# next is file setup.param
# parameters used by the "setup" script

# directory containing the raw image files
input_dir       /usr/tom1/data

# directory in which all intermediate and final output files go
output_dir      ../output

# directories in which the reference astrometric and photometric catalogs
#   can be found
astrom_refcat_dir      /home/tom/mk4/refcat
photom_refcat_dir      /home/tom/mk4/refcat
# directory in which all the XVista programs can be found 
xvista_dir      ../xvista
# name of any executable XVista program which has the "--version" option
#   as of 04/23/2003, the only one which does is 'sky'
xvista_exe      sky
# this is the name of a symbol table used by XVista programs 
#   we'll create it in the "output_dir"
xvista_symtable   symtable.dat

# directory in which the "match" programs can be found
match_dir        ../match

# directory in which the "photom" programs can be found
photom_dir       ../photom

# directory in which the "bait" programs can be found
bait_dir         ../bait
# name of an executable program in the bait directory,
#   from which we can get the version of the package
bait_exe       putsym

# name of the file we use to hold an ASCII list of image, with
#   properties of each one
imagelist_name    make_list.out

# observatory latitude (decimal degrees, positive North)
#   and longitude (decimal degrees, positive West of Greenwich)
latitude           41.83
longitude          88.33

# If you want to skip any image which is designated as "bad",
#   because some property of that image falls outside an acceptable range,
#   then set "skip_bad" to 1.  The pipeline will then set the "include"
#   field of any bad images to zero, and skip over them while processing.
# If you set "skip_bad" to 0, then even bad frames are processed.
skip_bad           1


# end of file setup.param
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