is observed. Limits are set on the slepton mass up to 500 GeV for massless $\chi_1^0$, assuming degeneracy of $\tilde{e}, \tilde{\mu}$, and $\tilde{\tau}$ exploiting the 2$\ell$ signature, see their Figure 6(b).

⁹KHACHATRYAN 17L searched in about 19 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with two $\tau$ (at least one decaying hadronically) and $\tilde{E}_T$. Results were interpreted to set constraints on the cross section for production of $\tilde{\tau}_L$ pairs for $m_{\chi_1^0} = 1$ GeV. No mass constraints are set, see their Fig. 7.

¹⁰AAD 16AA summarized and extended ATLAS searches for electroweak supersymmetry in final states containing several charged leptons, $\tilde{E}_T$, with or without hadronic leptons, in 20 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV. The paper reports 95% C.L. exclusion limits on the cross-section for production of $\tilde{\tau}_R$ and $\tilde{\tau}_L$ pairs for various $m_{\chi_1^0}$, using the 2 hadronic $\tau + \tilde{E}_T$ analysis. The $m_{\tilde{\tau}_{R/L}} = 109$ GeV is excluded for $m_{\chi_1^0} = 0$ GeV, with the constraints being stronger for $\tilde{\tau}_R$. See their Fig. 12.

¹¹AAD 12AF searched in 2 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV for events with two tau leptons, jets and large $\tilde{E}_T$ in a GMSB framework. No significant excess above the expected background was found and an upper limit on the visible cross section for new phenomena is set. A 95% C.L. lower limit of 32 TeV on the mGMSB breaking scale $\Lambda$ is set for $M_{mess} = 250$ TeV, $N_S = 3$, $\mu > 0$ and $C_{grav} = 1$, independent of $\tan\beta$.

¹²AAD 12AG searched in 2.05 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV for events with at least one hadronically decaying tau lepton, jets, and large $\tilde{E}_T$ in a GMSB framework. No significant excess above the expected background was found and an upper limit on the visible cross section for new phenomena is set. A 95% C.L. lower limit of 30 TeV on the mGMSB breaking scale $\Lambda$ is set for $M_{mess} = 250$ TeV, $N_S = 3$, $\mu > 0$ and $C_{grav} = 1$, independent of $\tan\beta$. For large values of $\tan\beta$, the limit on $\Lambda$ increases to 43 TeV.

¹³AAD 12CM searched in 4.7 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV for events with at least one tau lepton, zero or one additional light lepton ($e/\mu$) jets, and large $\tilde{E}_T$ in a GMSB framework. No significant excess above the expected background was found and an upper limit on the visible cross section for new phenomena is set. A 95% C.L. lower limit of 54 TeV on the mGMSB breaking scale $\Lambda$ is set for $M_{mess} = 250$ TeV, $N_S = 3$, $\mu > 0$ and $C_{grav} = 1$, for $\tan\beta > 20$. Here the $\tilde{\tau}_1$ is the NLSP.

¹⁴ABBIENDI 06B use data 600 pb⁻¹ of data from $\sqrt{s} = 189-209$ GeV. They look for events from pair-produced staus in a GMSB scenario with $\tilde{\tau}$ NLSP including prompt $\tilde{\tau}$ decays to ditau + $\tilde{e}$ final states, large impact parameters, kinked tracks and heavy stable charged particles. Limits on the cross-section are computed as a function of $m(\tilde{\tau})$ and the lifetime, see their Fig. 7. The limit is compared to the $\sigma \cdot BR^2$ from a scan over the GMSB parameter space.

¹⁵ABDALLAH 04H use data from LEP 1 and $\sqrt{s} = 192-208$ GeV. They re-use results or re-analyze the data from ABDALLAH 03M to put limits on the parameter space of anomaly-mediated supersymmetry breaking (AMSB), which is scanned in the region $1<m_{3/2}<50$ TeV, $0<m_0<1000$ GeV, 1.5<tan$\beta$<35, both signs of $\mu$. The constraints are obtained from the searches for mass degenerate chargino and neutralino, for SM-like and invisible Higgs, for leptonically decaying charginos and from the limit on non-SM Z width of 3.2 MeV. The limit is for $m_{\tilde{\tau}} = 174.3$ GeV (see Table 2 for other $m_{\tilde{\tau}}$ values). The limit improves to 75 GeV for $\mu < 0$.

## R-parity violating $\tilde{\tau}$ (Stau) mass limit

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).

<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;1200</td><td>95</td><td>1 AAD</td><td>21Y ATLS</td><td>≥ 4ℓ, λ<sub>12k</sub> ≠ 0, m<sub>χ<sub>1</sub><sup>0</sup></sub> = 900 GeV (mass-degenerate <span style="text-decoration: overline;">ℓ<sub>L</sub></span> and <span style="text-decoration: overline;">ν</span> of all 3 generations)</td></tr><tr><td>> 870</td><td>95</td><td>1 AAD</td><td>21Y ATLS</td><td>≥ 4ℓ, λ<sub>133</sub> ≠ 0, m<sub>χ<sub>1</sub><sup>0</sup></sub> = 450 GeV (mass-degenerate <span style="text-decoration: overline;">ℓ<sub>L</sub></span> and <span style="text-decoration: overline;">ν</span> of all 3 generations)</td></tr><tr><td>>1060</td><td>95</td><td>2 AABOUD</td><td>18Z ATLS</td><td>≥ 4ℓ, λ<sub>12k</sub> ≠ 0, m<sub>χ<sub>1</sub><sup>0</sup></sub> = 600 GeV (mass-degenerate left-handed sleptons and sneutrinos of all 3 generations)</td></tr><tr><td>> 780</td><td>95</td><td>2 AABOUD</td><td>18Z ATLS</td><td>≥ 4ℓ, λ<sub>133</sub> ≠ 0, m<sub>χ<sub>1</sub><sup>0</sup></sub> = 300 GeV (mass-degenerate left-handed sleptons and sneutrinos of all 3 generations)</td></tr><tr><td>> 90</td><td>95</td><td>3 ABDALLAH</td><td>04M DLPH</td><td>τ<sub>R</sub>, indirect, Δm > 5 GeV</td></tr><tr><td>• • •</td><td></td><td>• • •</td><td></td><td>We do not use the following data for averages, fits, limits, etc.</td></tr><tr><td>> 74</td><td>95</td><td>4 ABBIENDI</td><td>04F OPAL</td><td>τ<sub>L</sub></td></tr></tbody></table>

¹AAD 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 up to two hadronically decaying taus). No significant excess above the Standard Model expectations is observed. Limits are set on Tchln12-GGM, and RPV models similar to Tchln21, Tglu1A (with $q = u, d, s, c, b$, with equal branching fractions), and $\tilde{e}_L/\tilde{\nu} \to \ell^\pm/\nu$ (mass-degenerate $\tilde{\tau}_L$ and $\tilde{\nu}$ of all 3 generations), all with $\chi_1^0 \to \ell^\pm\ell^\mp\nu$ via $\lambda_{12k}$ or $\lambda_{133}$ (where $i,k = 1,2$), see their Figure 11.

²AABOUD 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 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 R-parity violating decays of the LSP via $\lambda_{12k}$ or $\lambda_{133}$ to charged leptons, see their Figures 7, 8.

³ABDALLAH 04M use data from $\sqrt{s} = 192-208$ GeV to derive limits on sparticle masses under the assumption of RPV with $LLE$ couplings. The results are valid for $\Delta m > 200$ GeV, $\tan\beta > 1.5$, $\Delta m > 5$ GeV and assuming a BR of 1 for the given decay. The limit quoted is for indirect decays using the neutralino constraint of 39.5 GeV, also derived in ABDALLAH 04M. For indirect decays via $LLE$ the limit decreases to 86 GeV if the constraint from the neutralino is not used. Supersedes the result of ABREU 00u.

⁴ABBIENDI 04F use data from $\sqrt{s} = 189-209$ GeV. They derive limits on sparticle masses under the assumption of RPV with $LLE$ or $LQD$ couplings. The results are valid for

$\tan\beta = 1.5$, $\mu = -200$ GeV, with, in addition, $\Delta m > 5$ GeV for indirect decays via $LQD$. The limit quoted applies to direct decays with $LLE$ couplings and improves to 75 GeV for $LQD$ couplings. The limit on the $\tilde{\tau}_R$ mass for indirect decays is 92 GeV for $LLE$ couplings with $m_{\chi_1^0} = 10$ GeV and no exclusion is obtained for $LQD$ couplings. Supersedes the results of ABBIENDI 00.

## Long-lived $\tilde{\ell}$ (Slepton) mass limit

Limits on scalar leptons which leave detector before decaying. Limits from Z decays are independent of lepton flavor. Limits from continuum $e^+e^-$ annihilation are also independent of flavor for muons and staus. Selectron limits from $e^+e^-$ collisions in the continuum depend on MSSM parameters because of the additional neutralino exchange contribution.

<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>>520</td><td>95</td><td>1 AAD</td><td>23BQ ATLS</td><td>2ℓ slightly displaced, long-lived <span style="text-decoration: overline;">μ</span>, <span style="text-decoration: overline;">μ</span> → <span style="text-decoration: overline;">μ</span>G, <span style="text-decoration: overline;">m</span><sub>μR</sub> = <span style="text-decoration: overline;">m</span><sub>μL</sub>, <span style="text-decoration: overline;">τ</span><sub>μ</sub> = 10 ps</td></tr><tr><td>>190</td><td>95</td><td>1 AAD</td><td>23BQ ATLS</td><td>2ℓ slightly displaced, long-lived <span style="text-decoration: overline;">μ</span>, <span style="text-decoration: overline;">μ</span> → <span style="text-decoration: overline;">μ</span>G, <span style="text-decoration: overline;">m</span><sub>μR</sub> = <span style="text-decoration: overline;">m</span><sub>μL</sub>, <span style="text-decoration: overline;">τ</span><sub>μ</sub> = 1 ps</td></tr><tr><td>none 220-360</td><td>95</td><td>2 AAD</td><td>23G ATLS</td><td>direct <span style="text-decoration: overline;">τ</span> pair, <span style="text-decoration: overline;">τ</span> → <span style="text-decoration: overline;">τ</span>G, <span style="text-decoration: overline;">τ</span>, <span style="text-decoration: overline;">τ</span> = 10 ns</td></tr><tr><td>none 150-220</td><td>95</td><td>3 TUMASYAN</td><td>23AG CMS</td><td>2 hadronic <span style="text-decoration: overline;">τ</span> + <span style="text-decoration: overline;">E</span><sub>T</sub>, <span style="text-decoration: overline;">τ</span> → <span style="text-decoration: overline;">τ</span><span style="text-decoration: overline;">χ</span><sub>1</sub><sup>0</sup>, maximally mixed scenario with <span style="text-decoration: overline;">c</span>τ = 0.1 mm, <span style="text-decoration: overline;">m</span><sub>χ<sub>1</sub><sup>0</sup></sub> = 1 GeV</td></tr><tr><td>>610</td><td>95</td><td>4 TUMASYAN</td><td>22AF CMS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">e</span>, <span style="text-decoration: overline;">e</span> → <span style="text-decoration: overline;">e</span>G, <span style="text-decoration: overline;">m</span><sub>eR</sub> = <span style="text-decoration: overline;">m</span><sub>eL</sub>, <span style="text-decoration: overline;">c</span>τ = 0.7 cm</td></tr><tr><td>>610</td><td>95</td><td>4 TUMASYAN</td><td>22AF CMS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">μ</span>, <span style="text-decoration: overline;">μ</span> → <span style="text-decoration: overline;">μ</span>G, <span style="text-decoration: overline;">m</span><sub>μR</sub> = <span style="text-decoration: overline;">m</span><sub>μL</sub>, <span style="text-decoration: overline;">c</span>τ = 3 cm</td></tr><tr><td>>405</td><td>95</td><td>4 TUMASYAN</td><td>22AF CMS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">τ</span>, <span style="text-decoration: overline;">τ</span> → <span style="text-decoration: overline;">τ</span>G, <span style="text-decoration: overline;">m</span><sub>τR</sub> = <span style="text-decoration: overline;">m</span><sub>τL</sub>, <span style="text-decoration: overline;">c</span>τ = 2 cm</td></tr><tr><td>>270</td><td>95</td><td>4 TUMASYAN</td><td>22AF CMS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">e</span><sub>L</sub>, <span style="text-decoration: overline;">e</span> → <span style="text-decoration: overline;">e</span>G, <span style="text-decoration: overline;">m</span><sub>eR</sub> = <span style="text-decoration: overline;">m</span><sub>eL</sub>, <span style="text-decoration: overline;">m</span> → <span style="text-decoration: overline;">m</span>μ = <span style="text-decoration: overline;">m</span><sub>τ</sub>, 0.005 cm <span style="text-decoration: overline;">c</span>τ <span style="text-decoration: overline;">&lt;</span> 265 cm</td></tr><tr><td>>680</td><td>95</td><td>4 TUMASYAN</td><td>22AF CMS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">e</span><sub>L</sub>, <span style="text-decoration: overline;">e</sub> → <span style="text-decoration: overline;">e</span>G, <span style="text-decoration: overline;">m</span><sub>eR</sub> = <span style="text-decoration: overline;">m</span><sub>eL</sub>, <span style="text-decoration: overline;">m</span> → <span style="text-decoration: overline;">m</span>μ = <span style="text-decoration: overline;">m</span><sub>τ</sub>, <span style="text-decoration: overline;">c</span>τ = 2 cm</td></tr><tr><td>>720</td><td>95</td><td>5 AAD</td><td>21AL ATLS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">e</span>, <span style="text-decoration: overline;">e</span> → <span style="text-decoration: overline;">e</span>G, <span style="text-decoration: overline;">m</span><sub>eR</sub> = <span style="text-decoration: overline;">m</span><sub>eL</sub>, <span style="text-decoration: overline;">τ</span> <span style="text-decoration: overline;">τ</span> = 0.1 ns</td></tr><tr><td>>680</td><td>95</td><td>5 AAD</td><td>21AL ATLS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">μ</span>, <span style="text-decoration: overline;">μ</span> → <span style="text-decoration: overline;">μ</span>G, <span style="text-decoration: overline;">m</span><sub>μR</sub> = <span style="text-decoration: overline;">m</span><sub>μL</sub>, <span style="text-decoration: overline;">τ</span><sub>μ</sub> = 0.1 ns</td></tr><tr><td>>340</td><td>95</td><td>5 AAD</td><td>21AL ATLS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">τ</span>, <span style="text-decoration: overline;">τ</span> → <span style="text-decoration: overline;">τ</span>G, mixing sin$\theta_{\tau} = 0.95$, <span style="text-decoration: overline;">τ</span><sub>τ</sub> = 0.1 ns</td></tr><tr><td>>820</td><td>95</td><td>5 AAD</td><td>21AL ATLS</td><td>2ℓ displaced, long-lived <span style="text-decoration: overline;">e</span><sub>L</sub>, <span style="text-decoration: overline;">e</sub> → <span style="text-decoration: overline;">e</span>G, <span style="text-decoration: overline;">m</span><sub>eR</sub> = <span style="text-decoration: overline;">m</span><sub>eL</sub>, <span style="text-decoration: overline;">m</span> → <span style="text-decoration: overline;">m</span>μ = <span style="text-decoration: overline;">m</span><sub>τ</sub>, <span style="text-decoration: overline;">τ</span><sub>τ</sub> = 0.1 ns</td></tr><tr><td>>430</td><td>95</td><td>6 AABOUD</td><td>19AT ATLS</td><td>long-lived <span style="text-decoration: overline;">τ</span>, GMSB</td></tr><tr><td>>490</td><td>95</td><td>7 KHACHATRY...16BW CMS</td><td>16BW CMS</td><td>long-lived <span style="text-decoration: overline;">τ</span> from inclusive production, mGMSB SPS line 7 scenario</td></tr><tr><td>>240</td><td>95</td><td>7 KHACHATRY...16BW CMS</td><td>16BW CMS</td><td>long-lived <span style="text-decoration: overline;">τ</span> from direct pair production, mGMSB SPS line 7 scenario</td></tr><tr><td>>440</td><td>95</td><td>8 AAD</td><td>15AE ATLS</td><td>mGMSB, <span style="text-decoration: overline;">m</span><sub>mess</sub> = 250 TeV, <span style="text-decoration: overline;">N</span><sub>S</sub> = 3, <span style="text-decoration: overline;">μ</span> > 0, <span style="text-decoration: overline;">c</span><span style="text-decoration: overline;">grav</span> = 5000, <span style="text-decoration: overline;">tan</span><sub>β</sub> = 10</td></tr><tr><td>>385</td><td>95</td><td>8 AAD</td><td>15AE ATLS</td><td>mGMSB, <span style="text-decoration: overline;">m</span><sub>mess</sub> = 250 TeV, <span style="text-decoration: overline;">N</span><sub>S</sub> = 3, <span style="text-decoration: overline;">μ</span> > 0, <span style="text-decoration: overline;">c</span><span style="text-decoration: overline;">grav</span> = 5000, <span style="text-decoration: overline;">tan</span><sub>β</sub> = 50</td></tr><tr><td>>266</td><td>95</td><td>8 AAD</td><td>15AE ATLS</td><td>direct <span style="text-decoration: overline;">τ</span> production</td></tr><tr><td>none 124-309</td><td>95</td><td>9 AAJ</td><td>15BD LHCB</td><td>long-lived <span style="text-decoration: overline;">τ</span>, mGMSB, SPS7</td></tr><tr><td>> 98</td><td>95</td><td>10 ABBIENDI</td><td>03L OPAL</td><td><span style="text-decoration: overline;">τ</span><sub>R</sub>, <span style="text-decoration: overline;">τ</span></td></tr><tr><td>> 87</td><td>95</td><td>11 ABREU</td><td>00Q DLPH</td><td><span style="text-decoration: overline;">τ</span><sub>R</sub>, <span style="text-decoration: overline;">τ</span></td></tr><tr><td>> 81.2</td><td>95</td><td>12 ACCIARRI</td><td>99H L3</td><td><span style="text-decoration: overline;">τ</span><sub>R</sub>, <span style="text-decoration: overline;">τ</span></td></tr><tr><td>> 81</td><td>95</td><td>13 BARATE</td><td>98K ALEP</td><td><span style="text-decoration: overline;">τ</span><sub>R</sub>, <span style="text-decoration: overline;">τ</span></td></tr><tr><td>• • •</td><td></td><td></td><td></td><td>We do not use the following data for averages, fits, limits, etc.</td></tr><tr><td>>300</td><td>95</td><td>14 AAD</td><td>13AA ATLS</td><td>long-lived <span style="text-decoration: overline;">τ</span>, GMSB, <span style="text-decoration: overline;">tan</span><sub>β</sub> = 5-20</td></tr><tr><td>>339</td><td>95</td><td>15 ABAZOV</td><td>13B D0</td><td>long-lived <span style="text-decoration: overline;">τ</span>, 100 <span style="text-decoration: overline;">c</span><span style="text-decoration: overline;">τ</span> <span style="text-decoration: overline;">&lt;</span> 300 GeV</td></tr><tr><td>>500</td><td>95</td><td>16,17 CHATRCHYAN 13AB CMS</td><td>13AB CMS</td><td>long-lived <span style="text-decoration: overline;">τ</span>, direct <span style="text-decoration: overline;">τ</span> pair prod., minimal GMSB, SPS line 7</td></tr><tr><td>>314</td><td>95</td><td>19 CHATRCHYAN 12L CMS</td><td>12L CMS</td><td>long-lived <span style="text-decoration: overline;">τ</span>, <span style="text-decoration: overline;">τ</span><sub>τ</sub> from direct pair prod. and from decay of heavier SUSY particles, minimal GMSB, SPS line 7</td></tr><tr><td>>136</td><td>95</td><td>20 AAD</td><td>11P ATLS</td><td>stable <span style="text-decoration: overline;">τ</span>, GMSB scenario, <span style="text-decoration: overline;">tan</span><sub>β</sub> = 5</td></tr></tbody></table>

<table><tbody><tr><td>• • •</td><td></td><td></td><td></td><td>We do not use the following data for averages, fits, limits, etc.</td></tr><tr><td>>300</td><td>95</td><td>14 AAD</td><td>13AA ATLS</td><td>long-lived <span style="text-decoration: overline;">τ</span>, GMSB, <span style="text-decoration: overline;">tan</span><sub>β</sub> = 5-20</td></tr><tr><td>>339</td><td>95</td><td>15 ABAZOV</td><td>13B D0</td><td>long-lived <span style="text-decoration: overline;">τ</span>, 100 <span style="text-decoration: overline;">c</span><span style="text-decoration: overline;">τ</span> <span style="text-decoration: overline;">&lt;</span> 300 GeV</td></tr><tr><td>>500</td><td>95</td><td>16,17 CHATRCHYAN 13AB CMS</td><td>13AB CMS</td><td>long-lived <span style="text-decoration: overline;">τ</span>, direct <span style="text-decoration: overline;">τ</span> pair prod., minimal GMSB, SPS line 7</td></tr><tr><td>>314</td><td>95</td><td>19 CHATRCHYAN 12L CMS</td><td>12L CMS</td><td>long-lived <span style="text-decoration: overline;">τ</span>, <span style="text-decoration: overline;">τ</span><sub>τ</sub> from decay of heavier SUSY particles, minimal GMSB, SPS line 7</td></tr><tr><td>>136</td><td>95</td><td>20 AAD</td><td>11P ATLS</td><td>stable <span style="text-decoration: overline;">τ</span>, GMSB scenario, <span style="text-decoration: overline;">tan</span><sub>β</sub> = 5</td></tr></tbody></table>

¹AAD 23BQ searched in 139 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for pair production of long-lived $\tilde{\mu}$ in events with muons with impact parameters in the millimeter range. No significant excess above the Standard Model predictions is observed. Limits are set on $m_{\tilde{\mu}}$ as a function of the $\tilde{\mu}$ lifetime, assuming the $\tilde{\mu} \to \mu G$ decay and mass-degenerate $\tilde{\mu}L$ and $\tilde{\mu}R$. See Figure 4.

²AAD 23G searched in 139 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for stau pair production in events with high-p tracks with large ionisation in the pixel detector. No significant excess above the Standard Model predictions is observed. Limits are set on the stau mass as a function of its lifetime, see Figure 19.
³TUMASYAN 23AG searched in 138 fb⁻¹ of pp collisions at √s = 13 TeV for or direct pair production of tau sleptons in events with two hadronically decaying tau leptons. No significant excess above the Standard Model expectations is observed. Limits are set for the maximally mixed scenario with long-lived tau sleptons and τ lifetimes of 0.01 mm to 2.5 mm, see their figure 8. Limits are also set on the mass of the tau slepton in models with τ̃ → τχ̃₁₀ for mass-degenerate, pure left-handed and pure right-handed tau sleptons, see their figures 4–7.

⁴TUMASYAN 22AF searched for evidence of new long-lived particles decaying to 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 → bτ̃ and t → dτ̃, 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 slepton and the lightest SUSY particle a gravitino Ĝ, 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.

⁵AAD 21AL searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for pair production of long-lived sleptons in events with highly displaced leptons. No significant excess above the Standard Model predictions is observed. Limits are set on m̃e, m̃μ, m̃τ as a function of the slepton lifetime, assuming the t̃ → ℓ Ĝ decay and mass-degenerate t̃L and t̃R. See Figures 2.

⁶AABOUD 19AT searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for metastable and stable R-hadrons. Multiple search strategies for a wide range of lifetimes, corresponding to path lengths of a few meters, are defined. No significant deviations from the expected Standard Model background are observed. Results are interpreted in terms of exclusion limits on long-lived tau in the context of GMSB models. Lower limits on the mass for direct production of staus are set at 430 GeV, see their Fig. 10 (left).

⁷KHACHATRYAN 16BW searched in 2.5 fb⁻¹ of pp collisions at √s = 13 TeV for events with heavy stable charged particles, identified by their anomalously high energy deposits in the silicon tracker and/or long time-of-flight measurements by the muon system. No evidence for an excess over the expected background is observed. Limits are derived for pair production of tau sleptons as a function of mass, depending on their direct or inclusive production in a minimal GMSB scenario along the Snowmass Points and Slopes (SPS) line 7, see Fig. 4 and Table 7.

⁸AAD 15AE searched in 19.1 fb⁻¹ of pp collisions at √s = 8 TeV for heavy long-lived charged particles, measured through their specific ionization energy loss in the ATLAS pixel detector or their time-of-flight in the ALTAS muon system. In the absence of an excess of events above the expected backgrounds, limits are set on stable τ̃ sleptons in various scenarios, see Figs. 5–7.

⁹AAIJ 15BD searched in 3.0 fb⁻¹ of pp collisions at √s = 7 and 8 TeV for evidence of Drell-Yan pair production of long-lived τ̃ particles. No evidence for such particles is observed and 95% C.L. upper limits on the cross section of τ̃ pair production are derived, see Fig. 7. In the mGMSB, assuming the SPS7 benchmark scenario τ̃ masses between 124 and 309 GeV are excluded at 95% C.L.

¹⁰ABBENDI 03L used e⁺e⁻ data at √s = 130–209 GeV to select events with two high momentum tracks with anomalous dE/dx. The excluded cross section is compared to the theoretical expectation as a function of the heavy particle mass in their Fig. 3. The limit improves to 98.5 GeV for µ̃L and τ̃L. The bounds are valid for colorless spin 0 particles with lifetimes longer than 10⁻⁶ s. Supersedes the results from ACKERSTAFF 98P.

¹¹ABREU 00Q searches for the production of pairs of heavy, charged stable particles in e⁺e⁻ annihilation at √s = 130–189 GeV. The upper bound improves to 88 GeV for µ̃L, τ̃L. These limits include and update the results of ABREU 98P.

¹²ACCIARRI 99H searched for production of pairs of back-to-back heavy charged particles at √s = 130–183 GeV. The upper bound improves to 82.2 GeV for µ̃L, τ̃L.

¹³The BARATE 98k mass limit improves to 82 GeV for µ̃L, τ̃L. Data collected at √s = 161–184 GeV.

¹⁴AAD 13AA searched in 4.7 fb⁻¹ of pp collisions at √s = 7 TeV for events containing long-lived massive particles in a GMSB framework. No significant excess above the expected background was found. A 95% C.L. lower limit of 300 GeV is placed on long-lived τ̃'s in the GMSB model with M<sub>mess</sub> = 250 TeV, N<sub>S</sub> = 3, μ > 0, for tanβ = 5–20. The lower limit on the GMSB breaking scale Λ was found to be 99–110 TeV, for tanβ values between 5 and 40, see Fig. 4 (top). Also, directly produced long-lived sleptons, or sleptons decaying to long-lived ones, are excluded at 95% C.L. up to a τ̃ mass of 278 GeV for models with slepton splittings smaller than 50 GeV.

¹⁵ABAZOV 13B looked in 6.3 fb⁻¹ of pp collisions at √s = 1.96 TeV for charged massive long-lived particles in events with muon-back particles that have both speed and ionization energy loss inconsistent with muons produced in beam collisions. In the absence of an excess, limits are set at 95% C.L. on the production cross section of stau leptons in the mass range 100–300 GeV, see their Table 20 and Fig. 23.

¹⁶CHATRCHYAN 13AB looked in 5.0 fb⁻¹ of pp collisions at √s = 7 TeV and in 18.8 fb⁻¹ of pp collisions at √s = 8 TeV for events with heavy stable particles, identified by their anomalous dE/dx in the tracker or additionally requiring that it be identified as muon in the muon chambers, from pair production of τ̃₁'s. No evidence for an excess over the expected background is observed. Supersedes CHATRCHYAN 12L.

¹⁷CHATRCHYAN 13AB limits are derived for pair production of τ̃γ as a function of mass in minimal GMSB scenarios along the Snowmass Points and Slopes (SPS) line 7 (see Fig. 8 and Table 7). The limit given here is valid for direct pair τ̃₁ production.

¹⁸CHATRCHYAN 13AB limits are derived for the production of τ̃₁ as a function of mass in minimal GMSB scenarios along the Snowmass Points and Slopes (SPS) line 7 (see Fig. 8 and Table 7). The limit given here is valid for the production of τ̃₁ from both direct pair production and from the decay of heavier supersymmetric particles.

¹⁹CHATRCHYAN 12L looked in 5.0 fb⁻¹ of pp collisions at √s = 7 TeV for events with heavy stable particles, identified by their anomalous dE/dx in the tracker or additionally requiring that it be identified as muon in the muon chambers, from pair production of τ̃₁'s. No evidence for an excess over the expected background is observed. Limits are derived for the production of τ̃₁ as a function of mass in minimal GMSB scenarios along the Snowmass Points and Slopes (SPS) line 7 (see Fig. 3). The limit given here is valid for the production of τ̃₁ in the decay of heavier supersymmetric particles.

²⁰AAD 11P looked in 37 pb⁻¹ of pp collisions at √s = 7 TeV for events with two heavy stable particles, reconstructed in the Inner tracker and the Muon System and identified by their time of flight in the Muon System. No evidence for an excess over the SM expectation is observed. Limits on the mass are derived, see Fig. 3, for τ̃ in a GMSB scenario and for sleptons produced by electroweak processes only, in which case the limit degrades to 110 GeV.

## $\tilde{q}$ (Squark) mass limit

For $m_{\tilde{q}} > 60–70$ GeV, it is expected that squarks 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.

Limits from $e^+e^-$ collisions depend on the mixing angle of the lightest mass eigenstate $\tilde{q}_1 = \tilde{q}_R \sin\theta_q + \tilde{q}_L \cos\theta_q$. It is usually assumed that only the bottom and stop squarks have non-trivial mixing angles (see the stop and bottom sections). Here, unless otherwise noted, squarks are always taken to be either left/right degenerate, or purely of left or right type. Data from Z decays have set squark mass limits above 40 GeV, in the case of $\tilde{q} \to q\tilde{\chi}_1$ decays if $\Delta m = m_{\tilde{q}} - m_{\tilde{\chi}_1^0} \gtrsim 5$ GeV. For smaller values of $\Delta m$, current constraints on the invisible width of the Z ($\Delta\Gamma_{inv} < 2.0$ MeV, LEP 00) exclude $m_{\tilde{u}_L, R} < 44$ GeV, $m_{\tilde{d}_L} < 33$ GeV, $m_{\tilde{d}_L} < 44$ GeV and, assuming all squarks degenerate, $m_{\tilde{q}} < 48$ GeV.

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 $\tilde{q}$ (Squark) mass limit

<table><thead><tr><th>VALUE (GeV)</th><th>CL<sup>95</sup></th><th>DOCUMENT ID</th><th>TECN</th><th>COMMENT</th></tr></thead><tbody><tr><td>&gt;1550</td><td>95</td><td>1 AAD</td><td>23AE ATLS</td><td>2 SFOS t̃, jets, E<sub>T</sub>, Tsqk2, m<sub>χ̃2</sub><sup>0</sup> = (m̃q + m<sub>χ̃1</sub><sup>0</sup>)/2, m<sub>χ̃1</sub><sup>0</sup> = 100 GeV</td></tr><tr><td>none<br>1200–2500</td><td>95</td><td>2 TUMASYAN</td><td>23X CMS</td><td>2 AK8 jets + 1 AK4 jet, q̃ → qχ̃<sub>2</sub><sup>0</sup> and χ̃<sub>2</sub><sup>0</sup> → H<sub>1</sub>χ̃<sub>2</sub><sup>0</sup>, 40 &lt; m<sub>H<sub>1</sub></sub> &lt; 120 GeV</td></tr><tr><td>&gt;1400</td><td>95</td><td>3 AAD</td><td>21AK ATLS</td><td>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tsqk3, 4 degenerate light q̃ℓ, m<sub>χ̃1</sub><sup>±</sup> = (m̃q + m<sub>χ̃1</sub><sup>0</sup>)/2, m<sub>χ̃1</sub><sup>0</sup> &lt; 200 GeV</td></tr><tr><td>&gt;1040</td><td>95</td><td>3 AAD</td><td>21AK ATLS</td><td>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tsqk3, 1 light q̃ℓ, m<sub>χ̃1</sub><sup>±</sup> = (m̃q + m<sub>χ̃1</sub><sup>0</sup>)/2, m<sub>χ̃1</sub><sup>0</sup> &lt; 200 GeV</td></tr><tr><td>&gt; 925</td><td>95</td><td>4 AAD</td><td>21F ATLS</td><td>≥ 1 jet + E<sub>T</sub>, Tsqk1, m̃q = m<sub>χ̃1</sub><sup>0</sup></td></tr><tr><td>&gt; 550</td><td>95</td><td>4 AAD</td><td>21F ATLS</td><td>≥ 1 jet + E<sub>T</sub>, Tstop3, m<sub>χ̃1</sub><sup>0</sup> = 5 GeV</td></tr><tr><td>&gt; 550</td><td>95</td><td>4 AAD</td><td>21F ATLS</td><td>≥ 1 jet + E<sub>T</sub>, Tstop4, m<sub>χ̃1</sub><sup>0</sup> = 5 GeV</td></tr><tr><td>&gt; 545</td><td>95</td><td>4 AAD</td><td>21F ATLS</td><td>≥ 1 jet + E<sub>T</sub>, Tsbot1, m<sub>b</sub> = m<sub>χ̃1</sub><sup>0</sup> = 5 GeV</td></tr><tr><td>&gt;1850</td><td>95</td><td>5 AAD</td><td>21L ATLS</td><td>jets + E<sub>T</sub>, Tsqk1, 8 degenerate q̃, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1220</td><td>95</td><td>5 AAD</td><td>21L ATLS</td><td>jets + E<sub>T</sub>, Tsqk1, 1 non-degenerate q̃, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1310</td><td>95</td><td>5 AAD</td><td>21L ATLS</td><td>jets + E<sub>T</sub>, Tsqk3, 4 degenerate q̃ℓ, m<sub>χ̃1</sub><sup>±</sup> = (m̃q + m<sub>χ̃1</sub><sup>0</sup>)/2, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;3000</td><td>95</td><td>5 AAD</td><td>21L ATLS</td><td>jets + E<sub>T</sub>, combined q̃g̃, g̃q̃, q̃q̃ production, g̃ → qq̃'χ̃<sub>1</sub><sup>0</sup>, q̃ → qχ̃<sub>1</sub><sup>0</sup>, m̃q = m̃g̃, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1800</td><td>95</td><td>6 SIRUNYAN</td><td>21M CMS</td><td>ℓ<sup>±</sup>ℓ<sup>±</sup> + E<sub>T</sub>, Tsqk2A, m<sub>χ̃2</sub><sup>0</sup> = 1500 GeV, m<sub>χ̃1</sub><sup>0</sup> = 100 GeV</td></tr><tr><td>&gt;1590</td><td>95</td><td>7 SIRUNYAN</td><td>19AG CMS</td><td>2γ + E<sub>T</sub>, Tsqk4B, 500 GeV &lt;m<sub>χ̃1</sub><sup>0</sup> &lt; 1500 GeV</td></tr><tr><td>&gt;1130</td><td>95</td><td>8 SIRUNYAN</td><td>19CH CMS</td><td>jets + E<sub>T</sub>, Tsqk1, 1 light flavour, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1630</td><td>95</td><td>8 SIRUNYAN</td><td>19CH CMS</td><td>jets + E<sub>T</sub>, Tsqk1, 8 degenerate light flavours, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt;1430</td><td>95</td><td>9 SIRUNYAN</td><td>19K CMS</td><td>γ + ℓ + E<sub>T</sub>, Tsqk4A, m<sub>χ̃1</sub><sup>0</sup> = 1200 GeV</td></tr><tr><td>&gt;1200</td><td>95</td><td>10 AABOUD</td><td>18BJ ATLS</td><td>ℓ<sup>±</sup>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tsqk2, m<sub>χ̃1</sub><sup>0</sup> = 1 GeV, any m<sub>χ̃2</sub><sup>0</sup></td></tr><tr><td>&gt; 850</td><td>95</td><td>11 AABOUD</td><td>18BV ATLS</td><td>c-jets + E<sub>T</sub>, Tsqk1 (charm only), m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>&gt; 710</td><td>95</td><td>12 AABOUD</td><td>18I ATLS</td><td>≥ 1 jets + E<sub>T</sub>, Tsqk1, m̃q ~ m<sub>χ̃1</sub><sup>0</sup></td></tr></tbody></table>
# Searches Particle Listings

## Supersymmetric Particle Searches

<table><tbody><tr><td>&gt;1820</td><td>95</td><td>13 AABOUD</td><td>18U ATLS</td><td>2 &gamma; + E<sub>T</sub>, GGM, Tsqk4B, any NLSP mass</td><td>&gt;1430</td><td>95</td><td>39 CHATRCHYAN 13H CMS</td><td>2&gamma; + &ge;4 jets + low &not;E<sub>T</sub>, stealth SUSY model</td></tr><tr><td>&gt;1550</td><td>95</td><td>14 AABOUD</td><td>18V ATLS</td><td>jets + E<sub>T</sub>, Tsqk1, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;750</td><td>95</td><td>40 CHATRCHYAN 13T CMS</td><td>jets + E<sub>T</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td></tr><tr><td>&gt;1150</td><td>95</td><td>15 AABOUD</td><td>18V ATLS</td><td>jets + E<sub>T</sub>, Tsqk3, m<sub>&chi;</sub><sup>&plusmn;</sup><sub>1</sub> = 0.5 (m<sub>q&#773;</sub> + m<sub>&chi;</sub><sup>0</sup><sub>1</sub>), m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;820</td><td>95</td><td>41 AAD</td><td>12AX ATLS &ell; + jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr><tr><td>&gt;1650</td><td>95</td><td>16 SIRUNYAN</td><td>18AA CMS</td><td>&ge; 1&gamma; + E<sub>T</sub>, Tsqk4A</td><td>&gt;1200</td><td>95</td><td>42 AAD</td><td>&ell;<sup>&plusmn;</sup> + jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr><tr><td>&gt;1750</td><td>95</td><td>16 SIRUNYAN</td><td>18AA CMS</td><td>&ge; 1&gamma; + E<sub>T</sub>, Tsqk4B</td><td>&gt;870</td><td>95</td><td>43 AAD</td><td>2&gamma; + E<sub>T</sub>, GMSB, bino NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &gt; 50 GeV</td></tr><tr><td>&gt; 675</td><td>95</td><td>17 SIRUNYAN</td><td>18AY CMS</td><td>jets + E<sub>T</sub>, Tsqk1, 1 light flavor state, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;950</td><td>95</td><td>44 AAD</td><td>12W ATLS jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr><tr><td>&gt;1320</td><td>95</td><td>17 SIRUNYAN</td><td>18AY CMS</td><td>jets + E<sub>T</sub>, Tsqk1,8 degenerate light flavor states, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;760</td><td>95</td><td>45 CHATRCHYAN 12 CMS</td><td>e, &mu;, jets, razor, CMSSM</td></tr><tr><td>&gt;1220</td><td>95</td><td>18 AABOUD</td><td>17AR ATLS</td><td>1&ell; + jets + E<sub>T</sub>, Tsqk3, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;760</td><td>95</td><td>46 CHATRCHYAN 12AE CMS</td><td>jets + E<sub>T</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> = 0.5 GeV</td></tr><tr><td>&gt;1000</td><td>95</td><td>19 AABOUD</td><td>17N ATLS</td><td>2 same-flavour, opposite-sign &ell; + jets + E<sub>T</sub>, Tsqk2, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;1110</td><td>95</td><td>47 CHATRCHYAN 12AT CMS</td><td>200 GeV</td></tr><tr><td>&gt;1150</td><td>95</td><td>20 KHACHATRY..17P CMS</td><td></td><td>1 or more jets + E<sub>T</sub>, Tsqk1, 4(flav- vor) &times; 2(isospin) = 8 mass degenerate states, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;1180</td><td>95</td><td>47 CHATRCHYAN 12AT CMS</td><td>jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr><tr><td>&gt; 575</td><td>95</td><td>20 KHACHATRY..17P CMS</td><td></td><td>1 or more jets + E<sub>T</sub>, Tsqk1, one light flavor state, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;1080</td><td>95</td><td>48 AABOUD</td><td>18V ATLS jets + E<sub>T</sub>, Tsqk5, (m<sub>&chi;</sub><sup>0</sup><sub>2</sub> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub>)/ (m<sub>q&#773;</sub> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub>) &lt; 0.95, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 60 GeV</td></tr><tr><td>&gt;1370</td><td>95</td><td>21 KHACHATRY..17V CMS</td><td></td><td>2 &gamma; + E<sub>T</sub>, GGM, Tsqk4, any NLSP mass</td><td>&gt;300</td><td>95</td><td>49 KHACHATRY..16BT CMS</td><td>19-parameter pMSSM model, global Bayesian analysis, flat prior</td></tr><tr><td>&gt;1600</td><td>95</td><td>22 SIRUNYAN</td><td>17AY CMS</td><td>&gamma; + jets + E<sub>T</sub>, Tsqk4B, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>50 AAD</td><td></td><td>50 AAD ATLS &ell;<sup>&plusmn;</sup> + jets + E<sub>T</sub></td><td></td></tr><tr><td>&gt;1370</td><td>95</td><td>22 SIRUNYAN</td><td>17AY CMS</td><td>&gamma; + jets + E<sub>T</sub>, Tsqk4A, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;1650</td><td>95</td><td>28 AAD</td><td>15BV ATLS jets + E<sub>T</sub>, m<sub>q&#773;</sub> = m<sub>q&#773;</sub>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 1 GeV</td></tr><tr><td>&gt;1050</td><td>95</td><td>23 SIRUNYAN</td><td>17AZ CMS</td><td>&ge; 1 jets + E<sub>T</sub>, Tsqk1, single light flavor state, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;790</td><td>95</td><td>28 AAD</td><td>15BV ATLS jets + E<sub>T</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> &rarr; qW&#773;&chi;<sup>0</sup><sub>1</sub>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td></tr><tr><td>&gt;1550</td><td>95</td><td>23 SIRUNYAN</td><td>17AZ CMS</td><td>&ge; 1 jets + E<sub>T</sub>, Tsqk1, 4(flav- vor) &times; 2(isospin) = 8 degenerate mass states, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;820</td><td>95</td><td>28 AAD</td><td>15BV ATLS 2 or 3 leptons + jets, q&#773; decays via sleptons, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td></tr><tr><td>&gt;1390</td><td>95</td><td>24 SIRUNYAN</td><td>17P CMS</td><td>jets + E<sub>T</sub>, Tsqk1, 4(flav- vor) &times; 2(isospin) = 8 degenerate mass states, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;850</td><td>95</td><td>28 AAD</td><td>&tau;, q&#773; decays via staus, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 50 GeV</td></tr><tr><td>&gt; 950</td><td>95</td><td>24 SIRUNYAN</td><td>17P CMS</td><td>jets + E<sub>T</sub>, Tsqk1, one light flavor state, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;700</td><td>95</td><td>51 KHACHATRY..15AR CMS</td><td>q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> &rarr; s&#773;g, s&#773; &rarr; s&#773;G, s&#773; &rarr; gg, m<sub>g&#773;</sub> = 100 GeV, m<sub>S</sub> = 90 GeV</td></tr><tr><td>&gt; 608</td><td>95</td><td>25 AABOUD</td><td>16D ATLS</td><td>&ge; 1 jet + E<sub>T</sub>, Tsqk1, m<sub>q&#773;</sub> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 5 GeV</td><td>&gt;550</td><td>95</td><td>51 KHACHATRY..15AR CMS</td><td>&ell;<sup>&plusmn;</sup>, q&#773; &rarr; q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub>, q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub> &rarr; s&#773;W<sup>&plusmn;</sup>, s&#773; &rarr; s&#773;G, s&#773; &rarr; gg, m<sub>g&#773;</sub> = 100 GeV, m<sub>S</sub> = 90 GeV</td></tr><tr><td>&gt;1030</td><td>95</td><td>26 AABOUD</td><td>16N ATLS</td><td>&ge; 2 jets + E<sub>T</sub>, Tsqk1, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;1500</td><td>95</td><td>52 KHACHATRY..15AZ CMS</td><td>&ge; 2 &gamma;, &ge; 1 jet, (Razor), bino- like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt; 600</td><td>95</td><td>27 KHACHATRY..16BS CMS</td><td></td><td>jets + E<sub>T</sub>, Tsqk1, single light squark, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;1000</td><td>95</td><td>52 KHACHATRY..15AZ CMS</td><td>&ge; 1 &gamma;, &ge; 2 jet, wino-like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt;1260</td><td>95</td><td>27 KHACHATRY..16BS CMS</td><td></td><td>jets + E<sub>T</sub>, Tsqk1, 8 degenerate light squarks, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;670</td><td>95</td><td>53 AAD</td><td>14E ATLS &ell;<sup>&plusmn;</sup> &ell;(&ell;+)&plusmn; jets, q&#773; &rarr; q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub>, q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub> &rarr; W(*)&plusmn; q&#773;&chi;<sup>0</sup><sub>2</sub>, q&#773;&chi;<sup>0</sup><sub>2</sub> &rarr; Z(*) q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 300 GeV</td></tr><tr><td>&gt; 850</td><td>95</td><td>28 AAD</td><td>15BV ATLS</td><td>jets + E<sub>T</sub>, q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td><td>&gt;780</td><td>95</td><td>53 AAD</td><td>14E ATLS &ell;<sup>&plusmn;</sup> &ell;(&ell;+)&plusmn; jets, q&#773; &rarr; q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub>, q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub> &rarr; &ell;<sup>&plusmn;</sup>&nu;<sub>1</sub>, q&#773;&chi;<sup>0</sup><sub>2</sub>, q&#773;&chi;<sup>0</sup><sub>2</sub> &rarr; &ell;<sup>&plusmn;</sup>&ell;(&nu;&nu;) q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model</td></tr><tr><td>&gt; 250</td><td>95</td><td>29 AAD</td><td>15CS ATLS</td><td>photon + E<sub>T</sub>, p&rho; &rarr; q&#773;q&#773;&chi;<sup>0</sup>, q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub>, m<sub>q&#773;</sub> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = m<sub>c</sub></td><td>&gt;700</td><td>95</td><td>54 CHATRCHYAN 13AO CMS</td><td>&ell;<sup>&plusmn;</sup>&ell;+ jets + E<sub>T</sub>, CMSSM, m<sub>0</sub> &lt; 700 GeV</td></tr><tr><td>&gt; 490</td><td>95</td><td>30 AAD</td><td>15K ATLS</td><td>&zeta; &rarr; c&#773;&chi;<sup>0</sup><sub>1</sub>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 200 GeV</td><td>&gt;1350</td><td>95</td><td>55 CHATRCHYAN 13AV CMS</td><td>jets + (leptons) + E<sub>T</sub>, CMSSM, m<sub>g&#773;</sub> = m<sub>q&#773;</sub></td></tr><tr><td>&gt; 875</td><td>95</td><td>31 KHACHATRY..15AF CMS</td><td></td><td>&zeta; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub>, simplified model, 8 degenerate light q&#773;, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td><td>&gt;800</td><td>95</td><td>56 CHATRCHYAN 13W CMS</td><td>&ge; 1 photons + jets + E<sub>T</sub>, GGM, wino-like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt; 520</td><td>95</td><td>31 KHACHATRY..15AF CMS</td><td></td><td>&zeta; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub>, simplified model, single light squark, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0</td><td>&gt;1000</td><td>95</td><td>56 CHATRCHYAN 13W CMS</td><td>&ge; 2 photons + jets + E<sub>T</sub>, GGM, bino-like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt;1450</td><td>95</td><td>31 KHACHATRY..15AF CMS</td><td></td><td>CMSSM, tan&beta; = 30, A<sub>0</sub> = -2max(m<sub>0</sub>, m<sub>1/2</sub>), &mu; &gt; 0</td><td>&gt;340</td><td>95</td><td>57 DREINER</td><td>12A THEO m<sub>q&#773;</sub> ~ m<sub>&chi;</sub><sup>0</sup><sub>1</sub></td></tr><tr><td>&gt; 850</td><td>95</td><td>32 AAD</td><td>14AE ATLS</td><td>jets + E<sub>T</sub>, q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, mass degenerate first and second generation squarks, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td>&gt;650</td><td>95</td><td>58 DREINER</td><td>12A THEO m<sub>q&#773;</sub> ~ m<sub>&chi;</sub><sup>0</sup><sub>1</sub></td></tr><tr><td>&gt; 440</td><td>95</td><td>32 AAD</td><td>14AE ATLS</td><td>jets + E<sub>T</sub>, q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, single light-flavour squark, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td><td></td><td></td><td></td><td></td></tr><tr><td>&gt;1700</td><td>95</td><td>32 AAD</td><td>14AE ATLS</td><td>jets + E<sub>T</sub>, mSUGRA/CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td><td></td><td></td><td></td><td></td></tr><tr><td>&gt; 800</td><td>95</td><td>33 CHATRCHYAN 14AH CMS</td><td></td><td>jets + E<sub>T</sub>, q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 50 GeV</td><td></td><td></td><td></td><td></td></tr><tr><td>&gt; 780</td><td>95</td><td>34 CHATRCHYAN 14I CMS</td><td></td><td>multijets + E<sub>T</sub>, q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 200 GeV</td><td></td><td></td><td></td><td></td></tr><tr><td>&gt;1360</td><td>95</td><td>35 AAD</td><td>13L ATLS</td><td>jets + E<sub>T</sub>, CMSSM, m<sub>g&#773;</sub> = m<sub>q&#773;</sub></td><td></td><td></td><td></td><td></td></tr><tr><td>&gt;1200</td><td>95</td><td>36 AAD</td><td>13Q ATLS</td><td>&gamma;+b + E<sub>T</sub>, higgino-like neutralino, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &gt; 220 GeV, GMSB</td><td></td><td></td><td></td><td></td></tr><tr><td>&gt;1250</td><td>95</td><td>37 CHATRCHYAN 13 CMS</td><td></td><td>&ell;<sup>&plusmn;</sup> &ell;<sup>&plusmn;</sup> + jets + E<sub>T</sub>, CMSSM</td><td></td><td></td><td></td><td></td></tr><tr><td></td><td></td><td>38 CHATRCHYAN 13G CMS</td><td></td><td>0,1,2, &ge; 3 b-jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td><td></td><td></td><td></td><td></td></tr></tbody></table>

<table><tbody><tr><td>&gt;1430</td><td>95</td><td>39 CHATRCHYAN 13H CMS</td><td>2&gamma; + &ge;4 jets + low &not;E<sub>T</sub>, stealth SUSY model</td></tr><tr><td>&gt;750</td><td>95</td><td>40 CHATRCHYAN 13T CMS</td><td>jets + E<sub>T</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 0 GeV</td></tr><tr><td>&gt;820</td><td>95</td><td>41 AAD</td><td>12AX ATLS &ell; + jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr><tr><td>&gt;1200</td><td>95</td><td>42 AAD</td><td>12CJ ATLS &ell;<sup>&plusmn;</sup> + jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr><tr><td>&gt;870</td><td>95</td><td>43 AAD</td><td>12CP ATLS 2&gamma; + E<sub>T</sub>, GMSB, bino NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &gt; 50 GeV</td></tr><tr><td>&gt;950</td><td>95</td><td>44 AAD</td><td>12W ATLS jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr><tr><td>&gt;760</td><td>95</td><td>45 CHATRCHYAN 12 CMS</td><td>e, &mu;, jets, razor, CMSSM</td></tr><tr><td>&gt;760</td><td>95</td><td>46 CHATRCHYAN 12AE CMS</td><td>jets + E<sub>T</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> = 0.5 GeV</td></tr><tr><td>&gt;1110</td><td>95</td><td>47 CHATRCHYAN 12AT CMS</td><td>200 GeV</td></tr><tr><td>&gt;1180</td><td>95</td><td>47 CHATRCHYAN 12AT CMS</td><td>jets + E<sub>T</sub>, CMSSM, m<sub>q&#773;</sub> = m<sub>g&#773;</sub></td></tr></tbody></table>

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

<table><tbody><tr><td>&gt;1080</td><td>95</td><td>48 AABOUD</td><td>18V ATLS jets + E<sub>T</sub>, Tsqk5, (m<sub>&chi;</sub><sup>0</sup><sub>2</sub> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub>)/ (m<sub>q&#773;</sub> - m<sub>&chi;</sub><sup>0</sup><sub>1</sub>) &lt; 0.95, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 60 GeV</td></tr><tr><td>&gt;300</td><td>95</td><td>49 KHACHATRY..16BT CMS</td><td>19-parameter pMSSM model, global Bayesian analysis, flat prior</td></tr><tr><td>&gt;1650</td><td>95</td><td>50 AAD</td><td>15AI ATLS &ell;<sup>&plusmn;</sup> + jets + E<sub>T</sub></td></tr><tr><td>&gt;790</td><td>95</td><td>28 AAD</td><td>15BV ATLS jets + E<sub>T</sub>, m<sub>q&#773;</sub> = m<sub>q&#773;</sub>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 1 GeV</td></tr><tr><td>&gt;820</td><td>95</td><td>28 AAD</td><td>15BV ATLS jets + E<sub>T</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> &rarr; qW&#773;&chi;<sup>0</sup><sub>1</sub>, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td></tr><tr><td>&gt;850</td><td>95</td><td>28 AAD</td><td>15BV ATLS 2 or 3 leptons + jets, q&#773; decays via sleptons, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 100 GeV</td></tr><tr><td>&gt;700</td><td>95</td><td>51 KHACHATRY..15AR CMS</td><td>q&#773; &rarr; q&#773;&chi;<sup>0</sup><sub>1</sub>, q&#773;&chi;<sup>0</sup><sub>1</sub> &rarr; s&#773;g, s&#773; &rarr; s&#773;G, s&#773; &rarr; gg, m<sub>g&#773;</sub> = 100 GeV, m<sub>S</sub> = 90 GeV</td></tr><tr><td>&gt;550</td><td>95</td><td>51 KHACHATRY..15AR CMS</td><td>&ell;<sup>&plusmn;</sup>, q&#773; &rarr; q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub>, q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub> &rarr; s&#773;W<sup>&plusmn;</sup>, s&#773; &rarr; s&#773;G, s&#773; &rarr; gg, m<sub>g&#773;</sub> = 100 GeV, m<sub>S</sub> = 90 GeV</td></tr><tr><td>&gt;1500</td><td>95</td><td>52 KHACHATRY..15AZ CMS</td><td>&ge; 2 &gamma;, &ge; 1 jet, (Razor), bino- like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt;1000</td><td>95</td><td>52 KHACHATRY..15AZ CMS</td><td>&ge; 1 &gamma;, &ge; 2 jet, wino-like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt;670</td><td>95</td><td>53 AAD</td><td>14E ATLS &ell;<sup>&plusmn;</sup> &ell;(&ell;+)&plusmn; jets, q&#773; &rarr; q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub>, q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub> &rarr; W(*)&plusmn; q&#773;&chi;<sup>0</sup><sub>2</sub>, q&#773;&chi;<sup>0</sup><sub>2</sub> &rarr; Z(*) q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> &lt; 300 GeV</td></tr><tr><td>&gt;780</td><td>95</td><td>53 AAD</td><td>14E ATLS &ell;<sup>&plusmn;</sup> &ell;(&ell;+)&plusmn; jets, q&#773; &rarr; q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub>, q&#773;&chi;<sup>&plusmn;</sup><sub>1</sub> &rarr; &ell;<sup>&plusmn;</sup>&nu;<sub>1</sub>, q&#773;&chi;<sup>0</sup><sub>2</sub>, q&#773;&chi;<sup>0</sup><sub>2</sub> &rarr; &ell;<sup>&plusmn;</sup>&ell;(&nu;&nu;) q&#773;&chi;<sup>0</sup><sub>1</sub> simplified model</td></tr><tr><td>&gt;1000</td><td>95</td><td>54 CHATRCHYAN 13AO CMS</td><td>&ell;<sup>&plusmn;</sup>&ell;+ jets + E<sub>T</sub>, CMSSM, m<sub>0</sub> &lt; 700 GeV</td></tr><tr><td>&gt;1350</td><td>95</td><td>55 CHATRCHYAN 13AV CMS</td><td>jets + (leptons) + E<sub>T</sub>, CMSSM, m<sub>g&#773;</sub> = m<sub>q&#773;</sub></td></tr><tr><td>&gt;800</td><td>95</td><td>56 CHATRCHYAN 13W CMS</td><td>&ge; 1 photons + jets + E<sub>T</sub>, GGM, wino-like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt;1000</td><td>95</td><td>56 CHATRCHYAN 13W CMS</td><td>&ge; 2 photons + jets + E<sub>T</sub>, GGM, bino-like NLSP, m<sub>&chi;</sub><sup>0</sup><sub>1</sub> = 375 GeV</td></tr><tr><td>&gt;340</td><td>95</td><td>57 DREINER</td><td>12A THEO m<sub>q&#773;</sub> ~ m<sub>&chi;</sub><sup>0</sup><sub>1</sub></td></tr><tr><td>&gt;650</td><td>95</td><td>58 DREINER</td><td>12A THEO m<sub>q&#773;</sub> ~ m<sub>&chi;</sub><sup>0</sup><sub>1</sub></td></tr></tbody></table>

<footnote n="1">1 AAD 23AE searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for events with 2 &ell; with same flavour and opposite sign, plus jets and E<sub>T</sub>, defining signal region with the dilepton invariant mass both on- and off-shell with respect to the Z boson. No significant excess above the Standard Model predictions is observed. Limits are set on models of strong and electroweak production. In this case, limits are placed on the mass of pair-produced squarks, assuming a scenario like in Tsqk2, see figure 16.</footnote>

<footnote n="2">2 TUMASYAN 23x searched in 138 fb⁻¹ of pp collisions at √s = 13 TeV for squark pair production with cascade decays to CP-even singlet-like Higgs bosons (H<sub>1</sub>), leading to final states with small missing transverse momentum. This search targets H<sub>1</sub> decays to b&bar;B-pairs that are reconstructed in large-area (AKB) jets. No significant excess above the Standard Model expectations is observed. Limits are set in the next-to-minimal supersymmetric extension of the SM, where a singlino of low mass leads to squark and gluino cascade decays that can predominantly end in a highly Lorentz-boosted singlet-like H<sub>1</sub> and a singlino-like neutralino q&#773;&chi;<sup>0</sup><sub>S</sub> of small transverse momentum. The eight first- and second-generation squarks are assumed mass-degenerate, and the gluino mass is set at 1% larger.</footnote>

<footnote n="3">3 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.</footnote>
⁴AAD 21f searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for pair production of squarks in events with a high-pT jet and $E_T$. No significant excess above the Standard Model predictions is observed. Limits are set on the t̄ mass in the Tstop3 and Tstop4, on the b̄ mass in the Tsbot1, and on the q̄ mass in the Tsqk1 simplified model (four-flavour, two chirality states degeneracy).

⁵AAD 21l searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for pair production of gluino 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.

⁶SIRUNYAN 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 $E_T$. 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 $\tilde{\chi}_2^0$ and $\tilde{\chi}_1^\pm$ mass in Tch1n2Fa, see their Figure 11, on the $\tilde{\chi}_1^0$ mass in Tn1n1C and Tn1n1B for $m_{\tilde{\chi}_2^0} = m_{\tilde{\chi}_1^\pm} = m_{\tilde{\chi}_1^0}$, see their Figure 12. Limits are also set on the light squark mass for the simplified model Tsqk2A, on the bottom mass in Tsbot3, see their Figure 13, and on the slepton mass in direct electroweak pair production of mass-degenerate left- and right-handed sleptons (selectrons and smuons), see their Figure 14.

⁷SIRUNYAN 19AG searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with two photons and large $E_T$. 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.

⁸SIRUNYAN 19CH searched in 137 fb⁻¹ of pp collisions at √s = 13 TeV for events containing 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 and Tglu3A simplified models, see their Figure 13. Limits are also set on squark, bottom and stop masses in the Tsqk1, Tsbot1, Tstop1 simplified models, see their Figure 14.

⁹SIRUNYAN 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 $E_T$. 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 Tch1n1A 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.

¹⁰AABOUD 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 Tsqk2 model in case of $m_{\tilde{\chi}_1^0} = 1$ GeV: for any $m_{\tilde{\chi}_2^0}$, squark masses below 1200 GeV are excluded, see their Fig. 14(b).

¹¹AABOUD 18BV searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one jet identified as c-jet, large missing transverse energy and no leptons. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in Tsqk1 models considering only $\tilde{c}_1$. In scenarios with massless neutralinos, squark masses below 850 GeV are excluded. If the differences of the $\tilde{c}_1$ and $\tilde{\chi}_1^0$ masses are below 100 GeV, squark masses below 500 GeV are excluded. See their Fig.6 and Fig.7.

¹²AABOUD 18I searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one jet with a transverse momentum above 250 GeV and no leptons. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in Tsqk1 models. In the compressed scenario with similar squark and neutralino masses, squark masses below 710 GeV are excluded. See their Fig.10(b).

¹³AABOUD 18V 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 are interpreted in terms of lower limits on the masses of squark in Tsqk4B models. Masses below 1820 GeV are excluded for any NLSP mass, see their Fig. 9.

¹⁴AABOUD 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 Tsqk1 model: squark masses below 1550 GeV are excluded for massless LSP, see their Fig. 13(a).

¹⁵AABOUD 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 Tsqk3 model. Assuming that $m_{\tilde{\chi}_1^\pm} = 0.5 (m_{\tilde{q}} + m_{\tilde{\chi}_1^0})$, squark masses below 1150 GeV are excluded for massless LSP, see their Fig. 14(a). Exclusions are also shown assuming $m_{\tilde{\chi}_1^0} = 60$ GeV, see their Fig. 14(b).

¹⁶SIRUNYAN 18AA searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one photon and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on wino masses in a general gauge-mediated SUSY breaking (GGM) scenario with bino-like $\tilde{\chi}_1^0$ and wino-like $\tilde{\chi}_1^\pm$ and $\tilde{\chi}_1^0$, see Figure 7. Limits are also set on the NLSP mass in the Tch1n1A and Tch1n1A 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.

¹⁷SIRUNYAN 18AY searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events containing one or more jets and significant $E_T$. 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, bottom 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 $< c_T < 10^5$ mm, see their Figure 4.

¹⁸AABOUD 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 1.25 TeV are set on the 1st and 2nd generation squark masses in Tsqk3 simplified models, with $x = (m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_1^0}) / (m_{\tilde{q}} - m_{\tilde{\chi}_1^0}) = 1/2$. Similar limits are obtained for variable x and fixed neutralino mass, $m_{\tilde{\chi}_1^0} = 60$ GeV. See their Figure 13.

¹⁹AABOUD 17N searched in 14.7 fb⁻¹ of pp collisions at √s = 13 TeV for events with 2 same-flavour, opposite-sign leptons (electrons or muons), jets and large missing transverse momentum. The results are interpreted as 95% C.L. limits in Tsqk2 models, assuming $m_{\tilde{\chi}_1^0} = 0$ GeV and $m_{\tilde{\chi}_2^0} = 600$ GeV. See their Fig. 12 for exclusion limits as a function of $m_{\tilde{\chi}_2^0}$.

²⁰KHACHATRYAN 17P searched in 2.3 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, 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.

²¹KHACHATRYAN 17V searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for events with two photons and large $E_T$. 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.

²²SIRUNYAN 17AY searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one photon, jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu4A and Tglu4B simplified models, and on the squark mass in the Tsqk4A and Tsqk4B simplified models, see their Figure 6.

²³SIRUNYAN 17AZ 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 Tsqk1 simplified model (for single light squark and for 8 degenerate light squarks), on the bottom mass in the Tsbot1 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.

²⁴SIRUNYAN 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 Tsqk1 simplified model, on the stop mass in the Tstop1 simplified model, and on the bottom mass in the Tsbot1 simplified model, see Fig. 13.

²⁵AABOUD 16D searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events with an energetic jet and large missing transverse momentum. The results are interpreted as 95% C.L. limits on masses of first and second generation squarks decaying into a quark and the lightest neutralino in scenarios with $m_{\tilde{q}} - m_{\tilde{\chi}_1^0} < 25$ GeV. See their Fig. 6.

²⁶AABOUD 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. First- and second-generation squark masses below 1030 GeV are excluded at the 95% C.L. decaying to quarks and a massless lightest neutralino. See their Fig. 7a.

²⁷KHACHATRYAN 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 $M_{T2}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the squark mass in the Tsqk1 simplified model, both in the assumption of a single light squark and of 8 degenerate squarks, see Fig. 11 and Table 3.

²⁸AAD 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 squark mass in several R-parity conserving models. See their Figs. 9, 11, 18, 22, 24, 27, 28.

²⁹AAD 15CS searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for evidence of pair production of squarks, decaying into a quark and a neutralino, where a photon was radiated either from an initial-state quark, from an intermediate quark, or from a final-state quark. No evidence was found for an excess above the expected level of Standard Model background and a 95% C.L. exclusion limit is set on the squark mass as a function of the squark-neutralino mass difference, see Fig. 19.

³⁰AAD 15K searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for events containing at least two jets, where the two leading jets are each identified as originating from c-quarks, 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 mass of superpartners of charm quarks (c̄). Assuming that the decay $c̄ → c\tilde{\chi}_1^0$ takes place 100% of the time, a scalar charm mass below 490 GeV is excluded for $m_{\tilde{\chi}_1^0} < 200$ GeV. For more details, see their Fig. 2.

³¹KHACHATRYAN 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 squark mass in simplified models where the decay $\tilde{q} → q\tilde{\chi}_1^0$ takes place with a branching ratio of 100%, both for the case of a single light squark or 8 degenerate squarks, 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.

³²AAD 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 over the expected SM background is observed. Exclusion limits are derived in simplified models containing squarks that decay via $\tilde{q} → q\tilde{\chi}_1^0$, where either a single light state or two degenerate generations of squarks are assumed, see Fig. 10.

³³CHATRCHYAN 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 squark masses in simplified models where the decay $\tilde{q} → q\tilde{\chi}_1^0$ 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.

34 CHATRCHYAN 141 searched in $19.5 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 8$ 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 squarks that decay via $\tilde{q} \to q\tilde{\chi}_1^0$, where either a single light state or two degenerate generations of squarks are assumed, see Fig. 7a.

35 AAD 13L searched in $4.7 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for the production of squarks and gluinos in events containing jets, missing transverse momentum and no high-$p_T$ electrons or muons. No excess over the expected SM background is observed. In mSUGRA/CMSSM models with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, squarks and gluinos of equal mass are excluded for masses below 1360 GeV at 95% C.L. In a simplified model containing only squarks of the first two generations, a gluino octet and a massless neutralino, squark masses below 1320 GeV are excluded at 95% C.L. for gluino masses below 2 TeV. See Figures 10–15 for more precise bounds.

36 AAD 13Q searched in $4.7 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events containing a high-$p_T$ isolated photon, at least one jet identified as originating from a bottom quark, and high missing transverse momentum. Such signatures may originate from supersymmetric models with gauge-mediated supersymmetry breaking in events in which one of a pair of higgsino-like neutralinos decays into a photon and a gravitino while the other decays into a Higgs boson and a graviton. No significant excess above the expected background was found and limits were set on the squark mass as a function of the neutralino mass in a generalized GMSB model (GGM) with a higgsino-like neutralino NLSP, see their Fig. 4. For neutralino masses greater than 220 GeV, squark masses below 1020 GeV are excluded at 95% C.L.

37 CHATRCHYAN 13R looked in $4.98 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with two opposite-sign leptons $(e, \mu, \tau)$, jets and missing transverse energy. No excess beyond the Standard Model expectation is observed. Exclusion limits are derived in the mSUGRA/CMSSM model with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, see Fig. 6.

38 CHATRCHYAN 13G searched in $4.98 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for the production of squarks and gluinos in events containing 0,1,2, $\ge 3$ b-jets, missing transverse momentum and no electrons or muons. No excess over the expected SM background is observed. In mSUGRA/CMSSM models with $\tan\beta = 10$, $A_0 = 0$, and $\mu > 0$, squarks and gluinos of equal mass are excluded for masses below 1250 GeV at 95% C.L. Exclusions are also derived in various simplified models, see Fig. 7.

39 CHATRCHYAN 13H searched in $4.96 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with two photons, $\ge 4$ jets and low $E_T$ due to $\tilde{q} \to \gamma\tilde{\chi}_1^0$ decays in a stealth SUSY framework, where the $\tilde{\chi}_1^0$ decays through a singino ($\tilde{s}$) intermediate state to $\gamma S\tilde{G}$, with the singlet state $S$ decaying to two jets. No significant excess above the expected background was found and limits were set in a particular R-parity conserving stealth SUSY model. The model assumes $m_{\tilde{\chi}_1^0} = 0.5 m_{\tilde{q}}$, $m_{\tilde{s}} = 100$ GeV and $m_S = 90$ GeV. Under these assumptions, squark masses less than 1430 GeV were excluded at the 95% C.L.

40 CHATRCHYAN 13T searched in $11.7 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events with at least two energetic jets and significant $E_T$, using the $\alpha_T$ variable to discriminate between processes with genuine and misreconstructed $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on squark masses in simplified models where the decay $\tilde{q} \to q\tilde{\chi}_1^0$ takes place with a branching ratio of 100%, assuming an eightfold degeneracy of the masses of the first two generation squarks, see Fig. 8 and Table 9. Also limits in the case of a single light squark are given.

41 AAD 12AX searched in $1.04 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for supersymmetry in events containing jets, missing transverse momentum and one isolated electron or muon. No excess over the expected SM background is observed and model-independent limits are set on the cross section of new physics contributions to the signal regions. In mSUGRA/CMSSM models with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, squarks and gluinos of equal mass are excluded for masses below 820 GeV at 95% C.L. Limits are also set on simplified models for squark production and decay via an intermediate chargino and on supersymmetric models with bilinear R-parity violation. Supersedes AAD 11G.

42 AAD 12CJ searched in $4.7 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events containing one or more isolated leptons (electrons or muons) and $E_T$. The observations are in good agreement with the SM expectations and exclusion limits have been set in number of SUSY models. In the mSUGRA/CMSSM model with $\tan\beta = 10$, $A_0 = 0$, and $\mu > 0$, 95% C.L. exclusion limits have been derived for $m_{\tilde{q}} < 1200$ GeV, assuming equal squark and gluino masses. In minimal GMSB, values of the effective SUSY breaking scale $\Lambda < 50$ TeV are excluded at 95% C.L. for $\tan\beta < 45$. Also exclusion limits in a number of simplified models have been presented, see Figs. 10 and 12.

43 AAD 12CP searched in $4.8 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with two photons and large $E_T$ due to $\tilde{q} \to \gamma\tilde{G}$ decays in a GMSB framework. No significant excess above the expected background was found and limits were set on the squark mass as a function of the neutralino mass in a generalized GMSB model (GGM) with a bino-like neutralino NLSP. The other sparticle masses were decoupled, $\tan\beta = 2$ and $c\tau_{NLSP} < 0.1$ mm. Also, in the framework of the SP8 model, a 95% C.L. lower limit was set on the breaking scale $\Lambda$ of 196 TeV.

44 AAD 12W searched in $1.04 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for the production of squarks and gluinos in events containing jets, missing transverse momentum and no electrons or muons. No excess over the expected SM background is observed. In mSUGRA/CMSSM models with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, squarks and gluinos of equal mass are excluded for masses below 950 GeV at 95% C.L. In a simplified model containing only squarks of the first two generations, a gluino octet and a massless neutralino, squark masses below 875 GeV are excluded at 95% C.L.

45 CHATRCHYAN 12 looked in $35 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with $e$ and/or $\mu$ and/or jets, a large total transverse energy, and $E_T$. The event selection is based on the dimensionless razor variable $R$, related to the $E_T$ and $M_T$, an indicator of the heavy particle mass scale. No evidence for an excess over the expected background is observed. Limits are derived in the CMSSM ($m_0, m_{1/2}$) plane for $\tan\beta = 3, 10$ and 50 (see Fig. 7 and 8). Limits are also obtained for Simplified Model Spectra.

46 CHATRCHYAN 12AE searched in $4.98 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with at least three jets and large missing transverse momentum. No significant excess over the expected SM backgrounds are observed and 95% C.L. limits on the production cross section of squarks in a scenario where $\tilde{q} \to q\tilde{\chi}_1^0$ with a 100% branching ratio, see Fig. 3. For $m_{\tilde{\chi}_1^0} < 200$ GeV, values of $m_{\tilde{q}}$ below 760 GeV are excluded at 95% C.L. Also limits in the CMSSM are presented, see Fig. 2.

47 CHATRCHYAN 12AT searched in $4.73 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for the production of squarks and gluinos in events containing jets, missing transverse momentum and no electrons or muons. No excess over the expected SM background is observed. In

mSUGRA/CMSSM models with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, squarks with masses below 1110 GeV are excluded at 95% C.L. Squarks and gluinos of equal mass are excluded for masses below 1180 GeV at 95% C.L. Exclusions are also derived in various simplified models, see Fig. 6.

48 AABOUD 18V searched in $36.1 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 13$ 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 Tskq5 model. Squark masses below 1100 GeV are excluded if $(m_{\tilde{\chi}_2^0} - m_{\tilde{\chi}_1^0})/(m_{\tilde{q}} - m_{\tilde{\chi}_1^0}) < 0.95$ and $m_{\tilde{\chi}_1^0} = 60$ GeV, see their Fig. 16(a).

49 KHACHATRYAN 16BT performed a global Bayesian analysis of a wide range of CMS results obtained with data samples corresponding to $5.0 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV and in $19.5 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 8$ 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.

50 AAD 15AI searched in $20 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 8$ 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 squark masses in the CMSSM/mSUGRA, see Fig. 15, in the NUHMG, see Fig. 16, and in various simplified models, see Figs. 19–21.

51 KHACHATRYAN 15AR searched in $19.7 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 8$ TeV for events containing jets, either a charged lepton or a photon, and low missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the squark mass in a stealth SUSY model where the decays $\tilde{q} \to q\tilde{\chi}_1^0$, $\tilde{\chi}_1^\pm \to \tilde{S}W^\pm$, $\tilde{S} \to S\tilde{G}$ and $S \to gg$, with $m_{\tilde{S}} = 100$ GeV and $m_S = 90$ GeV, take place with a branching ratio of 100%. See Fig. 6 for $\gamma$ or Fig. 7 for $\ell^\pm$ analyses.

52 KHACHATRYAN 15AZ searched in $19.7 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 8$ 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.

53 AAD 14E searched in $20.3 \text{ fb}^{-1}$ 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. 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 $\tilde{q} \to q'\tilde{\chi}_1^\pm, \tilde{\chi}_1^\pm \to W^(*)\tilde{\chi}_2^0, \tilde{\chi}_2^0 \to Z^(*)\tilde{\chi}_1^0$ simplified model, the following assumptions have been made: $m_{\tilde{\chi}_1^\pm} = 0.5 m_{\tilde{\chi}_1^0} + m_{\tilde{g}}, m_{\tilde{\chi}_2^0} = 0.5 (m_{\tilde{\chi}_1^0} + m_{\tilde{\chi}_1^\pm})$. In the $\tilde{q} \to q'\tilde{\chi}_1^0$ or $\tilde{q} \to q'\tilde{\chi}_2^0, \tilde{\chi}_1^\pm \to \ell^\pm\nu\tilde{\chi}_1^0$ or $\tilde{\chi}_2^0 \to \ell^\pm\ell^\pm(\nu\nu)\tilde{\chi}_1^0$ simplified model, the following assumptions have been made: $m_{\tilde{\chi}_1^\pm} = m_{\tilde{\chi}_1^0} = 0.5 (m_{\tilde{\chi}_1^0} + m_{\tilde{g}}), m_{\tilde{\chi}_1^0} < 460$ GeV. Limits are also derived in the mSUGRA/CMSSM, bRPV and GMSB models, see their Fig. 8.

54 CHATRCHYAN 13AO searched in $4.98 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with two opposite-sign isolated leptons accompanied by hadronic jets and $E_T$. No significant excesses over the expected SM backgrounds are observed and 95% C.L. exclusion limits are derived in the mSUGRA/CMSSM model with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, see Fig. 8.

55 CHATRCHYAN 13AV searched in $4.7 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for new heavy particle pairs decaying into jets (possibly b-tagged), leptons and $E_T$ using the Razor variables. No significant excess over the expected SM backgrounds are observed and 95% C.L. exclusion limits are derived in the mSUGRA/CMSSM model with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, see Fig. 3. The results are also interpreted in various simplified models, see Fig. 4.

56 CHATRCHYAN 13W searched in $4.93 \text{ fb}^{-1}$ of pp collisions at $\sqrt{s} = 7$ TeV for events with one or more photons, hadronic jets and $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on squark masses in the general gauge-mediated SUSY breaking model (GGM), for both a wino-like and bino-like neutralino NLSP scenario, see Fig. 5.

57 DREINER 12A reassesses constraints from CMS (at 7 TeV, $\sim 4.4 \text{ fb}^{-1}$) under the assumption that the first and second generation squarks and the lightest SUSY particle are quasi-degenerate in mass (compressed spectrum).

58 DREINER 12A reassesses constraints from CMS (at 7 TeV, $\sim 4.4 \text{ fb}^{-1}$) under the assumption that the first and second generation squarks, the gluino, and the lightest SUSY particle are quasi-degenerate in mass (compressed spectrum).

## R-parity violating $\tilde{q}$ (Squark) 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 100–720</td><td>95</td><td>1 SIRUNYAN</td><td>18EA CMS</td><td>2 large jets with four-parton sub-structure, $\tilde{q} \to 4q$</td></tr><tr><td>&gt;1600</td><td>95</td><td>2 KHACHATRY...16BX CMS</td><td></td><td>$\tilde{q} \to q\tilde{\chi}_1^0, \tilde{\chi}_1^0 \to \ell\ell\nu, \lambda_{121}$ or $\lambda_{122} \neq 0, m_{\tilde{g}} = 2400$ GeV</td></tr><tr><td>&gt;1000</td><td>95</td><td>3 AAD</td><td>15CB ATLS</td><td>jets, $\tilde{q} \to q\tilde{\chi}_1^0, \tilde{\chi}_1^0 \to \ell\ell qq, m_{\tilde{\chi}_1^0} = 108$ GeV and $2.5 &lt; c\tau_{\tilde{\chi}_1^0} < 200$ mm</td></tr><tr><td></td><td></td><td>4 AAD</td><td>12AX ATLS</td><td>$\ell +jets + \ell^T$, CMSSM, $m_{\tilde{q}} = m_{\tilde{g}} \ge 3\ell^\pm$</td></tr><tr><td></td><td></td><td>5 CHATRCHYAN 12AL CMS</td><td></td><td></td></tr></tbody></table>

1 SIRUNYAN 18EA searched in $38.2 \text{ fb}^{-1}$ 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.

2 KHACHATRYAN 16BX searched in $19.5 \text{ fb}^{-1}$ 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 $\lambda_{121} \neq 0$.
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.

³AAD 15CB searched for events containing at least one long-lived particle that decays to 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 multilayer 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. 14–20.

⁴AAD 12AX searched in 1.04 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV for supersymmetry in events containing jets, missing transverse momentum and one isolated electron or muon. No excess over the expected SM background is observed and model-independent limits are set on the cross section of new physics contributions to the signal regions. In mSUGRA/CMSSM models with $\tan\beta = 10$, $A_0 = 0$ and $\mu > 0$, squarks and gluinos of equal mass are excluded for masses below 820 GeV at 95% C.L. Limits are also set on simplified models for squark production and decay via an intermediate chargino and on supersymmetric models with bilinear R-parity violation. Supersedes AAD 11G.

⁵CHATRCHYAN 12AL looked in 4.98 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV for anomalous production of events with three or more isolated leptons. Limits on squark and gluino masses are set in RPV SUSY models with leptonic LLE couplings, $\lambda_{123} > 0.05$, and hadronic UDD couplings, $\chi''_{112} > 0.05$, see their Fig. 5. In the UDD case the leptons arise from supersymmetric cascade decays. A very specific supersymmetric spectrum is assumed. All decays are prompt.

## Long-lived $\tilde{q}$ (Squark) mass limit

The following are bounds on long-lived scalar squarks, assumed to hadronise into hadrons with lifetime long enough to escape the detector prior to a possible decay. Limits may depend on the mixing angle of mass eigenstates: $\tilde{q}_1 = \tilde{q}_L \cos\theta_q + \tilde{q}_R \sin\theta_q$.

The coupling to the $Z^0$ boson vanishes for up-type squarks when $\theta_u=0.98$, and for down type squarks when $\theta_d=1.17$.

<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;1250</td><td>95</td><td>1 AABOUD</td><td>19AT ATLS</td><td>$\tilde{b}$ R-hadrons</td></tr><tr><td>&gt;1340</td><td>95</td><td>2 AABOUD</td><td>19AT ATLS</td><td>$\tilde{t}$ R-hadrons</td></tr><tr><td>&gt;1600</td><td>95</td><td>3 SIRUNYAN</td><td>19BH CMS</td><td>long-lived $\tilde{t}$, RPV, $\tilde{t} \to \overline{d}\overline{d}$, 10 mm &lt; $\zeta\tau$ &lt; 110 mm</td></tr><tr><td>&gt;1350</td><td>95</td><td>3 SIRUNYAN</td><td>19BH CMS</td><td>long-lived $\tilde{t}$, RPV, $\tilde{t} \to b\ell$, 7 mm &lt; $\zeta\tau$ &lt; 110 mm</td></tr><tr><td>&gt; 805</td><td>95</td><td>4 AABOUD</td><td>16B ATLS</td><td>$\tilde{b}$ R-hadrons</td></tr><tr><td>&gt; 890</td><td>95</td><td>5 AABOUD</td><td>16B ATLS</td><td>$\tilde{t}$ R-hadrons</td></tr><tr><td>&gt;1040</td><td>95</td><td>6 KHACHATRY...16BW CMS</td><td>$\tilde{t}$ R-hadrons, cloud interaction model</td><td></td></tr><tr><td>&gt;1000</td><td>95</td><td>6 KHACHATRY...16BW CMS</td><td>$\tilde{t}$ R-hadrons, charge-suppressed interaction model</td><td></td></tr><tr><td>&gt; 845</td><td>95</td><td>7 AAD</td><td>15AE ATLS</td><td>$\tilde{b}$ R-hadron, stable, Regge model</td></tr><tr><td>&gt; 900</td><td>95</td><td>7 AAD</td><td>15AE ATLS</td><td>$\tilde{t}$ R-hadron, stable, Regge model</td></tr><tr><td>&gt;1500</td><td>95</td><td>7 AAD</td><td>15AE ATLS</td><td>$\tilde{g}$ decaying to 300 GeV stable sleptons, LeptoSUSY model</td></tr><tr><td>&gt; 751</td><td>95</td><td>8 AAD</td><td>15BM ATLS</td><td>$\tilde{b}$ R-hadron, stable, Regge model</td></tr><tr><td>&gt; 766</td><td>95</td><td>8 AAD</td><td>15BM ATLS</td><td>$\tilde{t}$ R-hadron, stable, Regge model</td></tr><tr><td>&gt; 525</td><td>95</td><td>9 KHACHATRY...15AK CMS</td><td>$\tilde{t}$ R-hadrons, 10 $\mu$s &lt; $\tau$ &lt; 1000 s</td><td></td></tr><tr><td>&gt; 470</td><td>95</td><td>9 KHACHATRY...15AK CMS</td><td>$\tilde{t}$ R-hadrons, 1 $\mu$s &lt; $\tau$ &lt; 1000 s</td><td></td></tr></tbody></table>

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

<table><tbody><tr><td>&gt; 683</td><td>95</td><td>10 AAD</td><td>13AA ATLS</td><td>$\tilde{t}$, R-hadrons, generic interaction model</td></tr><tr><td>&gt; 612</td><td>95</td><td>11 AAD</td><td>13AA ATLS</td><td>$\tilde{b}$, R-hadrons, generic interaction model</td></tr><tr><td>&gt; 344</td><td>95</td><td>12 AAD</td><td>13BC ATLS</td><td>R-hadrons, $\tilde{t} \to b\chi_1^0$, Regge model, lifetime between 10<sup>-5</sup> and 10<sup>3</sup> s, $m_{\chi_1^0} = 100$ GeV</td></tr><tr><td>&gt; 379</td><td>95</td><td>13 AAD</td><td>13BC ATLS</td><td>R-hadrons, $\tilde{t} \to t\chi_1^0$, Regge model, lifetime between 10<sup>-5</sup> and 10<sup>3</sup> s, $m_{\chi_1^0} = 100$ GeV</td></tr><tr><td>&gt; 935</td><td>95</td><td>14 CHATRCHYAN 13AB CMS</td><td></td><td>long-lived $\tilde{t}$ forming R-hadrons, cloud interaction model</td></tr></tbody></table>

¹AABOUD 19AT searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for metastable and stable R-hadrons. Multiple search strategies for a wide range of lifetimes, corresponding to path lengths of a few meters, are defined. No significant deviations from the expected Standard Model background are observed. Sbottom R-hadrons are excluded at 95% C.L. for masses below 1250 GeV. Less stringent constraints are achieved with the muon-spectrometer agnostic analysis. See their Figure 9 (bottom-left).

²AABOUD 19AT searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for metastable and stable R-hadrons. Multiple search strategies for a wide range of lifetimes, corresponding to path lengths of a few meters, are defined. No significant deviations from the expected Standard Model background are observed. Stop R-hadrons are excluded at 95% C.L. for masses below 1340 GeV. Similar constraints are achieved with the muon-spectrometer agnostic analysis. See their Figure 9 (bottom-right).

³SIRUNYAN 19BH searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for long-lived particles decaying into jets, with each long-lived particle having a decay vertex well displaced from the production vertex. The selected events are found to be consistent with standard model predictions. Limits are set on the gluino mass in a GMSB model where the gluino is decaying via $\tilde{g} \to g\tilde{G}$, see their Figure 4 and in an RPV model of supersymmetry where the gluino is decaying via $\tilde{g} \to \overline{t}\overline{d}\overline{s}$, see their Figures 5. Limits are also set on the stop mass in two RPV models, see their Figure 6 (for $\tilde{t} \to b\ell$ decays) and Figure 7 (for $\tilde{t} \to \overline{d}\overline{d}$ decays).

⁴AABOUD 16b searched in 3.2 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for long-lived R-hadrons using observables related to large ionization losses and slow propagation velocities, which are signatures of heavy charged particles traveling significantly slower than the speed of light. Exclusion limits at 95% C.L. are set on the long-lived bottom masses exceeding 805 GeV. See their Fig. 5.

⁵AABOUD 16b searched in 3.2 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for long-lived R-hadrons using observables related to large ionization losses and slow propagation velocities, which are signatures of heavy charged particles traveling significantly slower than the speed of light. Exclusion limits at 95% C.L. are set on the long-lived bottom masses exceeding 890 GeV. See their Fig. 5.

⁶KHACHATRYAN 16BW searched in 2.5 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for events with heavy stable charged particles, identified by their anomalously high energy deposits in the silicon tracker and/or long time-of-flight measurements by the muon system. No evidence for an excess over the expected background is observed. Limits are derived for pair production of top squarks as a function of mass, depending on the interaction model, see Fig. 4 and Table 7.

⁷AAD 15AE searched in 19.1 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for heavy long-lived charged particles, measured through their specific ionization energy loss in the ATLAS pixel detector or their time-of-flight in the ALTAS muon system. In the absence of an excess of events above the expected backgrounds, limits are set R-hadrons in various scenarios, see Fig. 11. Limits are also set in LeptoSUSY models where the gluino decays to stable 300 GeV leptons, see Fig. 9.

⁸AAD 15BM searched in 18.4 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for stable and metastable non-relativistic charged particles through their anomalous specific ionization energy loss in the ATLAS pixel detector. In absence of an excess of events above the expected backgrounds, limits are set on stable bottom and top squark R-hadrons, see Table 5.

⁹KHACHATRYAN 15AK looked in a data set corresponding to fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV, and a search interval corresponding to 281 h of trigger lifetime, for long-lived particles that have stopped in the CMS detector. No evidence for an excess over the expected background in a cloud interaction model is observed. Assuming the decay $\tilde{t} \to t\chi_1^0$ and lifetimes between 1 $\mu$s and 1000 s, limits are derived on $\tilde{t}$ production as a function of $m_{\chi_1^0}$, see Figs. 4 and 7. The exclusions require that $m_{\chi_1^0}$ is kinematically consistent with the minimum values of the jet energy thresholds used.

¹⁰AAD 13AA searched in 4.7 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV for events containing colored long-lived particles that hadronize forming R-hadrons. No significant excess above the expected background was found. Long-lived R-hadrons containing a $\tilde{t}$ are excluded for masses up to 683 GeV at 95% C.L in a general interaction model. Also, limits independent of the fraction of R-hadrons that arrive charged in the muon system were derived, see Fig. 6.

¹¹AAD 13AA searched in 4.7 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV for events containing colored long-lived particles that hadronize forming R-hadrons. No significant excess above the expected background was found. Long-lived R-hadrons containing a $\tilde{b}$ are excluded for masses up to 612 GeV at 95% C.L in a general interaction model. Also, limits independent of the fraction of R-hadrons that arrive charged in the muon system were derived, see Fig. 6.

¹²AAD 13BC searched in 5.0 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV and in 22.9 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for bottom squark R-hadrons that have come to rest within the ATLAS calorimeter and decay at some later time to hadronic jets and a neutralino. In absence of an excess of events above the expected backgrounds, limits are set on bottom masses for the decay $\tilde{b} \to b\chi_1^0$, for different lifetimes, and for a neutralino mass of 100 GeV, see their Table 6 and Fig. 10.

¹³AAD 13BC searched in 5.0 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV and in 22.9 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for bottom squark R-hadrons that have come to rest within the ATLAS calorimeter and decay at some later time to hadronic jets and a neutralino. In absence of an excess of events above the expected backgrounds, limits are set on stop masses for the decay $\tilde{t} \to t\chi_1^0$, for different lifetimes, and for a neutralino mass of 100 GeV, see their Table 6 and Fig. 10.

¹⁴CHATRCHYAN 13AB looked in 5.0 fb⁻¹ of pp collisions at $\sqrt{s} = 7$ TeV and in 18.8 fb⁻¹ of pp collisions at $\sqrt{s} = 8$ TeV for events with heavy stable particles, identified by their anomalous $dE/dx$ in the tracker or additionally requiring that it be identified as muon in the muon chambers, from pair production of $t_1$s. No evidence for an excess over the expected background is observed. Limits are derived for pair production of stops as a function of mass in the cloud interaction model (see Fig. 8 and Table 6). In the charge-suppressed model, the limit decreases to 818 GeV.

## $\tilde{b}$ (Sottom) mass limit

Limits in $e^+e^-$ depend on the mixing angle of the mass eigenstate $\tilde{b}_1 = b_L \cos\theta_b + b_R \sin\theta_b$. Coupling to the Z vanishes for $\theta_b \sim 1.17$. As a consequence, no absolute constraint in the mass region $\lesssim 40$ GeV is available in the literature at this time from $e^+e^-$ collisions. In the Listings below, we use $\Delta m = m_{\tilde{b}_1} - m_{\tilde{\chi}_1^0}$.

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 $\tilde{b}$ (Sottom) 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>&gt; 850</td><td>95</td><td>1 AAD</td><td>21AM ATLS</td><td>$\tau^\pm$s + b-jets + $\ell_T$, Tsbot4, $m_{\chi_2^0} - m_{\chi_1^0} = 130$ GeV, $m_{\chi_2^0} &lt; 180$ GeV</td></tr><tr><td>&gt;1270</td><td>95</td><td>2 AAD</td><td>21S ATLS</td><td>b-jets + $\ell_T$, Tsbot1, $m_{\chi_1^0} = 0$ GeV</td></tr><tr><td>&gt; 660</td><td>95</td><td>2 AAD</td><td>21S ATLS</td><td>b-jets + $\ell_T$, Tsbot1, $m_{\tilde{b}_1} - m_{\tilde{\chi}_1^0} = 10$ GeV</td></tr><tr><td>&gt;1600</td><td>95</td><td>3 SIRUNYAN</td><td>21M CMS</td><td>$\ell^\pm \ell^\pm + \ell_T$, Tsbot3, $m_{\chi_2^0} = 1500$ GeV, $m_{\chi_1^0} = 100$ GeV</td></tr><tr><td>&gt; 750</td><td>95</td><td>4 AAD</td><td>20V ATLS</td><td>same-sign $\ell^\pm \ell^\pm$ + jets, Tsbot2, $m_{\tilde{\chi}_1^0} = m_{\tilde{\chi}_1^0} + 100$ GeV, $m_{\tilde{\chi}_1^0} \sim 50$ GeV</td></tr></tbody></table>
# Searches Particle Listings

## Supersymmetric Particle Searches

> 850 95 5 SIRUNYAN 20T CMS same-sign $\ell^\pm\ell^\pm$ or $\ge 3\ell^\pm + \text{jets, Tsbot2, }m_{\tilde{\chi}_1}^\pm < 800$ GeV, $m_{\tilde{\chi}_1}^0 = 50$ GeV

>1500 95 6 AAD 19H ATLS $\ge 3$ b-jets + $\not{E}_T$, Tsbot4, $\ge 1$ $h(\to b\bar{b})$, $m_{\tilde{\chi}_1}^0 = 60$ GeV

>1300 95 7 AAD 19H ATLS $\ge 3$ b-jets + $\not{E}_T$, Tsbot4, $\ge 1$ $h(\to b\bar{b})$, $m_{\tilde{\chi}_2}^0 = m_{\tilde{\chi}_1}^0 + 130$ GeV

>1220 95 8 SIRUNYAN 19CH CMS jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 530 95 9 SIRUNYAN 19CI CMS $\ge 1$ $H(\to \gamma\gamma)$ + jets + $\not{E}_T$, Tsbot4, $m_{\tilde{\chi}_2}^0 = m_{\tilde{\chi}_1}^0 + 130$ GeV, $m_{\tilde{\chi}_1}^0 = 1$ GeV

> 430 95 10 AABOUD 18I ATLS $\ge 1$ jets + $\not{E}_T$, Tsbot1, $m_{\tilde{b}} - m_{\tilde{\chi}_1}^0 \sim m_b$

> 840 95 11 SIRUNYAN 18AL CMS $\ge 3$ $\ell^\pm + \text{jets} + \not{E}_T$, Tsbot2, $m_{\tilde{\chi}_1}^0 = 50$ GeV

> 975 95 12 SIRUNYAN 18AR CMS $\ell^\pm\ell^\pm + \text{jets} + \not{E}_T$, Tsbot3, $m_{\tilde{b}} = (m_{\tilde{\chi}_2}^0+m_{\tilde{\chi}_1}^0)/2$, $m_{\tilde{\chi}_1}^0 = 100$ GeV

>1060 95 13 SIRUNYAN 18AY CMS jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

>1230 95 14 SIRUNYAN 18B CMS jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 420 95 15 SIRUNYAN 18X CMS $\ge 1$ $H(\to \gamma\gamma)$ + jets + $\not{E}_T$, Tsbot4, $m_{\tilde{\chi}_2}^0 = m_{\tilde{\chi}_1}^0 + 130$ GeV, $m_{\tilde{\chi}_1}^0 < 225$ GeV

> 700 95 16 AABOUD 17AJ ATLS same-sign $\ell^\pm\ell^\pm / 3 \ell^\pm + \text{jets} + \not{E}_T$, Tsbot2, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 950 95 17 AABOUD 17AX ATLS 2 b-jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 880 95 18 AABOUD 17AX ATLS 2 b-jets + $\not{E}_T$, mixture Tsbot1 and Tsbot2 BR=50%, $m_{\tilde{\chi}_1}^0 = 0$ GeV, $m_{\tilde{\chi}_1}^\pm - m_{\tilde{\chi}_1}^0 = 1$ GeV

> 315 95 19 KHACHATRY...17A CMS 2 VBF jets + $\not{E}_T$, Tsbot1, $m_{\tilde{b}} - m_{\tilde{\chi}_1}^0 = 5$ GeV

> 450 95 20 KHACHATRY...17AW CMS $\ge 3$ $\ell^\pm$, 2 jets, Tsbot2, $m_{\tilde{\chi}_1}^0 = 50$ GeV, $m_{\tilde{\chi}_1}^\pm = 200$ GeV

> 800 95 21 KHACHATRY...17P CMS 1 or more jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

>1175 95 22 SIRUNYAN 17AZ CMS $\ge 1$ jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 890 95 23 SIRUNYAN 17K CMS jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 810 95 24 SIRUNYAN 17S CMS same-sign $\ell^\pm\ell^\pm + \text{jets} + \not{E}_T$, Tsbot2, $m_{\tilde{\chi}_1}^0 = 50$ GeV, $m_{\tilde{\chi}_1}^\pm = 100$ GeV

> 323 95 25 AABOUD 16D ATLS $\ge 1$ jet + $\not{E}_T$, Tsbot1, $m_{\tilde{b}} - m_{\tilde{\chi}_1}^0 = 5$ GeV

> 840 95 26 AABOUD 16Q ATLS 2 b-jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 100$ GeV

> 540 95 27 AAD 16BB ATLS 2 same-sign/3 $\ell^\pm + \text{jets} + \not{E}_T$, Tsbot2, $m_{\tilde{\chi}_1}^0 < 55$ GeV

> 680 95 28 KHACHATRY...16BJ CMS same-sign $\ell^\pm\ell^\pm$, Tsbot2, $m_{\tilde{\chi}_1}^\pm < 550$ GeV, $m_{\tilde{\chi}_1}^0 = 50$ GeV

> 880 95 29 KHACHATRY...16BS CMS jets + $\not{E}_T$, Tsbot1, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 550 95 30 KHACHATRY...16BY CMS opposite-sign $\ell^\pm\ell^\pm$, Tsbot3, $m_{\tilde{\chi}_1}^0 = 100$ GeV

> 600 95 31 AAD 15CJ ATLS $\tilde{b} \to b \tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 < 250$ GeV

> 440 95 31 AAD 15CJ ATLS $\tilde{b} \to t \tilde{\chi}_1^\pm, \tilde{\chi}_1^\pm \to W^*(\tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 = 60$ GeV, $m_{\tilde{b}} - m_{\tilde{\chi}_1}^0 < m_t$

> 640 95 32 KHACHATRY...15AF CMS $\tilde{b} \to b \tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 = 0$

> 650 95 33 KHACHATRY...15AH CMS $\tilde{b} \to b \tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 = 0$

> 250 95 33 KHACHATRY...15AH CMS $\tilde{b} \to b \tilde{\chi}_1^0, m_{\tilde{b}} - m_{\tilde{\chi}_1}^0 < 10$ GeV

> 570 95 34 KHACHATRY...15I CMS $\tilde{b} \to t \tilde{\chi}_1^\pm, \tilde{\chi}_1^\pm \to W^*(\tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 = 50$ GeV, $150<m_{\tilde{\chi}_1}^\pm < 300$ GeV

> 255 95 35 AAD 14T ATLS $\tilde{b}_1 \to b \tilde{\chi}_1^0, m_{\tilde{b}_1}^0 - m_{\tilde{\chi}_1}^0 \approx m_b$

> 400 95 36 CHATRCHYAN 14AH CMS jets + $\not{E}_T$, $\tilde{b} \to b \tilde{\chi}_1^0$ simplified model, $m_{\tilde{\chi}_1}^0 = 50$ GeV

>37 CHATRCHYAN 14R CMS $\ge 3$ $\ell^\pm, \tilde{b} \to t \tilde{\chi}_1^\pm, \tilde{\chi}_1^\pm \to W^*(\tilde{\chi}_1^0)$ simplified model, $m_{\tilde{\chi}_1}^0 = 50$ GeV

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

> 440 95 38 KHACHATRY...15AD CMS $\ell^\pm\ell^\mp + \text{jets} + \not{E}_T$, $\tilde{b} \to b \tilde{\chi}_1^0$

none 340-600 95 39 AAD 14AX ATLS $\ge 3$ b-jets + $\not{E}_T$, $\tilde{b} \to b \tilde{\chi}_2^0$ simplified model with $\tilde{\chi}_1^0 \to h \tilde{\chi}_1^0$, $m_{\tilde{\chi}_1}^0 = 60$ GeV, $m_{\tilde{\chi}_2}^0 = 300$ GeV

> 440 95 40 AAD 14E ATLS $\ell^\pm\ell^\pm(\ell^\mp) + \text{jets}, \tilde{b}_1 \to t \tilde{\chi}_1^\pm$ with $\tilde{\chi}_1^\pm \to W^*(\ell^\pm)\tilde{\chi}_1^0$ simplified model, $m_{\tilde{\chi}_1}^\pm = 2$ $m_{\tilde{\chi}_1}^0$

> 500 95 41 CHATRCHYAN 14H CMS same-sign $\ell^\pm\ell^\pm, \tilde{b} \to t \tilde{\chi}_1^\pm$, $\tilde{\chi}_1^\pm \to W^*(\tilde{\chi}_1^0)$ simplified model, $m_{\tilde{\chi}_1}^\pm = 2$ GeV, $m_{\tilde{\chi}_1}^0 = 100$ GeV

> 620 95 42 AAD 13AU ATLS 2 b-jets + $\not{E}_T$, $\tilde{b}_1 \to b \tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 < 120$ GeV

> 550 95 43 CHATRCHYAN 13AT CMS jets + $\not{E}_T$, $\tilde{b} \to b \tilde{\chi}_1^0$ simplified model, $m_{\tilde{\chi}_1}^0 = 50$ GeV

> 600 95 44 CHATRCHYAN 13T CMS jets + $\not{E}_T$, $\tilde{b} \to b \tilde{\chi}_1^0$ simplified model, $m_{\tilde{\chi}_1}^0 = 0$ GeV

> 450 95 45 CHATRCHYAN 13V CMS same-sign $\ell^\pm\ell^\pm + \ge 2$ b-jets, $\tilde{b} \to t \tilde{\chi}_1^\pm, \tilde{\chi}_1^\pm \to W^*(\tilde{\chi}_1^0)$ simplified model, $m_{\tilde{\chi}_1}^0 = 50$ GeV

> 390 95 46 AAD 12AN ATLS $\tilde{b}_1 \to b \tilde{\chi}_1^0$, simplified model, $m_{\tilde{\chi}_1}^0 < 60$ GeV

> 410 95 47 CHATRCHYAN 12AI CMS $\ell^\pm\ell^\pm + \text{jets} + \not{E}_T$, $\tilde{b}_1 \to b \tilde{\chi}_1^0$, simplified model, $m_{\tilde{\chi}_1}^0 = 50$ GeV

> 294 95 49 AAD 11K ATLS stable $b$

> 50 AAD 110 ATLS $\tilde{g} \to \tilde{b}_1 b, \tilde{b}_1 \to b \tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 = 60$ GeV

> 230 95 51 CHATRCHYAN 11D CMS $\tilde{b}_1, \tilde{l} \to b$

> 247 95 52 AALTONEN 10R CDF $\tilde{b}_1 \to b \tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 < 70$ GeV

> 53 ABAZOV 10L D0 $\tilde{b}_1 \to b \tilde{\chi}_1^0, m_{\tilde{\chi}_1}^0 = 0$ GeV

1 AAD 21AM searched in 139 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for pair production of bottom squarks in events with hadronically decaying $\tau^\pm$-leptons, b-tagged jets, and large $\not{E}_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom squark mass in the Tsbot4 simplified model, assuming $m_{\tilde{\chi}_1}^0 - m_{\tilde{\chi}_2}^0 = 130$ GeV, see their Figure 8.

2 AAD 21S searched in 139 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for pair production of bottom squarks, LQ or dark matter in events with b-jets and $\not{E}_T$, also using dedicated secondary-vertex-finding techniques. No significant excess above the Standard Model predictions is observed. Limits are set on $m_{\tilde{b}_1}$ in the Tsbot1 simplified model, on the LQ masses depending on the BR in $b\nu$, on scalar and pseudoscalar dark matter mediator masses. See Figures 8, 9, 10.

3 SIRUNYAN 21M searched in 137 fb⁻¹ of pp collisions at $\sqrt{s} = 13$ TeV for supersymmetry in events with two opposite-sign same-flavor leptons (electrons, muons) and $\not{E}_T$. 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 $\tilde{\chi}_2^0$ and $\tilde{\chi}_1^\pm$ mass in Tchl12Fa, see their Figure 11, on the $\tilde{\chi}_1^0$ mass in Tn1n1C and Tn1n1B for $m_{\tilde{\chi}_2}^0=m_{\tilde{\chi}_1}^\pm=m_{\tilde{\chi}_1}^0$, see their Figure 12. Limits are also set on the light squark mass for the simplified model Tsqk2A, on the bottom mass in Tsbot3, see their Figure 13, and on the slepton mass in direct electroweak pair production of mass-degenerate left- and right-handed sleptons (selectrons and muons), see their Figure 14.

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 bottom squark masses in the Tsbot2 simplified model for $m_{\tilde{\chi}_1}^\pm = m_{\tilde{\chi}_1}^0 + 100$ GeV, see their Fig. 8(a).

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 $\tilde{g} \to q\bar{q}\bar{q} + e/\mu/\tau$ or via $\tilde{g} \to t\bar{b}$, see Figure 12.
7 AAD 19h searched in 139 fb⁻¹ of pp collisions at √s = 13 TeV for events with no charged leptons, three or more b-jets, and large E<sub>T</sub>. Higgs boson candidates are reconstructed as b-jet pairs. No significant excess above the Standard Model expectations is observed. Limits up to 1300 GeV are set on the bottom mass in the Tsbot4 simplified model, see Figure 8(b), for m<sub>χ̃0</sub> = m<sub>χ̃0</sub> + 130 GeV and m<sub>χ̃0</sub> from 200 to 750 GeV.

8 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, Tsbot1, Tstop1 simplified models, see their Figure 14.

9 SIRUNYAN 19ci searched in 77.5 fb⁻¹ of pp collisions at √s = 13 TeV for events with one or more high-momentum Higgs bosons, decaying to pairs of photons, jets and E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom mass in the Tsbot4 simplified model, see Figure 3, and on the wino mass in the Tchi1n2E simplified model, see their Figure 4. Limits are also set on the higgsino mass in the Tn1n1A and Tn1n1B simplified models, see their Figure 5.

10 AABOUD 18i searched in 36.1 fb⁻¹ of pp collisions at √s = 13 TeV for events with at least one jet with a transverse momentum above 250 GeV and no leptons. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in Tsbot1 models. In the compressed scenario with bottom and neutralino masses differing by m<sub>b</sub>, bottom masses below 430 GeV are excluded. For m<sub>χ̃0</sub> = 0 they exclude bottom masses up to 610 GeV. See their Fig. 10(a).

11 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.

12 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 model, see their Figure 8, and on the neutralino 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.

13 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 simplified model, see their Figure 7. Limits are also set on the chargino/neutralino mass in the Tchi1n2E simplified model, see their Figure 8. and on the neutralino 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.

14 SIRUNYAN 18b searched in 35.9 fb⁻¹ of pp collisions at √s = 13 TeV for the pair production of third-generation squarks in events with jets and large E<sub>T</sub>. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom mass in the Tsbot1 simplified model, see their Figure 5, and on the stop mass in the Tstop4 simplified model, see their Figure 6.

15 SIRUNYAN 18x 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 photons, jets and E<sub>T</sub>. The razor variables (M<sub>R</sub> and R²) are used to categorise the events. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom mass in the Tsbot4 simplified model and on the wino mass in the Tchi1n2E simplified model, see their Figure 5. Limits are also set on the higgsino mass in the Tn1n1A and Tn1n1B simplified models, see their Figure 6.

16 AABOUD 17a 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 700 GeV are set on the bottom squark mass in Tsbot2 simplified models assuming m<sub>χ̃0</sub> = 0 GeV.

See their Figure 4(d).

17 AABOUD 17ax searched in 36 fb⁻¹ of pp collisions at √s = 13 TeV for events containing two jets identified as originating from b-quarks 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 bottom squarks. In the Tsbot1 simplified model, a b̄1 mass below 950 GeV is excluded for m<sub>χ̃0</sub> = 0 (<420) GeV. See their Fig. 7(a).

18 AABOUD 17ax searched in 36 fb⁻¹ of pp collisions at √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 bottom squarks. Assuming 50% BR for Tsbot1 and Tsbot2 simplified models, a b̄1 mass below 880 (860) GeV is excluded for m<sub>χ̃0</sub> = 0 (<250) GeV. See their Fig. 7(b).

19 KHACHATRYAN 17a searched in 18.5 fb⁻¹ of pp collisions at √s = 8 TeV for events with two forward jets, produced through vector boson fusion, and missing transverse momentum. No significant excess above the Standard Model expectations is observed. A limit is set on bottom masses in the Tsbot1 simplified model, see Fig. 3.

20 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.

21 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 Figure 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.

22 SIRUNYAN 17az searched in 35.9 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 simplified models, see their Figures 6. Limits are also set on the squark mass in the Tsqk1 simplified model, see their Fig. 7. Finally, limits are set on the stop mass in the Tstop2 simplified model, see their Fig. 8. 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 Tsbot1 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.

23 SIRUNYAN 17k searched in 2.3 fb⁻¹ of pp collisions at √s = 13 TeV for direct production of stop or bottom pairs in events with multiple jets and significant E<sub>T</sub>. 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 Tsbot1 simplified model, see Fig. 10 (also here, only the results of the all-hadronic search are used).

24 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<sub>T</sub>. 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 Tglu1B simplified models, see their Figures 5 and 6, and on the bottom mass in the Tsbot2 simplified model, see their Figure 6.

25 AABOUD 16d searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events with an energetic jet and large missing transverse momentum. The results are interpreted as 95% C.L. limits on mass of bottom decaying into a b-quark and the lightest neutralino in scenarios with m<sub>b̄1</sub> - m<sub>χ̃0</sub> between 5 and 20 GeV. See their Fig. 6.

26 AABOUD 16q searched in 3.2 fb⁻¹ of pp collisions at √s = 13 TeV for events containing two jets identified as originating from b-quarks 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. Assuming that the decay b̄1 → b̄χ̃0 1 (Tsbot1) takes place 100% of the time, a b̄1 mass below 840 (800) GeV is excluded for m<sub>χ̃0</sub> < 100 (360) GeV. Differences in mass above 100 GeV between the b̄1 and the χ̃0 1 are excluded up to a b̄1 mass of 500 GeV. For more details, see their Fig. 4.

27 AAD 16B 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<sub>T</sub>. No significant excess over the Standard Model expectation is found. Exclusion limits at 95% C.L. are set on the bottom mass for the Tsbot2 model, assuming m<sub>χ̃1±</sub> = m<sub>χ̃0</sub> + 100 GeV. See their Fig. 4c.

28 KHACHATRYAN 16Bj 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<sub>T</sub>, using the transverse mass variable MT2 to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom mass in the Tsbot1 simplified model, see Fig. 11 and Table 3.

29 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 Tglu4C simplified model, see Fig. 4, and on bottom masses in the Tsbot3 simplified model, see Fig. 5.

30 AAD 15Cj searched in 20 fb⁻¹ of pp collisions at √s = 8 TeV for evidence of third generation squarks by combining a large number of searches covering various final states. Limits on the bottom mass are shown, either assuming the b̄ → b̄χ̃0 1 decay, see Fig. 11, or assuming the b̄ → tχ̃1± decay, with tχ̃1± → W(*)χ̃0 1, see Fig. 12a, or assuming the b̄ → b̄χ̃0 2 decay, with χ̃2 0 → hχ̃0 1, see Fig. 12b. Interpretations in the pMSSM are also discussed, see Figures 13-15.

31 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<sub>T</sub>, using the transverse mass variable MT2 to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom mass in simplified models where the decay b̄ → b̄χ̃0 1 takes place with a branching ratio of 100%, see Fig. 12. See also Table 5. Exclusions in the CMSSM, assuming tanβ = 30, A0 = -2 max(m0, m1/2) and μ > 0, are also presented, see Fig. 15.

32 KHACHATRYAN 15AH searched in 19.4 or 19.7 fb⁻¹ of pp collisions at √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 bottom mass in simplified models where the decay b̄ → b̄χ̃0 1 takes place with a branching ratio of 100%, see Fig. 12. Limits are also set in a simplified model where the decay b̄ → cχ̃1± takes place with a branching ratio of 100%, see Fig. 12.

33 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 bottom mass in a simplified model where the decay b̄ → tχ̃1±, with tχ̃1± → W±χ̃0 1, takes place with a branching ratio of 100%, see Fig. 7.

34 AAD 14T searched in 20.3 fb⁻¹ of pp collisions at √s = 8 TeV for monojet-like 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 b̄1 → b̄χ̃0 1 takes place 100% of the time, see Fig. 12.

35 CHATRCHYAN 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<sub>T</sub>, using the razor variables (M<sub>R</sub> and R²) 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 b̄ → b̄χ̃0 1 takes place with a branching ratio of 100%, see Figs. 28 and 29. Exclusions in the CMSSM, assuming tanβ = 10, A0 = 0 and μ > 0, are also presented, see Fig. 26.

36 CHATRCHYAN 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 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, see their Fig. 7. Finally, limits are set on the stop mass in the Tstop1, Tstop3, Tstop4, Tstop6 and Tstop7 simplified models, see Fig. 8.
excess above the Standard Model where the decay $\tilde{b} \to t \tilde{\chi}_1^\pm$, with $\tilde{\chi}_1^\pm \to W^\pm \tilde{\chi}_1^0$, takes place with a branching ratio of 100%, see Fig. 11.

38 KHACHATRYAN 15AD searched in 19.4 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 8$ 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 bottom pair production where the bottom decays into a b-quark, two opposite-sign dileptons and a neutralino LSP, through an intermediate state containing either an off-shell Z-boson or a slepton, see Fig. 8.

39 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 $\tan\beta = 30$, $A_0 = -2$ $m_0$ and $\mu > 0$, see their Fig. 14. Also, exclusion limits are set in simplified models containing scalar bottom quarks, where the decay $\tilde{b} \to b \tilde{\chi}_2^0$ and $\tilde{\chi}_2^0 \to h \tilde{\chi}_1^0$ takes place with a branching ratio of 100%, see their Figures 11.

40 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. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing bottom, see Fig. 7. Limits are also derived in the mSUGRA/CMSSM, bRPV and GMSB models, see their Fig. 8.

41 CHATRCHYAN 14H 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 bottom mass in a simplified models where the decay $\tilde{b} \to t \tilde{\chi}_1^\pm$, $\tilde{\chi}_1^\pm \to W^\pm \tilde{\chi}_1^0$ takes place with a branching ratio of 100%, with varying mass of the $\tilde{\chi}_1^\pm$, for $m_{\tilde{\chi}_1^0} = 50$ GeV, see Fig. 6.

42 AAD 13AU searched in 20.1 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 8$ TeV for events containing two jets identified as originating from b-quarks 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. Assuming that the decay $\tilde{b}_1 \to b \tilde{\chi}_1^0$ takes place 100% of the time, a $\tilde{b}_1$ mass below 620 GeV is excluded for $m_{\tilde{\chi}_1^0} < 120$ GeV. For more details, see their Fig. 5.

43 CHATRCHYAN 13AT provides interpretations of various searches for supersymmetry by the CMS experiment based on 4.73–4.98 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 7$ TeV in the framework of simplified models. Limits are set on the bottom mass in a simplified models where bottom quarks are pair-produced and the decay $\tilde{b} \to b \tilde{\chi}_1^0$ takes place with a branching ratio of 100%, see Fig. 4.

44 CHATRCHYAN 13T searched in 11.7 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 8$ TeV for events with at least two energetic jets and significant $E_T$, using the $\alpha_T$ variable to discriminate between processes with genuine and misreconstructed $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on bottom masses in simplified models where the decay $\tilde{b} \to b \tilde{\chi}_1^0$ takes place with a branching ratio of 100%, see Fig. 8 and Table 9.

45 CHATRCHYAN 13v searched in 10.5 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 8$ TeV for events with two isolated same-sign dileptons and at least two b-jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom mass in a simplified models where the decay $\tilde{b} \to t \tilde{\chi}_1^\pm$, $\tilde{\chi}_1^\pm \to W^\pm \tilde{\chi}_1^0$ takes place with a branching ratio of 100%, with varying mass of the $\tilde{\chi}_1^\pm$, for $m_{\tilde{\chi}_1^0} = 50$ GeV, see Fig. 4.

46 AAD 12AN searched in 2.05 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 7$ TeV for scalar bottom quarks in events with large missing transverse momentum and two b-jets in the final state. The data are found to be consistent with the Standard Model expectations. Limits are set in an R-parity conserving minimal supersymmetric scenario, assuming $B(\tilde{b}_1 \to b \tilde{\chi}_1^0) = 100\%$, see their Fig. 2.

47 CHATRCHYAN 12AI looked in 4.98 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 7$ TeV for events with two same-sign leptons (e, $\mu$), but not necessarily same flavor, at least 2 b-jets and missing transverse energy. No excess beyond the Standard Model expectation is observed. Exclusion limits are derived in a simplified model for bottom pair production, where the bottom decays through $\tilde{b}_1 \to t \tilde{\chi}_1 W$, see Fig. 8.

48 CHATRCHYAN 12B0 searched in 4.7 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 7$ TeV for scalar bottom quarks in events with large missing transverse momentum and two b-jets in the final state. The data are found to be consistent with the Standard Model expectations. Limits are set in an R-parity conserving minimal supersymmetric scenario, assuming $B(\tilde{b}_1 \to b \tilde{\chi}_1^0) = 100\%$, see their Fig. 2.

49 AAD 11K looked in 34 pb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 7$ TeV for events with heavy stable particles, identified by their anomalous $dE/dx$ in the tracker or time of flight in the tile calorimeter, from pair production of $\tilde{b}$. No evidence for an excess over the SM expectation is observed and limits on the mass are derived for pair production of bottom, see Fig. 4.

50 AAD 11O looked in 35 pb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 7$ TeV for events with jets, of which at least one is a b-jet, and $E_T$. No excess above the Standard Model was found. Limits are derived in the $(m_{\tilde{g}}, m_{\tilde{b}_1})$ plane (see Fig. 2) under the assumption of 100% branching ratios and $\tilde{b}_1$ being the lightest squark. The quoted limit is valid for $m_{\tilde{b}_1} < 500$ GeV. A similar approach for $\tilde{t}_1$ as the lightest squark with $\tilde{g} \to \tilde{t}_1 t$ and $\tilde{t}_1 \to b \tilde{\chi}_1^\pm$ with 100% branching ratios leads to a gluino mass limit of 520 GeV for 130 < $m_{\tilde{t}_1} < 300$ GeV. Limits are also derived in the CMSSM ($m_0, m_{1/2}$) plane for $\tan\beta = 40$, see Fig. 4, and in scenarios based on the gauge group SO(10).

51 CHATRCHYAN 11D looked in 35 pb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 7$ TeV for events with $\ge 2$ jets, at least one of which is b-tagged, and $E_T$, where the b-jets are decay products of $\tilde{t}$ or $\tilde{b}$. No evidence for an excess over the expected background is observed. Limits are derived in the CMSSM ($m_0, m_{1/2}$) plane for $\tan\beta = 50$ (see Fig. 2).

52 AALTONEN 10R searched in 2.65 fb$^{-1}$ of $p\bar{p}$ collisions at $\sqrt{s} = 1.96$ TeV for events with $E_T$ and exactly two jets, at least one of which is b-tagged. The results are in agreement with the SM prediction, and a limit on the cross section of 0.1 pb is obtained for the

range of masses $80 < m_{\tilde{b}_1} < 280$ GeV assuming that the bottom decays exclusively to $b \tilde{\chi}_1^0$. The excluded mass region in the framework of conserved $R_p$ is shown in a plane of $(m_{\tilde{b}_1}, m_{\tilde{\chi}_1^0})$, see their Fig. 2.

53 ABAZOV 10L looked in 5.2 fb$^{-1}$ of $p\bar{p}$ collisions at $\sqrt{s} = 1.96$ TeV for events with at least 2 b-jets and $E_T$ from the production of $\tilde{b}_1 \tilde{b}_1$. No evidence for an excess over the SM expectation is observed, and a limit on the cross section is derived under the assumption of 100% branching ratio. The excluded mass region in the framework of conserved $R_p$ is shown in a plane of $(m_{\tilde{b}_1}, m_{\tilde{\chi}_1^0})$, see their Fig. 3b. The exclusion also extends to $m_{\tilde{\chi}_1^0} = 110$ GeV for $160 < m_{\tilde{b}_1} < 200$ GeV.

## R-parity violating $\tilde{b}$ (Sbottom) 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>>307</td><td>95</td><td>1 KHACHATRY...16BX</td><td>CMS</td><td>RPV, b&#x0304; &rarr; td or ts, &lambda;''<sub>332</sub> or &lambda;''<sub>331</sub> coupling</td></tr></tbody></table>

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

$$2 \text{AAD} \qquad 14E \text{ATLS} \qquad \begin{aligned} & \ell^{\pm} \ell^{\pm} (\ell^{\mp}) + \text{jets}, \tilde{b}_1 \to t \tilde{\chi}_1^{\pm} \\ & \text{with } \tilde{\chi}_1^{\pm} \to W^{(\pm)} \pm \tilde{\chi}_1^0 \text{ simplified model, } m_{\tilde{\chi}_1^{\pm}} = \frac{2}{3} m_{\tilde{\chi}_1^0} \end{aligned} \qquad \bullet \bullet \bullet$$

1 KHACHATRYAN 16BX searched in 19.5 fb$^{-1}$ of $pp$ collisions at $\sqrt{s} = 8$ TeV for events containing 2 leptons coming from R-parity-violating decays of supersymmetric particles. No excess over the expected background is observed. Limits are derived on the bottom mass, assuming the RPV $\tilde{b} \to td$ or $\tilde{b} \to ts$ decay, see Fig. 15.

2 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. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing bottom, see Fig. 7. Limits are also derived in the mSUGRA/CMSSM, bRPV and GMSB models, see their Fig. 8.

## $\tilde{t}$ (Stop) mass limit

Limits depend on the decay mode. In $e^+e^-$ collisions they also depend on the mixing angle of the mass eigenstate $\tilde{t}_1 = \tilde{t}_1 \cos\theta_t + \tilde{t}_1 \sin\theta_t$. The coupling to the Z vanishes when $\theta_t = 0.98$. In the Listings below, we use $\Delta m \equiv m_{\tilde{t}_1} - m_{\tilde{\chi}_1^0}$ or $\Delta m \equiv m_{\tilde{t}_1} - m_{\tilde{\nu}_t}$, depending on relevant decay mode. See also bounds in "$\tilde{q}$ (Squark) MASS LIMIT."

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 $\tilde{t}$ (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>>1430</td><td>95</td><td>1 HAYRAPETY...23E</td><td>CMS</td><td>γ + jets + E<sub>T</sub>, Tstop13, m<sub>χ̃1</sub><sup>0</sup> = 1170 GeV</td></tr><tr><td>>1150</td><td>95</td><td>2 TUMASYAN</td><td>23AB CMS</td><td>≥ 1 π<sup>±</sup> + E<sub>T</sub>, Tstop16, m<sub>χ̃1</sub><sup>0</sup> = 1 GeV</td></tr><tr><td>> 480</td><td>95</td><td>3 TUMASYAN</td><td>23K CMS</td><td>1 high-ρ<sub>t</sub> jet, 1 low-ρ<sub>t</sub> e or μ, Tstop3, m<sub>χ̃1</sub><sup>0</sup> - m<sub>χ̃1</sub><sup>0</sup> = 10</td></tr><tr><td>> 700</td><td>95</td><td>3 TUMASYAN</td><td>23K CMS</td><td>GeV<br>1 high-ρ<sub>t</sub> jet, 1 low-ρ<sub>t</sub> e or μ, Tstop3, m<sub>χ̃1</sub><sup>0</sup> - m<sub>χ̃1</sub><sup>0</sup> = 80</td></tr><tr><td>> 480</td><td>95</td><td>4 TUMASYAN</td><td>22Q CMS</td><td>GeV<br>2 or 3 ℓ (soft), E<sub>T</sub>; Tstop2, m<sub>χ̃1</sub><sup>0</sup> - m<sub>χ̃1</sub><sup>0</sup> = 30 GeV</td></tr><tr><td>> 540</td><td>95</td><td>4 TUMASYAN</td><td>22Q CMS</td><td>2 or 3 ℓ (soft), E<sub>T</sub>; Tstop3, m<sub>χ̃1</sub><sup>0</sup> - m<sub>χ̃1</sub><sup>0</sup> = 30 GeV</td></tr><tr><td>>1400</td><td>95</td><td>5 AAD</td><td>21AW ATLS</td><td>τ<sup>±</sup> + jets + b-jets + E<sub>T</sub>, Tstop5, m<sub>χ̃1</sub><sup>0</sup> = 1200 GeV</td></tr><tr><td>>1200</td><td>95</td><td>6 AAD</td><td>21O ATLS</td><td>ℓ<sup>±</sup> + jet + E<sub>T</sub>, Tstop1, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>> 710</td><td>95</td><td>6 AAD</td><td>21O ATLS</td><td>ℓ<sup>±</sup> + jet + E<sub>T</sub>, Tstop1, m<sub>χ̃1</sub><sup>0</sup> = 580 GeV</td></tr><tr><td>> 640</td><td>95</td><td>6 AAD</td><td>21O ATLS</td><td>ℓ<sup>±</sup> + jet + E<sub>T</sub>, Tstop3, m<sub>χ̃1</sub><sup>0</sup> = 580 GeV</td></tr><tr><td>>1000</td><td>95</td><td>7 AAD</td><td>21P ATLS</td><td>ℓ<sup>±</sup>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tstop1, m<sub>χ̃1</sub><sup>0</sup> = 0 GeV</td></tr><tr><td>> 600</td><td>95</td><td>7 AAD</td><td>21P ATLS</td><td>ℓ<sup>±</sup>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tstop2, m<sub>χ̃1</sub><sup>0</sup> = 500 GeV</td></tr><tr><td>> 550</td><td>95</td><td>7 AAD</td><td>21P ATLS</td><td>ℓ<sup>±</sup>ℓ<sup>±</sup> + jets + E<sub>T</sub>, Tstop3, m<sub>χ̃1</sub><sup>0</sup> = 500 GeV</td></tr><tr><td>>1310</td><td>95</td><td>8 SIRUNYAN</td><td>21AD CMS</td><td>jets + E<sub>T</sub>, Tstop1, m<sub>χ̃1</sub><sup>0</sup> < 300 GeV</td></tr><tr><td>>1170</td><td>95</td><td>8 SIRUNYAN</td><td>21AD CMS</td><td>jets + E<sub>T</sub>, Tstop2, m<sub>χ̃1</sub><sup>0</sup> = (m<sub>χ̃1</sub> + m<sub>χ̃0</sub>)/2, m<sub>χ̃1</sub><sup>0</sup> < 100 GeV</td></tr><tr><td>>1150</td><td>95</td><td>8 SIRUNYAN</td><td>21AD CMS</td><td>jets + E<sub>T</sub>, Tstop1 (50%) or Tstop2 (50%), m<sub>χ̃1</sub><sup>0</sup> - m<sub>χ̃1</sub><sup>0</sup> = 5 GeV, m<sub>χ̃1</sub><sup>0</sup> = 100 GeV</td></tr></tbody></table>
Searches Particle Listings
Supersymmetric Particle Searches

<table>
  <tbody>
    <tr>
      <td>&gt; 640</td>
      <td>95</td>
      <td>8 SIRUNYAN</td>
      <td>21AD CMS jets + E<sub>T</sub>, Tstop3, m<sub>t</sub> - m<sub>t</sub><sup>0</sup></td>
      <td>&gt;1070</td>
      <td>95</td>
      <td>17 SIRUNYAN</td>
      <td>20AH CMS &ell;<sup>&pm;</sup> + jet + E<sub>T</sub>, Tstop8, m<sub>t</sub><sup>&pm;</sup> - m<sub>t</sub><sup>0</sup> = 5 GeV, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
    </tr>
    <tr>
      <td>&gt; 620</td>
      <td>95</td>
      <td>8 SIRUNYAN</td>
      <td>21AD CMS jets + E<sub>T</sub>, Tstop3, 10 GeV &lt; m<sub>t</sub> - m<sub>t</sub><sup>0</sup> &lt; 60 GeV</td>
      <td>&gt;1050</td>
      <td>95</td>
      <td>17 SIRUNYAN</td>
      <td>20AH CMS &ell;<sup>&pm;</sup> + jet + E<sub>T</sub>, Tstop8, m<sub>t</sub><sup>&pm;</sup> - m<sub>t</sub><sup>0</sup> = 5 GeV, m<sub>t</sub><sup>0</sup> &lt; 350 GeV</td>
    </tr>
    <tr>
      <td>&gt; 740</td>
      <td>95</td>
      <td>8 SIRUNYAN</td>
      <td>21AD CMS jets + E<sub>T</sub>, Tstop2, m<sub>t</sub> - m<sub>t</sub><sup>0</sup></td>
      <td>= 80 GeV</td>
      <td></td>
      <td>18 SIRUNYAN</td>
      <td>20T CMS same-sign &ell;<sup>&pm;</sup>&ell;<sup>&pm;</sup> or &ge; 3&ell;<sup>&pm;</sup> + jets, Tstop7, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> = 175 GeV, m<sub>t</sub> = 200 GeV, B(t<sub>2</sub> &rarr; t<sub>1</sub> H) = 100%</td>
    </tr>
    <tr>
      <td>&gt; 720</td>
      <td>95</td>
      <td>8 SIRUNYAN</td>
      <td>21AD CMS jets + E<sub>T</sub>, Tstop2, 40 GeV &lt; m<sub>t</sub> - m<sub>t</sub><sup>0</sup> &lt; 80 GeV</td>
      <td></td>
      <td>&gt; 730</td>
      <td>95</td>
      <td>18 SIRUNYAN</td>
      <td>20T CMS same-sign &ell;<sup>&pm;</sup>&ell;<sup>&pm;</sup> or &ge; 3&ell;<sup>&pm;</sup> + jets, Tstop7, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> = 175 GeV, m<sub>t</sub> = 200 GeV, B(t<sub>2</sub> &rarr; t<sub>1</sub> Z) = 100%</td>
    </tr>
    <tr>
      <td>&gt; 595</td>
      <td>95</td>
      <td>8 SIRUNYAN</td>
      <td>21AD CMS jets + E<sub>T</sub>, Tstop2, m<sub>t</sub> - m<sub>t</sub><sup>0</sup></td>
      <td>= 10 GeV</td>
      <td></td>
      <td>18 SIRUNYAN</td>
      <td>20T CMS same-sign &ell;<sup>&pm;</sup>&ell;<sup>&pm;</sup> or &ge; 3&ell;<sup>&pm;</sup> + jets, Tstop7, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> = 175 GeV, m<sub>t</sub> = 200 GeV, B(t<sub>2</sub> &rarr; t<sub>1</sub> Z) = B(t<sub>2</sub> &rarr; t<sub>1</sub> H) = 50%</td>
    </tr>
    <tr>
      <td>&gt; 630</td>
      <td>95</td>
      <td>8 SIRUNYAN</td>
      <td>21AD CMS jets + E<sub>T</sub>, Tstop4, m<sub>t</sub> - m<sub>t</sub><sup>0</sup></td>
      <td>&gt; 890</td>
      <td>95</td>
      <td>19 SIRUNYAN</td>
      <td>20U CMS &tau;<sup>&pm;</sup>&tau;<sup>&pm;</sup> + b-jets + E<sub>T</sub>, Tstop11, m<sub>t</sub><sup>&pm;</sup> = 0.5 (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>), m<sub>t</sub> = 0.5 m<sub>t</sub><sup>&pm;</sup>, m<sub>t</sub><sup>0</sup> = 0</td>
    </tr>
    <tr>
      <td>none 200-920</td>
      <td>95</td>
      <td>9 SIRUNYAN</td>
      <td>21B CMS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> + b-jets + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td></td>
      <td>20 SIRUNYAN</td>
      <td>19AU CMS &gamma; + jets + b-jets + E<sub>T</sub>, Tstop13, m<sub>t</sub><sup>0</sup> = 1 GeV</td>
    </tr>
    <tr>
      <td>none 250-810</td>
      <td>95</td>
      <td>9 SIRUNYAN</td>
      <td>21B CMS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> + b-jets + E<sub>T</sub>, Tstop2, m<sub>t</sub><sup>0</sup> = (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>)/2, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td>&gt; 760</td>
      <td>95</td>
      <td>20 SIRUNYAN</td>
      <td>19AU CMS &gamma; + jets + b-jets + E<sub>T</sub>, Tstop13, m<sub>t</sub><sup>0</sup> = 800 GeV</td>
    </tr>
    <tr>
      <td>&gt;1300</td>
      <td>95</td>
      <td>9 SIRUNYAN</td>
      <td>21B CMS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> + b-jets + E<sub>T</sub>, Tstop11, m<sub>t</sub><sup>&pm;</sup> = (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>)/2, m<sub>t</sub><sup>0</sup> = (m<sub>t</sub><sup>&pm;</sup> + m<sub>t</sub><sup>0</sup>)/2 + m<sub>t</sub><sup>0</sup>, m<sub>t</sub><sup>0</sup> = 0</td>
      <td>&gt;1100</td>
      <td>95</td>
      <td>21 SIRUNYAN</td>
      <td>19CH CMS jets + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
    </tr>
    <tr>
      <td>none 400-1180</td>
      <td>95</td>
      <td>9 SIRUNYAN</td>
      <td>21B CMS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> + b-jets + E<sub>T</sub>, Tstop11, m<sub>t</sub><sup>&pm;</sup> = (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>)/2, m<sub>t</sub><sup>0</sup> = 0.05 (m<sub>t</sub><sup>&pm;</sup> + m<sub>t</sub><sup>0</sup>) + m<sub>t</sub><sup>0</sup>, m<sub>t</sub><sup>0</sup> = 0</td>
      <td></td>
      <td></td>
      <td>22 SIRUNYAN</td>
      <td>19S CMS 1 or 2 &ell; + jets + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> &lt; 200 GeV</td>
    </tr>
    <tr>
      <td>&gt;1400</td>
      <td>95</td>
      <td>9 SIRUNYAN</td>
      <td>21B CMS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> + b-jets + E<sub>T</sub>, Tstop11, m<sub>t</sub><sup>&pm;</sup> = (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>)/2, m<sub>t</sub><sup>0</sup> = 0.95 (m<sub>t</sub><sup>&pm;</sup> + m<sub>t</sub><sup>0</sup>) + m<sub>t</sub><sup>0</sup>, m<sub>t</sub><sup>0</sup> = 0</td>
      <td></td>
      <td>&gt;1190</td>
      <td>95</td>
      <td>24 AABOUD</td>
      <td>18AQ ATLS 1&ell; + jets + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> = 0</td>
    </tr>
    <tr>
      <td>&gt;1325</td>
      <td>95</td>
      <td>10 TUMASYAN</td>
      <td>21I CMS &ge; 2 jets + E<sub>T</sub> + 0,1,2 &ell;, Tstop1, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td>&gt; 208</td>
      <td>95</td>
      <td>23 SIRUNYAN</td>
      <td>19U CMS e<sup>&pm;</sup>&mu;<sup>&mp;</sup> + &ge; 1b-jet, Tstop1, m<sub>t</sub><sup>0</sup> - m<sub>t</sub><sup>0</sup> = 175 GeV</td>
    </tr>
    <tr>
      <td>&gt;1150</td>
      <td>95</td>
      <td>10 TUMASYAN</td>
      <td>21I CMS &ge; 2 jets + E<sub>T</sub> + 0,1,2 &ell;, Tstop1, m<sub>t</sub><sup>0</sup> = 700 GeV</td>
      <td></td>
      <td>&gt; 235</td>
      <td>95</td>
      <td>23 SIRUNYAN</td>
      <td>19U CMS e<sup>&pm;</sup>&mu;<sup>&mp;</sup> + &ge; 1b-jet, Tstop1, m<sub>t</sub><sup>0</sup> - m<sub>t</sub><sup>0</sup> = 182.5 GeV</td>
    </tr>
    <tr>
      <td>&gt;1260</td>
      <td>95</td>
      <td>10 TUMASYAN</td>
      <td>21I CMS &ge; 2 jets + E<sub>T</sub> + 0,1,2 &ell;, Tstop2, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td>&gt; 242</td>
      <td>95</td>
      <td>23 SIRUNYAN</td>
      <td>19U CMS e<sup>&pm;</sup>&mu;<sup>&mp;</sup> + &ge; 1b-jet, Tstop1, m<sub>t</sub><sup>0</sup> - m<sub>t</sub><sup>0</sup> = 167.5 GeV</td>
    </tr>
    <tr>
      <td>&gt;1000</td>
      <td>95</td>
      <td>10 TUMASYAN</td>
      <td>21I CMS &ge; 2 jets + E<sub>T</sub> + 0,1,2 &ell;, Tstop2, m<sub>t</sub><sup>0</sup> &lt; 575 GeV</td>
      <td></td>
      <td>&gt; 940</td>
      <td>95</td>
      <td>24 AABOUD</td>
      <td>18AQ ATLS 1&ell; + jets + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> = 0</td>
    </tr>
    <tr>
      <td>&gt;1175</td>
      <td>95</td>
      <td>10 TUMASYAN</td>
      <td>21I CMS &ge; 2 jets + E<sub>T</sub> + 0,1,2 &ell;, Tstop1 (50%) or Tstop2 (50%), m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td>&gt; 270</td>
      <td>95</td>
      <td>25 AABOUD</td>
      <td>18AQ ATLS 1&ell; + jets + E<sub>T</sub>, Tstop3, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> = 20 GeV</td>
    </tr>
    <tr>
      <td>&gt;1000</td>
      <td>95</td>
      <td>10 TUMASYAN</td>
      <td>21I CMS &ge; 2 jets + E<sub>T</sub> + 0,1,2 &ell;, Tstop1 (50%) or Tstop2 (50%), m<sub>t</sub><sup>0</sup> = 570 GeV</td>
      <td></td>
      <td>&gt; 840</td>
      <td>95</td>
      <td>26 AABOUD</td>
      <td>18AQ ATLS 1&ell; + jets + E<sub>T</sub>, Tstop2, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> = 10 GeV</td>
    </tr>
    <tr>
      <td>none 145-295</td>
      <td>95</td>
      <td>10 TUMASYAN</td>
      <td>21I CMS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> + jets + E<sub>T</sub>, Tstop1, |m<sub>t</sub> - m<sub>t</sub><sup>0</sup> - 175 GeV| &lt; 30 GeV</td>
      <td></td>
      <td>&gt; 500</td>
      <td>95</td>
      <td>27 AABOUD</td>
      <td>18BV ATLS c-jets + E<sub>T</sub>, Tstop4, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> &lt; 100 GeV</td>
    </tr>
    <tr>
      <td>none, 170-230</td>
      <td>95</td>
      <td>11 AABOUD</td>
      <td>20 ATLS e<sup>&pm;</sup>&mu;<sup>&mp;</sup> + &ge; 1b-jet, Tstop1, m<sub>t</sub><sup>0</sup> = 0.5 GeV</td>
      <td></td>
      <td>&gt; 850</td>
      <td>95</td>
      <td>28 AABOUD</td>
      <td>18BV ATLS c-jets + E<sub>T</sub>, Tstop4, m<sub>t</sub><sup>0</sup> = 0</td>
    </tr>
    <tr>
      <td>none, 170-220</td>
      <td>95</td>
      <td>11 AABOUD</td>
      <td>20 ATLS e<sup>&pm;</sup>&mu;<sup>&mp;</sup> + &ge; 1b-jet, Tstop1, m<sub>t</sub><sup>0</sup> &lt; 62 GeV</td>
      <td></td>
      <td>&gt; 390</td>
      <td>95</td>
      <td>29 AABOUD</td>
      <td>18I ATLS &ge; 1 jets + E<sub>T</sub>, Tstop3, m<sub>t</sub> ~ m<sub>t</sub><sup>0</sup></td>
    </tr>
    <tr>
      <td>&gt;1220</td>
      <td>95</td>
      <td>12 AAD</td>
      <td>20AS ATLS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> or 2 b-jets and E<sub>T</sub>, Tstop6, m<sub>t</sub><sup>0</sup> = 900 GeV</td>
      <td></td>
      <td>&gt; 430</td>
      <td>95</td>
      <td>30 AABOUD</td>
      <td>18I ATLS &ge; 1 jets + E<sub>T</sub>, Tstop4, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> = 5 GeV</td>
    </tr>
    <tr>
      <td>&gt; 860</td>
      <td>95</td>
      <td>13 AAD</td>
      <td>20AS ATLS &ell;<sup>&pm;</sup>&ell;<sup>&mp;</sup> or 2 b-jets and E<sub>T</sub>, t<sub>2</sub> with t<sub>2</sub> &rarr; t<sub>1</sub> Z, t<sub>1</sub> &rarr; b&ell; &ell;&#773;<sub>1</sub>, &Delta;m(t<sub>1</sub>, m<sub>t</sub><sup>0</sup>) = 40 GeV</td>
      <td></td>
      <td>&gt; 450</td>
      <td>95</td>
      <td>31 AABOUD</td>
      <td>18Y ATLS 2&ell; (&ge; 1 hadronic &tau;) + b-jets + E<sub>T</sub>, Tstop5, m<sub>t</sub> ~ 800 GeV</td>
    </tr>
    <tr>
      <td>none 400-1250</td>
      <td>95</td>
      <td>14 AAD</td>
      <td>20S ATLS jets + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td>&gt; 720</td>
      <td>95</td>
      <td>32 SIRUNYAN</td>
      <td>18AJ CMS 2&ell; (soft) + E<sub>T</sub>, Tstop10, m<sub>t</sub><sup>&pm;</sup> = (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>)/2, m<sub>t</sub> - m<sub>t</sub><sup>0</sup> = 40 GeV</td>
    </tr>
    <tr>
      <td>none 300-660</td>
      <td>95</td>
      <td>15 AAD</td>
      <td>20S ATLS jets + E<sub>T</sub>, Tstop3, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td></td>
      <td></td>
      <td>33 SIRUNYAN</td>
      <td>18AL CMS &ge; 3&ell;<sup>&pm;</sup> + jets + E<sub>T</sub>, Tstop7, m<sub>t</sub><sup>0</sup> - m<sub>t</sub><sup>0</sup> = 175 GeV, m<sub>t</sub> = 200 GeV, BR(t<sub>2</sub> &rarr; t<sub>1</sub> H) = 100%</td>
    </tr>
    <tr>
      <td>&gt; 765</td>
      <td>95</td>
      <td>16 AAD</td>
      <td>20V ATLS same-sign &ell;<sup>&pm;</sup>&ell;<sup>&pm;</sup> + jets, m<sub>t</sub> &rarr; t&#773;<sub>2</sub>, m<sub>t</sub><sup>0</sup> &rarr; m<sub>t</sub><sup>0</sup> W, m<sub>t</sub><sup>0</sup> &rarr; m<sub>t</sub><sup>0</sup> W, m<sub>t</sub><sup>0</sup> ~ m<sub>t</sub><sup>0</sup></td>
      <td></td>
      <td>&gt; 780</td>
      <td>95</td>
      <td>33 SIRUNYAN</td>
      <td>18AL CMS &ge; 3&ell;<sup>&pm;</sup> + jets + E<sub>T</sub>, Tstop7, m<sub>t</sub><sup>0</sup> - m<sub>t</sub><sup>0</sup> = 175 GeV, m<sub>t</sub> = 200 GeV, BR(t<sub>2</sub> &rarr; t<sub>1</sub> Z) = 100%</td>
    </tr>
    <tr>
      <td>&gt;1200</td>
      <td>95</td>
      <td>17 SIRUNYAN</td>
      <td>20AH CMS &ell;<sup>&pm;</sup> + jet + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup></td>
      <td>= 0 GeV</td>
      <td></td>
      <td></td>
      <td>33 SIRUNYAN</td>
      <td>18AL CMS &ge; 3&ell;<sup>&pm;</sup> + jets + E<sub>T</sub>, Tstop7, m<sub>t</sub><sup>0</sup> - m<sub>t</sub><sup>0</sup> = 175 GeV, m<sub>t</sub> = 200 GeV, BR(t<sub>2</sub> &rarr; t<sub>1</sub> Z) = BR(t<sub>2</sub> &rarr; t<sub>1</sub> H) = 50%</td>
    </tr>
    <tr>
      <td>&gt;1175</td>
      <td>95</td>
      <td>17 SIRUNYAN</td>
      <td>20AH CMS &ell;<sup>&pm;</sup> + jet + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> &lt; 425 GeV</td>
      <td></td>
      <td>&gt; 710</td>
      <td>95</td>
      <td>34 SIRUNYAN</td>
      <td>18AN CMS 1 or 2 &gamma; + &ell; + jets, GGM, Tstop12, m<sub>t</sub><sup>0</sup> = 150 GeV</td>
    </tr>
    <tr>
      <td>none 230-1140</td>
      <td>95</td>
      <td>17 SIRUNYAN</td>
      <td>20AH CMS &ell;<sup>&pm;</sup> + jet + E<sub>T</sub>, Tstop2, m<sub>t</sub><sup>&pm;</sup> = (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>)/2, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
      <td></td>
      <td>&gt; 730</td>
      <td>95</td>
      <td>34 SIRUNYAN</td>
      <td>18AN CMS 1 or 2 &gamma; + &ell; + jets, GGM, Tstop12, m<sub>t</sub><sup>0</sup> = 500 GeV</td>
    </tr>
    <tr>
      <td>&gt;1100</td>
      <td>95</td>
      <td>17 SIRUNYAN</td>
      <td>20AH CMS &ell;<sup>&pm;</sup> + jet + E<sub>T</sub>, Tstop2, m<sub>t</sub><sup>&pm;</sup> = (m<sub>t</sub> + m<sub>t</sub><sup>0</sup>)/2, 50 &lt; m<sub>t</sub><sup>0</sup> &lt; 425 GeV</td>
      <td></td>
      <td>&gt;1000</td>
      <td>95</td>
      <td>35 SIRUNYAN</td>
      <td>18AY CMS jets + E<sub>T</sub>, Tstop1, m<sub>t</sub><sup>0</sup> = 0 GeV</td>
    </tr>
    <tr>
      <td></td>
      <td></td>
      <td></td>
      <td></td>
      <td>&gt; 500</td>
      <td>95</td>
      <td>35 SIRUNYAN</td>
      <td>18AY CMS jets + E<sub>T</sub>, Tstop4, m<sub>t</sub><sup>0</sup> = 420 GeV</td>
    </tr>
  </tbody>
</table>
# Searches Particle Listings

## Supersymmetric Particle Searches

> 510 95 36 SIRUNYAN 18B CMS jets+E_T, Tstop4, m̃_t - m̃_χ₀ = > 610 95

> 800 95 37 SIRUNYAN 18C CMS ℓ±ℓ∓ + b-jets + E_T, Tstop1, m̃_χ₀ = 0 > 590 95

> 750 95 37 SIRUNYAN 18C CMS ℓ±ℓ∓ + b-jets + E_T, Tstop2, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_χ₁ = 0 none 280-640 95

>1050 95 37 SIRUNYAN 18C CMS Combination of all-hadronic, 1 ℓ± and ℓ∓ℓ∓ searches, Tstop1, m̃_χ₀ = 0 > 350 95

>1000 95 37 SIRUNYAN 18C CMS Combination of all-hadronic, 1 ℓ± and ℓ∓ℓ∓ searches, Tstop2, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_χ₁ = 0 > 280 95

>1200 95 37 SIRUNYAN 18C CMS ℓ±ℓ∓ + b-jets + E_T, Tstop11, m̃_χ₁ = 0.5 (m̃_t + m̃_χ₀), m̃_χ₁ = 0.5 m̃_χ₁, m̃_χ₀ = 0 > 240 95

>1300 95 37 SIRUNYAN 18C CMS ℓ±ℓ∓ + b-jets + E_T, Tstop11, m̃_χ₁ = 0.5 (m̃_t + m̃_χ₀), m̃_χ₁ = 0.95 m̃_χ₁, m̃_χ₀ = 0 > 225 95

>1300 95 37 SIRUNYAN 18C CMS ℓ±ℓ∓ + b-jets + E_T, Tstop11, m̃_χ₁ = 0.5 (m̃_t + m̃_χ₀), m̃_χ₁ = 0.95 m̃_χ₁, m̃_χ₀ = 0 > 325 95

none 460-1060 95 37 SIRUNYAN 18C CMS ℓ±ℓ∓ + b-jets + E_T, Tstop11, m̃_χ₁ = 0.5 (m̃_t + m̃_χ₀), m̃_χ₁ = 0.05 m̃_χ₁, m̃_χ₀ = 0 > 400 95

>1020 95 38 SIRUNYAN 18D CMS top quark (hadronically decaying) + jets + E_T, Tstop1, m̃_χ₀ = 0 GeV > 500 95

> 420 95 39 SIRUNYAN 18DI CMS ℓ± + jet + E_T, Tstop3, m̃_χ₁ = m̃_χ₀ = 10 GeV >1120 95

> 560 95 39 SIRUNYAN 18DI CMS ℓ± + jet + E_T, Tstop3, m̃_χ₁ = m̃_χ₀ = 80 GeV >1000 95

> 540 95 39 SIRUNYAN 18DI CMS ℓ±, Tstop10, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_t - m̃_χ₁ = 40 GeV > 980 95

> 590 95 39 SIRUNYAN 18DI CMS Combination of all-hadronic and 1 ℓ± searches, Tstop3, m̃_χ₁ = m̃_χ₀ = 30 GeV >1040 95

> 670 95 39 SIRUNYAN 18DI CMS Combination of all-hadronic and 1 ℓ± searches, Tstop10, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_t - m̃_χ₀ = 60 GeV > 750 95

> 450 95 40 SIRUNYAN 18DN CMS ℓ±ℓ∓, Tstop1, m̃_t - m̃_χ₀ = > 540 95

none 225-325 95 40 SIRUNYAN 18DN CMS ℓ±ℓ∓, Tstop2, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_t - m̃_χ₁ = 2 > 480 95

none 210-690 95 40 SIRUNYAN 18DN CMS ℓ±ℓ∓, Tstop1, m̃_χ₁ = 0 GeV > 530 95

none 250-600 95 40 SIRUNYAN 18DN CMS ℓ±ℓ∓, Tstop2, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_χ₁ = 0 GeV >1070 95

> 700 95 41 AABOUD 17AJ ATLS same-sign ℓ±ℓ∓ / 3 ℓ ± jets + E_T, Tstop11, m̃_χ₂ = m̃_χ₁ + 100 GeV > 900 95

> 880 95 42 AABOUD 17AX ATLS b-jets+E_T, mixture Tstop1 and Tstop2 with BR=50%, m̃_χ₁ = 0 GeV, m̃_χ₁ - m̃_χ₁ = 1 GeV >1020 95

none 250-1000 95 43 AABOUD 17AY ATLS jets+E_T, Tstop1, m̃_χ₁ = 0 GeV > 540 95

none 450-850 95 44 AABOUD 17AY ATLS jets+E_T, mixture of Tstop1 and Tstop2 with BR=50%, m̃_χ₁ = m̃_χ₀ = 1 GeV > 700 95

> 720 95 45 AABOUD 17BE ATLS ℓ±ℓ∓ + E_T, Tstop1, m̃_χ₀ = 0 GeV > 160 95

> 400 95 46 AABOUD 17BE ATLS ℓ±ℓ∓ + E_T, Tstop3, m̃_χ₁ = m̃_χ₀ = 40 GeV > 160 95

> 430 95 47 AABOUD 17BE ATLS ℓ±ℓ∓ + E_T, Tstop1 (offshell t), m̃_t - m̃_χ₀ ~ m_W none 230-960 95

> 700 95 48 AABOUD 17BE ATLS ℓ±ℓ∓ + E_T, Tstop2, m̃_t - m̃_χ₁ = 10 GeV, m̃_χ₁ = 0 GeV > 990 95

> 750 95 49 KHACHATRY...17 CMS jets+E_T, Tstop1, m̃_χ₀ = 100 GeV > 323 95

none 250-740 95 50 KHACHATRY...17AD CMS jets+b-jets+E_T, Tstop1, m̃_χ₁ = 0 GeV none, 745-780 95

51 KHACHATRY...17AD CMS jets+b-jets+E_T, mixture Tstop1 and Tstop2 with BR=50%, m̃_χ₀ = 60 GeV

52 KHACHATRY...17P CMS 1 or more jets+E_T, Tstop8, m̃_χ₁ = m̃_χ₀ = 5 GeV, m̃_χ₁ = 100 GeV

52 KHACHATRY...17P CMS 1 or more jets+E_T, Tstop1, m̃_χ₀ = 0 GeV

52 KHACHATRY...17P CMS 1 or more jets+E_T, Tstop4, 10 GeV < m̃_t - m̃_χ₀ < 80 GeV

52 KHACHATRY...17P CMS 1 or more jets+E_T, Tstop3, 10 GeV < m̃_t - m̃_χ₀ < 80 GeV

52 KHACHATRY...17P CMS 1 or more jets+E_T, Tstop9, 10 GeV < m̃_t - m̃_χ₀ < 80 GeV

53 KHACHATRY...17S CMS jets+E_T, Tstop4, m̃_t - m̃_χ₀ = 10 GeV

54 KHACHATRY...17S CMS jets+E_T, Tstop3, m̃_t - m̃_χ₀ = 10 GeV

55 KHACHATRY...17S CMS jets+E_T, Tstop2, m̃_χ₁ = 0.25 m̃_t + 0.75 m̃_χ₀, m̃_χ₀ = 225 GeV

56 KHACHATRY...17S CMS jets+E_T, Tstop2, m̃_χ₁ = 0.75 m̃_t + 0.25 m̃_χ₀, m̃_χ₀ = 0 GeV

57 KHACHATRY...17S CMS jets+E_T, Tstop1, m̃_χ₀ = 0 GeV

58 SIRUNYAN 17AS CMS 1ℓ+jets+E_T, Tstop1, m̃_χ₀ = 0 GeV

58 SIRUNYAN 17AS CMS 1ℓ+jets+E_T, Tstop2, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_χ₁ = 0 GeV

58 SIRUNYAN 17AS CMS 1ℓ+jets+E_T, Tstop8, m̃_χ₁ = m̃_χ₀ = 5 GeV, m̃_χ₀ = 0 GeV

59 SIRUNYAN 17AT CMS jets+E_T, Tstop1, m̃_χ₀ = 0 GeV

59 SIRUNYAN 17AT CMS jets+E_T, Tstop2, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_χ₁ = 0 GeV

59 SIRUNYAN 17AT CMS jets+E_T, Tstop8, m̃_χ₁ = m̃_χ₀ = 5 GeV, m̃_χ₀ = 100 GeV

59 SIRUNYAN 17AT CMS jets+E_T, Tstop3, 10 GeV < m̃_t - m̃_χ₀ < 80 GeV

59 SIRUNYAN 17AT CMS jets+E_T, Tstop4, 10 GeV < m̃_t - m̃_χ₀ < 80 GeV

59 SIRUNYAN 17AT CMS jets+E_T, Tstop10, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, 10 GeV < m̃_t - m̃_χ₀ < 80 GeV

60 SIRUNYAN 17AZ CMS ≥ 1 jets+E_T, Tstop1, m̃_χ₀ = 0 GeV

60 SIRUNYAN 17AZ CMS ≥ 1 jets+E_T, Tstop2, m̃_χ₁ = (m̃_t + m̃_χ₀)/2, m̃_χ₁ = 0 GeV

60 SIRUNYAN 17AZ CMS ≥ 1 jets+E_T, Tstop8, m̃_χ₁ = m̃_χ₀ = 5 GeV, m̃_χ₁ = 100 GeV

60 SIRUNYAN 17AZ CMS ≥ 1 jets+E_T, Tstop4, 10 GeV < m̃_t - m̃_χ₀ < 80 GeV

61 SIRUNYAN 17K CMS 0, 1 ℓ±+jets+E_T (combination), Tstop1, m̃_χ₁ = 0 GeV

61 SIRUNYAN 17K CMS 0, 1 ℓ±+jets+E_T (combination), Tstop8, m̃_χ₁ = m̃_χ₀ = 5 GeV, m̃_χ₀ = 100 GeV

61 SIRUNYAN 17K CMS jets+E_T, Tstop4, 10 < m̃_t - m̃_χ₀ < 80 GeV

62 SIRUNYAN 17P CMS jets+E_T, Tstop1, m̃_χ₁ = 0 GeV

62 SIRUNYAN 17P CMS jets+E_T, Tstop1, m̃_χ₀ = 0 GeV

63 AABOUD 16D ATLS ≥ 1 jet + E_T, Tstop4, m̃_t - m̃_χ₀ = 5 GeV

64 AABOUD 16J ATLS 1 ℓ± + ≥ 4 jets + E_T, Tstop1, m̃_χ₀ = 0 GeV
> 490-650 95 65 AAD 16AY ATLS 2ℓ (including hadronic τ) + $E_T$, Tstop5, 87 GeV < $m_\tilde{\tau}$ < $m_{\tilde{\tau}_1}$

> 700 95 66 KHACHATRY...16AV CMS 1 or 2 $\ell^\pm$+jets+b-jets+$E_T$, Tstop1, $m_{\tilde{\chi}_0^0}$ < 250 GeV

> 700 95 66 KHACHATRY...16AV CMS 1 or 2 $\ell^\pm$+jets+b-jets $E_T$, Tstop2, $m_{\tilde{\chi}_0^0}$ = 0 GeV, $m_{\tilde{\chi}_1^\pm}$ = 0.75 $m_{\tilde{\tau}_1}$ + 0.25 $m_{\tilde{\chi}_1^0}$

> 775 95 67 KHACHATRY...16BK CMS jets+$E_T$, Tstop1, $m_{\tilde{\chi}_1^0}$ < 200GeV

> 620 95 67 KHACHATRY...16BK CMS jets+$E_T$, Tstop2, $m_{\tilde{\chi}_1^0}$ = 0 GeV

> 800 95 68 KHACHATRY...16BS CMS jets+$E_T$, Tstop1, $m_{\tilde{\chi}_1^0}$ = 0 GeV

> 316 95 69 KHACHATRY...16Y CMS 1 or 2 soft $\ell^\pm$ + jets + $E_T$, Tstop3, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ = 25 GeV

> 250 95 70 AAD 15CJ ATLS $B(\tilde{t} \to c\tilde{\chi}_0^0) + B(\tilde{t} \to b f' \tilde{\chi}_1^0) = 1$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ = 10 GeV

> 270 95 70 AAD 15CJ ATLS $\tilde{t} \to c\tilde{\chi}_1^0$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ = 80 GeV

none, 200-700 95 70 AAD 15CJ ATLS $\tilde{t} \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 0

> 500 95 70 AAD 15CJ ATLS $B(\tilde{t} \to t\tilde{\chi}_0^0) + B(\tilde{t} \to b\tilde{\chi}_1^0) = 1$, $\tilde{\chi}_1^\pm \to W^(*)\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^\pm} = 2m_{\tilde{\chi}_1^0}$, $m_{\tilde{\chi}_1^0}$ < 160 GeV

> 600 95 70 AAD 15CJ ATLS $\tilde{t}_2 \to Z\tilde{\tau}_1$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ = 180 GeV, $m_{\tilde{\chi}_1^0}$ = 0

> 600 95 70 AAD 15CJ ATLS $\tilde{t}_2 \to h\tilde{\tau}_1$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ = 180 GeV, $m_{\tilde{\chi}_1^0}$ = 0

none, 172.5-191 95 71 AAD 15J ATLS $\tilde{t} \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 1 GeV

> 450 95 72 KHACHATRY...15AF CMS $\tilde{t} \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 0, $m_{\tilde{\tau}_1} > m_t + m_{\tilde{\chi}_1^0}$

> 560 95 73 KHACHATRY...15AH CMS $\tilde{t} \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 0, $m_{\tilde{\tau}_1} > m_t + m_{\tilde{\chi}_1^0}$

> 250 95 74 KHACHATRY...15AH CMS $\tilde{t} \to c\tilde{\chi}_1^0$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ < 10 GeV

> 730 95 75 KHACHATRY...15X CMS $\tilde{t} \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 100 GeV, $m_{\tilde{\tau}_1} > m_t + m_{\tilde{\chi}_1^0}$

none 400-645 95 75 KHACHATRY...15X CMS $\tilde{t} \to t\tilde{\chi}_1^0$ or $\tilde{t} \to b\tilde{\chi}_1^\pm$, $m_{\tilde{\chi}_1^0} = 100$ GeV, $m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_1^0} = 5$ GeV

none 270-645 95 76 AAD 14AJ ATLS $\geq 4$ jets + $E_T$, $\tilde{t}_1 \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ < 30 GeV

none 250-550 95 76 AAD 14AJ ATLS $\geq 4$ jets + $E_T$, $B(\tilde{t}_1 \to b\tilde{\chi}_1^\pm) = 50\%$, $m_{\tilde{\chi}_1^\pm} = 2m_{\tilde{\chi}_1^0}$, $m_{\tilde{\chi}_1^0}$ < 60 GeV

none 210-640 95 77 AAD 14BD ATLS $\ell^\pm$ + jets + $E_T$, $\tilde{t}_1 \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 0 GeV

> 500 95 77 AAD 14BD ATLS $\ell^\pm$ + jets + $E_T$, $\tilde{t}_1 \to b\tilde{\chi}_1^\pm$, $m_{\tilde{\chi}_1^\pm} = 2m_{\tilde{\chi}_1^0}$, 100 GeV < $m_{\tilde{\chi}_1^0}$ < 150 GeV

none 150-445 95 78 AAD 14F ATLS $\ell^\pm \tilde{t}^+$ final state, $\tilde{t}_1 \to b\tilde{\chi}_1^\pm$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^\pm} = 10$ GeV, $m_{\tilde{\chi}_1^0} = 1$ GeV

none 215-530 95 78 AAD 14F ATLS $\ell^\pm \tilde{t}^+$ final state, $\tilde{t}_1 \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 1 GeV

> 270 95 79 AAD 14T ATLS $\tilde{t}_1 \to c\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ = 200 GeV

> 240 95 79 AAD 14T ATLS $\tilde{t}_1 \to c\tilde{\chi}_1^0$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ < 85 GeV

> 255 95 79 AAD 14T ATLS $\tilde{t}_1 \to b f' \tilde{\chi}_1^0$, $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ ≈ $m_b$

> 400 95 80 CHATRCHYAN 14AH CMS jets + $E_T$, $\tilde{t} \to t\tilde{\chi}_1^0$ simplified model, $m_{\tilde{\chi}_1^0}$ = 50 GeV

81 CHATRCHYAN 14R CMS $\geq 3\ell^\pm$, $\tilde{t} \to (b\tilde{\chi}_1^0/t\tilde{\chi}_1^0)$, $\tilde{\chi}_1^\pm \to (qq'/\ell\nu)\tilde{\chi}_1^0$, $\tilde{\chi}_1^0 \to (H/Z)\tilde{G}$, GMSB, natural higgsino NLSP scenario

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

> 850 95 82 AABOUD 17AF ATLS $2\ell$+jets+b-jets+$E_T$, Tstop6, $m_{\tilde{\chi}_1^0}$ = 0

> 800 95 83 AABOUD 17AF ATLS $2\ell$+jets+b-jets+$E_T$, Tstop7 with 100% decays via Z, $m_{\tilde{\chi}_1^0}$ = 50 GeV

> 880 95 84 AABOUD 17AF ATLS $2\ell$+jets+b-jets+$E_T$, Tstop7 with 100% decays via higgs, $m_{\tilde{\chi}_1^0}$ = 50 GeV

> 230 95 85 AABOUD 17AY ATLS jets+$E_T$, pMSSM-inspired ROLBIECKI 15 THEO WW xsection, $\tilde{t}_1 \to bW\tilde{\chi}_1^0$, $m_{\tilde{\tau}_1} \approx m_b + m_W + m_{\tilde{\chi}_1^0}$

> 600 95 86 AAD 14B ATLS $Z+bE_T$, $\tilde{t}_2 \to Z\tilde{t}_1$, $\tilde{t}_1 \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ < 200 GeV

> 540 95 86 AAD 14B ATLS $Z+bE_T$, $\tilde{t}_1 \to t\tilde{\chi}_1^0$, $\tilde{\chi}_1^0 \to Z\tilde{G}$, natural GMSB, 100 GeV < $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ < $m_{\tilde{\tau}_1} - 10$ GeV

> 360 95 87 CHATRCHYAN 14U CMS $\tilde{t}_1 \to b\tilde{\chi}_1^\pm r$, $\tilde{\chi}_1^\pm \to f'\tilde{\chi}_1^0$, $\tilde{\chi}_1^0 \to H\tilde{G}$ simplified model, $m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_1^0}$ = 5 GeV, GMSB $\tilde{t} \to t\tilde{\chi}_1^0$, $m_{\tilde{\chi}_1^0}$ < 10 GeV

> 215 95 CZAKON 14 $\tilde{t}_2 \to H\tilde{t}_1$ or $\tilde{t}_2 \to Z\tilde{t}_1$ simplified model

1 HAYRAPETYAN 23E searched in 137 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for evidence of gluino, top squark and electroweakino pair production in events with at least one photon, multiple jets, and large $E_T$. 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 Tchi1chi1A assumes higgsino-like cross sections and includes $\tilde{\chi}_1^0 \tilde{\chi}_1^2$ and $\tilde{\chi}_{1,2}^0 \tilde{\chi}_1^2$ production. For $\tilde{\chi}_1^0 \tilde{\chi}_1^2$ alone no mass point can be excluded in the model Tchi1chi1A, but in another model for $\tilde{\chi}_1^0 \tilde{\chi}_1^2$ production, Tn1n2A.

2 TUMASYAN 23AB searched in 138 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for evidence of top squark pair production in a final state with at least one hadronically decaying tau lepton and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the mass of $\tilde{t}$ for the model Tstop16, see their Figure 9. The exclusion limits are not very sensitive to the choice of the $\tilde{t}$ mass parameter, chosen between 0.25 < $(m_{\tilde{\tau}_1^\pm} - m_{\tilde{\chi}_1^0})/(m_{\tilde{\tau}_1^0} - m_{\tilde{\chi}_1^0}) < 0.75$ because of the complementary nature of the signal diagrams.

3 TUMASYAN 23k searched in 138 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for evidence of top squark pair production in events with a high-momentum jet, an electron or muon with low transverse momentum, and significant $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the top squark mass in the simplified model Tstop3 for 10 GeV < $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0}$ < 80 GeV, see their Figure 10.

4 TUMASYAN 22q searched in up to 137 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for evidence of electroweakino and top squark pair production with a small mass difference between the two produced supersymmetric particles and the lightest neutralino in events with two or three low-momentum leptons and missing transverse momentum. 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 model Tchi1n2F, see their Figure 8. Limits are also set in a higgsino simplified model with both $\tilde{\chi}_2^0 \tilde{\chi}_1^\pm$ and $\tilde{\chi}_2^0 \tilde{\chi}_1^0$ production, where $\tilde{\chi}_2^0 \to Z\tilde{\chi}_1^0$ and $m_{\tilde{\chi}_2^0} = 1/2(m_{\tilde{\chi}_2^0} + m_{\tilde{\chi}_1^0})$. A model inspired by the pMSSM is used for further interpretations in the case of a higgsino LSP, see their Figure 9. Limits are also set on the mass of the top squark in the models Tstop2 and Tstop3, see their Figure 10.

5 AAD 21AW searched in 139 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for pair production of stops in events with one or two hadronically decaying τ leptons, jets, b-jets and $E_T$. No significant excess above the Standard Model predictions is observed. Limits are set on the $\tilde{t}_1$ mass as a function of the $\tilde{t}_1$ in the Tstop5 scenario. See their Fig. 8.

6 AAD 21O searched in 139 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for pair production of top squarks in events with one electron or muon, jets, and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the top squark mass in the Tstop1 and Tstop3 simplified models and dark matter models, see their Figures 13, 14 and 15.

7 AAD 21P searched in 139 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for pair production of top squarks in events with two opposite-sign leptons, jets, and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the top squark mass in the Tstop1, Tstop2, and Tstop3 simplified models, see their Figures 14,

8 SIRUNYAN 21AD searched in 137 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for supersymmetry in events with multiple jets, no leptons, and large $E_T$. 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 $m_{\tilde{\chi}_1^\pm} = (m_{\tilde{\tau}_1} + m_{\tilde{\chi}_1^0})/2$, and a 50:50 mixture of these with $m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_1^0}$ = 5 GeV, see their Fig. 8. Limits are also set on the top squark mass for 10 GeV < $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^\pm}$ < 80 GeV in the simplified models Tstop2, Tstop3, 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 $m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0} = 20$ GeV, and Tglu3D with $m_{\tilde{\chi}_1^\pm} - m_{\tilde{\chi}_1^0}$ = 5 GeV, see their Figure 10.

9 SIRUNYAN 21B searched in 137 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for the pair production of top squarks in events with two oppositely charged leptons (electrons or muons), jets identified as originating from a b-quark and significant $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1, Tstop2 and Tstop11 simplified models, see their Figures 6 and 7.

10 TUMASYAN 21I searched in 137 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for evidence of top squarks in events with at least two jets and large $E_T$, categorized into events with 0, 1, or 2 leptons. No significant excess above the Standard Model expectations is observed. Limits are set on the top squark mass in the simplified model Tstop1 in the top corridor $|m_{\tilde{\tau}_1} - m_{\tilde{\chi}_1^0} - 175$ GeV| < 30 GeV using dilepton events, see their Figure 7.

7. Limits are also set for a combination of earlier searches with 0, 1, and 2 leptons in
the models Tstop1, Tstop2 and a 50:50 mixture of these models, see their Fig. 9. The results are interpreted in an alternative signal model of dark matter production via a spin-0 mediator in association with a top quark pair as well.

<footnote n="11">11 AABOUD 20 searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events containing one electron-muon pair with opposite charge. The search targets a region of parameter space where the kinematics of top squark pair production and top quark pair production is very similar and makes use of the double-differential angular distributions of the leptons. No excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1 model, see Figures 16 and 17.</footnote>

<footnote n="12">12 AAD 20AS searched in 139 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for evidence of top squarks in events containing either a pair of jets consistent with SM Higgs boson decay into b-quarks or a same-flavour opposite-sign dilepton pair with an invariant mass consistent with a Z boson. No significant excess over the expected background is observed. Limits at 95% C.L. are set in Tstop6 simplified model. Assuming $m_{\tilde{\chi}_1^0} = 0$ GeV, $\tilde{t}_1$ masses up to 1220 GeV are excluded for $m_{\tilde{\chi}_2^0}$ around 900 GeV. Limits reduce down to $\tilde{t}_1$ masses up to 900 GeV for $m_{\tilde{\chi}_2^0} = 130$ GeV. See their Fig. 10. Limits are presented also in case of $B(\tilde{\chi}_2^0 \to \tilde{\chi}_1^0 h) = 0$ and 1, see their Fig. 11.</footnote>

<footnote n="13">13 AAD 20AS searched in 139 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for evidence of top squarks in events containing either a pair of jets consistent with SM Higgs boson decay into b-quarks or a same-flavour opposite-sign dilepton pair with an invariant mass consistent with a Z boson. No significant excess over the expected background is observed. Limits at 95% C.L. are set in simplified model featuring $\tilde{t}_2$ pair production, $\tilde{t}_2 \to \tilde{t}_1 Z$ and $\tilde{t}_1 \to b f' f' \tilde{\chi}_1^0$. Assuming $m_{\tilde{\chi}_1^0} = 300$ GeV, and a mass difference between $\tilde{t}_1$ and $\tilde{\chi}_1^0$ of 40 GeV, $\tilde{t}_2$ masses up to 860 GeV are excluded. See their Fig. 12.</footnote>

<footnote n="14">14 AAD 20s searched in 139 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events containing multiple jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Exclusion limits at 95% C.L. are set on top squark masses in the Tstop1 model up to 1250 GeV for lightest neutralino masses below 200 GeV. Additional constraints are set in the case where $m_{\tilde{t}} - m_{\tilde{\chi}_1^0} \sim m_t$ for which top squark masses in the range 300–630 GeV are excluded. See their Fig. 13.</footnote>

<footnote n="15">15 AAD 20s searched in 139 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events containing multiple jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Exclusion limits at 95% C.L. are set on top squark masses in the Tstop3 model in the range 300–660 GeV. In case $m_{\tilde{t}} - m_{\tilde{\chi}_1^0} \sim 5$ GeV or above, $m_{\tilde{t}}$ below 500 GeV are excluded. See their Fig. 13(b).</footnote>

<footnote n="16">16 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 top squark mass up to 765 GeV assuming $\tilde{t}_1 \to t \tilde{\chi}_2^0$ with $\tilde{\chi}_2^0 \to \tilde{\chi}_1^\pm W$ and $\tilde{\chi}_1^\pm \to \tilde{\chi}_1^0 W$. Masses of the charginos and lightest neutralinos are set as $m_W = m_{\tilde{\chi}_1^0} = m_{\tilde{t}_1} - 275$ GeV, $m_{\tilde{\chi}_2^0} = m_{\tilde{\chi}_1^0} + 100$ GeV and $m_{\tilde{\chi}_1^\pm} \sim m_{\tilde{\chi}_1^0}$. See their Fig. 8(b).</footnote>

<footnote n="17">17 SIRUNYAN 20AH searched in 137 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for pair production of top squarks in events with a single isolated electron or muon, multiple 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 Figures 6, 7 and 8, respectively.</footnote>

<footnote n="18">18 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 $\tilde{g} \to q \bar{q} q \bar{q} + e/\mu/\tau$ or via $\tilde{g} \to t b s$, see Figure 12.</footnote>

<footnote n="19">19 SIRUNYAN 20u searched in 77.2 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for the pair production of top squarks in events with two hadronically decaying taus, jets identified as originating from a b-quark and large $E_T$. No significant excess above the Standard Model expectations are observed. Limits are set on the stop mass in the Tstop11 simplified model assuming the final state leptons are taus. Different values of the scalar tau mass are considered; the impact on the lower bound is negligible.</footnote>

<footnote n="20">20 SIRUNYAN 19AU searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events with at last one photon, jets, some of which are identified as originating from b-quarks, and large $E_T$. No significant excess above the Standard Model expectations is observed. In the framework of GMSB, limits are set on the gluino mass in the Tglu1A, Tglu1C, Tglu2A and Tglu3A simplified models, and on the top squark mass in the Tstop13 simplified model, see their Figure 5.</footnote>

<footnote n="21">21 SIRUNYAN 19CH searched in 137 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events containing 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 and Tglu3A simplified models, see their Figure 13. Limits are also set on squark, bottom and stop masses in the Tsqk1, Tsbtol, Tstop1 simplified models, see their Figure 14.</footnote>

<footnote n="22">22 SIRUNYAN 19s searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events with zero or one charged leptons, jets and $E_T$. 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.</footnote>

<footnote n="23">23 SIRUNYAN 19u searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events containing one electron-muon pair with opposite charge. The search targets a region of parameter space where the kinematics of top squark pair production and top quark pair production is very similar, due to the mass difference between the top squark and the neutralino being close to the top quark mass. No excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop1 model, with $m_{\tilde{t}_1} - m_{\tilde{\chi}_1^0}$ close to $m_t$, see Figure 5.</footnote>

<footnote n="24">24 AABOUD 18AQ searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for top squark pair production in final states with one isolated electron or muon, several energetic jets, and missing transverse momentum. No significant excess over the Standard Model prediction is observed. In case of Tstop1 models, top squark masses up to 940 GeV are excluded</footnote>

<footnote>assuming $m_{\tilde{\chi}_1^0} = 0$ GeV, see their Fig. 20. If the top quark is not on-shell (3-body) decay, exclusions up to 500 GeV are obtained for $m_{\tilde{\chi}_1^0} = 300$ GeV. Exclusions as a function of $m_{\tilde{t}_1} - m_{\tilde{\chi}_1^0}$ are given in their Fig. 21.</footnote>

<footnote n="25">25 AABOUD 18AQ searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for top squark pair production in final states with one isolated electron or muon, several energetic jets, and missing transverse momentum. No significant excess over the Standard Model prediction is observed. In case of Tstop3 models (4-body), top squark masses up to 370 GeV are excluded for $m_{\tilde{t}_1} - m_{\tilde{\chi}_1^0}$ as low as 20 GeV. Top squark masses below 195 GeV are excluded for all $m_{\tilde{\chi}_1^0}$. See their Fig. 20 and Fig. 21.</footnote>

<footnote n="26">26 AABOUD 18AQ searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for top squark pair production in final states with one isolated electron or muon, several energetic jets, and missing transverse momentum. No significant excess over the Standard Model prediction is observed. In case of Tstop2 models, top squark masses up to 840 GeV are excluded for $m_{\tilde{t}_1} - m_{\tilde{\chi}_1^\pm} = 10$ GeV. See their Fig. 23. Exclusion limits for this decay mode are presented also in the context of Higgsino-LSP phenomenological MSSM models, where $m_{\tilde{t}_1} - m_{\tilde{\chi}_1^0} = 5$ GeV, see their Fig. 26.</footnote>

<footnote n="27">27 AABOUD 18BV searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events with at least one jet identified as c-jet, large missing transverse energy and no leptons. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in Tstop4 models. In scenarios with differences of the stop and neutralino masses below 100 GeV, stop masses below 500 GeV are excluded. See their Fig.6 and Fig.7.</footnote>

<footnote n="28">28 AABOUD 18BV searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events with at least one jet identified as c-jet, large missing transverse energy and no leptons. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in Tstop1 models. In scenarios with massless neutralinos, top squark masses below 850 GeV are excluded. See their Fig.6.</footnote>

<footnote n="29">29 AABOUD 18I searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events with at least one jet with a transverse momentum above 250 GeV and no leptons. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in Tstop3 models. Stop masses below 390 GeV are excluded for $m_{\tilde{t}_1} - m_{\tilde{\chi}_1^0} = m_b$. See their Fig.9(b).</footnote>

<footnote n="30">30 AABOUD 18I searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events with at least one jet with a transverse momentum above 250 GeV and no leptons. Good agreement is observed between the number of events in data and Standard Model predictions. The results are translated into exclusion limits in Tstop4 models. In scenarios with differences of the stop and neutralino masses around 5 GeV, stop masses below 430 GeV are excluded. See their Fig.9(a).</footnote>

<footnote n="31">31 AABOUD 18Y searched in 36.1 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for direct pair production of top squarks in final states with two tau leptons, b-jets, and missing transverse momentum. At least one hadronic $\tau$ is required. No significant deviation from the SM predictions is observed in the data. The analysis results are interpreted in Tstop5 models with a nearly massless gravitino. Top squark masses up to 1.16 TeV and tau slepton masses up to 1 TeV are excluded, see their Fig. 7.</footnote>

<footnote n="32">32 SIRUNYAN 18AJ searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events containing two low-momentum, oppositely charged leptons (electrons or muons) and $E_T$. No excess over the expected background is observed. Limits are derived on the tau mass in the Tchi1n2F simplified model, see their Figure 5. Limits are also set on the stop mass in the Tstop10 simplified model, see their Figure 6. Finally, limits are set on the Higgsino mass in the Tchi1n2G simplified model, see Figure 8 and in the pMSSM, see Figure 7.</footnote>

<footnote n="33">33 SIRUNYAN 18AL searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events with at least three charged leptons, in any combination of electrons and muons, jets and 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="34">34 SIRUNYAN 18AN searched in 19.7 fb⁻¹ of pp collisions at $\sqrt{s}$ = 8 TeV for events containing one or two photons and a pair of top quarks from the decay of a pair of top squark in a natural gauge-mediated scenario. The final state consists of a lepton (electron or muon), jets and one or two photons. No significant excess above the Standard Model expectations is observed. Limits are set on the stop mass in the Tstop12 simplified model, see their Figure 6.</footnote>

<footnote n="35">35 SIRUNYAN 18AY searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for events containing one or more jets and significant $E_T$. 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, bottom and stop masses in the Tsqk1, Tsbtol, 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 $< c_T < 10^5$ mm, see their Figure 4.</footnote>

<footnote n="36">36 SIRUNYAN 18B searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for the pair production of third-generation squarks in events with jets and large $E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the bottom mass in the Tsbtol1 simplified model, see their Figure 5, and on the stop mass in the Tstop4 simplified model, see their Figure 6.</footnote>

<footnote n="37">37 SIRUNYAN 18C searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for the pair production of top squarks in events with two oppositely charged leptons (electrons or muons) jets identified as originating from a b-quark 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 Tstop11 simplified models, see their Figures 11 and 12. The Tstop1 and Tstop2 results are combined with complementary searches in the all-hadronic and single lepton channels, see their Figures 13 and 14.</footnote>

<footnote n="38">38 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.</footnote>

<footnote n="39">39 SIRUNYAN 18D1 searched in 35.9 fb⁻¹ of pp collisions at $\sqrt{s}$ = 13 TeV for pair production of top squarks in events with a low transverse momentum lepton (electron or muon), a high-momentum jet and significant missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits are set on the</footnote>