CaloSwClcon_g3.cxx

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/*
  Copyright (C) 2002-2020 CERN for the benefit of the ATLAS collaboration
*/
 
/********************************************************************
 
NAME:     CaloSwClcon_g3.cxx
PACKAGE:  offline/Calorimeter/CaloClusterCorrection
 
AUTHORS:  S. Rajagopalan
CREATED:  Dec. 15, 1999
 
PURPOSE:  correction for the finite containment for a given cluster size
          (Tuned using 50 GeV Et photons)
      Base class: CaloClusterCorrection
          Correction tuned on G3 samples.
 
Atrecon Orig: emrecon/qclcon.F
          
Updated:  May 10, 2000    (SR, HM)
          Migrated to Athena Framework from PASO
 
Updated:  Jan 5, 2001    (HM)
          QA. 
 
Updated:  Feb 2003 (LC)
          New corrections for DC1 geometry
 
Updated:  May 5, 2004    (Sven Menke)
      base class changed from algo to tool
 
Updated:  June, 2004    (sss)
          Use ToolWithConstants to get correction constants.
********************************************************************/
 
 
#include "CaloSwClcon_g3.h"
#include "AthenaKernel/errorcheck.h"
#include "GaudiKernel/MsgStream.h"
#include <cmath>
 
 
using xAOD::CaloCluster;
 
// apply correction to one cluster.
void CaloSwClcon_g3::makeCorrection (const Context& myctx,
                                     CaloCluster* cluster) const
{
  const float etamin = m_etamin (myctx);
  const float etamax = m_etamax (myctx);
 
  float eta = cluster->eta();
  float aeta = fabs(eta);
  if (aeta < etamin || aeta >= etamax) return;
 
  const CxxUtils::Array<1> correction = m_correction (myctx);
  if (correction.size() == 0) return;
  
  // Determine the correction
  double granularity = (etamax - etamin) / correction.size();
  int i = static_cast<int> ((aeta - etamin)/granularity);
  float qclcon = correction[i];
 
  // Do the Correction
  setenergy(cluster, qclcon * cluster->e());
}
 

int CaloSwClcon_g3::version() const
{
  return 1;
}