radius jets in an event. No evidence was found for excess above the expected level of Standard Model background. Exclusion limits at 95% C.L. are set on the gluino mass assuming the gluino decays to various quark flavors, and for various neutralino masses. See their Fig. 11-16.

30 AAD 14AX searched in 20.1 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for the strong production of supersymmetric particles in events containing either zero or at last one high-$p_T$ lepton, large missing transverse momentum, high jet multiplicity and at least three jets identified as originating from b-quarks. No excess over the expected SM background is observed. Limits are derived in mSUGRA/CMSSM models with $\tan\beta = 30, A_0 = -2m_0$ and $\mu > 0$, see their Fig. 14. Also, exclusion limits in simplified models containing gluinos and scalar top and bottom quarks are set, see their Figures 12, 13.

31 AAD 14E searched in 20.3 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for strongly produced supersymmetric particles in events containing jets and two same-sign leptons or three leptons. The search also utilises jets originating from b-quarks, missing transverse momentum and other variables. The sensitivity of the search is enhanced by considering the number of mSUGRA/CMSSM models containing gluinos and squarks, see Figures 5 and 6. In the $\tilde{g} \to qq'\tilde{\chi}_1^\pm, \tilde{\chi}_1^\pm \to W^(*)\tilde{\chi}_2^0 \to Z^(*)\tilde{\chi}_1^0$ simplified model, the following assumptions have been made: $m_{\tilde{\chi}_1^0} = 0.5, m_{\tilde{\chi}_1^0} + m_{\tilde{g}} = m_{\tilde{\chi}_2^0} = 0.5, (m_{\tilde{\chi}_1^0} + m_{\tilde{\chi}_1^0}), m_{\tilde{\chi}_1^0} < 520$ GeV. In the $\tilde{g} \to qq'\tilde{\chi}_1^\pm, \tilde{\chi}_1^\pm \to \ell^\pm\nu\tilde{\chi}_1^0$ or $\tilde{g} \to qq'\tilde{\chi}_2^0, \tilde{\chi}_2^0 \to \ell^\pm\ell\mp(\nu\ell)\tilde{\chi}_1^0$ simplified model, the following assumptions have been made: $m_{\tilde{\chi}_1^0} = m_{\tilde{\chi}_2^0} = 0.5, (m_{\tilde{\chi}_1^0} + m_{\tilde{g}}), m_{\tilde{\chi}_1^0} < 660$ GeV. Limits are also derived in the mSUGRA/CMSSM, DRPV and GMSB models, see their Fig. 8.

32 CHATRCHYAN 14Hγ searched in 19.5 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the R-parity violating decay $\tilde{g} \to tbs$ takes place with a branching ratio of 100%, see Fig. 8.

## Long-lived $\tilde{g}$ (Gluino) mass limit

Limits on light gluinos ($m_{\tilde{g}} < 5$ GeV) were last listed in our PDG 14 edition: K. Olive, et al. (Particle Data Group), Chinese Physics C38 070001 (2014) (http://pdg.lbl.gov).

<table><thead><tr><th>VALUE (GeV)</th><th>CL%</th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&gt;2050</td><td>95</td><td>1 AAD</td><td>23G ATLS</td><td>R-hadrons, Tglu1A, stable, m<sub>χ̃1</sub> = 100 GeV</td></tr><tr><td>&gt;2270</td><td>95</td><td>1 AAD</td><td>23G ATLS</td><td>R-hadrons, Tglu1A, τ = 20 ns, m<sub>χ̃1</sub> = 100 GeV</td></tr><tr><td>&gt;2050</td><td>95</td><td>1 AAD</td><td>23G ATLS</td><td>R-hadrons, Tglu1A, stable, m<sub>g̃</sub> = m<sub>χ̃1</sub> = 30 GeV</td></tr><tr><td>&gt;2050</td><td>95</td><td>1 AAD</td><td>23G ATLS</td><td>R-hadrons, Tglu1A, τ = 20 ns, m<sub>g̃</sub> = m<sub>χ̃1</sub> = 30 GeV</td></tr><tr><td>&gt;2500</td><td>95</td><td>2 SIRUNYAN</td><td>21AF CMS</td><td>long-lived <i>g̃</i>, Tglu2RPV, λ<sub>323</sub><sup>′</sup> coupling, 0.6 mm &lt; cτ &lt; 90 mm</td></tr><tr><td>&gt;2450</td><td>95</td><td>3 SIRUNYAN</td><td>21U CMS</td><td>long-lived <i>g̃</i>, pp → <i>g̃g̃</i>, <i>g̃</i> → g<i>g̃</i>, GMSB, 6 &lt; cτ &lt; 550 mm</td></tr><tr><td>&gt;2500</td><td>95</td><td>3 SIRUNYAN</td><td>21U CMS</td><td>long-lived <i>g̃</i>, pp → <i>g̃g̃</i>, <i>g̃</i> → q<i>g̃</i><i>χ̃1</i><sup>0</sup>, mini-split, m<sub>χ̃1</sub><sup>0</sup> = 100 GeV, 7 &lt; cτ &lt; 360 mm</td></tr><tr><td>&gt;2500</td><td>95</td><td>3 SIRUNYAN</td><td>21U CMS</td><td>long-lived <i>g̃</i>, pp → <i>g̃g̃</i>, <i>g̃</i> → tbs, λ<sub>323</sub><sup>′</sup> coupling, 3 &lt; cτ &lt; 1000 mm</td></tr><tr><td>&gt;1980</td><td>95</td><td>4 AABOUD</td><td>19AT ATLS</td><td>R-hadrons, Tglu1A, metastable</td></tr><tr><td>&gt;2060</td><td>95</td><td>5 AABOUD</td><td>19C ATLS</td><td>R-hadrons, Tglu1A, τ ≥ 10 ns, m<sub>χ̃1</sub> = 100 GeV</td></tr><tr><td>&gt;1890</td><td>95</td><td>5 AABOUD</td><td>19C ATLS</td><td>R-hadrons, Tglu1A, stable</td></tr><tr><td>&gt;2400</td><td>95</td><td>6 SIRUNYAN</td><td>19BH CMS</td><td>long-lived <i>g̃</i>, RPV, <i>g̃</i> → t<b>D</b>s, 10 mm &lt; cτ &lt; 250 mm</td></tr><tr><td>&gt;2300</td><td>95</td><td>6 SIRUNYAN</td><td>19BH CMS</td><td>long-lived <i>g̃</i>, GMSB, <i>g̃</i> → g<i>g̃</i>, 20 mm &lt; cτ &lt; 110 mm</td></tr><tr><td>&gt;2100</td><td>95</td><td>7 SIRUNYAN</td><td>19BT CMS</td><td>long-lived <i>g̃</i>, GMSB, <i>g̃</i> → g<i>g̃</i>, 0.3 m &lt; cτ &lt; 30 mm</td></tr></tbody></table>