$
>\mathbf {30.4}
$
|
>20.4
|
95 |
1 |
|
CMS |
$
>20
$
|
$>\mathbf {30}$
|
95 |
2 |
|
ATLS |
• • • We do not use the following data for averages, fits, limits, etc. • • • |
$
>15.8
$
|
>21.8
|
95 |
3 |
|
ATLS |
$
> 12.0
$
|
>15.2
|
95 |
4 |
|
CMS |
$
> 12.5
$
|
> 16.7
|
95 |
5 |
|
ATLS |
$
> 9.6
$
|
> 12.9
|
95 |
6 |
|
ATLS |
$
> 9.5
$
|
> 13.1
|
95 |
7 |
|
CMS |
$
> 8.0
$
|
> 7.0
|
95 |
8 |
|
ATLS |
1
SIRUNYAN 2019AC limits are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV.
|
2
AABOUD 2017AT limits are from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit uses a uniform positive prior in 1/${{\mathit \Lambda}^{2}}$.
|
3
AABOUD 2016U limits are from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV. The quoted limit uses a uniform positive prior in 1/${{\mathit \Lambda}^{2}}$.
|
4
KHACHATRYAN 2015AE limit is from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV.
|
5
AAD 2014BE limits are from ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 8 TeV. The quoted limit uses a uniform positive prior in 1/${{\mathit \Lambda}^{2}}$.
|
6
AAD 2013E limis are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
|
7
CHATRCHYAN 2013K limis are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
|
8
AAD 2012AB limis are from ${{\mathit \mu}^{+}}{{\mathit \mu}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
|