WARNING: VERY EARLY VERSION!!
This code compares the H -> WW -> lvlv variables distributions with the pp -> HXX -> WWXX -> lvlvXX variables distributions.
To get the code and setup ROOT type:
git clone git@github.com:NTrevisani/DarkMatter.git
cd DarkMatter
source setup_slc6.sh
The samples are stored on lxplus:
H->WW: /afs/cern.ch/user/n/ntrevisa/public/latinoHWW
HXX->WWXX: /afs/cern.ch/user/d/dburns/public/HWWSignalMC/
To exploit the HXX sample variables to build a latino-like tree, and ease the comparison:
c++ -O2 -lm `root-config --cflags --glibs` -o latinoDM latinoDM.cpp
./latinoDM
To apply selection cuts at the latino's H->WW samples, and do a proper comparison with the Dark Matter sample:
c++ -O2 -lm `root-config --cflags --glibs` -o latinoSelections latinoSelections.cpp
./latinoSelections
To plot the distributions of the variables in the two cases (SM and Dark Matter), on the same canvas, at 8TeV and 13TeV:
root -l -b 'macro.C(8)'
root -l -b 'macro.C(13)'