$
> 4.5
$
|
> 12.8
|
95 |
1 |
|
ZEUS |
$
> 23.9
$
|
> 16.8
|
95 |
2 |
|
CMS |
$
\bf{>24}
$
|
>37
|
95 |
3 |
|
ATLS |
$
> 8.4
$
|
$\mathbf {>10.2}$
|
95 |
4 |
|
DLPH |
$
\bf{> 9.4}
$
|
>5.6
|
95 |
5 |
|
ALEP |
$
\mathbf { > 9.4}
$
|
>4.9
|
95 |
4 |
|
ALEP |
$
\bf{>23.3}
$
|
>12.5
|
95 |
6 |
|
RVUE |
$
\bf{>11.1}
$
|
>26.4
|
95 |
6 |
|
RVUE |
• • • We do not use the following data for averages, fits, limits, etc. • • • |
$
> 15.5
$
|
> 19.5
|
95 |
7 |
|
ATLS |
$
> 13.5
$
|
>18.3
|
95 |
8 |
|
CMS |
$
> 16.4
$
|
> 20.7
|
95 |
9 |
|
ATLS |
$
> 9.5
$
|
> 12.1
|
95 |
10 |
|
ATLS |
$
> 10.1
$
|
> 9.4
|
95 |
11 |
|
ATLS |
$
> 4.2
$
|
> 4.0
|
95 |
12 |
|
H1 |
$
> 3.8
$
|
> 3.8
|
95 |
13 |
|
DLPH |
$
> 12.9
$
|
> 7.2
|
95 |
14 |
|
ALEP |
$
> 3.7
$
|
> 5.9
|
95 |
15 |
|
CDF |
1
ABRAMOWICZ 2019 limits are from Q${}^{2}$ spectrum measurements of ${{\mathit e}^{\pm}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit e}^{\pm}}{{\mathit X}}$ .
|
2
SIRUNYAN 2019AC limits are from ${{\mathit e}^{+}}{{\mathit e}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\sqrt {s }$ = 13 TeV.
|
3
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/${{\mathit \Lambda}^{2}}$.
|
4
ABDALLAH 2009 and SCHAEL 2007A limits are from $\mathit R_{b}$, $\mathit A{}^{b}_{FB}$.
|
5
SCHAEL 2007A limits are from $\mathit R_{c}$, $\mathit Q{}^{depl}_{FB}$, and hadronic cross section measurements.
|
6
CHEUNG 2001B is an update of BARGER 1998E.
|
7
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/${{\mathit \Lambda}^{2}}$.
|
8
KHACHATRYAN 2015AE limit is from ${{\mathit e}^{+}}{{\mathit e}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 8 TeV.
|
9
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/${{\mathit \Lambda}^{2}}$.
|
10
AAD 2013E limis are from ${{\mathit e}^{+}}{{\mathit e}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
|
11
AAD 2012AB limis are from ${{\mathit e}^{+}}{{\mathit e}^{-}}$ mass distribution in ${{\mathit p}}{{\mathit p}}$ collisions at $\mathit E_{{\mathrm {cm}}}$ = 7 TeV.
|
12
AARON 2011C limits are from ${{\mathit Q}^{2}}$ spectrum measurements of ${{\mathit e}^{\pm}}$ ${{\mathit p}}$ $\rightarrow$ ${{\mathit e}^{\pm}}{{\mathit X}}$ .
|
13
ABDALLAH 2011 limit is from ${{\mathit e}^{+}}$ ${{\mathit e}^{-}}$ $\rightarrow$ ${{\mathit t}}{{\overline{\mathit c}}}$ cross section. ${{\mathit \Lambda}_{{LL}}}$ = ${{\mathit \Lambda}_{{LR}}}$ = ${{\mathit \Lambda}_{{RL}}}$ = ${{\mathit \Lambda}_{{RR}}}$ is assumed.
|
14
SCHAEL 2007A limit assumes quark flavor universality of the contact interactions.
|
15
ABULENCIA 2006L limits are from ${{\mathit p}}{{\overline{\mathit p}}}$ collisions at $\sqrt {s }$ = 1.96 TeV.
|