# PARAMETER FILE FOR cflatf_conventional.sh OR cflatf_advanced.sh

# default name (change if either cflatf_conventional.sh or cflatf_advanced.sh is used)
name='flatfield_con' # <- for cflatf_conventional.sh
# name='flatfield_adv' # <- for cflatf_advanced.sh

# (mandatory) PATH VARIABLES
# (mainpath = the run, night = the night, block = subfolder for observing block
# during that night)
mainpath=/work1/herenz/pmas/run197/
night=/night3/
block=/skyflat/ # skyflat == twilight-flat

# instrument parameter file
parfile=${p3d_path}/data/instruments/pmas/larr4k.prm

# user parameter file
userparfile=${mainpath}qsos.prm

# inputfile(s) (if a comma separated list is given, the combined
# exposure will be extracted, which is usefull for e.g. twilight
# flats) (note: only provide quadrant a) 
# !!! VARIABLE NAME IS ALWAYS inputfile, even if more than one file is in the list !!!
inputfile='run197_01506a.fits,run197_01507a.fits,run197_01508a.fits,run197_01509a.fits'

# tracemask (leave empty if you want to calculate the trace mask from
# the (combined) input raw data file - i.e. tracemask=
#tracemask=${mainpath}${night}${block}/tracemask/tracemask_comb_05-24-12--2101_run197_01507_imcmb_trace.fits
tracemask=

# master bias
masterbias=${mainpath}${night}/bias/masterbias/Q308+0129_mbias.fits

# dispersion mask (mandatory)
dispmask=${mainpath}${night}${block}/dispmask/dispmask_05-24-12--2221_run197_01510_imcmb_dmask.fits

# special parameters:
# (best used for switches - for flatfielding the following are possible:
# /biaspx, /biaspy, /biasox, /biasoy, /biasconstant, /exemonitor(?), /compress, 
# /gui, /cinv, /scattlightsubtract, /crclean, /nocrmask, /imagemethod, /imageclean,
# /nocrmask, /imageclean, /writeall, /showcrgui, /satmask (!) 
special_params=''

# TODO: finish(ed?) - for traditional method