EVNDISP.reconstruction.SW18_noDoublePass.runparameter

eventdisplay reconstruction parameter file
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parameter file used for e.g. DST DQM, laser gain calibration
(should not be used for any data analysis)
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Note: all line without '*' in the beginning are ignored

Remember that after changing any values here, you have to redo lookup tables,
effective areas and radial acceptances
(so don't do it)

The following file describes the reconstruction parameters for eventdisplay:

i) trace integration and image cleaning parameter

ii) quality cuts applied before the array analysis 
(reconstruction of shower core and direction).

   Each set of cuts listed below correspond to one set of array parameters in the
   eventdisplay output file (showerpars tree): 
   for example: first set of cuts to Xcore[0], Ycore[0], etc., second set to Xcore[1], Ycore[1], ...

   The maximum number of different set is 100 
   (can be changed in VGlobalRunParameter: variable VDST_MAXRECMETHODS

   mscw_energy reads the results of one set only, choose with -arrayrecid=RECID 
   (e.g. for cut set 13: -arrayrecid=13)

   (Note: There is some confusion between the words method and cut set in the array analysis code of
   eventdisplay.)

Note that these values override parameters given at the command line (!)
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i) trace integration and image cleaning parameter
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 trace integration <integration method (0=off/1=default/2=sliding window)>
* -1 FADCANALYSIS 1
 double pass method 
    Par1: <doublepass (on=1, off=0)>
    Par2: <integration window length for pass 1> 
    Par3: <integration method for pass 1 (1/2)>
    Par4: <double pass error option (0/1)> (don't change if you don't understand)
    Par5: <maximum time difference between LG and HG T0 (default -4 samples)>
* -1 FADCDOUBLEPASS 0 4 2 0 -4
 trace integration window <window 1> <window 2>
* -1 FADCSUMMATIONWINDOW 16 16
 trace integration start (for window 1 for integration method 1)
    Par1: <sample # of window start> 
    Par2: <shift of window start for double pass>
    Par3: <timing method used for calculation of window start (FIXED/TZERO/TAVERAGE)>
    Par4: <max difference between T0 and trace integration start>
* -1 FADCSUMMATIONSTART 2 -1 T0

 image cleaning <method=TWOLEVELCLEANING/TIMECLUSTERCLEANING> <FIXED/VARIABLE>
* -1 IMAGECLEANINGMETHOD TWOLEVELCLEANING VARIABLE
 image cleaning thresholds <image> <border> <remove single image/border pairs (1=on)>
* -1 IMAGECLEANINGTHRESHOLDS 5. 2.5 1

 image calculation at the edge of the camera <start fit for image with at least this loss> <min number of tubes>
* -1 LLEDGEFIT 0.05 5

 quality cut on distance of image/border pixel (applied for all cuts defined below)
 (this is currently used for plotting only)
 -1 BRIGHTSTARS CATALOGUENAME MIN_B_MAGNITUDE MIN_DISTANCE_DEG <apply cut for images with less then minimum number of tubes>
* -1 BRIGHTSTARS Hipparcos_MAG8_1997.dat 3.0 0. 15

ii) quality cuts applied before the array analysis 
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USAGE:

   to start a new set of cuts:

   '* -1 RECMETHOD 4'

   syntax:

     <telescope type> <variable name> <variable value>

   all line without '*' in the beginning are ignored

   all operators are '>' or '<' (except for number of images, where it is '>=')

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Set 0 = default reconstruction methods / quality cuts
        for 4-telescope runs

* -1 RECMETHOD 4
* -1 MINANGLE 10.
* -1 MINTUBES 5
* -1 MINSIZE 100
* -1 MAXLOSS 0.2
* -1 MINWIDTH 0.02
* -1 MAXDIST 1.75