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\section{Interpretation}
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In this section, we interpret the results of the targeted search in the context of the \wzmet\ model depicted in Fig.~\ref{fig:diagrams} (right)
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and a gauge-mediated SUSY breaking (GMSB) model that produces a signature of \zzmet\ will be added. The results of the targeted search presented here
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will be combined with those of the trilepton ewkino search for the final \wzmet\ interpretation, and with the quadlepton ewkino search
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for the final GMSB \zzmet\ interpretation.
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The exclusion is performed using the results of simultaneous counting experiments in the exclusive \MET\ signal regions defined by \MET\ $>$ 80 GeV,
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as summarized in Table~\ref{tab:results_targ} (commonly referred to as a ``shape analysis'').
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For the \wzmet\ model, the signal efficiency times acceptance and cross section upper limits are displayed in Fig.~\ref{fig:results_wzmet},
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along with the observed and expected exclusion contours, which are compared to the 2011 observed exclusion contour.
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Figure~\ref{fig:results_wzmetpoints} shows the excluded points used to derive the exclusion contours. We note that the map of exclusion
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contours appears quite ragged since for many of the points the cross section upper limit is very close to the theory cross section.
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Therefore we do not expect the ragged exclusion region to be an issue for the final results since
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we currently have 9.2 fb$^{-1}$ and expect the luminosity to increase significantly. A {\bf VERY APPROXIMATE} projection of the expected excluded region
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for an integrated luminosity of 15 fb$^{-1}$ (a rough guess at the final HCP data sample) is obtained by scaling the expected cross section limits by
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$\sqrt{(9.2 \rm{fb}^{-1})/(15 \rm{fb}^{-1})}$, as displayed in Fig.~\ref{fig:results_15fb}.
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\begin{figure}[!ht]
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\begin{center}
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\begin{tabular}{cc}
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\includegraphics[width=0.45\textwidth]{plots/wzsms_eff.pdf}
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\includegraphics[width=0.45\textwidth]{plots/wzsms_xsec.pdf}
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\end{tabular}
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\caption{ Interpretation of the targeted analysis in the \wzmet\ model. The acceptance times efficiency (left) and cross section
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upper limit (right) and displayed. The observed and expected exclusion contours are indicated and compared to the observed
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exclusion from the 2011 analysis.
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\label{fig:results_wzmet}}
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\end{center}
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\end{figure}
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\begin{figure}[!hb]
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\begin{center}
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\includegraphics[width=0.75\textwidth]{plots/wzsms_points.pdf}
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\caption{ Observed (left) and expected (right) excluded points for the \wzmet\ interpretation, with the corresponding exclusion contours overlaid.
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\label{fig:results_wzmetpoints}}
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\end{center}
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\end{figure}
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\clearpage
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\begin{figure}[!ht]
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\begin{center}
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\includegraphics[width=0.5\textwidth]{plots/wzsms_expected_15fb.pdf}
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\caption{ A {\bf VERY APPROXIMATE} projection of the expected excluded points for an integrated luminosity of 15$^{-1}$.
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\label{fig:results_15fb}}
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\end{center}
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\end{figure}
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The results of the interpretation in the GMSB \zzmet\ model are displayed in Fig.~\ref{fig:results_gmsb},
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as a function of the chargino and neutralino mass parameter $\mu$. These results exclude the range $X < \mu < Y$~GeV.
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\begin{figure}[!hb]
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\begin{center}
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\includegraphics[width=0.75\textwidth]{plots/ZDIJET_GMSB.pdf}
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\caption{ Interpretation of the targeted analysis in the GMSB \zzmet\ model.
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\label{fig:results_gmsb}}
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\end{center}
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\end{figure}
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