Index: trunk/MagicSoft/Simulation/Detector/Camera/camera.h
===================================================================
--- trunk/MagicSoft/Simulation/Detector/Camera/camera.h	(revision 313)
+++ trunk/MagicSoft/Simulation/Detector/Camera/camera.h	(revision 316)
@@ -19,7 +19,7 @@
 //=
 //= $RCSfile: camera.h,v $
-//= $Revision: 1.1.1.1 $
+//= $Revision: 1.2 $
 //= $Author: harald $ 
-//= $Date: 1999-11-05 11:59:31 $
+//= $Date: 1999-11-10 07:42:41 $
 //=
 //=//////////////////////////////////////////////////////////////////////
@@ -236,5 +236,5 @@
 //!@{
 
-#define QE_FILE     "qe.dat"
+#define QE_FILE     "../Data/qe.dat"
 
 //!@}
@@ -278,4 +278,227 @@
 /*
  *$Log: not supported by cvs2svn $
+ *Revision 1.1.1.1  1999/11/05 11:59:31  harald
+ *This the starting point for CVS controlled further developments of the
+ *camera program. The program was originally written by Jose Carlos. 
+ *But here you can find a "rootified" version to the program. This means 
+ *that there is no hbook stuff in it now. Also the output of the
+ *program changed to the MagicRawDataFormat. 
+ *
+ *The "rootification" was done by Dirk Petry and Harald Kornmayer. 
+ *
+ *In the following you can see the README file of that version:
+ *
+ *==================================================
+ *
+ *Fri Oct 22  1999   D.P.
+ *
+ *The MAGIC Monte Carlo System
+ *
+ *Camera Simulation Programme
+ *---------------------------
+ *
+ *1) Description
+ *
+ *This version is the result of the fusion of H.K.'s
+ *root_camera which is described below (section 2)
+ *and another version by D.P. which had a few additional
+ *useful features.
+ *
+ *The version compiles under Linux with ROOT 2.22 installed
+ *(variable ROOTSYS has to be set).
+ *
+ *Compile as before simply using "make" in the root_camera
+ *directory.
+ *
+ *All features of H.K.'s root_camera were retained.
+ *
+ *Additional features of this version are:
+ *
+ *  a) HBOOK is no longer used and all references are removed.
+ *
+ *  b) Instead of HBOOK, the user is given now the possibility of 
+ *     having Diagnostic data in ROOT format as a complement
+ *     to the ROOT Raw data.
+ *
+ *     This data is written to the file which is determined by
+ *     the new input parameter "diag_file" in the camera parameter
+ *     file.
+ *
+ *     All source code file belonging to this part have filenames
+ *     starting with "MDiag".
+ *
+ *     The user can read the output file using the following commands
+ *     in an interactive ROOT session:
+ *
+ *       	root [0] .L MDiag.so
+ *	root [1] new TFile("diag.root");
+ *	root [2] new TTreeViewer("T");
+ *	
+ *     This brings up a viewer from which all variables of the
+ *     TTree can be accessed and histogrammed. This example
+ *     assumes that you have named the file "diag.root", that
+ *     you are using ROOT version 2.22 or later and that you have
+ *     the shared object library "MDiag.so" which is produced
+ *     by the Makefile along with the executable "camera".
+ *       
+ * !   The contents of the so-called diag file is not yet fixed.
+ * !   At the moment it is what J.C.G. used to put into the HBOOK
+ * !   ntuple. In future versions the moments calculation can be
+ * !   removed and the parameter list be modified correspondingly.
+ *
+ *  c) Now concatenated reflector files can be read. This is useful
+ *     if you have run the reflector with different parameters but
+ *     you want to continue the analysis with all reflector data
+ *     going into ONE ROOT outputfile.
+ *
+ *     The previous camera version contained a bug which made reading 
+ *     of two or more concatenated reflector files impossible.
+ *
+ *  d) The reflector output format was changed. It is now version
+ *     0.4 .
+ *     The change solely consists in a shortening of the flag
+ *     definition in the file 
+ *
+ *           include-MC/MCCphoton.hxx  
+ *
+ * !   IF YOU WANT TO READ REFLECTOR FORMAT 0.3, you can easily
+ * !   do so by recompiling camera with the previous version of
+ * !   include-MC/MCCphoton.hxx.
+ *
+ *     The change was necessary for saving space and better
+ *     debugging. From now on, this format can be frozen.
+ *
+ * !   For producing reflector output in the new format, you
+ * !   of course have to recompile your reflector with the
+ * !   new include-MC/MCCphoton.hxx .
+ *
+ *  e) A first version of the pixelization with the larger
+ *     outer pixels is implemented. THIS IS NOT YET FULLY
+ *     TESTED, but first rough tests show that it works
+ *     at least to a good approximation.
+ *
+ *     The present version implements the camera outline
+ *     with 18 "gap-pixels" and 595 pixels in total as
+ *     shown in 
+ *
+ *        http://sarastro.ifae.es/internal/home/hardware/camera/numbering.ps
+ *
+ *     This change involved 
+ *
+ *	(i) The file pixels.dat is no longer needed. Instead
+ *          the coordinates are generated by the program itself
+ *          (takes maybe 1 second). In the file 
+ *
+ *		pixel-coords.txt
+ *
+ *	  in the same directory as this README, you find a list
+ *          of the coordinates generated by this new routine. It
+ *          has the format
+ *
+ *              number   i   j   x  y  size-factor
+ *
+ *          where i and j are J.C.G.'s so called biaxis hexagonal
+ *          coordinates (for internal use) and x and y are the
+ *          coordinates of the pixel centers in the standard camera
+ *          coordinate system in units of centimeters. The value
+ *          of "size-factor" determines the linear size of the pixel
+ *          relative to the central pixels. 
+ *
+ *        (ii) The magic.def file has two additional parameters
+ *          which give the number of central pixels and the
+ *          number of gap pixels
+ *
+ *        (iii) In camera.h and camera.cxx several changes were 
+ *          necessary, among them the introduction of several
+ *          new functions 
+ *
+ *     The newly suggested outline with asymmetric Winston cones
+ *     will be implemented in a later version.
+ *
+ *  f) phe files can no longer be read since this contradicts
+ *     our philosophy that the analysis should be done with other
+ *     programs like e.g. EVITA and not with "camera" itself.
+ *     This possibility was removed. 
+ *
+ *  g) ROOT is no longer invoked with an interactive interface.
+ *     In this way, camera can better be run as a batch program and
+ *     it uses less memory.
+ *
+ *  h) small changes concerning the variable "t_chan" were necessary in
+ *     order to avoid segmentation faults: The variable is used as an
+ *     index and it went sometimes outside the limits when camera
+ *     was reading proton data. This is because the reflector files
+ *     don't contain the photons in a chronological order and also
+ *     the timespread can be considerably longer that the foreseen
+ *     digitisation timespan. Please see the source code of camera.cxx
+ *     round about line 1090.
+ *
+ *  j) several unused variables were removed, a few warning messages
+ *     occur when you compile camera.cxx but these can be ignored at
+ *     the moment.
+ *
+ *In general the program is of course not finished. It still needs
+ *debugging, proper trigger simulation, simulation of the asymmetric
+ *version of the outer pixels, proper NSB simulation, adaption of
+ *the diag "ntuple" contents to our need and others small improvements.
+ *
+ *In the directory rfl-files there is now a file in reflector format 0.4
+ *containing a single event produced by the starfiled adder. It has
+ *a duration of 30 ns and represents the region around the Crab Nebula.
+ *Using the enclosed input parameter file, camera should process this
+ *file without problems.
+ *
+ *2) The README for the previous version of root_camera
+ *
+ *README for a preliminary version of the 
+ *root_camera program. 
+ *
+ *root_camera is based on the program "camera"of Jose Carlos
+ *Gonzalez. It was changed in the way that only the pixelisation 
+ *and the distibution of the phe to the FADCs works in a 
+ *first version. 
+ *
+ *Using the #undef command most possibilities of the orignal 
+ *program are switched of. 
+ *
+ *The new parts are signed by 
+ *
+ *- ROOT or __ROOT__ 
+ *  nearly all  important codelines for ROOT output are enclosed 
+ *  in structures like 
+ *  #ifdef __ROOT__ 
+ *  
+ *    code 
+ *
+ *  #endif __ROOT__ 
+ *
+ *  In same case the new lines are signed by a comment with the word 
+ *  ROOT in it. 
+ *
+ *  For timing of the pulse some variable names are changed. 
+ *  (t0, t1, t  -->  t_ini, t_fin, t_1st, t_chan,...) 
+ *  Look also for this changes. 
+ *
+ *  For the new root-file is also a change in readparm-files
+ *
+ *
+ *- __DETAIL_TRIGGER__
+ *
+ *  This is for the implementation of the current work on trigger 
+ *  studies. Because the class MTrigger is not well documented it 
+ *  isn´t a part of this tar file. Only a dummy File exists. 
+ *
+ *
+ *
+ *With all files in the archive, the root_camera program should run. 
+ *
+ *A reflector file is in the directory rfl-files
+ *
+ *==================================================
+ *
+ *From now on, use CVS for development!!!!
+ *
+ *
+ *
  *Revision 1.3  1999/10/22 15:32:56  petry
  *tidied-up version, really sent to H.K. and N.M., 22-10-99
