$> 780$ 
95 
^{ 1} 

ATLS 
$> 1060$ 
95 
^{ 1} 

ATLS 
$\bf{> 410}$ 
95 
^{ 2} 

ATLS 
• • • We do not use the following data for averages, fits, limits, etc. • • • 
$> 87$ 
95 
^{ 3} 

DLPH 
$>81$ 
95 
^{ 4} 

ALEP 
^{1}
AABOUD 2018Z searched in 36.1 ${\mathrm {fb}}{}^{1}$ of ${{\mathit p}}{{\mathit p}}$ 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 Higgsino 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 Rparity violating decays of the LSP via ${{\mathit \lambda}_{{12k}}}$ or ${{\mathit \lambda}_{{i33}}}$ to charged leptons, see their Figures 7, 8.

^{2}
AAD 2014X searched in 20.3 fb${}^{1}$ of ${{\mathit p}}{{\mathit p}}$ 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 slepton mass in an Rparity violating simplified model where the decay ${{\widetilde{\mathit \ell}}}$ $\rightarrow$ ${{\mathit \ell}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , with ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\mathit \nu}}$ , takes place with a branching ratio of 100$\%$, see Fig. 9.

^{3}
ABDALLAH 2004M use data from $\sqrt {s }$ = $192  208$~GeV to derive limits on sparticle masses under the assumption of RPV with ${{\mathit L}}{{\mathit L}}{{\overline{\mathit E}}}$ or ${{\overline{\mathit U}}}{{\overline{\mathit D}}}{{\overline{\mathit D}}}$ couplings. The results are valid for ${{\mathit \mu}}$ = $200$~GeV, tan ${{\mathit \beta}}$ = 1.5, $\Delta \mathit m$ $>$ 5~GeV and assuming a BR of 1 for the given decay. The limit quoted is for indirect ${{\overline{\mathit U}}}{{\overline{\mathit D}}}{{\overline{\mathit D}}}$ decays using the neutralino constraint of 39.5 GeV for ${{\mathit L}}{{\mathit L}}{{\overline{\mathit E}}}$ and of 38.0 GeV for ${{\overline{\mathit U}}}{{\overline{\mathit D}}}{{\overline{\mathit D}}}$ couplings, also derived in ABDALLAH 2004M. For indirect decays via ${{\mathit L}}{{\mathit L}}{{\overline{\mathit E}}}$ the limit improves to 90 GeV if the constraint from the neutralino is used and remains at 87 GeV if it is not used. For indirect decays via ${{\overline{\mathit U}}}{{\overline{\mathit D}}}{{\overline{\mathit D}}}$ couplings it degrades to 85 GeV when the neutralino constraint is not used. Supersedes the result of ABREU 2000U.

^{4}
HEISTER 2003G searches for the production of smuons in the case of RPV prompt decays with $\mathit LL\bar E$, $\mathit LQ\bar D$ or $\bar U \bar D \bar D$ couplings at $\sqrt {s }$ = $189  209~$GeV. The search is performed for direct and indirect decays, assuming one coupling at a time to be nonzero. The limit holds for direct decays mediated by RPV $\mathit LQ\bar D$ couplings and improves to 90 GeV for indirect decays (for $\Delta \mathit m>$ 10 GeV). Limits are also given for $\mathit LL\bar E$ direct (${\mathit m}_{{{\widetilde{\mathit \mu}}}{{\mathit R}}}$ $>$ 87~GeV) and indirect decays (${\mathit m}_{{{\widetilde{\mathit \mu}}}{{\mathit R}}}$ $>$ 96 GeV for ${{\mathit m}}({{\widetilde{\mathit \chi}}_{{1}}^{0}}$) $>$ 23 GeV from BARATE 1998S) and for $\bar U \bar D \bar D$ indirect decays (${\mathit m}_{{{\widetilde{\mathit \mu}}}{{\mathit R}}}$ $>$ 85 GeV for $\Delta \mathit m>$ 10 GeV). Supersedes the results from BARATE 2001B.

