/* ======================================================================== *\ ! ! * ! * This file is part of MARS, the MAGIC Analysis and Reconstruction ! * Software. It is distributed to you in the hope that it can be a useful ! * and timesaving tool in analysing Data of imaging Cerenkov telescopes. ! * It is distributed WITHOUT ANY WARRANTY. ! * ! * Permission to use, copy, modify and distribute this software and its ! * documentation for any purpose is hereby granted without fee, ! * provided that the above copyright notice appear in all copies and ! * that both that copyright notice and this permission notice appear ! * in supporting documentation. It is provided "as is" without express ! * or implied warranty. ! * ! ! ! Author(s): Thomas Bretz, 5/2003 ! ! Copyright: MAGIC Software Development, 2000-2003 ! ! \* ======================================================================== */ ///////////////////////////////////////////////////////////////////////////// // // MCurrents (PRELIMINARY) // ///////////////////////////////////////////////////////////////////////////// #include "MCurrents.h" #include #include "MLog.h" #include "MLogManip.h" ClassImp(MCurrents); using namespace std; // -------------------------------------------------------------------------- // // Default constructor. // MCurrents::MCurrents(Int_t size, const char *name, const char *title) : fArray(size) { fName = name ? name : "MCurrents"; fTitle = title ? title : "Storage container for the pixel currents"; } // -------------------------------------------------------------------------- // // Print the hillas Parameters to *fLog // void MCurrents::Print(Option_t *) const { *fLog << all << underline << GetDescriptor() << endl; for (int i=0; i