Difference: PhysicsResultsSUS14016 (10 vs. 11)

Revision 112015-09-03 - JohannesSchulz

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META TOPICPARENT name="SUSYPhotonWorkingGroup"
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Figure 8: Measurement of the trigger efficiency of the photon part as a function of the transverse momentum of the photon with the highest transverse momentum. The plateau region is reached for $p_{\text{T}}$ = 40 GeV and the efficiency for $p_{\text{T}}$ $>$ 40 GeV is given by $\varepsilon_{\text{$\gamma$-req}}$ = (88.0 $\pm$ 0.7({stat.)}) $\%$.
Figure 9: Control region where the $V\gamma$ and $\gamma$jets background simulations are fitted to the data using the template variable $E_{\mathrm{T}}^{\text{miss}}$/$\sqrt{\text{ $H_{\text{T}}$}}$.
Table 3: Number of signal events and the selection efficiency after each selection step for three signal points, each corresponding to a different signal scenario. The TChiNg_500 point corresponds to a NLSP mass of 500 GeV, The TChiWg_650 point corresponds to a NLSP mass of 650 GeV and the GGM_640_630 point corresponds to a wino mass of 640 GeV and a bino mass of 630 GeV.
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Figure 10: Efficiencies for the GGM signal points in the plane spanned by of the wino and bino mass.
Figure 11: Effciencies for the TChiNg signal scenario depending on the mass of the NLSP after the full selection.
Figure 12: Effciencies for the TChiWg signal scenario depending on the mass of the NLSP after the full selection. The TChiWg simulation has a higher granularity compared to the TChiNg simulation.
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Figure 10: Efficiencies for the GGM signal points in the plane spanned by of the wino and bino mass. Electronic version: WinoBino_Acceptance.root
Figure 11: Effciencies for the TChiNg signal scenario depending on the mass of the NLSP after the full selection. Eelectronic version: TChiNg_acc.root
Figure 12: Effciencies for the TChiWg signal scenario depending on the mass of the NLSP after the full selection. The TChiWg simulation has a higher granularity compared to the TChiNg simulation. Electronic version: TChiwg_acc.root
 

-- JohannesSchulz - 2015-07-22

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