Login

VBF Analysis Group Meeting

→ Europe/Brussels
G/0-G.0.46 - Z Room (Building G)

G/0-G.0.46 - Z Room

Building G

20
Description

Zoom room

    • 1
      Round table
      Speakers: Andrea Malara, Chaochen Yuan (ULB), Hugues EVARD (ULB), Longsheng Tan (Université libre de Bruxelles), Muhammad Aamir Shahzad (ULB, Bruxelles)
      25_06_11_status_report.pdf
      progress_6_16.pdf

      Longshen 

      • Limits
        - What integrated luminosity did you assume?
        - Run without any systematic uncertainty and verify that the limit indeed changes by sqrt(10) when scaling the integrated lumi x10 or /10. 
        - Perform the same check (integrated lumi x10 or /10) with JECs uncty applied). How is the limit affected?
      • VBF
        - clarify what the VBF selection is. 

       

      Andrea

      - Update the plots after removing duplicate events from the JetHT dataset. 
      - Make a table of all systematics that are already Run 3 and the ones that are missing. 
      - Add table of yields in signal region. (similar to https://cms-results.web.cern.ch/cms-results/public-results/publications/HIG-20-003/CMS-HIG-20-003_Table_0A8.pdf ) 

       

       Laurent:

      • contact IC to understand their plans before the talk at Higgs rare

       

      Chaochen

      • Make the training using signal: ggH+VBF H, and background: EWK+strong Z and W (=4 backgrounds). should consider in the future to have 4 outputs instead of 2: EWK V, strong V, ggH, VBF H.

       

      Aamir

      • EGM SF: maybe try to fit a smaller (100/1000 x smaller) dataset? Maybe try to adapt the number of bins in the M(ee) distribution: instead of 1 bin/GeV, use 5 bins/GeV? 
Powered by Indico v3.3.8