This repository is ready for CMSSW. Also, the shell scripts stored in subrepository/bin folder inform you how to use the exeutables compiled in this repository.
# note that this code is no more support CMSSW9 now.
# if you want to use ROOT 6.22 (for RDataFrame and RDF::Node). it is recommended to use CMSSW12
# CMSSW version follows Higgs Combine releases.
export USER_CXXFLAGS="-Wno-error=unused-variable -Wno-error=unused-but-set-variable -DEDM_ML_DEBUG -g"
cmsrel CMSSW_11_3_4
cd CMSSW_11_3_4/src
git clone https://github.com/ltsai323/xPhoton.git -b main || exit
git clone https://github.com/youyingli/ShowerShapeCorrection.git || exit
scram b -j8 || (echo -e '\n\n compile failed in xPhoton\n\n '; exit)
git clone https://github.com/cms-analysis/HiggsAnalysis-CombinedLimit.git HiggsAnalysis/CombinedLimit -b v9.0.0 || exit
scram b -j8 || (echo -e '\n\n compile failed in Higgs Combine \n\n'; exit)inherited from RS's xPhoton_HFJet.C Run the whole xPhotonn code. First argument is input root file from ggAnalyzer and second output is a integer which is only used for output naming.
The code to add additional information in each event. First argument is the MC cross section, second and third argument are the input and output root file from xPhoton.
Input the files to massively send crab job and read content to connect primary dataset and text file. To extract MC informations in primary dataset.
Building... For Zee.
- macro/step2.test.makehisto/step2_makehisto.C requires ROOT version > 6.14. So Only CMSSW12_0_0 or above version are able to run this code.
- However, lots of xPhoton code are written in python2, which is not compatible for python3.