additional_resources:
- {description: Param card for Gluino-Slepton 2000-1300 model, location: param_card_GG_N2_SLN1_2000_1300_2LMET100.dat}
- {description: Run card for Gluino-Slepton 2000-1300 model, location: run_card_GG_N2_SLN1_2000_1300_2LMET100.dat}
- {description: Param card for Gluino-Z* 800-700 model, location: param_card_GG_N2_offshellZN1_800_700_2LMET100.dat}
- {description: Run card for Gluino-Z* 800-700 model, location: run_card_GG_N2_offshellZN1_800_700_2LMET100.dat}
- {description: Param card for Squark-Z* 1200-700 model, location: param_card_SS_N2_ZN1_1200_700_2LMET100.dat}
- {description: Run card for Squark-Z* 1200-700 model, location: run_card_SS_N2_ZN1_1200_700_2LMET100.dat}
- description: run_card.dat used for the C1pN2 100 60 sample
  location: C1pN2_100_60_run_card.dat
- description: param_card.dat used for the C1pN2 100 60 sample
  location: C1pN2_100_60_param_card.dat
- description: madspin_card_C1N2_WZ.dat used for the C1pN2 100 60 sample
  location: C1pN2_100_60_madspin_card_C1N2_WZ.dat
- description: run_card.dat used for the C1mN2 100 60 sample
  location: C1mN2_100_60_run_card.dat
- description: param_card.dat used for the C1mN2 100 60 sample
  location: C1mN2_100_60_param_card.dat
- description: madspin_card_C1N2_WZ.dat used for the C1mN2 100 60 sample
  location: C1mN2_100_60_madspin_card_C1N2_WZ.dat
- description: run_card.dat used for the C1pN2 150 70 sample
  location: C1pN2_150_70_run_card.dat
- description: param_card.dat used for the C1pN2 150 70 sample
  location: C1pN2_150_70_param_card.dat
- description: madspin_card_C1N2_WZ.dat used for the C1pN2 150 70 sample
  location: C1pN2_150_70_madspin_card_C1N2_WZ.dat
- description: run_card.dat used for the C1mN2 150 70 sample
  location: C1mN2_150_70_run_card.dat
- description: param_card.dat used for the C1mN2 150 70 sample
  location: C1mN2_150_70_param_card.dat
- description: madspin_card_C1N2_WZ.dat used for the C1mN2 150 70 sample
  location: C1mN2_150_70_madspin_card_C1N2_WZ.dat
- description: run_card.dat used for the C1N2 250 100 sample
  location: C1N2_250_100_run_card.dat
- description: param_card.dat used for the C1N2 250 100 sample
  location: C1N2_250_100_param_card.dat
- description: run_card.dat used for the C1N2 400 200 sample
  location: C1N2_400_200_run_card.dat
- description: param_card.dat used for the C1N2 400 200 sample
  location: C1N2_400_200_param_card.dat
- description: run_card.dat used for the C1N2 650 250 sample
  location: C1N2_650_250_run_card.dat
- description: param_card.dat used for the C1N2 650 250 sample
  location: C1N2_650_250_param_card.dat
- description: run_card.dat used for the GMSB 200 sample
  location: GMSB_200_run_card.dat
- description: param_card.dat used for the GMSB 200 sample
  location: GMSB_200_param_card.dat
- description: run_card.dat used for the GMSB 500 sample
  location: GMSB_500_run_card.dat
- description: param_card.dat used for the GMSB 500 sample
  location: GMSB_500_param_card.dat
- description: run_card.dat used for the GMSB 700 sample
  location: GMSB_700_run_card.dat
- description: param_card.dat used for the GMSB 700 sample
  location: GMSB_700_param_card.dat
### SimpleAnalysis
- {description: Code for RJR regions in SimpleAnalysis, location: ANA-SUSY-2018-05_RJR.cxx}
- {description: Code for EWK regions in SimpleAnalysis, location: ANA-SUSY-2018-05_EWK.cxx}
- {description: Code for Strong regions in SimpleAnalysis, location: ANA-SUSY-2018-05_Strong.cxx}
### Likelihoods
- {description: Collection of JSON-based likelihoods, location: llh_jsons.tar}
- {description: README describing llh files, location: README.md}
---
data_file: dummy.yaml
data_license: {description: "", name: "", url: ""}
description: '- - - - - - - - Overview of HEPData Record - - - - - - - - <br/><br/>
<b>EWK SR distributions:</b> <a href="116034?version=1&table=Figure 11a">SR-High_8-EWK</a>; <a href="116034?version=1&table=Figure 11b">SR-ℓℓ𝑏𝑏-EWK</a>; <a href="116034?version=1&table=Figure 11c">SR-Int-EWK</a>; <a href="116034?version=1&table=Figure 11d">SR-Low-EWK</a>; <a href="116034?version=1&table=Figure 11e">SR-OffShell-EWK</a><br/><br/>
<b>Strong SR distributions:</b> <a href="116034?version=1&table=Figure 13a">SRC-STR</a>; <a href="116034?version=1&table=Figure 13b">SRLow-STR</a>; <a href="116034?version=1&table=Figure 13c">SRMed-STR</a>; <a href="116034?version=1&table=Figure 13d">SRHigh-STR</a><br/><br/>

<b>RJR SR Yields:</b> <a href="116034?version=1&table=Table 16">SR2l-Low-RJR, SR2l-ISR-RJR</a><br/><br/>
<b>EWK SR Yields:</b> <a href="116034?version=1&table=Table 18">SR-High_16a-EWK, SR-High_8a-EWK, SR-1J-High-EWK, SR-ℓℓ𝑏𝑏-EWK, SR-High_16b-EWK, SR-High_8b-EWK</a>; <a href="116034?version=1&table=Table 19">SR-Int_a-EWK, SR-Low_a-EWK, SR-Low-2-EWK, SR-OffShell_a-EWK, SR-Int_b-EWK, SR-Low_b-EWK, SR-OffShell_b-EWK </a><br/><br/>
<b>Strong SR Yields:</b> <a href="116034?version=1&table=Table 21">SRC-STR, SRLow-STR, SRMed-STR, SRHigh-STR</a>; <a href="116034?version=1&table=Table 22">SRZLow-STR, SRZMed-STR, SRZHigh-STR</a><br/><br/>

<b>C1N2 Model Limits:</b> <a href="116034?version=1&table=Table 15a C1N2 Observed Limit">Obs</a>; <a href="116034?version=1&table=Table 15a C1N2 Expected Limit">Exp</a>; <a href="116034?version=1&table=Auxiliary Figure 34a C1N2 Expected XS Upper Limit">Upper Limits</a><br/><br/>
<b>GMSB Model Limits:</b> <a href="116034?version=1&table=Table 15b GMSB Observed Limit">Obs</a>; <a href="116034?version=1&table=Table 15b GMSB Expected Limit">Exp</a>; <a href="116034?version=1&table=Auxiliary Figure 34b GMSB Expected XS Upper Limit">Upper Limits</a><br/><br/>
<b>Gluon-Slepton Model Limits:</b> <a href="116034?version=1&table=Figure 16a Observed Limit">Obs</a>; <a href="116034?version=1&table=Figure 16a Expected Limit">Exp</a>; <a href="116034?version=1&table=Auxiliary Figure 23a XS Upper Limit">Upper Limits</a><br/><br/>
<b>Gluon-Z* Model Limits:</b> <a href="116034?version=1&table=Figure 16b Observed Limit">Obs</a>; <a href="116034?version=1&table=Figure 16b Expected Limit">Exp</a>; <a href="116034?version=1&table=Auxiliary Figure 23b XS Upper Limit">Upper Limits</a><br/><br/>
<b>Squark-Z* Model Limits:</b> <a href="116034?version=1&table=Figure 16c Observed Limit">Obs</a>; <a href="116034?version=1&table=Figure 16c Expected Limit">Exp</a>; <a href="116034?version=1&table=Auxiliary Figure 23c XS Upper Limit">Upper Limits</a><br/><br/>

<b>EWK VR distributions:</b> <a href="116034?version=1&table=Figure 4a S_ETmiss in VR-High-Sideband-EWK">VR-High-Sideband-EWK</a>; <a href="116034?version=1&table=Figure 4b S_Etmiss in VR-High-R-EWK">VR-High-R-EWK</a>; <a href="116034?version=1&table=Figure 4c S_Etmiss in VR-1J-High-EWK">VR-1J-High-EWK</a>; <a href="116034?version=1&table=Figure 4d S_Etmiss in VR-llbb-EWK">VR-ℓℓ𝑏𝑏-EWK</a>; <a href="116034?version=1&table=Figure 5a S_Etmiss in VR-Int-EWK">VR-Int-EWK</a>; <a href="116034?version=1&table=Figure 5b S_Etmiss in VR-Low-EWK">VR-Low-EWK</a>; <a href="116034?version=1&table=Figure 5c S_Etmiss in VR-Low-2-EWK">VR-Low-2-EWK</a>; <a href="116034?version=1&table=Figure 5d S_Etmiss in VR-OffShell-EWK">VR-OffShell-EWK</a><br/><br/>
<b>Strong VR distributions:</b> <a href="116034?version=1&table=Figure 6a">VRC-STR</a>; <a href="116034?version=1&table=Figure 6b">VRLow-STR</a>; <a href="116034?version=1&table=Figure 6c">VRMed-STR</a>; <a href="116034?version=1&table=Figure 6d">VRHigh-STR</a>; <a href="116034?version=1&table=Figure 8">VR3L-STR</a><br/><br/>

<b>Other Strong distributions:</b> <a href="116034?version=1&table=Auxiliary Figure 17a">SRLow-STR + VRLow-STR</a><br/><br/>
<b>Other EWK distributions:</b> <a href="116034?version=1&table=Auxiliary Figure 33a Mjj in CR-Z-EWK and SR-Low-EWK">CR-Z-EWK + SR-Low-EWK</a>; <a href="116034?version=1&table=Auxiliary Figure 33b S_ETmiss in CR-Z-met-EWK">CR-Z-met-EWK</a><br/><br/>

<b>Strong Signal Cutflows:</b> <a href="116034?version=1&table=Auxiliary Table 30-31 SRC-STR Cutflow">SRC-STR GG_N2_ZN1</a>; <a href="116034?version=1&table=Auxiliary Table 30-31 SRMed-STR Cutflow">SRC-STR SS_N2_ZN1</a>; <a href="116034?version=1&table=Auxiliary Table 30-31 SRLow-STR Cutflow">SRLow-STR GG_N2_SLN1</a>; <a href="116034?version=1&table=Auxiliary Table 30-31 SRHigh-STR Cutflow">SRC-STR GG_N2_SLN1</a>; <a href="116034?version=1&table=Auxiliary Table 30-31 SRZLow-STR Cutflow">SRZLow-STR SS_N2_ZN1</a>; <a href="116034?version=1&table=Auxiliary Table 30-31 SRZMed-STR Cutflow">SRZMed-STR SS_N2_ZN1</a>; <a href="116034?version=1&table=Auxiliary Table 30-31 SRZHigh-STR Cutflow">SRZHigh-STR SS_N2_ZN1</a><br/><br/>
<b>EWK Signal Cutflows:</b> <a href="116034?version=1&table=Auxiliary Table 36 SR-OffShell_a-EWK Cutflow"> SR-OffShell_a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 37 SR-OffShell_b-EWK Cutflow"> SR-OffShell_b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 38 SR-Low_a-EWK Cutflow"> SR-Low_a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 39 SR-Low_b-EWK Cutflow"> SR-Low_b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 40 SR-Low-2-EWK Cutflow"> SR-Low-2-E</a>; <a href="116034?version=1&table=Auxiliary Table 41 SR-Int_a-EWK Cutflow"> SR-Int_a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 42 SR-Int_b-EWK Cutflow"> SR-Int_b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 43 SR-High_16a-EWK Cutflow"> SR-High_16a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 44 SR-High_16b-EWK Cutflow"> SR-High_16b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 45 SR-High_8a-EWK Cutflow"> SR-High_8a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 46 SR-High_8b-EWK Cutflow"> SR-High_8b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 47 SR-1J-High-EWK Cutflow"> SR-1J-Hig</a>; <a href="116034?version=1&table=Auxiliary Table 48 SR-llbb-EWK Cutflow"> SR-llbb-EWK</a><br/><br/>
<b>EWK Signal Number of MC Events:</b> <a href="116034?version=1&table=Auxiliary Table 36 SR-OffShell_a-EWK Generated"> SR-OffShell_a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 37 SR-OffShell_b-EWK Generated"> SR-OffShell_b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 38 SR-Low_a-EWK Generated"> SR-Low_a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 39 SR-Low_b-EWK Generated"> SR-Low_b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 40 SR-Low-2-EWK Generated"> SR-Low-2-E</a>; <a href="116034?version=1&table=Auxiliary Table 41 SR-Int_a-EWK Generated"> SR-Int_a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 42 SR-Int_b-EWK Generated"> SR-Int_b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 43 SR-High_16a-EWK Generated"> SR-High_16a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 44 SR-High_16b-EWK Generated"> SR-High_16b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 45 SR-High_8a-EWK Generated"> SR-High_8a-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 46 SR-High_8b-EWK Generated"> SR-High_8b-EWK</a>; <a href="116034?version=1&table=Auxiliary Table 47 SR-1J-High-EWK Generated"> SR-1J-Hig</a>; <a href="116034?version=1&table=Auxiliary Table 48 SR-llbb-EWK Generated"> SR-llbb-EWK</a><br/><br/>

<b>SRC-STR Signal Acceptance:</b> <a href="116034?version=1&table=GG_N2_SLN1 acc in SRC">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 acc in SRC">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 acc in SRC">SS_N2_ZN1</a><br/><br/>
<b>SRLow-STR Signal Acceptance:</b> <a href="116034?version=1&table=GG_N2_SLN1 acc in SRLow">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 acc in SRLow">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 acc in SRLow">SS_N2_ZN1</a><br/><br/>
<b>SRMed-STR Signal Acceptance:</b> <a href="116034?version=1&table=GG_N2_SLN1 acc in SRMed">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 acc in SRMed">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 acc in SRMed">SS_N2_ZN1</a><br/><br/>
<b>SRHigh-STR Signal Acceptance:</b> <a href="116034?version=1&table=GG_N2_SLN1 acc in SRHigh">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 acc in SRHigh">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 acc in SRHigh">SS_N2_ZN1</a><br/><br/>
<b>SRZLow-STR Signal Acceptance:</b> <a href="116034?version=1&table=GG_N2_ZN1 acc in SRZLow">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 acc in SRZLow">SS_N2_ZN1</a><br/><br/>
<b>SRZMed-STR Signal Acceptance:</b> <a href="116034?version=1&table=GG_N2_ZN1 acc in SRZMed">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 acc in SRZMed">SS_N2_ZN1</a><br/><br/>
<b>SRZHigh-STR Signal Acceptance:</b> <a href="116034?version=1&table=GG_N2_ZN1 acc in SRZHigh">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 acc in SRZHigh">SS_N2_ZN1</a><br/><br/>

<b>SRC-STR Signal Efficiency:</b> <a href="116034?version=1&table=GG_N2_SLN1 eff in SRC">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 eff in SRC">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 eff in SRC">SS_N2_ZN1</a><br/><br/>
<b>SRLow-STR Signal Efficiency:</b> <a href="116034?version=1&table=GG_N2_SLN1 eff in SRLow">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 eff in SRLow">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 eff in SRLow">SS_N2_ZN1</a><br/><br/>
<b>SRMed-STR Signal Efficiency:</b> <a href="116034?version=1&table=GG_N2_SLN1 eff in SRMed">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 eff in SRMed">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 eff in SRMed">SS_N2_ZN1</a><br/><br/>
<b>SRHigh-STR Signal Efficiency:</b> <a href="116034?version=1&table=GG_N2_SLN1 eff in SRHigh">GG_N2_SLN1</a>; <a href="116034?version=1&table=GG_N2_ZN1 eff in SRHigh">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 eff in SRHigh">SS_N2_ZN1</a><br/><br/>

<b>SRZLow-STR Signal Efficiency:</b> <a href="116034?version=1&table=GG_N2_ZN1 eff in SRZLow">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 eff in SRZLow">SS_N2_ZN1</a><br/><br/>
<b>SRZMed-STR Signal Efficiency:</b> <a href="116034?version=1&table=GG_N2_ZN1 eff in SRZMed">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 eff in SRZMed">SS_N2_ZN1</a><br/><br/>
<b>SRZHigh-STR Signal Efficiency:</b> <a href="116034?version=1&table=GG_N2_ZN1 eff in SRZHigh">GG_N2_ZN1</a>; <a href="116034?version=1&table=SS_N2_ZN1 eff in SRZHigh">SS_N2_ZN1</a><br/><br/>

<b>SR-OffShell_a-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-OffShell_a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-OffShell_a-EWK">C1N2</a>; <br/><br/>
<b>SR-OffShell_b-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-OffShell_b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-OffShell_b-EWK">C1N2</a>; <br/><br/>
<b>SR-Low_a-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in C1N2 acc in SR-Low_a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in C1N2 acc in SR-Low_a-EWK">C1N2</a>; <br/><br/>
<b>SR-Low_b-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-Low_b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-Low_b-EWK">C1N2</a>; <br/><br/>
<b>SR-Int_a-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-Int_a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-Int_a-EWK">C1N2</a>; <br/><br/>
<b>SR-Int_b-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-Int_b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-Int_b-EWK">C1N2</a>; <br/><br/>
<b>SR-High_16a-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-High_16a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-High_16a-EWK">C1N2</a>; <br/><br/>
<b>SR-High_16b-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-High_16b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-High_16b-EWK">C1N2</a>; <br/><br/>
<b>SR-High_8a-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-High_8a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-High_8a-EWK">C1N2</a>; <br/><br/>
<b>SR-High_8b-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-High_8b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-High_8b-EWK">C1N2</a>; <br/><br/>
<b>SR-1J-High-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-1J-High-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-1J-High-EWK">C1N2</a>; <br/><br/>
<b>SR-llbb-EWK Signal Acceptance:</b><a href="116034?version=1&table=GMSB acc in SR-llbb-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 acc in SR-llbb-EWK">C1N2</a>; <br/><br/>

<b>SR-OffShell_a-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-OffShell_a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-OffShell_a-EWK">C1N2</a>; <br/><br/>
<b>SR-OffShell_b-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-OffShell_b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-OffShell_b-EWK">C1N2</a>; <br/><br/>
<b>SR-Low_a-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in C1N2 eff in SR-Low_a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in C1N2 eff in SR-Low_a-EWK">C1N2</a>; <br/><br/>
<b>SR-Low_b-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-Low_b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-Low_b-EWK">C1N2</a>; <br/><br/>
<b>SR-Int_a-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-Int_a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-Int_a-EWK">C1N2</a>; <br/><br/>
<b>SR-Int_b-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-Int_b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-Int_b-EWK">C1N2</a>; <br/><br/>
<b>SR-High_16a-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-High_16a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-High_16a-EWK">C1N2</a>; <br/><br/>
<b>SR-High_16b-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-High_16b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-High_16b-EWK">C1N2</a>; <br/><br/>
<b>SR-High_8a-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-High_8a-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-High_8a-EWK">C1N2</a>; <br/><br/>
<b>SR-High_8b-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-High_8b-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-High_8b-EWK">C1N2</a>; <br/><br/>
<b>SR-1J-High-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-1J-High-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-1J-High-EWK">C1N2</a>; <br/><br/>
<b>SR-llbb-EWK Signal Efficiency:</b><a href="116034?version=1&table=GMSB eff in SR-llbb-EWK">GMSB</a>; <a href="116034?version=1&table=C1N2 eff in SR-llbb-EWK">C1N2</a>; <br/><br/>

<b>Truth Code snippets</b>, <b>SLHA files</b>, and <b>PYHF json likelihoods</b> are available under "Resources" (purple button on the left)

----
Record created with hepdata_lib 0.7.0: https://zenodo.org/record/4946277 and PYHF: https://doi.org/10.5281/zenodo.1169739'
keywords: []
name: Table of Contents
---
data_file: table_16.yaml
description: Breakdown of expected and observed yields in the two recursive-jigsaw
  reconstruction signal regions after a simultaneous fit of the the CRs. The two sets
  of regions are fit separately. The uncertainties include both statistical and systematic
  sources.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
location: Data from Table 16
name: Table 16
### END RJR START EWK
---
data_file: table_18.yaml
description: Breakdown of expected and observed yields in the electroweak search High
  and $\ell\ell bb$ signal regions after a simultaneous fit to the signal regions
  and control regions. All statistical and systematic uncertainties are included.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
location: Data from Table 18
name: Table 18
---
data_file: table_19.yaml
description: Breakdown of expected and observed yields in the electroweak search Int,
  Low, and OffShell signal regions after a simultaneous fit to the signal regions
  and control regions. All statistical and systematic uncertainties are included.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
location: Data from Table 19
name: Table 19
---
data_file: table_21.yaml
description: Breakdown of expected and observed yields in the four edge signal regions,
  integrated over the $m_{\ell\ell}$ distribution after a separate simultaneous fit
  to each signal region and control region pair. The uncertainties include both the
  statistical and systematic sources.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: observables
  values:
  - N
location: Data from Table 21
name: Table 21
---
data_file: table_22.yaml
description: Breakdown of expected and observed yields in the three on-$Z$ signal
  regions after a separate simultaneous fit to each signal region and control region
  pair. The uncertainties include both the statistical and systematic sources.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: observables
  values:
  - N
location: Data from Table 22
name: Table 22
---
additional_resources:
- description: Image file
  location: VR_High_Sideband_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_High_Sideband_EWK_met_Sign.png
data_file: figure_4a_s_etmiss_in_vr-high-sideband-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-High-Sideband-EWK
  (top-left), VR-High-R-EWK (top-right), VR-1J-High-EWK (bottom-left), and VR-$\ell\ell
  bb$-EWK (bottom-right) from the EWK search after a simultaneous fit of the control
  regions. The hatched band includes both the systematic and statistical uncertainties.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 4a
name: Figure 4a S_ETmiss in VR-High-Sideband-EWK
---
additional_resources:
- description: Image file
  location: VR_High_R_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_High_R_EWK_met_Sign.png
data_file: figure_4b_s_etmiss_in_vr-high-r-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-High-Sideband-EWK
  (top-left), VR-High-R-EWK (top-right), VR-1J-High-EWK (bottom-left), and VR-$\ell\ell
  bb$-EWK (bottom-right) from the EWK search after a simultaneous fit of the control
  regions. The hatched band includes both the systematic and statistical uncertainties.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 4b
name: Figure 4b S_Etmiss in VR-High-R-EWK
---
additional_resources:
- description: Image file
  location: VR_1J_High_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_1J_High_EWK_met_Sign.png
data_file: figure_4c_s_etmiss_in_vr-1j-high-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-High-Sideband-EWK
  (top-left), VR-High-R-EWK (top-right), VR-1J-High-EWK (bottom-left), and VR-$\ell\ell
  bb$-EWK (bottom-right) from the EWK search after a simultaneous fit of the control
  regions. The hatched band includes both the systematic and statistical uncertainties.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 4c
name: Figure 4c S_Etmiss in VR-1J-High-EWK
---
additional_resources:
- description: Image file
  location: VR_llbb_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_llbb_EWK_met_Sign.png
data_file: figure_4d_s_etmiss_in_vr-llbb-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-High-Sideband-EWK
  (top-left), VR-High-R-EWK (top-right), VR-1J-High-EWK (bottom-left), and VR-$\ell\ell
  bb$-EWK (bottom-right) from the EWK search after a simultaneous fit of the control
  regions. The hatched band includes both the systematic and statistical uncertainties.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 4d
name: Figure 4d S_Etmiss in VR-llbb-EWK
---
additional_resources:
- description: Image file
  location: VR_Int_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_Int_EWK_met_Sign.png
data_file: figure_5a_s_etmiss_in_vr-int-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-Int-EWK
  (top-left), VR-Low-EWK (top-right), VR-Low-2-EWK (bottom-left), and VR-OffShell-EWK
  (bottom-right) from the EWK search after a simultaneous fit of the control regions.
  The hatched band includes both the systematic and statistical uncertainties. The
  last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 5a
name: Figure 5a S_Etmiss in VR-Int-EWK
---
additional_resources:
- description: Image file
  location: VR_Low_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_Low_EWK_met_Sign.png
data_file: figure_5b_s_etmiss_in_vr-low-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-Int-EWK
  (top-left), VR-Low-EWK (top-right), VR-Low-2-EWK (bottom-left), and VR-OffShell-EWK
  (bottom-right) from the EWK search after a simultaneous fit of the control regions.
  The hatched band includes both the systematic and statistical uncertainties. The
  last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 5b
name: Figure 5b S_Etmiss in VR-Low-EWK
---
additional_resources:
- description: Image file
  location: VR_Low_2_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_Low_2_EWK_met_Sign.png
data_file: figure_5c_s_etmiss_in_vr-low-2-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-Int-EWK
  (top-left), VR-Low-EWK (top-right), VR-Low-2-EWK (bottom-left), and VR-OffShell-EWK
  (bottom-right) from the EWK search after a simultaneous fit of the control regions.
  The hatched band includes both the systematic and statistical uncertainties. The
  last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 5c
name: Figure 5c S_Etmiss in VR-Low-2-EWK
---
additional_resources:
- description: Image file
  location: VR_OffShell_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_VR_OffShell_EWK_met_Sign.png
data_file: figure_5d_s_etmiss_in_vr-offshell-ewk.yaml
description: Distributions of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in VR-Int-EWK
  (top-left), VR-Low-EWK (top-right), VR-Low-2-EWK (bottom-left), and VR-OffShell-EWK
  (bottom-right) from the EWK search after a simultaneous fit of the control regions.
  The hatched band includes both the systematic and statistical uncertainties. The
  last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 5d
name: Figure 5d S_Etmiss in VR-OffShell-EWK
---
additional_resources:
- description: Image file
  location: SF_VRC_log.png
- description: Thumbnail image file
  location: thumb_SF_VRC_log.png
data_file: figure_6a.yaml
description: Observed and expected dilepton mass distributions in VRC-STR (top-left),
  VRLow-STR (top-right), VRMed-STR (bottom-left), and VRHigh-STR (bottom-right). Each
  validation region is fit separately with the corresponding control region. All statistical
  and systematic uncertainties are included in the hatched band. The entries are normalized
  to the bin width, and the last bin is the overflow.
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 6a
name: Figure 6a
---
additional_resources:
- description: Image file
  location: SF_VRLow_log.png
- description: Thumbnail image file
  location: thumb_SF_VRLow_log.png
data_file: figure_6b.yaml
description: Observed and expected dilepton mass distributions in VRC-STR (top-left),
  VRLow-STR (top-right), VRMed-STR (bottom-left), and VRHigh-STR (bottom-right). Each
  validation region is fit separately with the corresponding control region. All statistical
  and systematic uncertainties are included in the hatched band. The entries are normalized
  to the bin width, and the last bin is the overflow.
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 6b
name: Figure 6b
---
additional_resources:
- description: Image file
  location: SF_VRMed_log.png
- description: Thumbnail image file
  location: thumb_SF_VRMed_log.png
data_file: figure_6c.yaml
description: Observed and expected dilepton mass distributions in VRC-STR (top-left),
  VRLow-STR (top-right), VRMed-STR (bottom-left), and VRHigh-STR (bottom-right). Each
  validation region is fit separately with the corresponding control region. All statistical
  and systematic uncertainties are included in the hatched band. The entries are normalized
  to the bin width, and the last bin is the overflow.
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 6c
name: Figure 6c
---
additional_resources:
- description: Image file
  location: SF_VRHigh_log.png
- description: Thumbnail image file
  location: thumb_SF_VRHigh_log.png
data_file: figure_6d.yaml
description: Observed and expected dilepton mass distributions in VRC-STR (top-left),
  VRLow-STR (top-right), VRMed-STR (bottom-left), and VRHigh-STR (bottom-right). Each
  validation region is fit separately with the corresponding control region. All statistical
  and systematic uncertainties are included in the hatched band. The entries are normalized
  to the bin width, and the last bin is the overflow.
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 6d
name: Figure 6d
---
additional_resources:
- description: Image file
  location: SF_VRLow_nJet30.png
- description: Thumbnail image file
  location: thumb_SF_VRLow_nJet30.png
data_file: figure_7a.yaml
description: Observed and expected jet multiplicity in VRLow-STR (top-left), VRMed-STR
  (top-right), and VRHigh-STR (bottom) after a fit performed on the $m_{\ell\ell}$
  distribution and corresponding control region. All statistical and systematic uncertainties
  are included in the hatched band. The last bin contains the overflow.
keywords:
- name: observables
  values:
  - Njets
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 7a
name: Figure 7a
---
additional_resources:
- description: Image file
  location: SF_VRMed_nJet30.png
- description: Thumbnail image file
  location: thumb_SF_VRMed_nJet30.png
data_file: figure_7b.yaml
description: Observed and expected jet multiplicity in VRLow-STR (top-left), VRMed-STR
  (top-right), and VRHigh-STR (bottom) after a fit performed on the $m_{\ell\ell}$
  distribution and corresponding control region. All statistical and systematic uncertainties
  are included in the hatched band. The last bin contains the overflow.
keywords:
- name: observables
  values:
  - Njets
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 7b
name: Figure 7b
---
additional_resources:
- description: Image file
  location: SF_VRHigh_nJet30.png
- description: Thumbnail image file
  location: thumb_SF_VRHigh_nJet30.png
data_file: figure_7c.yaml
description: Observed and expected jet multiplicity in VRLow-STR (top-left), VRMed-STR
  (top-right), and VRHigh-STR (bottom) after a fit performed on the $m_{\ell\ell}$
  distribution and corresponding control region. All statistical and systematic uncertainties
  are included in the hatched band. The last bin contains the overflow.
keywords:
- name: observables
  values:
  - Njets
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 7c
name: Figure 7c
---
additional_resources:
- description: Image file
  location: SF_VR3L_log.png
- description: Thumbnail image file
  location: thumb_SF_VR3L_log.png
data_file: figure_8.yaml
description: "Observed and expected dilepton mass distributions in VR3L-STR without\
  \ a fit to the data. The 'Other' category includes the negligible contributions\
  \ from $t\\bar{t}$ and $Z/\\gamma^*$+jets processes. The hatched band contains the\
  \ statistical uncertainty and the theoretical systematic uncertainties of the $WZ$/$ZZ$\
  \ prediction, which are the dominant sources of uncertainty. No fit is performed.\
  \ The last bin contains the overflow."
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 8
name: Figure 8
---
additional_resources:
- description: Image file
  location: SR_High_8_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_SR_High_8_EWK_met_Sign.png
data_file: figure_11a.yaml
description: Observed and expected distributions in five EWK search regions after
  a simultaneous fit to the SR and CR. In the top row, left-to-right, are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-High_8-EWK and $m_{bb}$ in SR-$\ell\ell bb$-EWK. In the middle row, left-to-right,
  are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in SR-Int-EWK and $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-Low-EWK. In the bottom row is $m_{\ell\ell}$ in SR-OffShell-EWK. Overlaid
  are example C1N2 and GMSB signal models, where the numbers in the brackets indicate
  the masses, in $\mathrm{GeV}$, of the $\tilde{\chi}_1^\pm$ and $\tilde{\chi}_2^0$
  or the mass of the $\tilde{\chi}_1^0$ and branching ratio to the Higgs boson respectively.
  All statistical and systematic uncertainties are included in the hatched bands.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 11a
name: Figure 11a
---
additional_resources:
- description: Image file
  location: SR_llbb_EWK_mbb.png
- description: Thumbnail image file
  location: thumb_SR_llbb_EWK_mbb.png
data_file: figure_11b.yaml
description: Observed and expected distributions in five EWK search regions after
  a simultaneous fit to the SR and CR. In the top row, left-to-right, are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-High_8-EWK and $m_{bb}$ in SR-$\ell\ell bb$-EWK. In the middle row, left-to-right,
  are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in SR-Int-EWK and $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-Low-EWK. In the bottom row is $m_{\ell\ell}$ in SR-OffShell-EWK. Overlaid
  are example C1N2 and GMSB signal models, where the numbers in the brackets indicate
  the masses, in $\mathrm{GeV}$, of the $\tilde{\chi}_1^\pm$ and $\tilde{\chi}_2^0$
  or the mass of the $\tilde{\chi}_1^0$ and branching ratio to the Higgs boson respectively.
  All statistical and systematic uncertainties are included in the hatched bands.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - N
  - Mbb
location: Data from Figure 11b
name: Figure 11b
---
additional_resources:
- description: Image file
  location: SR_Int_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_SR_Int_EWK_met_Sign.png
data_file: figure_11c.yaml
description: Observed and expected distributions in five EWK search regions after
  a simultaneous fit to the SR and CR. In the top row, left-to-right, are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-High_8-EWK and $m_{bb}$ in SR-$\ell\ell bb$-EWK. In the middle row, left-to-right,
  are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in SR-Int-EWK and $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-Low-EWK. In the bottom row is $m_{\ell\ell}$ in SR-OffShell-EWK. Overlaid
  are example C1N2 and GMSB signal models, where the numbers in the brackets indicate
  the masses, in $\mathrm{GeV}$, of the $\tilde{\chi}_1^\pm$ and $\tilde{\chi}_2^0$
  or the mass of the $\tilde{\chi}_1^0$ and branching ratio to the Higgs boson respectively.
  All statistical and systematic uncertainties are included in the hatched bands.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - N
  - SETmiss
location: Data from Figure 11c
name: Figure 11c
---
additional_resources:
- description: Image file
  location: SR_Low_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_SR_Low_EWK_met_Sign.png
data_file: figure_11d.yaml
description: Observed and expected distributions in five EWK search regions after
  a simultaneous fit to the SR and CR. In the top row, left-to-right, are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-High_8-EWK and $m_{bb}$ in SR-$\ell\ell bb$-EWK. In the middle row, left-to-right,
  are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in SR-Int-EWK and $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-Low-EWK. In the bottom row is $m_{\ell\ell}$ in SR-OffShell-EWK. Overlaid
  are example C1N2 and GMSB signal models, where the numbers in the brackets indicate
  the masses, in $\mathrm{GeV}$, of the $\tilde{\chi}_1^\pm$ and $\tilde{\chi}_2^0$
  or the mass of the $\tilde{\chi}_1^0$ and branching ratio to the Higgs boson respectively.
  All statistical and systematic uncertainties are included in the hatched bands.
  The last bin includes the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
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  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
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  - N
  - SETmiss
location: Data from Figure 11d
name: Figure 11d
---
additional_resources:
- description: Image file
  location: SR_OffShell_EWK_mll.png
- description: Thumbnail image file
  location: thumb_SR_OffShell_EWK_mll.png
data_file: figure_11e.yaml
description: Observed and expected distributions in five EWK search regions after
  a simultaneous fit to the SR and CR. In the top row, left-to-right, are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-High_8-EWK and $m_{bb}$ in SR-$\ell\ell bb$-EWK. In the middle row, left-to-right,
  are $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ in SR-Int-EWK and $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  in SR-Low-EWK. In the bottom row is $m_{\ell\ell}$ in SR-OffShell-EWK. Overlaid
  are example C1N2 and GMSB signal models, where the numbers in the brackets indicate
  the masses, in $\mathrm{GeV}$, of the $\tilde{\chi}_1^\pm$ and $\tilde{\chi}_2^0$
  or the mass of the $\tilde{\chi}_1^0$ and branching ratio to the Higgs boson respectively.
  All statistical and systematic uncertainties are included in the hatched bands.
  The last bin includes the overflow.
keywords:
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  - 13000
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  - SUSY
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  - proton-proton scattering
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  values:
  - N
  - Mll
location: Data from Figure 11e
name: Figure 11e
---
additional_resources:
- description: Image file
  location: SF_SRC_log.png
- description: Thumbnail image file
  location: thumb_SF_SRC_log.png
data_file: figure_13a.yaml
description: Observed and expected dilepton mass distributions in SRC-STR (top-left),
  SRLow-STR (top-right), SRMed-STR (bottom-left), and SRHigh-STR (bottom-right), with
  the binning used for interpretations after a separate simultaneous fit to each signal
  region and control region pair. The red dashed lines are example signal models overlaid
  on the figure. All statistical and systematic uncertainties are included in the
  hatched bands. The last bins are the overflow.
keywords:
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  - Mll
  - N
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  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
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  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
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  values:
  - '13000'
location: Data from Figure 13a
name: Figure 13a
---
additional_resources:
- description: Image file
  location: SF_SRLow_log.png
- description: Thumbnail image file
  location: thumb_SF_SRLow_log.png
data_file: figure_13b.yaml
description: Observed and expected dilepton mass distributions in SRC-STR (top-left),
  SRLow-STR (top-right), SRMed-STR (bottom-left), and SRHigh-STR (bottom-right), with
  the binning used for interpretations after a separate simultaneous fit to each signal
  region and control region pair. The red dashed lines are example signal models overlaid
  on the figure. All statistical and systematic uncertainties are included in the
  hatched bands. The last bins are the overflow.
keywords:
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  - N
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  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
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  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 13b
name: Figure 13b
---
additional_resources:
- description: Image file
  location: SF_SRMed_log.png
- description: Thumbnail image file
  location: thumb_SF_SRMed_log.png
data_file: figure_13c.yaml
description: Observed and expected dilepton mass distributions in SRC-STR (top-left),
  SRLow-STR (top-right), SRMed-STR (bottom-left), and SRHigh-STR (bottom-right), with
  the binning used for interpretations after a separate simultaneous fit to each signal
  region and control region pair. The red dashed lines are example signal models overlaid
  on the figure. All statistical and systematic uncertainties are included in the
  hatched bands. The last bins are the overflow.
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
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  values:
  - '13000'
location: Data from Figure 13c
name: Figure 13c
---
additional_resources:
- description: Image file
  location: SF_SRHigh_log.png
- description: Thumbnail image file
  location: thumb_SF_SRHigh_log.png
data_file: figure_13d.yaml
description: Observed and expected dilepton mass distributions in SRC-STR (top-left),
  SRLow-STR (top-right), SRMed-STR (bottom-left), and SRHigh-STR (bottom-right), with
  the binning used for interpretations after a separate simultaneous fit to each signal
  region and control region pair. The red dashed lines are example signal models overlaid
  on the figure. All statistical and systematic uncertainties are included in the
  hatched bands. The last bins are the overflow.
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
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  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 13d
name: Figure 13d
---
additional_resources:
- description: Image file
  location: c1n2_Output_Contours_clear_2.png
- description: Thumbnail image file
  location: thumb_c1n2_Output_Contours_clear_2.png
data_file: figure_15a_c1n2_observed_limit.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
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  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
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location: Data from Figure 15a
name: Figure 15a C1N2 Observed Limit
---
additional_resources:
- description: Image file
  location: c1n2_Output_Contours_clear_2.png
- description: Thumbnail image file
  location: thumb_c1n2_Output_Contours_clear_2.png
data_file: figure_15a_c1n2_observed_limit_+1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
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location: Data from Figure 15a
name: Figure 15a C1N2 Observed Limit +1sigma
---
additional_resources:
- description: Image file
  location: c1n2_Output_Contours_clear_2.png
- description: Thumbnail image file
  location: thumb_c1n2_Output_Contours_clear_2.png
data_file: figure_15a_c1n2_observed_limit_-1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
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location: Data from Figure 15a
name: Figure 15a C1N2 Observed Limit -1sigma
---
additional_resources:
- description: Image file
  location: c1n2_Output_Contours_clear_2.png
- description: Thumbnail image file
  location: thumb_c1n2_Output_Contours_clear_2.png
data_file: figure_15a_c1n2_expected_limit.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
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- name: observables
  values:
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location: Data from Figure 15a
name: Figure 15a C1N2 Expected Limit
---
additional_resources:
- description: Image file
  location: c1n2_Output_Contours_clear_2.png
- description: Thumbnail image file
  location: thumb_c1n2_Output_Contours_clear_2.png
data_file: figure_15a_c1n2_expected_limit_+1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
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location: Data from Figure 15a
name: Figure 15a C1N2 Expected Limit +1sigma
---
additional_resources:
- description: Image file
  location: c1n2_Output_Contours_clear_2.png
- description: Thumbnail image file
  location: thumb_c1n2_Output_Contours_clear_2.png
data_file: figure_15a_c1n2_expected_limit_-1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
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- name: observables
  values:
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location: Data from Figure 15a
name: Figure 15a C1N2 Expected Limit -1sigma
---
additional_resources:
- description: Image file
  location: gmsb_Output_Contours_100max_clear.png
- description: Thumbnail image file
  location: thumb_gmsb_Output_Contours_100max_clear.png
data_file: figure_15b_gmsb_observed_limit.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
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  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
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location: Data from Figure 15b
name: Figure 15b GMSB Observed Limit
---
additional_resources:
- description: Image file
  location: gmsb_Output_Contours_100max_clear.png
- description: Thumbnail image file
  location: thumb_gmsb_Output_Contours_100max_clear.png
data_file: figure_15b_gmsb_observed_limit_+1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
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- name: observables
  values:
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location: Data from Figure 15b
name: Figure 15b GMSB Observed Limit +1sigma
---
additional_resources:
- description: Image file
  location: gmsb_Output_Contours_100max_clear.png
- description: Thumbnail image file
  location: thumb_gmsb_Output_Contours_100max_clear.png
data_file: figure_15b_gmsb_observed_limit_-1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
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- name: observables
  values:
  - CLs
location: Data from Figure 15b
name: Figure 15b GMSB Observed Limit -1sigma
---
additional_resources:
- description: Image file
  location: gmsb_Output_Contours_100max_clear.png
- description: Thumbnail image file
  location: thumb_gmsb_Output_Contours_100max_clear.png
data_file: figure_15b_gmsb_expected_limit.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - CLs
location: Data from Figure 15b
name: Figure 15b GMSB Expected Limit
---
additional_resources:
- description: Image file
  location: gmsb_Output_Contours_100max_clear.png
- description: Thumbnail image file
  location: thumb_gmsb_Output_Contours_100max_clear.png
data_file: figure_15b_gmsb_expected_limit_+1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
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- name: observables
  values:
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location: Data from Figure 15b
name: Figure 15b GMSB Expected Limit +1sigma
---
additional_resources:
- description: Image file
  location: gmsb_Output_Contours_100max_clear.png
- description: Thumbnail image file
  location: thumb_gmsb_Output_Contours_100max_clear.png
data_file: figure_15b_gmsb_expected_limit_-1sigma.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294].'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
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- name: observables
  values:
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location: Data from Figure 15b
name: Figure 15b GMSB Expected Limit -1sigma
---
additional_resources:
- description: Image file
  location: c1n2_Output_Contours_upper_limit_obs_2.png
- description: Thumbnail image file
  location: thumb_c1n2_Output_Contours_upper_limit_obs_2.png
data_file: auxiliary_figure_34a_c1n2_xs_upper_limit.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294]. The grey numbers
  indicate the observed 95\% CLs upper limit on the cross section.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
location: Data from Auxiliary Figure 34a
name: Auxiliary Figure 34a C1N2 XS Upper Limit
---
additional_resources:
- description: Image file
  location: gmsb_Output_Contours_100max_upper_limit_obs.png
- description: Thumbnail image file
  location: thumb_gmsb_Output_Contours_100max_upper_limit_obs.png
data_file: auxiliary_figure_34b_gmsb_xs_upper_limit.yaml
description: 'Expected and observed exclusion contours from the EWK analysis for the
  C1N2 model (left) and GMSB model (right). The dashed line indicates the expected
  limits at 95$\%$ CL and the surrounding band shows the $1\sigma$ variation of the
  expected limit as a consequence of the uncertainties on the background prediction
  and experimental uncertainties on the signal ($\pm1\sigma_\mathrm{exp}$). The red
  dotted lines surrounding the observed limit contours indicate the variation resulting
  from changing the signal cross-section within its uncertainty ($\pm1\sigma_\mathrm{theory}^\mathrm{SUSY}$).
  The gray shaded areas indicate observed limits on these models from the two lepton
  channels of Ref.~[arXiv: 1803.02762] and Ref.~[arXiv: 1403.5294]. The grey numbers
  indicate the observed 95$\%$ CLs upper limit on the cross section.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Figure 34b
name: Auxiliary Figure 34b GMSB XS Upper Limit
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_SLN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_SLN1comb.png
data_file: figure_16a_observed_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16a
name: Figure 16a Observed Limit
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_SLN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_SLN1comb.png
data_file: figure_16a_observed_limit_+1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16a
name: Figure 16a Observed Limit +1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_SLN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_SLN1comb.png
data_file: figure_16a_observed_limit_-1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16a
name: Figure 16a Observed Limit -1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_SLN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_SLN1comb.png
data_file: figure_16a_expected_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16a
name: Figure 16a Expected Limit
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_SLN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_SLN1comb.png
data_file: figure_16a_expected_limit_+1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16a
name: Figure 16a Expected Limit +1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_SLN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_SLN1comb.png
data_file: figure_16a_expected_limit_-1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16a
name: Figure 16a Expected Limit -1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_SLN1comb_UL.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_SLN1comb_UL.png
data_file: auxiliary_figure_23a_xs_upper_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23].The grey numbers\
  \ indicated the observed 95\\% CL upper limit on the cross section."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 23a
name: Auxiliary Figure 23a XS Upper Limit
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_ZN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_ZN1comb.png
data_file: figure_16b_observed_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16b
name: Figure 16b Observed Limit
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_ZN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_ZN1comb.png
data_file: figure_16b_observed_limit_+1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16b
name: Figure 16b Observed Limit +1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_ZN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_ZN1comb.png
data_file: figure_16b_observed_limit_-1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16b
name: Figure 16b Observed Limit -1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_ZN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_ZN1comb.png
data_file: figure_16b_expected_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16b
name: Figure 16b Expected Limit
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_ZN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_ZN1comb.png
data_file: figure_16b_expected_limit_+1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16b
name: Figure 16b Expected Limit +1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_ZN1comb.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_ZN1comb.png
data_file: figure_16b_expected_limit_-1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16b
name: Figure 16b Expected Limit -1sigma
---
additional_resources:
- description: Image file
  location: contourOverlay_GG_N2_ZN1comb_UL.png
- description: Thumbnail image file
  location: thumb_contourOverlay_GG_N2_ZN1comb_UL.png
data_file: auxiliary_figure_23b_xs_upper_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23].The grey numbers\
  \ indicated the observed 95\\% CL upper limit on the cross section."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 23b
name: Auxiliary Figure 23b XS Upper Limit
---
data_file: figure_16c_observed_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16c
name: Figure 16c Observed Limit
---
data_file: figure_16c_observed_limit_+1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16c
name: Figure 16c Observed Limit +1sigma
---
data_file: figure_16c_observed_limit_-1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16c
name: Figure 16c Observed Limit -1sigma
---
data_file: figure_16c_expected_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16c
name: Figure 16c Expected Limit
---
data_file: auxiliary_figure_23c_xs_upper_limit.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23].The grey numbers\
  \ indicated the observed 95\\% CL upper limit on the cross section."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Auxiliary Figure 23c
name: Auxiliary Figure 23c XS Upper Limit
---
data_file: figure_16c_expected_limit_+1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16c
name: Figure 16c Expected Limit +1sigma
---
data_file: figure_16c_expected_limit_-1sigma.yaml
description: "Expected and observed exclusion contours derived from the combination\
  \ of all of the Strong search SRs for the $\\tilde{g}$--$\\tilde{\\ell}$ (top-left),\
  \ $\\tilde{g}$--$Z$ (top-right), and $\\tilde{s}--Z$ (bottom) models. The dashed\
  \ line indicates the expected limits at 95\\% CL and the surrounding band shows\
  \ the $1\\sigma$ variation of the expected limit as a consequence of the uncertainties\
  \ in the background prediction and experimental uncertainties of the signal ($\\\
  pm1\\sigma_\\mathrm{exp}$). The red dotted lines surrounding the observed limit\
  \ contours indicate the variation resulting from changing the signal cross-section\
  \ within its uncertainty ($\\pm1\\sigma_\\mathrm{theory}^\\mathrm{SUSY}$). The grey-shaded\
  \ area indicates the observed limits on these models from Ref. [23]."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - CLs
- name: cmenergies
  values:
  - '13000'
location: Data from Figure 16c
name: Figure 16c Expected Limit -1sigma
---
additional_resources:
- description: Image file
  location: SF_SRLow_val_log.png
- description: Thumbnail image file
  location: thumb_SF_SRLow_val_log.png
data_file: auxiliary_figure_17a.yaml
description: "The combined $E_{\\mathrm{T}}^{\\mathrm{miss}}$ distribution of VRLow-STR\
  \ and SRLow-STR (left), and the same region with the $\\Delta\\phi(\\boldsymbol{j}_{1,2},\\\
  boldsymbol{\\mathit{p}}_{\text{T}}^{\text{miss}})<0.4$ requirement, used as a control\
  \ region to normalize the $Z/\\gamma^*+\\mathrm{jets}$ process (right).  Separate\
  \ fits for the SR and VR are performed, as for the results in the paper, and the\
  \ resulting distributions are merged. All statistical and systematic uncertainties\
  \ are included in the hatched bands. The last bins contain the overflow."
keywords:
- name: observables
  values:
  - Mll
  - N
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
location: Data from Auxiliary Figure 17a
name: Auxiliary Figure 17a
---
data_file: auxiliary_table_30-31_src-str_cutflow.yaml
description: "Cutflow of expected events in the four Strong search edge signal regions.\
  \  `Leptons' refers to electrons and muons only. The gluino-$Z^{(*)}$ model with\
  \ $m_{\tilde{g}}=800~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRC-STR\
  \ with 60000 Monte Carlo (MC) events generated. The slepton-$Z^{(*)}$ model with\
  \ $m_{\tilde{\\ell}}=1200~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRMed-STR\
  \ with 30000 (MC) events generated.  The gluino-slepton model with $m_{\tilde{g}}=2~TeV$\
  \ and $m_{\tilde{\\ell}}=1.3~TeV$ is used for SRLow-STR and SRHigh-STR with 30000\
  \ MC events generated. The Generator Filter requires two 5~GeV leptons and 100~GeV\
  \ of \\met. The SUSY2 kernel requires at least two leptons with $p_{\\mathrm{T}}>9~GeV$\
  \ or at least one lepton with $p_{\\mathrm{T}}>25~GeV$ and a photon with  $p_{\\\
  mathrm{T}}>40~GeV$, with all objects within $|\\eta|=2.6$."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: observables
  values:
  - N
location: Data from Auxiliary Table 30-31
name: Auxiliary Table 30-31 SRC-STR Cutflow
---
data_file: auxiliary_table_30-31_srmed-str_cutflow.yaml
description: "Cutflow of expected events in the four Strong search edge signal regions.\
  \  `Leptons' refers to electrons and muons only. The gluino-$Z^{(*)}$ model with\
  \ $m_{\tilde{g}}=800~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRC-STR\
  \ with 60000 Monte Carlo (MC) events generated. The slepton-$Z^{(*)}$ model with\
  \ $m_{\tilde{\\ell}}=1200~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRMed-STR\
  \ with 30000 (MC) events generated.  The gluino-slepton model with $m_{\tilde{g}}=2~TeV$\
  \ and $m_{\tilde{\\ell}}=1.3~TeV$ is used for SRLow-STR and SRHigh-STR with 30000\
  \ MC events generated. The Generator Filter requires two 5~GeV leptons and 100~GeV\
  \ of \\met. The SUSY2 kernel requires at least two leptons with $p_{\\mathrm{T}}>9~GeV$\
  \ or at least one lepton with $p_{\\mathrm{T}}>25~GeV$ and a photon with  $p_{\\\
  mathrm{T}}>40~GeV$, with all objects within $|\\eta|=2.6$."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: observables
  values:
  - N
location: Data from Auxiliary Table 30-31
name: Auxiliary Table 30-31 SRMed-STR Cutflow
---
data_file: auxiliary_table_30-31_srlow-str_cutflow.yaml
description: "Cutflow of expected events in the four Strong search edge signal regions.\
  \  `Leptons' refers to electrons and muons only. The gluino-$Z^{(*)}$ model with\
  \ $m_{\tilde{g}}=800~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRC-STR\
  \ with 60000 Monte Carlo (MC) events generated. The slepton-$Z^{(*)}$ model with\
  \ $m_{\tilde{\\ell}}=1200~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRMed-STR\
  \ with 30000 (MC) events generated.  The gluino-slepton model with $m_{\tilde{g}}=2~TeV$\
  \ and $m_{\tilde{\\ell}}=1.3~TeV$ is used for SRLow-STR and SRHigh-STR with 30000\
  \ MC events generated. The Generator Filter requires two 5~GeV leptons and 100~GeV\
  \ of \\met. The SUSY2 kernel requires at least two leptons with $p_{\\mathrm{T}}>9~GeV$\
  \ or at least one lepton with $p_{\\mathrm{T}}>25~GeV$ and a photon with  $p_{\\\
  mathrm{T}}>40~GeV$, with all objects within $|\\eta|=2.6$."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: observables
  values:
  - N
location: Data from Auxiliary Table 30-31
name: Auxiliary Table 30-31 SRLow-STR Cutflow
---
data_file: auxiliary_table_30-31_srhigh-str_cutflow.yaml
description: "Cutflow of expected events in the four Strong search edge signal regions.\
  \  `Leptons' refers to electrons and muons only. The gluino-$Z^{(*)}$ model with\
  \ $m_{\tilde{g}}=800~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRC-STR\
  \ with 60000 Monte Carlo (MC) events generated. The slepton-$Z^{(*)}$ model with\
  \ $m_{\tilde{\\ell}}=1200~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for SRMed-STR\
  \ with 30000 (MC) events generated.  The gluino-slepton model with $m_{\tilde{g}}=2~TeV$\
  \ and $m_{\tilde{\\ell}}=1.3~TeV$ is used for SRLow-STR and SRHigh-STR with 30000\
  \ MC events generated. The Generator Filter requires two 5~GeV leptons and 100~GeV\
  \ of \\met. The SUSY2 kernel requires at least two leptons with $p_{\\mathrm{T}}>9~GeV$\
  \ or at least one lepton with $p_{\\mathrm{T}}>25~GeV$ and a photon with  $p_{\\\
  mathrm{T}}>40~GeV$, with all objects within $|\\eta|=2.6$."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: observables
  values:
  - N
location: Data from Auxiliary Table 30-31
name: Auxiliary Table 30-31 SRHigh-STR Cutflow
---
data_file: auxiliary_table_30-31_srzlow-str_cutflow.yaml
description: "Cutflow of expected events in the three Strong search on-$Z$ signal\
  \ regions. The cutflow up to the signal region specific requirements is the same\
  \ as in the Strong search edge cutflow. The slepton-$Z^{(*)}$ model with $m_{\t\
  ilde{\\ell}}=1200~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for all of the\
  \ on-$Z$ signal regions with 30000 (MC) events generated."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: observables
  values:
  - N
location: Data from Auxiliary Table 30-31
name: Auxiliary Table 30-31 SRZLow-STR Cutflow
---
data_file: auxiliary_table_30-31_srzmed-str_cutflow.yaml
description: "Cutflow of expected events in the three Strong search on-$Z$ signal\
  \ regions. The cutflow up to the signal region specific requirements is the same\
  \ as in the Strong search edge cutflow. The slepton-$Z^{(*)}$ model with $m_{\t\
  ilde{\\ell}}=1200~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for all of the\
  \ on-$Z$ signal regions with 30000 (MC) events generated."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: observables
  values:
  - N
location: Data from Auxiliary Table 30-31
name: Auxiliary Table 30-31 SRZMed-STR Cutflow
---
data_file: auxiliary_table_30-31_srzhigh-str_cutflow.yaml
description: "Cutflow of expected events in the three Strong search on-$Z$ signal\
  \ regions. The cutflow up to the signal region specific requirements is the same\
  \ as in the Strong search edge cutflow. The slepton-$Z^{(*)}$ model with $m_{\t\
  ilde{\\ell}}=1200~GeV$ and $m_{\tilde{\\chi}_1^0}=700~GeV$ is used for all of the\
  \ on-$Z$ signal regions with 30000 (MC) events generated."
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
  - p-p > squark-squark > Z-Z > ll+MET+jets
- name: observables
  values:
  - N
location: Data from Auxiliary Table 30-31
name: Auxiliary Table 30-31 SRZHigh-STR Cutflow
---
data_file: auxiliary_table_36_sr-offshell_a-ewk_cutflow.yaml
description: 'Table 36: Cutflow of expected events in the region SR-OffShell_a-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 36
name: Auxiliary Table 36 SR-OffShell_a-EWK Cutflow
---
data_file: auxiliary_table_36_sr-offshell_a-ewk_generated.yaml
description: 'Table 36: Cutflow of expected events in the region SR-OffShell_a-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 36
name: Auxiliary Table 36 SR-OffShell_a-EWK Generated
---
data_file: auxiliary_table_37_sr-offshell_b-ewk_cutflow.yaml
description: 'Table 37: Cutflow of expected events in the region SR-OffShell_b-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 37
name: Auxiliary Table 37 SR-OffShell_b-EWK Cutflow
---
data_file: auxiliary_table_37_sr-offshell_b-ewk_generated.yaml
description: 'Table 37: Cutflow of expected events in the region SR-OffShell_b-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 37
name: Auxiliary Table 37 SR-OffShell_b-EWK Generated
---
data_file: auxiliary_table_38_sr-low_a-ewk_cutflow.yaml
description: 'Table 38: Cutflow of expected events in the region SR-Low_a-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 38
name: Auxiliary Table 38 SR-Low_a-EWK Cutflow
---
data_file: auxiliary_table_38_sr-low_a-ewk_generated.yaml
description: 'Table 38: Cutflow of expected events in the region SR-Low_a-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 38
name: Auxiliary Table 38 SR-Low_a-EWK Generated
---
data_file: auxiliary_table_39_sr-low_b-ewk_cutflow.yaml
description: 'Table 39: Cutflow of expected events in the region SR-Low_b-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 39
name: Auxiliary Table 39 SR-Low_b-EWK Cutflow
---
data_file: auxiliary_table_39_sr-low_b-ewk_generated.yaml
description: 'Table 39: Cutflow of expected events in the region SR-Low_b-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 39
name: Auxiliary Table 39 SR-Low_b-EWK Generated
---
data_file: auxiliary_table_40_sr-low-2-ewk_cutflow.yaml
description: 'Table 40: Cutflow of expected events in the region SR-Low-2-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 40
name: Auxiliary Table 40 SR-Low-2-EWK Cutflow
---
data_file: auxiliary_table_40_sr-low-2-ewk_generated.yaml
description: 'Table 40: Cutflow of expected events in the region SR-Low-2-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 40
name: Auxiliary Table 40 SR-Low-2-EWK Generated
---
data_file: auxiliary_table_41_sr-int_a-ewk_cutflow.yaml
description: 'Table 41: Cutflow of expected events in the region SR-Int_a-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 41
name: Auxiliary Table 41 SR-Int_a-EWK Cutflow
---
data_file: auxiliary_table_41_sr-int_a-ewk_generated.yaml
description: 'Table 41: Cutflow of expected events in the region SR-Int_a-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 41
name: Auxiliary Table 41 SR-Int_a-EWK Generated
---
data_file: auxiliary_table_42_sr-int_b-ewk_cutflow.yaml
description: 'Table 42: Cutflow of expected events in the region SR-Int_b-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 42
name: Auxiliary Table 42 SR-Int_b-EWK Cutflow
---
data_file: auxiliary_table_42_sr-int_b-ewk_generated.yaml
description: 'Table 42: Cutflow of expected events in the region SR-Int_b-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 42
name: Auxiliary Table 42 SR-Int_b-EWK Generated
---
data_file: auxiliary_table_43_sr-high_16a-ewk_cutflow.yaml
description: 'Table 43: Cutflow of expected events in the region SR-High_16a-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 43
name: Auxiliary Table 43 SR-High_16a-EWK Cutflow
---
data_file: auxiliary_table_43_sr-high_16a-ewk_generated.yaml
description: 'Table 43: Cutflow of expected events in the region SR-High_16a-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 43
name: Auxiliary Table 43 SR-High_16a-EWK Generated
---
data_file: auxiliary_table_44_sr-high_16b-ewk_cutflow.yaml
description: 'Table 44: Cutflow of expected events in the region SR-High_16b-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 44
name: Auxiliary Table 44 SR-High_16b-EWK Cutflow
---
data_file: auxiliary_table_44_sr-high_16b-ewk_generated.yaml
description: 'Table 44: Cutflow of expected events in the region SR-High_16b-EWK.
  Requirements below the line are specific to this region. On the Generator Filter
  line, the total number of unweighted events simulated is given in brackets. `Leptons''
  refers to electrons and muons only. For C1N2 models, the Generator Filter requires
  at least two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below
  the Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 44
name: Auxiliary Table 44 SR-High_16b-EWK Generated
---
data_file: auxiliary_table_45_sr-high_8a-ewk_cutflow.yaml
description: 'Table 45: Cutflow of expected events in the region SR-High_8a-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 45
name: Auxiliary Table 45 SR-High_8a-EWK Cutflow
---
data_file: auxiliary_table_45_sr-high_8a-ewk_generated.yaml
description: 'Table 45: Cutflow of expected events in the region SR-High_8a-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 45
name: Auxiliary Table 45 SR-High_8a-EWK Generated
---
data_file: auxiliary_table_46_sr-high_8b-ewk_cutflow.yaml
description: 'Table 46: Cutflow of expected events in the region SR-High_8b-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 46
name: Auxiliary Table 46 SR-High_8b-EWK Cutflow
---
data_file: auxiliary_table_46_sr-high_8b-ewk_generated.yaml
description: 'Table 46: Cutflow of expected events in the region SR-High_8b-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 46
name: Auxiliary Table 46 SR-High_8b-EWK Generated
---
data_file: auxiliary_table_47_sr-1j-high-ewk_cutflow.yaml
description: 'Table 47: Cutflow of expected events in the region SR-1J-High-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 47
name: Auxiliary Table 47 SR-1J-High-EWK Cutflow
---
data_file: auxiliary_table_47_sr-1j-high-ewk_generated.yaml
description: 'Table 47: Cutflow of expected events in the region SR-1J-High-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 47
name: Auxiliary Table 47 SR-1J-High-EWK Generated
---
data_file: auxiliary_table_48_sr-llbb-ewk_cutflow.yaml
description: 'Table 48: Cutflow of expected events in the region SR-llbb-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 48
name: Auxiliary Table 48 SR-llbb-EWK Cutflow
---
data_file: auxiliary_table_48_sr-llbb-ewk_generated.yaml
description: 'Table 48: Cutflow of expected events in the region SR-llbb-EWK. Requirements
  below the line are specific to this region. On the Generator Filter line, the total
  number of unweighted events simulated is given in brackets. `Leptons'' refers to
  electrons and muons only. For C1N2 models, the Generator Filter requires at least
  two $7~\mathrm{GeV}$ leptons and for C1N2 models with mass splittings below the
  Z boson mass it also requires $75~\mathrm{GeV}$ of $E_{\mathrm{T}}^{\mathrm{miss}}$.
  For GMSB models, the Generator Filter requires at least two $3~\mathrm{GeV}$ leptons.
  For on-shell C1N2 models, the `Forced Decays'' require each Z boson to decay to
  a charged lepton pair (electron, muon, or tau) and each W boson to decay hadronically.
  For off-shell C1N2 models, each neutralino is forced to produce a charged lepton
  pair in its decay, and each chargino can produce any fermion pair. The SUSY2 kernel
  requires at least two leptons with $p_{\mathrm{T}}>9~\mathrm{GeV}$  or at least
  one lepton with $p_{\mathrm{T}}>25~\mathrm{GeV}$ and a photon with  $p_{\mathrm{T}}>40~\mathrm{GeV}$,
  with all objects within $|\eta|=2.6$.'
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
location: Data from Auxiliary Table 48
name: Auxiliary Table 48 SR-llbb-EWK Generated
---
additional_resources:
- description: Image file
  location: CR_Z_EWKSR_Low_EWK_mjj.png
- description: Thumbnail image file
  location: thumb_CR_Z_EWKSR_Low_EWK_mjj.png
data_file: auxiliary_figure_33a_mjj_in_cr-z-ewk_and_sr-low-ewk.yaml
description: The combined $m_{jj}$ distribution of CR-Z-EWK and SR-Low-EWK (left),
  and the $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ distribution in CR-Z-met-EWK
  (right), which removes the upper limit of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})
  < 9$ from the definition of CR-Z-EWK. This $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  tail overlaps other control and validation regions, but not signal regions. The
  arrows indicate the signal region SR-Low-EWK (left), and the $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  phase space which is not included in CR-Z-EWK (right). All EWK search control and
  signal regions are included in the fit. All statistical and systematic uncertainties
  are included in the hatched bands. The theoretical uncertainties from CR-Z-EWK are
  applied to CR-Z-met-EWK. The last bins contain the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - Mjj
location: Data from Auxiliary Figure 33a
name: Auxiliary Figure 33a Mjj in CR-Z-EWK and SR-Low-EWK
---
additional_resources:
- description: Image file
  location: CR_Z_met_EWK_met_Sign.png
- description: Thumbnail image file
  location: thumb_CR_Z_met_EWK_met_Sign.png
data_file: auxiliary_figure_33b_s_etmiss_in_cr-z-met-ewk.yaml
description: The combined $m_{jj}$ distribution of CR-Z-EWK and SR-Low-EWK (left),
  and the $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$ distribution in CR-Z-met-EWK
  (right), which removes the upper limit of $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})
  < 9$ from the definition of CR-Z-EWK. This $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  tail overlaps other control and validation regions, but not signal regions. The
  arrows indicate the signal region SR-Low-EWK (left), and the $\mathcal{S}(E_{\mathrm{T}}^{\mathrm{miss}})$
  phase space which is not included in CR-Z-EWK (right). All EWK search control and
  signal regions are included in the fit. All statistical and systematic uncertainties
  are included in the hatched bands. The theoretical uncertainties from CR-Z-EWK are
  applied to CR-Z-met-EWK. The last bins contain the overflow.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: observables
  values:
  - N
  - SETmiss
location: Data from Auxiliary Figure 33b
name: Auxiliary Figure 33b S_ETmiss in CR-Z-met-EWK
### END EWK START STRONG
#### Start eff/acc plots
---
additional_resources:
- description: Image file
  location: GMSB_SR_OffShell_a_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_OffShell_a_acc.png
data_file: gmsb_acc_in_sr-offshell_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 25
name: GMSB acc in SR-OffShell_a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_OffShell_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_OffShell_a_eff_nonoise.png
data_file: gmsb_eff_in_sr-offshell_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 25
name: GMSB eff in SR-OffShell_a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_OffShell_b_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_OffShell_b_acc.png
data_file: gmsb_acc_in_sr-offshell_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 25
name: GMSB acc in SR-OffShell_b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_OffShell_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_OffShell_b_eff_nonoise.png
data_file: gmsb_eff_in_sr-offshell_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 25
name: GMSB eff in SR-OffShell_b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Low_a_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Low_a_acc.png
data_file: gmsb_acc_in_sr-low_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 25
name: GMSB acc in SR-Low_a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Low_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Low_a_eff_nonoise.png
data_file: gmsb_eff_in_sr-low_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 25
name: GMSB eff in SR-Low_a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Low_b_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Low_b_acc.png
data_file: gmsb_acc_in_sr-low_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 25
name: GMSB acc in SR-Low_b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Low_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Low_b_eff_nonoise.png
data_file: gmsb_eff_in_sr-low_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 25
name: GMSB eff in SR-Low_b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Low_2_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Low_2_acc.png
data_file: gmsb_acc_in_sr-low-2-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 26
name: GMSB acc in SR-Low-2-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Low_2_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Low_2_eff_nonoise.png
data_file: gmsb_eff_in_sr-low-2-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 26
name: GMSB eff in SR-Low-2-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Int_a_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Int_a_acc.png
data_file: gmsb_acc_in_sr-int_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 26
name: GMSB acc in SR-Int_a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Int_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Int_a_eff_nonoise.png
data_file: gmsb_eff_in_sr-int_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 26
name: GMSB eff in SR-Int_a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Int_b_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Int_b_acc.png
data_file: gmsb_acc_in_sr-int_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 26
name: GMSB acc in SR-Int_b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_Int_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_Int_b_eff_nonoise.png
data_file: gmsb_eff_in_sr-int_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 26
name: GMSB eff in SR-Int_b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_16_a_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_16_a_acc.png
data_file: gmsb_acc_in_sr-high_16a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 27
name: GMSB acc in SR-High_16a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_16_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_16_a_eff_nonoise.png
data_file: gmsb_eff_in_sr-high_16a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 27
name: GMSB eff in SR-High_16a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_16_b_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_16_b_acc.png
data_file: gmsb_acc_in_sr-high_16b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 27
name: GMSB acc in SR-High_16b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_16_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_16_b_eff_nonoise.png
data_file: gmsb_eff_in_sr-high_16b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 27
name: GMSB eff in SR-High_16b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_8_a_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_8_a_acc.png
data_file: gmsb_acc_in_sr-high_8a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 27
name: GMSB acc in SR-High_8a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_8_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_8_a_eff_nonoise.png
data_file: gmsb_eff_in_sr-high_8a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 27
name: GMSB eff in SR-High_8a-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_8_b_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_8_b_acc.png
data_file: gmsb_acc_in_sr-high_8b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 27
name: GMSB acc in SR-High_8b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_8_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_8_b_eff_nonoise.png
data_file: gmsb_eff_in_sr-high_8b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 27
name: GMSB eff in SR-High_8b-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_4_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_4_acc.png
data_file: gmsb_acc_in_sr-1j-high-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 28
name: GMSB acc in SR-1J-High-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_High_4_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_High_4_eff_nonoise.png
data_file: gmsb_eff_in_sr-1j-high-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 28
name: GMSB eff in SR-1J-High-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_llbb_acc.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_llbb_acc.png
data_file: gmsb_acc_in_sr-llbb-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 28
name: GMSB acc in SR-llbb-EWK
---
additional_resources:
- description: Image file
  location: GMSB_SR_llbb_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_GMSB_SR_llbb_eff_nonoise.png
data_file: gmsb_eff_in_sr-llbb-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the GMSB model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Neutralino Neutralino -> h/Z G h/Z G
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 28
name: GMSB eff in SR-llbb-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_OffShell_a_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_OffShell_a_acc.png
data_file: c1n2_acc_in_sr-offshell_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 29
name: C1N2 acc in SR-OffShell_a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_OffShell_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_OffShell_a_eff_nonoise.png
data_file: c1n2_eff_in_sr-offshell_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 29
name: C1N2 eff in SR-OffShell_a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_OffShell_b_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_OffShell_b_acc.png
data_file: c1n2_acc_in_sr-offshell_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 29
name: C1N2 acc in SR-OffShell_b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_OffShell_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_OffShell_b_eff_nonoise.png
data_file: c1n2_eff_in_sr-offshell_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 29
name: C1N2 eff in SR-OffShell_b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Low_a_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Low_a_acc.png
data_file: c1n2_acc_in_sr-low_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 29
name: C1N2 acc in SR-Low_a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Low_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Low_a_eff_nonoise.png
data_file: c1n2_eff_in_sr-low_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 29
name: C1N2 eff in SR-Low_a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Low_b_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Low_b_acc.png
data_file: c1n2_acc_in_sr-low_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 29
name: C1N2 acc in SR-Low_b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Low_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Low_b_eff_nonoise.png
data_file: c1n2_eff_in_sr-low_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-OffShell-EWK and SR-Low-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 29
name: C1N2 eff in SR-Low_b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Low_2_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Low_2_acc.png
data_file: c1n2_acc_in_sr-low-2-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 30
name: C1N2 acc in SR-Low-2-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Low_2_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Low_2_eff_nonoise.png
data_file: c1n2_eff_in_sr-low-2-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 30
name: C1N2 eff in SR-Low-2-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Int_a_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Int_a_acc.png
data_file: c1n2_acc_in_sr-int_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 30
name: C1N2 acc in SR-Int_a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Int_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Int_a_eff_nonoise.png
data_file: c1n2_eff_in_sr-int_a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 30
name: C1N2 eff in SR-Int_a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Int_b_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Int_b_acc.png
data_file: c1n2_acc_in_sr-int_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 30
name: C1N2 acc in SR-Int_b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_Int_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_Int_b_eff_nonoise.png
data_file: c1n2_eff_in_sr-int_b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-Low-2-EWK and SR-Int-EWK. Acceptance is calculated by applying
  the signal-region requirements to particle-level objects, which do not suffer from
  identification inefficiencies or mismeasurements. For models with mass splittings
  below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 30
name: C1N2 eff in SR-Int_b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_16_a_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_16_a_acc.png
data_file: c1n2_acc_in_sr-high_16a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 31
name: C1N2 acc in SR-High_16a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_16_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_16_a_eff_nonoise.png
data_file: c1n2_eff_in_sr-high_16a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 31
name: C1N2 eff in SR-High_16a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_16_b_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_16_b_acc.png
data_file: c1n2_acc_in_sr-high_16b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 31
name: C1N2 acc in SR-High_16b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_16_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_16_b_eff_nonoise.png
data_file: c1n2_eff_in_sr-high_16b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 31
name: C1N2 eff in SR-High_16b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_8_a_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_8_a_acc.png
data_file: c1n2_acc_in_sr-high_8a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 31
name: C1N2 acc in SR-High_8a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_8_a_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_8_a_eff_nonoise.png
data_file: c1n2_eff_in_sr-high_8a-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 31
name: C1N2 eff in SR-High_8a-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_8_b_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_8_b_acc.png
data_file: c1n2_acc_in_sr-high_8b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 31
name: C1N2 acc in SR-High_8b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_8_b_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_8_b_eff_nonoise.png
data_file: c1n2_eff_in_sr-high_8b-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-High-EWK. Acceptance is calculated by applying the signal-region
  requirements to particle-level objects, which do not suffer from identification
  inefficiencies or mismeasurements. For models with mass splittings below the Z boson
  mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}} > 75~\mathrm{GeV}$.
  The efficiency is calculated with fully reconstructed objects with the acceptance
  divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 31
name: C1N2 eff in SR-High_8b-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_4_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_4_acc.png
data_file: c1n2_acc_in_sr-1j-high-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 32
name: C1N2 acc in SR-1J-High-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_High_4_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_High_4_eff_nonoise.png
data_file: c1n2_eff_in_sr-1j-high-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 32
name: C1N2 eff in SR-1J-High-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_llbb_acc.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_llbb_acc.png
data_file: c1n2_acc_in_sr-llbb-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Acc
location: Data from Auxiliary Figure 32
name: C1N2 acc in SR-llbb-EWK
---
additional_resources:
- description: Image file
  location: C1N2_SR_llbb_eff_nonoise.png
- description: Thumbnail image file
  location: thumb_C1N2_SR_llbb_eff_nonoise.png
data_file: c1n2_eff_in_sr-llbb-ewk.yaml
description: Signal region acceptance (left) and efficiency (right) for the C1N2 model
  in the regions SR-1J-High-EWK and SR-$\ell\ell bb$-EWK. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements. For models with mass
  splittings below the Z boson mass, this filter also requires $E_{\mathrm{T}}^{\mathrm{miss}}
  > 75~\mathrm{GeV}$. The efficiency is calculated with fully reconstructed objects
  with the acceptance divided out.
keywords:
- name: cmenergies
  values:
  - 13000
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
- name: reactions
  values:
  - p - p -> Chargino Neutralino -> W Z -> q q l+ l-
- name: observables
  values:
  - Eff
location: Data from Auxiliary Figure 32
name: C1N2 eff in SR-llbb-EWK
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRC_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRC_acc.png
data_file: gg_n2_sln1_acc_in_src.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 acc in SRC
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRC_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRC_eff.png
data_file: gg_n2_sln1_eff_in_src.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 eff in SRC
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRC_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRC_acc.png
data_file: gg_n2_zn1_acc_in_src.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 acc in SRC
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRC_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRC_eff.png
data_file: gg_n2_zn1_eff_in_src.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 eff in SRC
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRC_acc.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRC_acc.png
data_file: ss_n2_zn1_acc_in_src.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Squark
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 acc in SRC
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRC_eff.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRC_eff.png
data_file: ss_n2_zn1_eff_in_src.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Squark
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 eff in SRC
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRLow_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRLow_acc.png
data_file: gg_n2_sln1_acc_in_srlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 acc in SRLow
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRLow_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRLow_eff.png
data_file: gg_n2_sln1_eff_in_srlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 eff in SRLow
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRLow_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRLow_acc.png
data_file: gg_n2_zn1_acc_in_srlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 acc in SRLow
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRLow_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRLow_eff.png
data_file: gg_n2_zn1_eff_in_srlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
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- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 eff in SRLow
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRLow_acc.png
- description: Thumbnail image file
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data_file: ss_n2_zn1_acc_in_srlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
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  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Squark
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 acc in SRLow
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRLow_eff.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRLow_eff.png
data_file: ss_n2_zn1_eff_in_srlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Squark
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 eff in SRLow
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRMed_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRMed_acc.png
data_file: gg_n2_sln1_acc_in_srmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 acc in SRMed
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRMed_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRMed_eff.png
data_file: gg_n2_sln1_eff_in_srmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 eff in SRMed
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRMed_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRMed_acc.png
data_file: gg_n2_zn1_acc_in_srmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 acc in SRMed
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRMed_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRMed_eff.png
data_file: gg_n2_zn1_eff_in_srmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 eff in SRMed
---
additional_resources:
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  location: SS_N2_ZN1_SRMed_acc.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRMed_acc.png
data_file: ss_n2_zn1_acc_in_srmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Squark
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 acc in SRMed
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRMed_eff.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRMed_eff.png
data_file: ss_n2_zn1_eff_in_srmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Squark
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 eff in SRMed
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRHigh_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRHigh_acc.png
data_file: gg_n2_sln1_acc_in_srhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 acc in SRHigh
---
additional_resources:
- description: Image file
  location: GG_N2_SLN1_SRHigh_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_SLN1_SRHigh_eff.png
data_file: gg_n2_sln1_eff_in_srhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_SLN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > slepton-slepton > ll+MET+jets
location: Data from Auxiliary Figure 18
name: GG_N2_SLN1 eff in SRHigh
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRHigh_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRHigh_acc.png
data_file: gg_n2_zn1_acc_in_srhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 acc in SRHigh
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRHigh_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRHigh_eff.png
data_file: gg_n2_zn1_eff_in_srhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 19
name: GG_N2_ZN1 eff in SRHigh
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRHigh_acc.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRHigh_acc.png
data_file: ss_n2_zn1_acc_in_srhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Squark
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 acc in SRHigh
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRHigh_eff.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRHigh_eff.png
data_file: ss_n2_zn1_eff_in_srhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Squark
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 21
name: SS_N2_ZN1 eff in SRHigh
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRZLow_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRZLow_acc.png
data_file: gg_n2_zn1_acc_in_srzlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 20
name: GG_N2_ZN1 acc in SRZLow
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRZLow_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRZLow_eff.png
data_file: gg_n2_zn1_eff_in_srzlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 20
name: GG_N2_ZN1 eff in SRZLow
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRZLow_acc.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRZLow_acc.png
data_file: ss_n2_zn1_acc_in_srzlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Squark
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 22
name: SS_N2_ZN1 acc in SRZLow
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRZLow_eff.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRZLow_eff.png
data_file: ss_n2_zn1_eff_in_srzlow.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Squark
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 22
name: SS_N2_ZN1 eff in SRZLow
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRZMed_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRZMed_acc.png
data_file: gg_n2_zn1_acc_in_srzmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 20
name: GG_N2_ZN1 acc in SRZMed
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRZMed_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRZMed_eff.png
data_file: gg_n2_zn1_eff_in_srzmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 20
name: GG_N2_ZN1 eff in SRZMed
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRZMed_acc.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRZMed_acc.png
data_file: ss_n2_zn1_acc_in_srzmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Squark
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 22
name: SS_N2_ZN1 acc in SRZMed
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRZMed_eff.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRZMed_eff.png
data_file: ss_n2_zn1_eff_in_srzmed.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Squark
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 22
name: SS_N2_ZN1 eff in SRZMed
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRZHigh_acc.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRZHigh_acc.png
data_file: gg_n2_zn1_acc_in_srzhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Gluino
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 20
name: GG_N2_ZN1 acc in SRZHigh
---
additional_resources:
- description: Image file
  location: GG_N2_ZN1_SRZHigh_eff.png
- description: Thumbnail image file
  location: thumb_GG_N2_ZN1_SRZHigh_eff.png
data_file: gg_n2_zn1_eff_in_srzhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the GG_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Gluino
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > gluino-gluino > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 20
name: GG_N2_ZN1 eff in SRZHigh
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRZHigh_acc.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRZHigh_acc.png
data_file: ss_n2_zn1_acc_in_srzhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Acceptance
  - Squark
- name: observables
  values:
  - Acceptance
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 22
name: SS_N2_ZN1 acc in SRZHigh
---
additional_resources:
- description: Image file
  location: SS_N2_ZN1_SRZHigh_eff.png
- description: Thumbnail image file
  location: thumb_SS_N2_ZN1_SRZHigh_eff.png
data_file: ss_n2_zn1_eff_in_srzhigh.yaml
description: Signal region acceptance (left) and efficiency (right) over the full
  \mll\ range for the SS_N2_ZN1 model in Strong search regions. Acceptance is calculated
  by applying the signal-region requirements to particle-level objects, which do not
  suffer from identification inefficiencies or mismeasurements.  The efficiency is
  calculated with fully reconstructed objects with the acceptance divided out.
keywords:
- name: phrases
  values:
  - SUSY
  - Supersymmetry
  - proton-proton scattering
  - Efficiency
  - Squark
- name: observables
  values:
  - Efficiency
- name: cmenergies
  values:
  - '13000'
- name: reactions
  values:
  - p-p > squark-squark > Z-Z > ll+MET+jets
location: Data from Auxiliary Figure 22
name: SS_N2_ZN1 eff in SRZHigh
