# parameters used by the "ccdproc" TCL procedure
# 
input_dir    ../input
output_dir    ../output

# we use some of the columns along the edge of the chip to shift the
#   master dark frame before subtracting it from the image.
#   One can use the average of several columns by supplying multiple
#   values, like this:
#   
#   dark_cols    2 3 4
#  
#   If the "dark_cols" is set to the single value "-1",
#   then no shifting of the master dark is performed -- we just 
#   subtract it as-is.
box_start    10
#dark_cols     2051 2052 2053 2054 2055
dark_cols     -1

# these positions define a box within the raw image which contains
#   "good" sky data.  The values start at zero (first row is 0, not 1)
#   The "end" position is inclusive, so
#          start_row  10   end_row 20    
#   means a trimmed region with 11 (not 10!) rows.
#   The 'trim_box' value is the box number used temporarily for trimming.
#          
trim_box           10 
trim_start_row     20
trim_end_row     2030
trim_start_col     12
trim_end_col     2036