| 41 |
|
\end{itemize} |
| 42 |
|
|
| 43 |
|
|
| 44 |
< |
Good agreement between the observed and predicted MET distributions is observed for each MC sample, as well as between the two samples, as shown in figures \ref{fig:mcclosurepho} and \ref{fig:mcclosureqcd}. |
| 44 |
> |
Good agreement between the observed and predicted MET distributions is observed for each MC sample, |
| 45 |
> |
as well as between the two samples, as shown in figures \ref{fig:mcclosurepho} and \ref{fig:mcclosureqcd}. |
| 46 |
> |
Note that the low equivalent luminosity of the QCD samples ($\approx$ 300/pb) explains the lack of |
| 47 |
> |
statistics in the tails. |
| 48 |
|
|
| 49 |
|
\begin{figure}[hbt] |
| 50 |
|
\begin{center} |
| 83 |
|
\begin{tabular}{r|r|r|r|r} |
| 84 |
|
MET & $>$ 30 GeV & $>$ 60 GeV & $>$ 100 GeV & $>$ 200 \\ \hline |
| 85 |
|
%tr |
| 86 |
< |
data & 921 & 15 & 1 & 0 \\ |
| 87 |
< |
pred & 959.15 $\pm$ 27.00 & 19.39 $\pm$ 0.58 & 2.28 $\pm$ 0.09 & 0.07 $\pm$ 0.01 \\ |
| 86 |
> |
Z MC & 921 & 15 & 1 & 0 \\ |
| 87 |
> |
Prediction & 959.15 $\pm$ 27.00 & 19.39 $\pm$ 0.58 & 2.28 $\pm$ 0.09 & 0.07 $\pm$ 0.01 \\ |
| 88 |
|
|
| 89 |
|
%no tr |
| 90 |
|
% Z MC & 921 & 15 & 1 & 0 \\ |
