195 |
|
the boundaries using the method recommended by the SUSY |
196 |
|
group\cite{ref:smooth}. In addition, we show a limit |
197 |
|
curve based on the LO cross-section, as well as the |
198 |
< |
``expected'' limit curve. The expected limit curve is |
198 |
> |
``expected'' limit curve. The expected limit curve was |
199 |
|
calculated using the CLA function also available in cl95cms. |
200 |
< |
Cross-section uncertainties due to variations of the factorization |
200 |
> |
In general we found that the ``expected'' limit is very close |
201 |
> |
to the observed limit, which is not surprising since the |
202 |
> |
expected BG (1.4 $\pm$ 0.8 events) is fully consistent |
203 |
> |
with the observation (1 event). Because of the quantization, |
204 |
> |
we find that the expected and observed limits are either |
205 |
> |
identical or differ by one or at most two grid points. |
206 |
> |
We have approximated the expected limit as the observed limit |
207 |
> |
minus 10 GeV\footnote{We show the expected limit only because |
208 |
> |
this is what is recommended by SUSY management. We believe that |
209 |
> |
quoting the agreement between the expected BG and the |
210 |
> |
observation should be enough....}. |
211 |
> |
Finally, we note that the sross-section uncertainties due to |
212 |
> |
variations of the factorization |
213 |
|
and renormalization scale are not included for the LO curve. |
214 |
|
The results are shown in Figure~\ref{fig:msugra} |
215 |
|
|
250 |
|
we use the lognormal nuisance parameter model as the default. |
251 |
|
|
252 |
|
|
253 |
< |
\clearpage |
253 |
> |
% \clearpage |
254 |
|
|
255 |
|
|
256 |
|
\subsubsection{Effect of signal contamination} |