Heavy ${{\widetilde{\boldsymbol g}}}$ (Gluino) mass limit

For ${\mathit m}_{{{\widetilde{\mathit g}}}}$ $>$ 60$-$70 GeV, it is expected that gluinos would undergo a cascade decay via a number of neutralinos and/or charginos rather than undergo a direct decay to photinos as assumed by some papers. Limits obtained when direct decay is assumed are usually higher than limits when cascade decays are included.
Some earlier papers are now obsolete and have been omitted. They were last listed in our PDG 2014 edition: K. Olive, $\mathit et~al.$ (Particle Data Group), Chinese Physics C38 070001 (2014) (http://pdg.lbl.gov).

R-parity conserving heavy ${{\widetilde{\boldsymbol g}}}$ (Gluino) mass limit INSPIRE search

VALUE (GeV) CL% DOCUMENT ID TECN  COMMENT
$> 1975$ 95 1
SIRUNYAN
2020B
 CMS ${}\geq{}1{{\mathit \gamma}}$ + $\not E_T$, Tglu4A, BR( ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ )=0.5, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $\simeq{}{\mathit m}_{{{\widetilde{\mathit g}}}}$
$> 2000$ 95 2
AABOUD
2019I
 ATL ${}\geq{}$2 jets + 1 or 2 ${{\mathit \tau}}$ + $\not E_T$, Tglu1F, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1860$ 95 3
SIRUNYAN
2019AG
 CMS 2${{\mathit \gamma}}$ +$\not E_T$, Tglu4B, 500 GeV $<{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$ 1500 GeV
$>1920$ 95 4
SIRUNYAN
2019AU
 CMS ${{\mathit \gamma}}$ +jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu4D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 127 GeV
$> 1950$ 95 4
SIRUNYAN
2019AU
 CMS ${{\mathit \gamma}}$ + jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu4E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$> 1800$ 95 4
SIRUNYAN
2019AU
 CMS ${{\mathit \gamma}}$ + jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu4F, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$> 2090$ 95 4
SIRUNYAN
2019AU
 CMS ${{\mathit \gamma}}$ + jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu4D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1200 GeV
$> 2120$ 95 4
SIRUNYAN
2019AU
 CMS ${{\mathit \gamma}}$ + jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu4E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1200 GeV
$> 1970$ 95 4
SIRUNYAN
2019AU
 CMS ${{\mathit \gamma}}$ + jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu4F, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1200 GeV
$> 1700$ 95 5
SIRUNYAN
2019CE
 CMS 2 jets, Stealth SUSY, Tglu1A and ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\widetilde{\mathit S}}}$ ${{\mathit \gamma}}$ ( ${{\widetilde{\mathit S}}}$ $\rightarrow$ ${{\mathit S}}{{\widetilde{\mathit G}}}$ ), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 200 GeV
$\bf{> 2000}$ 95 6
SIRUNYAN
2019CH
 CMS jets+$\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$\bf{> 2030}$ 95 6
SIRUNYAN
2019CH
 CMS jets+$\not E_T$, Tglu1C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}={\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$= 0.5(${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 2270$ 95 6
SIRUNYAN
2019CH
 CMS jets+$\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 2180$ 95 6
SIRUNYAN
2019CH
 CMS jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1750$ 95 7
SIRUNYAN
2019K
 CMS ${{\mathit \gamma}}+{{\mathit \ell}}+\not E_T$, Tglu4A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1500 GeV
$> 2000$ 95 8
SIRUNYAN
2019S
 CMS 1 or 2 ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 700 GeV
$> 1900$ 95 8
SIRUNYAN
2019S
 CMS 1 or 2 ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu3C, 150 GeV $<$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 950 GeV
$> 1970$ 95 9
AABOUD
2018AR
 ATLS jets+${}\geq{}3{{\mathit b}}$-jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 300 GeV
$> 1920$ 95 10
AABOUD
2018AR
 ATLS jets+${}\geq{}3{{\mathit b}}$-jets+$\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 600 GeV
$> 1650$ 95 11
AABOUD
2018AS
 ATLS ${}\geq{}$4 jets and disappearing tracks from ${{\widetilde{\mathit \chi}}^{\pm}}$ $\rightarrow$ ${{\widetilde{\mathit \chi}}_{{1}}^{0}}{{\mathit \pi}^{\pm}}$ , modified Tglu1A or Tglu1B, ${{\widetilde{\mathit \chi}}^{\pm}}$ lifetime 0.2 ns, ${\mathit m}_{{{\widetilde{\mathit \chi}}^{\pm}}}$ = 460 GeV
$> 1850$ 95 12
AABOUD
2018BJ
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$ + jets + $\not E_T$, Tglu1G, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1650$ 95 13
AABOUD
2018BJ
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$ + jets + $\not E_T$, Tglu1H, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 2150$ 95 14
AABOUD
2018U
 ATLS 2 ${{\mathit \gamma}}$ + $\not E_T$, GGM, Tglu4B, any NLSP mass
$> 1600$ 95 15
AABOUD
2018U
 ATLS ${{\mathit \gamma}}$ + jets + $\not E_T$, GGM higgsino-bino, mix of Tglu4B and Tglu4C, any NLSP mass
$> 2030$ 95 16
AABOUD
2018V
 ATLS jets+$\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1980$ 95 17
AABOUD
2018V
 ATLS jets+$\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}=0.5({\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1750$ 95 18
AABOUD
2018V
 ATLS jets+$\not E_T$, Tglu1C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV, any ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ $>$ 100 GeV
$> 2000$ 95 19
SIRUNYAN
2018AA
 CMS ${}\geq{}1{{\mathit \gamma}}$ + $\not E_T$, Tglu4A
$> 2100$ 95 19
SIRUNYAN
2018AA
 CMS ${}\geq{}1{{\mathit \gamma}}$ + $\not E_T$, Tglu4B
$> 1800$ 95 20
SIRUNYAN
2018AC
 CMS 1${{\mathit \ell}}$+jets, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$650 GeV
$> 1700$ 95 20
SIRUNYAN
2018AC
 CMS 1${{\mathit \ell}}$+jets, Tglu3A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$1040 GeV
$> 1900$ 95 20
SIRUNYAN
2018AC
 CMS 1${{\mathit \ell}}$ + jets, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 300 GeV
$> 1250$ 95 20
SIRUNYAN
2018AC
 CMS 1${{\mathit \ell}}$ + jets, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 950 GeV
$> 1610$ 95 21
SIRUNYAN
2018AL
 CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1160$ 95 21
SIRUNYAN
2018AL
 CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu1C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1500$ 95 22
SIRUNYAN
2018AR
 CMS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$ + jets + $\not E_T$, GMSB, Tglu4C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1770$ 95 22
SIRUNYAN
2018AR
 CMS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$ + jets + $\not E_T$, GMSB, Tglu4C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1400 GeV
$> 1625$ 95 23
SIRUNYAN
2018AY
 CMS jets+$\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1825$ 95 23
SIRUNYAN
2018AY
 CMS jets+$\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1625$ 95 23
SIRUNYAN
2018AY
 CMS jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 2040$ 95 24
SIRUNYAN
2018D
 CMS top quark (hadronically decaying) + jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1930$ 95 24
SIRUNYAN
2018D
 CMS top quark (hadronically decaying) + jets + $\not E_T$, Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 175 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 200 GeV
$> 1690$ 95 24
SIRUNYAN
2018D
 CMS top quark (hadronically decaying) + jets + $\not E_T$, Tglu3C, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 20 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1990$ 95 24
SIRUNYAN
2018D
 CMS top quark (hadronically decaying) + jets + $\not E_T$, Tglu3E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 2010$ 95 25
SIRUNYAN
2018M
 CMS ${}\geq{}$1 ${{\mathit H}}$ ( $\rightarrow$ ${{\mathit b}}{{\mathit b}}$ ) + $\not E_T$, Tglu1I
$> 1825$ 95 25
SIRUNYAN
2018M
 CMS ${}\geq{}$1 ${{\mathit H}}$ ( $\rightarrow$ ${{\mathit b}}{{\mathit b}}$ ) + $\not E_T$, Tglu1J
$>1750$ 95 26
AABOUD
2017AJ
 ATLS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ $/$ 3 ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1570$ 95 27
AABOUD
2017AJ
 ATLS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ $/$ 3 ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1860$ 95 28
AABOUD
2017AJ
 ATLS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ $/$ 3 ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1G, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 200 GeV
$>2100$ 95 29
AABOUD
2017AR
 ATLS 1${{\mathit \ell}}$+jets+$\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1740$ 95 30
AABOUD
2017AR
 ATLS 1${{\mathit \ell}}$+jets+$\not E_T$, Tglu1E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1800$ 95 31
AABOUD
2017AY
 ATLS jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 5 GeV
$>1800$ 95 32
AABOUD
2017AZ
 ATLS ${}\geq{}$7 jets+$\not E_T$, large R-jets and/or ${{\mathit b}}$-jets, Tglu1E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1540$ 95 33
AABOUD
2017AZ
 ATLS ${}\geq{}$7 jets+$\not E_T$, large R-jets and/or ${{\mathit b}}$-jets, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1340$ 95 34
AABOUD
2017N
 ATLS 2 same-flavor, opposite-sign ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1H, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1310$ 95 35
AABOUD
2017N
 ATLS 2 same-flavor, opposite-sign ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1H, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$> 1700$ 95 36
AABOUD
2017N
 ATLS 2 same-flavor, opposite-sign ${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1G, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $\sim{}$ 1 GeV
$> 1400$ 95 37
KHACHATRYAN
2017
CMS jets+$\not E_T$,Tglu1A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200GeV
$> 1650$ 95 37
KHACHATRYAN
2017
CMS jets+$\not E_T$,Tglu2A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200 GeV
$> 1600$ 95 37
KHACHATRYAN
2017
CMS jets+$\not E_T$,Tglu3A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200GeV
$> 1550$ 95 38
KHACHATRYAN
2017AD
 CMS jets+${{\mathit b}}$-jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1450$ 95 39
KHACHATRYAN
2017AD
 CMS jets+${{\mathit b}}$-jets+$\not E_T$, Tglu3C, 200 $<$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$>1570$ 95 40
KHACHATRYAN
2017AS
 CMS 1${{\mathit \ell}}$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 600 GeV
$>1500$ 95 40
KHACHATRYAN
2017AS
 CMS 1${{\mathit \ell}}$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 775 GeV
$>1400$ 95 40
KHACHATRYAN
2017AS
 CMS 1${{\mathit \ell}}$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 725 GeV
$\text{none 1050 - 1350}$ 95 40
KHACHATRYAN
2017AS
 CMS 1${{\mathit \ell}}$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 850 GeV
$> 1175$ 95 41
KHACHATRYAN
2017AW
 CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$, 2 jets, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 825$ 95 41
KHACHATRYAN
2017AW
 CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$, 2 jets, Tglu1C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1350$ 95 42
KHACHATRYAN
2017P
 CMS 1 or more jets+$\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1545$ 95 42
KHACHATRYAN
2017P
 CMS 1 or more jets+$\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1120$ 95 42
KHACHATRYAN
2017P
 CMS 1 or more jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1300$ 95 42
KHACHATRYAN
2017P
 CMS 1 or more jets+$\not E_T$, Tglu3D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>780$ 95 42
KHACHATRYAN
2017P
 CMS 1 or more jets+$\not E_T$, Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 175 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$>790$ 95 42
KHACHATRYAN
2017P
 CMS 1 or more jets+$\not E_T$, Tglu3C, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 20 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1650$ 95 43
KHACHATRYAN
2017V
 CMS 2 ${{\mathit \gamma}}$ + $\not E_T$, GGM, Tglu4B, any NLSP mass
$> 1900$ 95 44
SIRUNYAN
2017AF
 CMS 1${{\mathit \ell}}$+jets+${{\mathit b}}$-jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1600$ 95 44
SIRUNYAN
2017AF
 CMS 1${{\mathit \ell}}$+jets+${{\mathit b}}$-jets+$\not E_T$, Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 175 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1800$ 95 45
SIRUNYAN
2017AY
 CMS ${{\mathit \gamma}}$ + jets+$\not E_T$, Tglu4B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1600$ 95 45
SIRUNYAN
2017AY
 CMS ${{\mathit \gamma}}$ + jets+$\not E_T$, Tglu4A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1860$ 95 46
SIRUNYAN
2017AZ
 CMS ${}\geq{}$1 jets + $\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 2025$ 95 46
SIRUNYAN
2017AZ
 CMS ${}\geq{}$1 jets+$\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1900$ 95 46
SIRUNYAN
2017AZ
 CMS ${}\geq{}$1 jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1825$ 95 47
SIRUNYAN
2017P
 CMS jets+$\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1950$ 95 47
SIRUNYAN
2017P
 CMS jets+$\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1960$ 95 47
SIRUNYAN
2017P
 CMS jets+$\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1800$ 95 47
SIRUNYAN
2017P
 CMS jets+$\not E_T$, Tglu1C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1870$ 95 47
SIRUNYAN
2017P
 CMS jets+$\not E_T$, Tglu3D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1000 GeV
$> 1520$ 95 48
SIRUNYAN
2017S
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1200$ 95 48
SIRUNYAN
2017S
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu3D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1370$ 95 48
SIRUNYAN
2017S
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 175 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1180$ 95 48
SIRUNYAN
2017S
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu3C, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 20 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1280$ 95 48
SIRUNYAN
2017S
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1300$ 95 48
SIRUNYAN
2017S
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ + jets + $\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 20 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1570$ 95 49
AABOUD
2016AC
 ATLS ${}\geq{}$2 jets + 1 or 2 ${{\mathit \tau}}$ + $\not E_T$, Tglu1F, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1460$ 95 50
AABOUD
2016J
 ATLS 1 ${{\mathit \ell}^{\pm}}$ + ${}\geq{}$4 jets + $\not E_T$, Tglu3C, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 5 GeV
$> 1650$ 95 51
AABOUD
2016M
 ATLS 2 ${{\mathit \gamma}}$ + $\not E_T$, Tglu1D, any NLSP mass
$> 1510$ 95 52
AABOUD
2016N
 ATLS ${}\geq{}$4 jets + $\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1500$ 95 53
AABOUD
2016N
 ATLS ${}\geq{}$4 jets + $\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=200GeV
$> 1780$ 95 54
AAD
2016AD
 ATLS 0${{\mathit \ell}}$, ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 800 GeV
$> 1760$ 95 55
AAD
2016AD
 ATLS 1${{\mathit \ell}}$, ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 700 GeV
$> 1300$ 95 56
AAD
2016BB
 ATLS 2 same-sign/3${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$ 600 GeV
$> 1100$ 95 56
AAD
2016BB
 ATLS 2 same-sign/3${{\mathit \ell}}$ + jets + $\not E_T$, Tglu1E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$ 300 GeV
$> 1200$ 95 56
AAD
2016BB
 ATLS 2 same-sign /3${{\mathit \ell}}$ + jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 600 GeV
$> 1600$ 57
AAD
2016BG
 ATLS 1${{\mathit \ell}}$, ${}\geq{}$4 jets, $\not E_T$, Tglu1B, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$= (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$= 100 GeV
$>1400$ 95 58
AAD
2016V
 ATLS ${}\geq{}$7 to ${}\geq{}$10 jets + $\not E_T$, Tglu1E, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 200 GeV
$>1400$ 95 58
AAD
2016V
 ATLS ${}\geq{}$7 to ${}\geq{}$10 jets + $\not E_T$, pMSSM ${{\mathit M}_{{1}}}$ = 60 GeV, ${{\mathit M}_{{2}}}$ = 3 TeV, tan${{\mathit \beta}}$=10, ${{\mathit \mu}}$ $<$ 0
$> 1100$ 95 59
KHACHATRYAN
2016AM
 CMS boosted ${{\mathit W}}+{{\mathit b}}$, Tglu3C, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$80GeV,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$400GeV
$>700$ 95 59
KHACHATRYAN
2016AM
 CMS boosted ${{\mathit W}}+{{\mathit b}}$, Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=175 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=0 GeV
$>1050$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 800 GeV
$>1300$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ ,Tglu3A,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=0
$>1140$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 20 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>850$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=20 GeV,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$700 GeV
$>950$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3D, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV
$>1100$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ ,Tglu1B,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$= 0.5(${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}),{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$400GeV
$> 830$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ ,Tglu1B,${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$= 0.5(${\mathit m}_{{{\widetilde{\mathit g}}}}+{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}),{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}<$700GeV
$>1300$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = ${\mathit m}_{{{\mathit t}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1050$ 95 60
KHACHATRYAN
2016BJ
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu3B, ${\mathit m}_{{{\widetilde{\mathit t}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = ${\mathit m}_{{{\mathit t}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 800 GeV
$>1725$ 95 61
KHACHATRYAN
2016BS
 CMS jets + $\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1750$ 95 61
KHACHATRYAN
2016BS
 CMS jets + $\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1550$ 95 61
KHACHATRYAN
2016BS
 CMS jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$> 1280$ 95 62
KHACHATRYAN
2016BY
 CMS opposite-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu4C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1000 GeV
$> 1030$ 95 62
KHACHATRYAN
2016BY
 CMS opposite-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , Tglu4C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$>1440$ 95 63
KHACHATRYAN
2016V
 CMS jets + $\not E_T$, Tglu1A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1600$ 95 63
KHACHATRYAN
2016V
 CMS jets + $\not E_T$, Tglu2A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1550$ 95 63
KHACHATRYAN
2016V
 CMS jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1450$ 95 63
KHACHATRYAN
2016V
 CMS jets + $\not E_T$, Tglu1C, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>820$ 95 64
AAD
2015BG
 ATLS GGM, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\widetilde{\mathit q}}}{{\mathit Z}}{{\widetilde{\mathit G}}}$ , tan ${{\mathit \beta}}$ = 30, ${{\mathit \mu}}$ $>$ 600 GeV
$>850$ 95 64
AAD
2015BG
 ATLS GGM, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\widetilde{\mathit q}}}{{\mathit Z}}{{\widetilde{\mathit G}}}$ , tan ${{\mathit \beta}}$ = 1.5, ${{\mathit \mu}}$ $>$ 450 GeV
$>1150$ 95 65
AAD
2015BV
 ATLS general RPC ${{\widetilde{\mathit g}}}$ decays, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$>700$ 95 66
AAD
2015BX
 ATLS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit X}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , independent of ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$
$>1290$ 95 67
AAD
2015CA
 ATLS ${}\geq{}$2 ${{\mathit \gamma}}$ + $\not E_T$, GGM, bino-like NLSP, any NLSP mass
$>1260$ 95 67
AAD
2015CA
 ATLS ${}\geq{}$1 ${{\mathit \gamma}}$ + ${{\mathit b}}$-jets + $\not E_T$, GGM, higgsino-bino admix. NLSP and ${{\mathit \mu}}<$0, m(NLSP)$>$450 GeV
$>1140$ 95 67
AAD
2015CA
 ATLS ${}\geq{}$1 ${{\mathit \gamma}}$ + jets + $\not E_T$, GGM, higgsino-bino admixture NLSP, all ${{\mathit \mu}}>$0
$> 1225$ 95 68
KHACHATRYAN
2015AF
 CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$> 1300$ 95 68
KHACHATRYAN
2015AF
 CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$> 1225$ 95 68
KHACHATRYAN
2015AF
 CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1550$ 95 68
KHACHATRYAN
2015AF
 CMS CMSSM, tan ${{\mathit \beta}}$=30, ${\mathit m}_{{{\widetilde{\mathit g}}}}={\mathit m}_{{{\widetilde{\mathit q}}}}$, $\mathit A_{0}=−$2max(${\mathit m}_{\mathrm {0}},{\mathit m}_{\mathrm {1/2}}$), $\mu >$0
$>1150$ 95 68
KHACHATRYAN
2015AF
 CMS CMSSM, tan ${{\mathit \beta}}$=30, $\mathit A_{0}=−$2max(${\mathit m}_{\mathrm {0}},{\mathit m}_{\mathrm {1/2}}$), $\mu >$0
$>1280$ 95 69
KHACHATRYAN
2015I
 CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0
$>1310$ 95 70
KHACHATRYAN
2015X
 CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1175$ 95 70
KHACHATRYAN
2015X
 CMS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$> 1330$ 95 71
AAD
2014AE
 ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 1700$ 95 71
AAD
2014AE
 ATLS jets + $\not E_T$, mSUGRA/CMSSM, ${\mathit m}_{{{\widetilde{\mathit q}}}}$ = ${\mathit m}_{{{\widetilde{\mathit g}}}}$
$> 1090$ 95 72
AAD
2014AG
 ATLS ${{\mathit \tau}}$ + jets + $\not E_T$, natural Gauge Mediation
$> 1600$ 95 72
AAD
2014AG
 ATLS ${{\mathit \tau}}$ + jets + $\not E_T$, mGMSB, M$_{mess}$ = 250 GeV, ${{\mathit N}_{{5}}}$ = 3, ${{\mathit \mu}}$ $>$ 0, ${{\mathit C}}_{grav}$ = 1
$> 640$ 95 73
AAD
2014X
 ATLS ${}\geq{}4{{\mathit \ell}^{\pm}}$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ , tan $\beta $ = 30, GGM
$> 1000$ 95 74
CHATRCHYAN
2014AH
 CMS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1350$ 95 74
CHATRCHYAN
2014AH
 CMS jets + $\not E_T$, CMSSM, ${\mathit m}_{{{\widetilde{\mathit g}}}}$ = ${\mathit m}_{{{\widetilde{\mathit q}}}}$
$> 1000$ 95 75
CHATRCHYAN
2014AH
 CMS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1000$ 95 76
CHATRCHYAN
2014AH
 CMS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
$> 1160$ 95 77
CHATRCHYAN
2014I
 CMS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$> 1130$ 95 77
CHATRCHYAN
2014I
 CMS multijets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$> 1210$ 95 77
CHATRCHYAN
2014I
 CMS multijets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 100 GeV
$> 1260$ 95 78
CHATRCHYAN
2014N
 CMS 1${{\mathit \ell}^{\pm}}$+ jets +${}\geq{}2{{\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\mathit \chi}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\mathit \chi}_{{1}}^{0}}}$=0 GeV, ${\mathit m}_{{{\widetilde{\mathit t}}}}>$ ${\mathit m}_{{{\widetilde{\mathit g}}}}$
79
CHATRCHYAN
2014R
 CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$, ${{\widetilde{\mathit g}}}$ $/$ ${{\widetilde{\mathit q}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ simplified model, GMSB, slepton co-NLSP scenario
80
CHATRCHYAN
2014R
 CMS ${}\geq{}3{{\mathit \ell}^{\pm}}$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model
• • • We do not use the following data for averages, fits, limits, etc. • • •
$> 1500$ 95 81
AABOUD
2018BJ
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$ + jets + $\not E_T$, Tglu1H, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV, any ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$
$> 1770$ 95 82
AABOUD
2018V
 ATLS jets+$\not E_T$, Tglu1C-like, 1/2 BR per decay mode, any ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV
$>1600$ 95 83
AABOUD
2017AZ
 ATLS ${}\geq{}$7 jets+$\not E_T$, large R-jets and/or ${{\mathit b}}$-jets, pMSSM, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 200 GeV
$>1600$ 95 84
KHACHATRYAN
2016AY
 CMS 1${{\mathit \ell}^{\pm}}$ + jets + ${{\mathit b}}$-jets + $\not E_T$, Tglu3A, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV
$> 500$ 95 85
KHACHATRYAN
2016BT
 CMS 19-parameter pMSSM model, global Bayesian analysis, flat prior
95 86
AAD
2015AB
 ATLS ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit S}}}{{\mathit g}}$ , c${{\mathit \tau}}$ = 1 m, ${{\widetilde{\mathit S}}}$ $\rightarrow$ ${{\mathit S}}{{\widetilde{\mathit G}}}$ and ${{\mathit S}}$ $\rightarrow$ ${{\mathit g}}{{\mathit g}}$ , BR = 100$\%$
95 87
AAD
2015AI
 ATLS ${{\mathit \ell}^{\pm}}$ + jets + $\not E_T$
$>1600$ 95 65
AAD
2015BV
 ATLS pMSSM, M$_{1}$ = 60 GeV, ${\mathit m}_{{{\widetilde{\mathit q}}}}$ $<$ 1500 GeV
$>1280$ 95 65
AAD
2015BV
 ATLS mSUGRA, ${\mathit m}_{\mathrm {0}}$ $>$ 2 TeV
$>1100$ 95 65
AAD
2015BV
 ATLS via ${{\widetilde{\mathit \tau}}}$, natural GMSB, all ${\mathit m}_{{{\widetilde{\mathit \tau}}}}$
$>1330$ 95 65
AAD
2015BV
 ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$>1500$ 95 65
AAD
2015BV
 ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit q}}}{{\mathit q}}$ , ${{\widetilde{\mathit q}}}$ $\rightarrow$ ${{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$>1650$ 95 65
AAD
2015BV
 ATLS jets + $\not E_T$, ${\mathit m}_{{{\widetilde{\mathit g}}}}$ = ${\mathit m}_{{{\widetilde{\mathit q}}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV
$>850$ 95 65
AAD
2015BV
 ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit g}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 550 GeV
$>1270$ 95 65
AAD
2015BV
 ATLS jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1150$ 95 65
AAD
2015BV
 ATLS jets + ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}{{\mathit Z}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1320$ 95 65
AAD
2015BV
 ATLS jets + ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ decays via sleptons, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1220$ 95 65
AAD
2015BV
 ATLS ${{\mathit \tau}}$, ${{\widetilde{\mathit q}}}$ decays via staus, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV
$>1310$ 95 65
AAD
2015BV
 ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$>1220$ 95 65
AAD
2015BV
 ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}$ and ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\mathit T}_{{1}}}}$ $<$ 1000 GeV
$>1180$ 95 65
AAD
2015BV
 ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}$ and ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${\mathit m}_{{{\mathit T}_{{1}}}}$ $<$ 1000 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV
$>1260$ 95 65
AAD
2015BV
 ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}$ and ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit c}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$
$>1200$ 95 65
AAD
2015BV
 ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit b}}_{{1}}}{{\mathit b}}$ and ${{\widetilde{\mathit b}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit b}}_{{1}}}}$ $<$ 1000 GeV
$>1250$ 95 65
AAD
2015BV
 ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$\text{none, 750 - 1250}$ 95 65
AAD
2015BV
 ATLS ${\mathit {\mathit b}}$-jets, ${{\widetilde{\mathit g}}}$ decay via offshell ${{\widetilde{\mathit t}}_{{1}}}$ and ${{\widetilde{\mathit b}}_{{1}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 500 GeV
$>1100$ 95 88
AAD
2015CB
 ATLS jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit Z}}{{\widetilde{\mathit G}}}$ , GGM, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 400 GeV and 3 $<$ c$\tau _{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 500 mm
$>1400$ 95 88
AAD
2015CB
 ATLS jets or $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , Split SUSY, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV and 15 $<$ c$\tau $ $<$ 300 mm
$>1500$ 95 88
AAD
2015CB
 ATLS $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , Split SUSY, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV and 20 $<$ c$\tau $ $<$ 250 mm
89
KHACHATRYAN
2015AD
 CMS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$ + jets + $\not E_T$, GMSB, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit Z}}{{\widetilde{\mathit G}}}$
$>1300$ 95 90
KHACHATRYAN
2015AZ
 CMS ${}\geq{}$2 ${{\mathit \gamma}}$, ${}\geq{}$1 jet, (Razor), bino-like NLSP, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 375 GeV
$>800$ 95 90
KHACHATRYAN
2015AZ
 CMS ${}\geq{}$1 ${{\mathit \gamma}}$, ${}\geq{}$2 jet, wino-like NLSP, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 375 GeV
$> 1280$ 95 91
AAD
2014AX
 ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, CMSSM
$> 1250$ 95 91
AAD
2014AX
 ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit b}}_{{1}}}{{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${{\widetilde{\mathit b}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV, ${\mathit m}_{{{\widetilde{\mathit b}}_{{1}}}}$ $<$ 900 GeV
$> 1190$ 95 91
AAD
2014AX
 ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $<$ 1000 GeV
$> 1180$ 95 91
AAD
2014AX
 ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}_{{1}}}{{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}=2{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=60 GeV, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}<$1000 GeV
$> 1250$ 95 91
AAD
2014AX
 ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$> 1340$ 95 91
AAD
2014AX
 ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$> 1300$ 95 91
AAD
2014AX
 ATLS ${}\geq{}$3 ${{\mathit b}}$-jets + $\not E_T$, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ simplified model, ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit f}}{{\mathit f}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 2 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 300 GeV
$> 950$ 95 92
AAD
2014E
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model
$> 1000$ 95 92
AAD
2014E
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit t}}_{{1}}}$ with ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $<$ 200 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 118 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV
$> 640$ 95 92
AAD
2014E
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit t}}_{{1}}}$ with ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit c}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 20 GeV
$> 860$ 95 92
AAD
2014E
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{(*)\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 2 ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV
$> 1040$ 95 92
AAD
2014E
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{(*)\pm}}{{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit Z}^{(*)}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 520 GeV
$> 1200$ 95 92
AAD
2014E
 ATLS ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$( ${{\mathit \ell}^{\mp}}$) + jets, ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $/$ ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \nu}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$( ${{\mathit \nu}}{{\mathit \nu}}$) ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model
$> 1050$ 95 93
CHATRCHYAN
2014H
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, massless ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$
$> 900$ 95 94
CHATRCHYAN
2014H
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 0.5 ${\mathit m}_{{{\widetilde{\mathit g}}}}$, massless ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$
$> 1050$ 95 95
CHATRCHYAN
2014H
 CMS same-sign ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\pm}}$ , ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 300 GeV, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 50 GeV
1  SIRUNYAN 2020B searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least one photon and large $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on chargino masses in a general gauge-mediated SUSY breaking (GGM) scenario Tchi1n12-GGM, see Figure 4. Limits are also set on the NLSP mass in the Tchi1chi1F and Tchi1chi1G simplified models, see their Figure 5. Finally, limits are set on the gluino mass in the Tglu4A simplified model, see Figure 6.
2  AABOUD 2019I searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with hadronic jets, 1 or two hadronically decaying ${{\mathit \tau}}$ and $\not E_T$. In Tglu1F, gluino masses are excluded at 95$\%$ C.L. up to 2000 GeV for neutralino masses of 100 GeV or below. Neutralino masses up to 1000 GeV are excluded for all gluino masses below 1400 GeV. See their Fig. 9. Limits are also presented in the context of Gauge-Mediated Symmetry Breaking models: in this case, values of ${{\mathit \Lambda}}$ below 110 TeV are excluded at the 95$\%$ CL for all values of tan${{\mathit \beta}}$ in the range 2 $<$ tan${{\mathit \beta}}$ $<$ 60, see their Fig 10.
3  SIRUNYAN 2019AG searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two photons and large $\not E_T$. 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.
4  SIRUNYAN 2019AU searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at last one photon, jets, some of which are identified as originating from ${{\mathit b}}$-quarks, and large $\not E_T$. No significant excess above the Standard Model expectations is observed. In the framework of GMSB, limits are set on the gluino mass in the Tglu4C, Tglu4D and Tglu4E simplified models, and on the top squark mass in the Tstop13 simplified model, see their Figure 5.
5  SIRUNYAN 2019CE searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for new particles decaying to a photon and two gluons in events with at least three large-radius jets of which two have substructure and are composed of a photon and two gluons. No statistically significant excess is observed above the SM background expectation. Upper limits at 95$\%$ confidence level on the cross section for gluino pair production are set, using a simplified Tglu1A-like stealth SUSY model. Gluino masses up to 1500-1700 GeV are excluded, depending on the neutralino mass, with the highest exclusion set for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 200 GeV. See their Fig 4.
6  SIRUNYAN 2019CH searched in 137 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing multiple jets and large $\not E_T$. 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, sbottom and stop masses in the Tsqk1, Tsbot1, Tstop1 simplified models, see their Figure 14.
7  SIRUNYAN 2019K searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with a photon, an electron or muon, and large $\not E_T$. 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 Tchi1n1A simplified model, see their Figure 6. Limits are also set on the gluino mass in the Tglu4A simplified model, and on the squark mass in the Tsqk4A simplified model, see their Figure 7.
8  SIRUNYAN 2019S searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with zero or one charged leptons, jets and $\not E_T$. The razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) 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.
9  AABOUD 2018AR searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for gluino pair production in events containing large missing transverse momentum and several energetic jets, at least three of which must be identified as originating from ${{\mathit b}}$-quarks. No excess is found above the predicted background. In Tglu3A models, gluino masses of less than 1.97 TeV are excluded for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ below 300 GeV, see their Fig. 10(a). Interpretations are also provided for scenarios where Tglu3A modes mix with Tglu2A and Tglu3D, see their Fig 11.
10  AABOUD 2018AR searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for gluino pair production in events containing large missing transverse momentum and several energetic jets, at least three of which must be identified as originating from ${{\mathit b}}$-quarks. No excess is found above the predicted background. In Tglu2A models, gluino masses of less than 1.92 TeV are excluded for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ below 600 GeV, see their Fig. 10(b). Interpretations are also provided for scenarios where Tglu2A modes mix with Tglu3A and Tglu3D, see their Fig 11.
11  AABOUD 2018AS searched for in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for gluino pair production in the context of AMSB or phenomenological MSSM scenarios with wino-like LSP and long-lived charginos. Events with a disappearing track due to a low-momentum pion accompanied by at least four jets are considered. No significant excess above the Standard Model expectations is observed. Exclusion limits are set at 95$\%$ confidence level on the mass of gluinos for different chargino lifetimes. Gluino masses up to 1.65 TeV are excluded assuming a chargino mass of 460 GeV and lifetime of 0.2 ns, corresponding to a mass-splitting between the charged and neutral wino of around 160 MeV. See their Fig. 9.
12  AABOUD 2018BJ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in events with two opposite-sign charged leptons (electrons and muons), jets and missing transverse momentum, with various requirements to be sensitive to signals with different kinematic endpoint values in the dilepton invariant mass distribution. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1G model: gluino masses below 1850 GeV are excluded for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV, see their Fig. 12(a).
13  AABOUD 2018BJ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in events with two opposite-sign charged leptons (electrons and muons), jets and missing transverse momentum, with various requirements to be sensitive to signals with different kinematic endpoint values in the dilepton invariant mass distribution. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1H model: gluino masses below 1650 GeV are excluded for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV, see their Fig. 13(a).
14  AABOUD 2018U searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in events with at least one isolated photon, possibly jets and significant transverse momentum targeting generalised models of gauge-mediated SUSY breaking. No significant excess of events is observed above the SM prediction. Results for the di-photon channel are interpreted in terms of lower limits on the masses of gluinos in Tglu4B models, which reach as high as 2.3 TeV. Gluinos with masses below 2.15 TeV are excluded for any NLSP mass, see their Fig. 8.
15  AABOUD 2018U searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in events with at least one isolated photon, possibly jets and significant transverse momentum targeting generalised models of gauge-mediated SUSY breaking. No significant excess of events is observed above the SM prediction. Results of the ${{\mathit \gamma}}$ + jets + $\not E_T$ channel are interpreted in terms of lower limits on the masses of gluinos in GGM higgsino-bino models (mix of Tglu4B and Tglu4C), which reach as high as 2050 GeV. Gluino masses below 1600 GeV are excluded for any NLSP mass provided that ${\mathit m}_{{{\widetilde{\mathit g}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}>$ 50 GeV. See their Fig. 11.
16  AABOUD 2018V searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 Tglu1A model: gluino masses below 2030 GeV are excluded for massless LSP, see their Fig. 13(b).
17  AABOUD 2018V searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 Tglu1B model. Assuming that ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 0.5 (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$), gluino masses below 1980 GeV are excluded for massless LSP, see their Fig. 14(c). Exclusions are also shown assuming ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV, see their Fig. 14(d).
18  AABOUD 2018V searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 Tglu1E model: gluino masses below 1750 GeV are excluded for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV and any ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ above 100 GeV, see their Fig. 15. Gluino mass exclusion up to 2 TeV is found for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = 1 TeV.
19  SIRUNYAN 2018AA searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least one photon and large $\not E_T$. 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 ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ and wino-like ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ and ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , see Figure 7. Limits are also set on the NLSP mass in the Tchi1n1A and Tchi1chi1A 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 Tskq4A and Tsqk4B simplified models, see their Figure 10.
20  SIRUNYAN 2018AC searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with a single electron or muon and multiple jets. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu1B simplified models, see their Figure 5.
21  SIRUNYAN 2018AL searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least three charged leptons, in any combination of electrons and muons, jets and significant $\not E_T$. 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 sbottom mass in the Tsbot2 simplified model, see their Figure 6, and on the stop mass in the Tstop7 simplified model, see their Figure 7.
22  SIRUNYAN 2018AR searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing two opposite-charge, same-flavour leptons (electrons or muons), jets and $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu4C simplified model, see their Figure 7. Limits are also set on the chargino/neutralino mass in the Tchi1n2F simplified models, see their Figure 8, and on the higgsino mass in the Tn1n1B and Tn1n1C simplified models, see their Figure 9. Finally, limits are set on the sbottom mass in the Tsbot3 simplified model, see their Figure 10.
23  SIRUNYAN 2018AY searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing one or more jets and significant $\not E_T$. 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, sbottom 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${{\mathit \tau}}$ $<$ $10^{5}$ mm, see their Figure 4.
24  SIRUNYAN 2018D searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing identified hadronically decaying top quarks, no leptons, and $\not E_T$. 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.
25  SIRUNYAN 2018M searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with one or more high-momentum Higgs bosons, decaying to pairs of ${{\mathit b}}$-quarks, and large $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1I and Tglu1J simplified models, see their Figure 3.
26  AABOUD 2017AJ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.75 TeV are set on the gluino mass in Tglu3A simplified models in case of off-shell top squarks and for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV. See their Figure 4(a).
27  AABOUD 2017AJ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.57 TeV are set on the gluino mass in Tglu1E simplified models (2-step models) for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 100 GeV. See their Figure 4(b).
28  AABOUD 2017AJ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two same-sign or three leptons, jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.86 TeV are set on the gluino mass in Tglu1G simplified models for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 200 GeV. See their Figure 4(c).
29  AABOUD 2017AR searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with one isolated lepton, at least two jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 2.1 TeV are set on the gluino mass in Tglu1B simplified models, with $\mathit x$ = (${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$) $/$ (${\mathit m}_{{{\widetilde{\mathit g}}}}−{\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$) = 1/2.Similar limits are obtained for variable $\mathit x$ and fixed neutralino mass, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV. See their Figure 13.
30  AABOUD 2017AR searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with one isolated lepton, at least two jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.74 TeV are set on the gluino mass in Tglu1E simplified model. Limits up to 1.7 TeV are also set on pMSSM models leading to similar signal event topologies. See their Figure 13.
31  AABOUD 2017AY searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least four jets and large missing transverse momentum. No significant excess above the Standard Model expectations is observed. Limits up to 1.8 TeV are set on the gluino mass in Tglu3A simplified models assuming ${\mathit m}_{{{\widetilde{\mathit t}}_{{1}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 5 GeV. See their Figure 13.
32  AABOUD 2017AZ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least seven jets and large missing transverse momentum. Selected events are further classified based on the presence of large R-jets or ${{\mathit b}}$-jets and no leptons. No significant excess above the Standard Model expectations is observed. Limits up to 1.8 TeV are set on the gluino mass in Tglu1E simplified models. See their Figure 6b.
33  AABOUD 2017AZ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least seven jets and large missing transverse momentum. Selected events are further classified based on the presence of large R-jets or ${{\mathit b}}$-jets and no leptons. No significant excess above the Standard Model expectations is observed. Limits up to 1.54 TeV are set on the gluino mass in Tglu3A simplified models. See their Figure 7a.
34  AABOUD 2017N searched in 14.7 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with 2 same-flavor, opposite-sign leptons (electrons or muons), jets and large missing transverse momentum. In Tglu1J models, gluino masses are excluded at 95$\%$ C.L. up to 1300 GeV for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 0 GeV and ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = 1100 GeV. See their Fig. 12 for exclusion limits as a function of ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$. Limits are also presented assuming ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 100 GeV, see their Fig. 13.
35  AABOUD 2017N searched in 14.7 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with 2 same-flavor, opposite-sign leptons (electrons or muons), jets and large missing transverse momentum. In Tglu1H models, gluino masses are excluded at 95$\%$ C.L. up to 1310 GeV for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 400 GeV and assuming ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2. See their Fig. 15.
36  AABOUD 2017N searched in 14.7 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with 2 same-flavor, opposite-sign leptons (electrons or muons), jets and large missing transverse momentum. In Tglu1G models, gluino masses are excluded at 95$\%$ C.L. up to 1700 GeV for small ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$. The results probe kinematic endpoints as small as ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = (${\mathit m}_{{{\widetilde{\mathit g}}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2 = 50 GeV. See their Fig. 14.
37  KHACHATRYAN 2017 searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing four or more jets, no more than one lepton, and missing transverse momentum, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. No evidence for an excess over the expected background is observed. Limits are derived on the gluino mass in the Tglu1A, Tglu2A and Tglu3A simplified models, see Figs. 16 and 17. Also, assuming gluinos decay only via three-body processes involving third-generation quarks plus a neutralino/chargino, and assuming ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + 5 GeV, a branching ratio-independent limit on the gluino mass is given, see Fig. 16.
38  KHACHATRYAN 2017AD searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing at least four jets (including ${{\mathit b}}$-jets), missing transverse momentum and tagged top quarks. No evidence for an excess over the expected background is observed. Gluino masses up to 1550 GeV and neutralino masses up to 900 GeV are excluded at 95$\%$ C.L. See Fig. 13.
39  KHACHATRYAN 2017AD searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing at least four jets (including ${{\mathit b}}$-jets), missing transverse momentum and tagged top quarks. No evidence for an excess over the expected background is observed. Gluino masses up to 1450 GeV and neutralino masses up to 820 GeV are excluded at 95$\%$ C.L. See Fig. 13.
40  KHACHATRYAN 2017AS searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with a single electron or muon and multiple jets. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu1B simplified models, see their Fig. 7.
41  KHACHATRYAN 2017AW searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least three charged leptons, in any combination of electrons and muons, and significant $\not E_T$. 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 sbottom mass in the Tsbot2 simplified model, see their Figure 4.
42  KHACHATRYAN 2017P searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with one or more jets and large $\not E_T$. 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 sbottom 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.
43  KHACHATRYAN 2017V searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two photons and large $\not E_T$. 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.
44  SIRUNYAN 2017AF searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with a single lepton (electron or muon), jets, including at least one jet originating from a ${{\mathit b}}$-quark, and large $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A and Tglu3B simplified models, see their Figure 2.
45  SIRUNYAN 2017AY searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least one photon, jets and large $\not E_T$. 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 Tskq4A and Tsqk4B simplified models, see their Figure 6.
46  SIRUNYAN 2017AZ searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with one or more jets and large $\not E_T$. 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 sbottom 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.
47  SIRUNYAN 2017P searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with multiple jets and large $\not E_T$. 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 sbottom mass in the Tsbot1 simplified model, see Fig. 13.
48  SIRUNYAN 2017S searched in 35.9 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two isolated same-sign leptons, jets, and large $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the mass of the gluino mass in the Tglu3A, Tglu3B, Tglu3C, Tglu3D and Tglu1B simplified models, see their Figures 5 and 6, and on the sbottom mass in the Tsbot2 simplified model, see their Figure 6.
49  AABOUD 2016AC searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with hadronic jets, 1 or two hadronically decaying ${{\mathit \tau}}$ and $\not E_T$. In Tglu1F, gluino masses are excluded at 95$\%$ C.L. up to 1570 GeV for neutralino masses of 100 GeV or below. Neutralino masses up to 700 GeV are excluded for all gluino masses between 800 GeV and 1500 GeV, while the strongest neutralino-mass exclusion of 750 GeV is achieved for gluino masses around 1400 GeV. See their Fig. 8. Limits are also presented in the context of Gauge-Mediated Symmetry Breaking models: in this case, values of ${{\mathit \Lambda}}$ below 92 TeV are excluded at the 95$\%$ CL, corresponding to gluino masses below 2000 GeV. See their Fig. 9.
50  AABOUD 2016J searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with one isolated electron or muon, hadronic jets, and $\not E_T$. Gluino-mediated pair production of stops with a nearly mass-degenerate stop and neutralino are targeted and gluino masses are excluded at 95$\%$ C.L. up to 1460 GeV. A 100$\%$ of stops decaying via charm + neutralino is assumed. The results are also valid in case of 4-body decays ${{\widetilde{\mathit t}}_{{1}}}$ $\rightarrow$ ${{\mathit f}}{{\mathit f}^{\,'}}{{\mathit b}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ . See their Fig. 8.
51  AABOUD 2016M searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two photons, hadronic jets and $\not E_T$. No significant excess above the Standard Model expectations is observed. Exclusion limits at 95$\%$ C.L. are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for bino-like NLSP. See their Fig.$~$3.
52  AABOUD 2016N searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing hadronic jets, large $\not E_T$, and no electrons or muons. No significant excess above the Standard Model expectations is observed. Gluino masses below 1510 GeV are excluded at the 95$\%$ C.L. in a simplified model with only gluinos and the lightest neutralino. See their Fig. 7b.
53  AABOUD 2016N searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing hadronic jets, large $\not E_T$, and no electrons or muons. No significant excess above the Standard Model expectations is observed. Gluino masses below 1500 GeV are excluded at the 95$\%$ C.L. in a simplified model with gluinos decaying via an intermediate ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ to two quarks, a ${{\mathit W}}$ boson and a ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 200 GeV. See their Fig 8.
54  AAD 2016AD searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events containing several energetic jets, of which at least three must be identified as ${{\mathit b}}$-jets, large $\not E_T$ and no electrons or muons. No significant excess above the Standard Model expectations is observed. For ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ below 800 GeV, gluino masses below 1780 GeV are excluded at 95$\%$ C.L. for gluinos decaying via bottom squarks. See their Fig. 7a.
55  AAD 2016AD searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of pp collisions at $\sqrt {s }$ = 13 TeV for events containing several energetic jets, of which at least three must be identified as ${{\mathit b}}$-jets, large $\not E_T$ and one electron or muon. Large-radius jets with a high mass are also used to identify highly boosted top quarks. No significant excess above the Standard Model expectations is observed. For ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ below 700 GeV, gluino masses below 1760 GeV are excluded at 95$\%$ C.L. for gluinos decaying via top squarks. See their Fig. 7b.
56  AAD 2016BB searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with exactly two same-sign leptons or at least three leptons, multiple hadronic jets, ${{\mathit b}}$-jets, and $\not E_T$. No significant excess over the Standard Model expectation is found. Exclusion limits at 95$\%$ C.L. are set on the gluino mass in various simplified models (Tglu1D, Tglu1E, Tglu3A). See their Figs. 4.a, 4.b, and 4.d.
57  AAD 2016BG searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in final states with one isolated electron or muon, hadronic jets, and $\not E_T$. The data agree with the SM background expectation in the six signal selections defined in the search, and the largest deviation is a 2.1 standard deviation excess. Gluinos are excluded at 95$\%$ C.L. up to 1600 GeV assuming they decay via the lightest chargino to the lightest neutralino as in the model Tglu1B for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$=100 GeV, assuming ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}=({\mathit m}_{{{\widetilde{\mathit g}}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$)/2. See their Fig.$~$6.
58  AAD 2016V searched in 3.2 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with $\not E_T$ various hadronic jet multiplicities from ${}\geq{}$7 to ${}\geq{}$10 and with various ${{\mathit b}}$-jet multiplicity requirements. No significant excess over the Standard Model expectation is found. Exclusion limits at 95$\%$ C.L. are set on the gluino mass in one simplified model (Tglu1E) and a pMSSM-inspired model. See their Fig. 5.
59  KHACHATRYAN 2016AM searched in 19.7 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with highly boosted ${{\mathit W}}$-bosons and ${{\mathit b}}$-jets, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3C and Tglu3B simplified models, see Fig. 12.
60  KHACHATRYAN 2016BJ searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the following simplified models: Tglu3A and Tglu3D, see Fig. 4, Tglu3B and Tglu3C, see Fig. 5, and Tglu1B, see Fig. 7.
61  KHACHATRYAN 2016BS searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least one energetic jet , no isolated leptons, and significant $\not E_T$, using the transverse mass variable ${{\mathit M}_{{T2}}}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu2A and Tglu3A simplified models, see Fig. 10 and Table 3.
62  KHACHATRYAN 2016BY searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 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 sbottom masses in the Tsbot3 simplified model, see Fig. 5.
63  KHACHATRYAN 2016V searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least four energetic jets and significant $\not E_T$, no identified isolated electron or muon or charged track. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu1A, Tglu1C, Tglu2A, and Tglu3A simplified models, see Fig. 8.
64  AAD 2015BG searched in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with jets, missing $\mathit E_{T}$, and two opposite-sign same flavor isolated leptons featuring either a kinematic edge, or a peak at the ${{\mathit Z}}$-boson mass, in the invariant mass spectrum. No evidence for a statistically significant excess over the expected SM backgrounds are observed and 95$\%$ C.L. exclusion limits are derived in a GGM simplified model of gluino pair production where the gluino decays into quarks, a ${{\mathit Z}}$-boson, and a massless gravitino LSP, see Fig. 12. Also, limits are set in simplified models with slepton/sneutrino intermediate states, see Fig. 13.
65  AAD 2015BV 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 ${\mathit {\mathit b}}$-jets in the $\sqrt {s }$ =8 TeV data set collected in 2012. The paper reports the results of new interpretations and statistical combinations of previously published analyses, as well as new analyses. Exclusion limits at 95$\%$ C.L. are set on the gluino mass in several R-parity conserving models, leading to a generalized constraint on gluino masses exceeding 1150 GeV for lightest supersymmetric particle masses below 100 GeV. See their Figs. 10, 19, 20, 21, 23, 25, 26, 29-37.
66  AAD 2015BX interpreted the results of a wide range of ATLAS direct searches for supersymmetry, during the first run of the LHC using the $\sqrt {s }$ =7 TeV and $\sqrt {s }$ = 8 TeV data set collected in 2012, within the wider framework of the phenomenological MSSM (pMSSM). The integrated luminosity was up to 20.3 ${\mathrm {fb}}{}^{-1}$. From an initial random sampling of 500 million pMSSM points, generated from the 19-parameter pMSSM, a total of 310,327 model points with ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ LSP were selected each of which satisfies constraints from previous collider searches, precision measurements, cold dark matter energy density measurements and direct dark matter searches. The impact of the ATLAS Run 1 searches on this space was presented, considering the fraction of model points surviving, after projection into two-dimensional spaces of sparticle masses. Good complementarity is observed between different ATLAS analyses, with almost all showing regions of unique sensitivity. ATLAS searches have good sensitivity at LSP mass below 800 GeV.
67  AAD 2015CA searched in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with one or more photons, hadronic jets or ${{\mathit b}}$-jets and $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on gluino masses in the general gauge-mediated SUSY breaking model (GGM), for bino-like or higgsino-bino admixtures NLSP, see Fig. 8, 10, 11
68  KHACHATRYAN 2015AF searched in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least two energetic jets and significant $\not E_T$, using the transverse mass variable ${{\mathit M}_{{T2}}}$ to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 13(a), or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 13(b), or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 13(c). See also Table 5. Exclusions in the CMSSM, assuming tan ${{\mathit \beta}}$ = 30, $\mathit A_{0}$ = $−$2 max(${\mathit m}_{\mathrm {0}}$, ${\mathit m}_{\mathrm {1/2}}$) and ${{\mathit \mu}}$ $>$ 0, are also presented, see Fig. 15.
69  KHACHATRYAN 2015I searched in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events in which ${\mathit {\mathit b}}$-jets and four ${{\mathit W}}$-bosons are produced. Five individual search channels are combined (fully hadronic, single lepton, same-sign dilepton, opposite-sign dilepton, multilepton). No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a simplified model where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 5. Also a simplified model with gluinos decaying into on-shell top squarks is considered, see Fig. 6.
70  KHACHATRYAN 2015X searched in 19.3${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least two energetic jets, at least one of which is required to originate from a ${\mathit {\mathit b}}$ quark, and significant $\not E_T$, using the razor variables ($\mathit M_{R}$) and $\mathit R{}^{2}$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ and the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ take place with branching ratios varying between 0, 50 and 100$\%$, see Figs. 13 and 14.
71  AAD 2014AE searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 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 gluinos and squarks, see Figures 5, 6 and 7. Limits are also derived in the mSUGRA/CMSSM with parameters tan $\beta $ = 30, ${{\mathit A}_{{0}}}$ = $-2$ ${\mathit m}_{\mathrm {0}}$ and ${{\mathit \mu}}$ $>$ 0, see their Fig. 8.
72  AAD 2014AG searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing one hadronically decaying ${{\mathit \tau}}$-lepton, zero or one additional light leptons (electrons or muons), jets and large missing transverse momentum. No excess of events above the expected level of Standard Model background was found. Exclusion limits at 95$\%$ C.L. are set in several SUSY scenarios. For an interpretation in the minimal GMSB model, see their Fig. 8. For an interpretation in the mSUGRA/CMSSM with parameters tan $\beta $ = 30, ${{\mathit A}_{{0}}}$ = $-2$ ${\mathit m}_{\mathrm {0}}$ and ${{\mathit \mu}}$ $>$ 0, see their Fig. 9. For an interpretation in the framework of natural Gauge Mediation, see Fig. 10. For an interpretation in the bRPV scenario, see their Fig. 11.
73  AAD 2014X searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least four leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a general gauge-mediation model (GGM) where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , with ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ , takes place with a branching ratio of 100$\%$, for two choices of tan $\beta $ = 1.5 and 30, see Fig. 11. Also some constraints on the higgsino mass parameter ${{\mathit \mu}}$ are discussed.
74  CHATRCHYAN 2014AH searched in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV for events with at least two energetic jets and significant $\not E_T$, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. No significant excess above the Standard Model expectations is observed. Limits are set on sbottom masses in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 28. Exclusions in the CMSSM, assuming tan $\beta $ = 10, ${{\mathit A}_{{0}}}$ = 0 and ${{\mathit \mu}}$ $>$ 0, are also presented, see Fig. 26.
75  CHATRCHYAN 2014AH searched in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV for events with at least two energetic jets and significant $\not E_T$, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. A second analysis requires at least one of the jets to be originating from a ${{\mathit b}}$-quark. No significant excess above the Standard Model expectations is observed. Limits are set on sbottom masses in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit b}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Figs. 28 and 29. Exclusions in the CMSSM, assuming tan $\beta $ = 10, ${{\mathit A}_{{0}}}$ = 0 and ${{\mathit \mu}}$ $>$ 0, are also presented, see Fig. 26.
76  CHATRCHYAN 2014AH searched in 4.7 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV for events with at least two energetic jets and significant $\not E_T$, using the razor variables (${{\mathit M}_{{R}}}$ and ${{\mathit R}^{2}}$) to discriminate between signal and background processes. A second analysis requires at least one of the jets to be originating from a ${{\mathit b}}$-quark. No significant excess above the Standard Model expectations is observed. Limits are set on sbottom masses in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Figs. 28 and 29. Exclusions in the CMSSM, assuming tan $\beta $ = 10, ${{\mathit A}_{{0}}}$ = 0 and ${{\mathit \mu}}$ $>$0, are also presented, see Fig. 26.
77  CHATRCHYAN 2014I searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing multijets and large $\not E_T$. No excess over the expected SM background is observed. Exclusion limits are derived in simplified models containing gluinos that decay via ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ with a 100$\%$ branching ratio, see Fig. 7b, or via ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ with a 100$\%$ branching ratio, see Fig. 7c, or via ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\overline{\mathit q}}}{{\mathit W}}$ $/$ ${{\mathit Z}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ , see Fig. 7d.
78  CHATRCHYAN 2014N searched in 19.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events containing a single isolated electron or muon and multiple jets, at least two of which are identified as originating from a ${{\mathit b}}$-quark. No significant excesses over the expected SM backgrounds are observed. The results are interpreted in three simplified models of gluino pair production with subsequent decay into virtual or on-shell top squarks, where each of the top squarks decays in turn into a top quark and a ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$, see Fig. 4. The models differ in which masses are allowed to vary.
79  CHATRCHYAN 2014R searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least three leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a slepton co-NLSP simplified model (GMSB) where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}{{\widetilde{\mathit G}}}$ takes place with a branching ratio of 100$\%$, see Fig. 8.
80  CHATRCHYAN 2014R searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with at least three leptons (electrons, muons, taus) in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in a simplified model where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, see Fig. 11.
81  AABOUD 2018BJ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV in events with two opposite-sign charged leptons (electrons and muons), jets and missing transverse momentum, with various requirements to be sensitive to signals with different kinematic endpoint values in the dilepton invariant mass distribution. The data are found to be consistent with the SM expectation. Results are interpreted in the Tglu1H model in case of ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 1 GeV: for any ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$, gluino masses below 1500 GeV are excluded, see their Fig. 14(a).
82  AABOUD 2018V searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 a Tglu1C-like model, assuming 50$\%$ BR for each gluino decay mode. Gluino masses below 1770 GeV are excluded for any ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ $−$ ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ and ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ = 60 GeV, see their Fig. 16(b).
83  AABOUD 2017AZ searched in 36.1 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with at least seven jets and large missing transverse momentum. Selected events are further classified based on the presence of large R-jets or ${{\mathit b}}$-jets and no leptons. No significant excess above the Standard Model expectations is observed. Limits are set for pMSSM models with ${{\mathit M}_{{1}}}$ = 60 GeV, tan(${{\mathit \beta}}$) = 10, ${{\mathit \mu}}$ $<$ 0 varying the soft-breaking parameters ${{\mathit M}_{{3}}}$ and ${{\mathit \mu}}$. Gluino masses up to 1600 GeV are excluded for ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 200 GeV. See their Figure 6a and text for details on the model.
84  KHACHATRYAN 2016AY searched in 2.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV for events with one isolated high transverse momentum lepton (${{\mathit e}}$ or ${{\mathit \mu}}$), hadronic jets of which at least one is identified as coming from a ${{\mathit b}}$-quark, and large $\not E_T$. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in the Tglu3A simplified model, see Fig. 10, and in the Tglu3B model, see Fig. 11.
85  KHACHATRYAN 2016BT performed a global Bayesian analysis of a wide range of CMS results obtained with data samples corresponding to 5.0 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 7 TeV and in 19.5 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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.
86  AAD 2015AB searched for the decay of neutral, weakly interacting, long-lived particles in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. Signal events require at least two reconstructed vertices possibly originating from long-lived particles decaying to jets in the inner tracking detector and muon spectrometer. No significant excess of events over the expected background was found. Results were interpreted in Stealth SUSY benchmark models where a pair of gluinos decay to long-lived singlinos, ${{\widetilde{\mathit S}}}$, which in turn each decay to a low-mass gravitino and a pair of jets. The 95$\%$ confidence-level limits are set on the cross section ${\times }$ branching ratio for the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit S}}}{{\mathit g}}$ , as a function of the singlino proper lifetime (c${{\mathit \tau}}$). See their Fig. 10(f)
87  AAD 2015AI searched in 20 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 gluino mass in the CMSSM/mSUGRA, see Fig. 15, in the NUHMG, see Fig. 16, and in various simplified models, see Figs. $18 - 22$.
88  AAD 2015CB searched for events containing at least one long-lived particle that decays at a significant distance from its production point (displaced vertex, DV) into two leptons or into five or more charged particles in 20.3 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 multitrak 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 $\mathit R$-parity violation, split supersymmetry, and gauge mediation. See their Fig. $12 - 20$.
89  KHACHATRYAN 2015AD searched in 19.4 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 ${{\mathit Z}}$-boson mass, in the invariant mass spectrum. No evidence for a statistically significant excess over the expected SM backgrounds is observed and 95$\%$ C.L. exclusion limits are derived in a simplified model of gluino pair production where the gluino decays into quarks, a ${{\mathit Z}}$-boson, and a massless gravitino LSP, see Fig. 9.
90  KHACHATRYAN 2015AZ searched in 19.7 ${\mathrm {fb}}{}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with either at least one photon, hadronic jets and $\not E_T$ (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.
91  AAD 2014AX searched in 20.1 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for the strong production of supersymmetric particles in events containing either zero or at last one high high-$p_T$ lepton, large missing transverse momentum, high jet multiplicity and at least three jets identified as originating from ${{\mathit b}}$-quarks. No excess over the expected SM background is observed. Limits are derived in mSUGRA/CMSSM models with tan $\beta $ = 30, ${{\mathit A}_{{0}}}$ = $-2{{\mathit m}_{{0}}}$ and ${{\mathit \mu}}$ $>$ 0, see their Fig. 14. Also, exclusion limits in simplified models containing gluinos and scalar top and bottom quarks are set, see their Figures 12, 13.
92  AAD 2014E searched in 20.3 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ 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 ${{\mathit b}}$-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 ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{(*)\pm}}{{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit Z}^{(*)}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, the following assumptions have been made: ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = 0.5 ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + ${\mathit m}_{{{\widetilde{\mathit g}}}}$, ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = 0.5 (${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 520 GeV. In the ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \nu}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ or ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{2}}^{0}}$ , ${{\widetilde{\mathit \chi}}_{{2}}^{0}}$ $\rightarrow$ ${{\mathit \ell}^{\pm}}{{\mathit \ell}^{\mp}}$( ${{\mathit \nu}}{{\mathit \nu}}$) ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$ simplified model, the following assumptions have been made: ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ = ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{2}}^{0}}}$ = 0.5 (${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ + ${\mathit m}_{{{\widetilde{\mathit g}}}}$), ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$ $<$ 660 GeV. Limits are also derived in the mSUGRA/CMSSM, bRPV and GMSB models, see their Fig. 8.
93  CHATRCHYAN 2014H searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit t}}}{{\mathit t}}$ , ${{\widetilde{\mathit t}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, with varying mass of the ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$, or where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\widetilde{\mathit b}}}{{\mathit b}}$ , ${{\widetilde{\mathit b}}}$ $\rightarrow$ ${{\mathit t}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, with varying mass of the ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$, see Fig. 5.
94  CHATRCHYAN 2014H searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit q}}{{\mathit q}^{\,'}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, with varying mass of the ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ and ${{\widetilde{\mathit \chi}}_{{1}}^{0}}$, see Fig. 7.
95  CHATRCHYAN 2014H searched in 19.5 fb${}^{-1}$ of ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV for events with two isolated same-sign dileptons and jets in the final state. No significant excess above the Standard Model expectations is observed. Limits are set on the gluino mass in simplified models where the decay ${{\widetilde{\mathit g}}}$ $\rightarrow$ ${{\mathit b}}{{\overline{\mathit t}}}{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ , ${{\widetilde{\mathit \chi}}_{{1}}^{\pm}}$ $\rightarrow$ ${{\mathit W}^{\pm}}{{\widetilde{\mathit \chi}}_{{1}}^{0}}$ takes place with a branching ratio of 100$\%$, for two choices of ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{\pm}}}$ and fixed ${\mathit m}_{{{\widetilde{\mathit \chi}}_{{1}}^{0}}}$, see Fig. 6.
  References:
SIRUNYAN 2020B
PL B801 135183 Combined search for supersymmetry with photons in proton-proton collisions at $\sqrt{s}=$ 13 TeV
AABOUD 2019I
PR D99 012009 Search for squarks and gluinos in final states with hadronically decaying $\tau$-leptons, jets, and missing transverse momentum using $pp$ collisions at $\sqrt{s}$ = 13 TeV with the ATLAS detector
SIRUNYAN 2019AU
EPJ C79 444 Search for supersymmetry in events with a photon, jets, $\mathrm {b}$ -jets, and missing transverse momentum in proton?proton collisions at 13 $\,\text {Te}\text {V}$
SIRUNYAN 2019S
JHEP 1903 031 Inclusive search for supersymmetry in pp collisions at $ \sqrt{s}=13 $ TeV using razor variables and boosted object identification in zero and one lepton final states
SIRUNYAN 2019K
JHEP 1901 154 Search for supersymmetry in events with a photon, a lepton, and missing transverse momentum in proton-proton collisions at $\sqrt{s} =$ 13 TeV
SIRUNYAN 2019CH
JHEP 1910 244 Search for supersymmetry in proton-proton collisions at 13 TeV in final states with jets and missing transverse momentum
SIRUNYAN 2019CE
PRL 123 241801 Search for physics beyond the standard model in events with overlapping photons and jets
SIRUNYAN 2019AG
JHEP 1906 143 Search for supersymmetry in final states with photons and missing transverse momentum in proton-proton collisions at 13 TeV
AABOUD 2018V
PR D97 112001 Search for squarks and gluinos in final states with jets and missing transverse momentum using 36??fb$^{-1}$ of $\sqrt{s}=13$??TeV pp collision data with the ATLAS detector
AABOUD 2018BJ
EPJ C78 625 Search for new phenomena using the invariant mass distribution of same-flavour opposite-sign dilepton pairs in events with missing transverse momentum in $\sqrt{s}=13$   $\text {Te}\text {V}$ pp collisions with the ATLAS detector
AABOUD 2018U
PR D97 092006 Search for photonic signatures of gauge-mediated supersymmetry in 13 TeV $pp$ collisions with the ATLAS detector
AABOUD 2018AR
JHEP 1806 107 Search for supersymmetry in final states with missing transverse momentum and multiple $b$-jets in proton-proton collisions at $ \sqrt{s}=13 $ TeV with the ATLAS detector
AABOUD 2018AS
JHEP 1806 022 Search for long-lived charginos based on a disappearing-track signature in pp collisions at $ \sqrt{s}=13 $ TeV with the ATLAS detector
SIRUNYAN 2018AY
JHEP 1805 025 Search for natural and split supersymmetry in proton-proton collisions at $ \sqrt{s}=13 $ TeV in final states with jets and missing transverse momentum
SIRUNYAN 2018AC
PL B780 384 Search for supersymmetry in events with one lepton and multiple jets exploiting the angular correlation between the lepton and the missing transverse momentum in proton-proton collisions at $\sqrt{s} = $ 13 TeV
SIRUNYAN 2018AA
PL B780 118 Search for gauge-mediated supersymmetry in events with at least one photon and missing transverse momentum in pp collisions at $\sqrt{s} = $ 13 TeV
SIRUNYAN 2018D
PR D97 012007 Search for Supersymmetry in Proton-Proton Collisions at 13 TeV using Identified Top Quarks
SIRUNYAN 2018AR
JHEP 1803 076 Search for new phenomena in final states with two opposite-charge, same-flavor leptons, jets, and missing transverse momentum in pp collisions at $ \sqrt{s}=13 $ TeV
SIRUNYAN 2018AL
JHEP 1802 067 Search for supersymmetry in events with at least three electrons or muons, jets, and missing transverse momentum in proton-proton collisions at $ \sqrt{s}=13 $ TeV
SIRUNYAN 2018M
PRL 120 241801 Search for Physics Beyond the Standard Model in Events with High-Momentum Higgs Bosons and Missing Transverse Momentum in Proton-Proton Collisions at 13 TeV
AABOUD 2017N
EPJ C77 144 Search for New Phenomena in Events Containing a Same-Flavour Opposite-Sign Dilepton Pair, Jets, and Large Missing Transverse Momentum in $\sqrt {s }$ = 13 ${{\mathit p}}{{\mathit p}}$ Collisions with the ATLAS Detector
AABOUD 2017AR
PR D96 112010 Search for squarks and gluinos in Events with an Isolated Lepton, Jets, and Missing Transverse Momentum at $\sqrt {s }$ = 13 TeV with the ATLAS Detector
AABOUD 2017AJ
JHEP 1709 084 Search for Supersymmetry in Final States with Two Same-Sign or Three Leptons and Jets using 36 ${\mathrm {fb}}{}^{-1}$ of $\sqrt {s }$ = 13 TeV ${{\mathit p}}{{\mathit p}}$ Collision Data with the ATLAS Detector
AABOUD 2017AY
JHEP 1712 085 Search for a Scalar Partner of the Top Quark in the Jets Plus Missing Transverse Momentum Final State at $\sqrt {s }$ = 13 TeV with the ATLAS Detector
AABOUD 2017AZ
JHEP 1712 034 Search for New Phenomena with Large Jet Multiplicities and Missing Transverse Momentum using Large-Radius Jets and Flavour-Tagging at ATLAS in 13 TeV ${{\mathit p}}{{\mathit p}}$ Collisions
KHACHATRYAN 2017
PR D95 012003 Inclusive Search for Supersymmetry using Razor Variables in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV
KHACHATRYAN 2017AW
EPJ C77 635 Search for New Phenomena with Multiple Charged Leptons in Proton-Proton Collisions at $\sqrt {s }$ = 13 TeV
KHACHATRYAN 2017P
EPJ C77 294 A Search for New Phenomena in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13TeV in Final States with Missing Transverse Momentum and at Least One Jet using the $\alpha _{T}$ Variable
KHACHATRYAN 2017AS
PR D95 012011 Search for Supersymmetry in Events with One Lepton and Multiple Jets in Proton-Proton Collisions at $\sqrt {s }$ = 13 TeV
KHACHATRYAN 2017AD
PR D96 012004 Search for Supersymmetry in the All-Hadronic Final State using Top Quark Tagging in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV
KHACHATRYAN 2017V
PL B769 391 Search for Supersymmetry in Events with Photons and Missing Transverse Energy in ${{\mathit p}}{{\mathit p}}$ Collisions at 13 TeV
SIRUNYAN 2017S
EPJ C77 578 Search for Physics beyond the Standard Model in Events with Two Leptons of Same Sign, Missing Transverse Momentum, and Jets in Proton-Proton Collisions at $\sqrt {s }$ = 13 TeV
SIRUNYAN 2017AY
JHEP 1712 142 Search for Supersymmetry in Events with at Least One Photon, Missing Transverse Momentum, and Large Transverse Event Activity in Proton-Proton Collisions at $\sqrt {s }$ =13 TeV
SIRUNYAN 2017AZ
EPJ C77 710 Search for New Phenomena with the $\mathit M_{T2}$ Variable in the All-Hadronic Final State Produced in Proton-Proton Collisions at $\sqrt {s }$ = 13 TeV
SIRUNYAN 2017P
PR D96 032003 Search for Supersymmetry in Multijet Events with Missing Transverse Momentum in Proton-Proton Collisions at 13 TeV
SIRUNYAN 2017AF
PRL 119 151802 Search for Supersymmetry in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV in the Single-Lepton Final State using the Sum of Masses of Large-Radius Jets
AABOUD 2016J
PR D94 052009 Search for Top Squarks in Final States with One Isolated Lepton, Jets, and Missing Transverse Momentum in $\sqrt {s }$ = 13 TeV ${{\mathit p}}{{\mathit p}}$ Collisions with the ATLAS Detector
AABOUD 2016N
EPJ C76 392 Search for Squarks and Gluinos in Final States with Jets and Missing Transverse Momentum at $\sqrt {s }$ = 13 TeV with the ATLAS Detector
AABOUD 2016AC
EPJ C76 683 Search for Squarks and Gluinos in Events with Hadronically Decaying tau leptons, jets and Missing Transverse Momentum in Proton-Proton Collisions at $\sqrt {s }$ = 13 TeV Recorded with the ATLAS Detector
AABOUD 2016M
EPJ C76 517 Search for Supersymmetry in a Final State Containing Two Photons and Missing Transverse Momentum in $\sqrt {s }$ = 13 TeV ${{\mathit p}}{{\mathit p}}$ Collisions at the LHC using the ATLAS Detector
AAD 2016BB
EPJ C76 259 Search for Supersymmetry at $\sqrt {s }$ = 13 TeV in Final States with Jets and Two Same-Sign Leptons or Three Leptons with the ATLAS Detector
AAD 2016AD
PR D94 032003 Search for Pair Production of Gluinos Decaying Via stop and sbottom in Events with ${\mathit {\mathit b}}$-Jets and Large Missing Transverse Momentum in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV with the ATLAS Detector
AAD 2016BG
EPJ C76 565 Search for Gluinos in Events with an Isolated Lepton, Jets and Missing Transverse Momentum at $\sqrt {s }$ = 13 Te V with the ATLAS Detector
AAD 2016V
PL B757 334 Search for New Phenomena in Final States with Large Jet Multiplicities and Missing Transverse Momentum with ATLAS using $\sqrt {s }$ = 13 TeV Proton-Proton Collisions
KHACHATRYAN 2016BY
JHEP 1612 013 Search for New Physics in Final States with Two Opposite-Sign, Same-Flavor leptons, jets, and Missing Transverse Momentum in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV
KHACHATRYAN 2016AY
JHEP 1608 122 Search for Supersymmetry in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV in the Single-Lepton Final State using the Sum of Masses of Large-Radius Jets
KHACHATRYAN 2016V
PL B758 152 Search for Supersymmetry in the Multijet and Missing Transverse Momentum Final State in ${{\mathit p}}{{\mathit p}}$ Collisions at 13 TeV
KHACHATRYAN 2016AM
PR D93 092009 Search for Supersymmetry in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV in Final States with Boosted ${{\mathit W}}$ Bosons and ${\mathit {\mathit b}}$ Jets using Razor Variables
KHACHATRYAN 2016BJ
EPJ C76 439 Search for New Physics in Same-sign Dilepton Events in Proton-Proton Collisions at $\sqrt {s }$ = 13 TeV
KHACHATRYAN 2016BS
JHEP 1610 006 Search for New Physics with the MT2 Variable in all-Jets Final States Produced in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 13 TeV
KHACHATRYAN 2016BT
JHEP 1610 129 Phenomenological MSSM Interpretation of CMS Searches in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 7 and 8 TeV
AAD 2015AI
JHEP 1504 116 Search for Squarks and Gluinos in Events with Isolated Leptons, Jets and Missing Transverse Momentum at $\sqrt {s }$ = 8 TeV with the ATLAS Detector
AAD 2015BG
EPJ C75 318 Search for Supersymmetry in Events Containing a Same-Flavour Opposite-Sign Dilepton Pair, Jets, and Large Missing Transverse Momentum in $\sqrt {s }$ = 8 TeV ${{\mathit p}}{{\mathit p}}$ Collisions with the ATLAS Detector
AAD 2015AB
PR D92 012010 Search for Long-Lived, Weakly Interacting Particles that Decay to Displaced Hadronic Jets in Proton-Proton Collisions at $\sqrt {s }$ = 8 TeV with the ATLAS Detector
AAD 2015CA
PR D92 072001 Search for Photonic Signatures of Gauge-Mediated Supersymmetry in 8 TeV ${{\mathit p}}{{\mathit p}}$ Collisions with the ATLAS Detector
AAD 2015CB
PR D92 072004 Search for Massive, Long-Lived Particles using Multitrack Displaced Vertices or Displaced Lepton Pairs in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV with the ATLAS Detector
AAD 2015BX
JHEP 1510 134 Summary of the ATLAS Experiment's Sensitivity to Supersymmetry after LHC Run 1 Interpreted in the Phenomenological MSSM
AAD 2015BV
JHEP 1510 054 Summary of the Searches for Squarks and Gluinos using $\sqrt {s }$ = 8 TeV ${{\mathit p}}{{\mathit p}}$ Collisions with the ATLAS Experiment at the LHC
KHACHATRYAN 2015AF
JHEP 1505 078 Searches for Supersymmetry using the $\mathit M_{T2}$ Variable in Hadronic Events Produced in ${{\mathit p}}{{\mathit p}}$ Collisions at 8 TeV
KHACHATRYAN 2015AZ
PR D92 072006 Search for Supersymmetry with Photons in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV
KHACHATRYAN 2015X
PR D91 052018 Search for Supersymmetry Using Razor Variables in Events with ${\mathit {\mathit b}}$-Tagged Jets in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV
KHACHATRYAN 2015I
PL B745 5 Searches for Supersymmetry Based on Events with ${\mathit {\mathit b}}$ Jets and Four ${{\mathit W}}$ Bosons in ${{\mathit p}}{{\mathit p}}$ Collisions at 8 TeV
KHACHATRYAN 2015AD
JHEP 1504 124 Search for Physics Beyond the Standard Model in Events with Two Leptons, Jets, and Missing Transverse Momentum in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV
AAD 2014AX
JHEP 1410 024 Search for Strong Production of Supersymmetric Particles in Final States with Missing Transverse Momentum and at Least Three ${\mathit {\mathit b}}$-Jets at $\sqrt {s }$ = 8 TeV Proton-Proton Collisions with the ATLAS Detector
AAD 2014E
JHEP 1406 035 Search for Supersymmetry at $\sqrt {s }$ = 8 TeV in Final States with Jets and Two Same-Sign Leptons or Three Leptons with the ATLAS Detector
AAD 2014X
PR D90 052001 Search for Supersymmetry in Events with Four or More Leptons in $\sqrt {s }$ = 8 TeV ${{\mathit p}}{{\mathit p}}$ Collisions with the ATLAS Detector
AAD 2014AG
JHEP 1409 103 Search for Supersymmetry in Events with Large Missing Transverse Momentum, Jets, and at least one tau Lepton in 20 fb${}^{-1}$ of $\sqrt {s }$ = 8 TeV Proton-Proton Collision Data with the ATLAS Detector
AAD 2014AE
JHEP 1409 176 Search for squarks and gluinos with the ATLAS Detector in Final States with Jets and Missing Transverse Momentum using $\sqrt {s }$ = 8 TeV Proton-Proton Collision Data
CHATRCHYAN 2014R
PR D90 032006 Search for Anomalous Production of Events with Three or More Leptons in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV
CHATRCHYAN 2014AH
PR D90 112001 Search for Supersymmetry with Razor Variables in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 7 TeV
CHATRCHYAN 2014I
JHEP 1406 055 Search for New Physics in the Multijet and Missing Transverse Momentum Final State in Proton-Proton Collisions at $\sqrt {s }$ = 8 TeV
CHATRCHYAN 2014H
JHEP 1401 163 Search for New Physics in Events with Same-Sign Dileptons and Jets in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV
CHATRCHYAN 2014N
PL B733 328 Search for Supersymmetry in ${{\mathit p}}{{\mathit p}}$ Collisions at $\sqrt {s }$ = 8 TeV in Events with a Single Lepton, Large Jet Multiplicity, and Multiple $\mathit b$ Jets