I have 14 wcs-calibrated images that I am using to experiment with ZP derivation. The first 4 are B, the next 10 are Gunn r.
# Here are the images
ls -1 /home/sco/A_wcsf/Run_apr17/local_red/WCS/20*fits > list.ZP0
cat list.ZP0
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T020222.8_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T022042.6_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T032156.5_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T035223.8_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T061218.4_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T070902.2_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T072507.6_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T083937.3_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T092518.0_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T100533.3_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T101258.1_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T102445.6_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T104913.4_acm_sci_proc.fits
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T105144.7_acm_sci_proc.fits
For now (Apr17) I am proceesing each image with the code usno_photcal:
% usno_photcal
Usage: usno_photcal ./S/20180206T022042.6_acm_sci_proc.fits Y
arg1 - Name of FITS image (can be full path)
arg2 - run in debug mode (Y/N)
% setenv fullfits /home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T061218.4_acm_sci_proc.fits
% usno_photcal $fullfits N
I get the following:
% ls
20180206T061218.4_acm_sci_proc.fits 20180206T061218.4_acm_sci_proc.png zp.table
20180206T061218.4_acm_sci_proc.info 20180206T061218.4_acm_sci_proc-usno.cdfp zp.parlab
The real info for now is in zp.tablea, to see:
xyplotter_auto zp BmR ZP 1
xyplotter_auto zp Peak ZP 1
What I need:
1) Notification of filter
2) graphical filter of ZP values and stats for selected ZP values.
*** zpadopt, now installed in usno_photcal, has a graphical filter to
isolate good zp data and get mean values
Images to use:
setenv fullfits /home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T105144.7_acm_sci_proc.fits
usno_photcal $fullfits N
I ran these in: /home/sco/A_wcsf/Run_apr17/ZP0
X=Peak AVap
------------- --------------
Blue
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T020222.8_acm_sci_proc.fits -5.564 0.195 2 -3.634 0.043 2
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T022042.6_acm_sci_proc.fits -3.320 0.137 6 -3.320 0.137 6
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T032156.5_acm_sci_proc.fits -3.316 0.041 3 -3.316 0.041 3
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T035223.8_acm_sci_proc.fits -2.997 0.034 2 -2.997 0.034 2
Red
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T061218.4_acm_sci_proc.fits -3.166 0.074 2 -3.063 0.106 5
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T070902.2_acm_sci_proc.fits -2.281 0.000 1 -2.473 0.154 6
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T072507.6_acm_sci_proc.fits -2.874 0.118 2 -3.593 0.723 3
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T083937.3_acm_sci_proc.fits -3.078 0.054 4
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T092518.0_acm_sci_proc.fits -2.640 0.056 3
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T100533.3_acm_sci_proc.fits -2.389 0.197 8
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T101258.1_acm_sci_proc.fits -2.528 0.154 5
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T102445.6_acm_sci_proc.fits -2.775 0.142 5
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T104913.4_acm_sci_proc.fits -3.372 0.085 9 -3.345 0.072 9
/home/sco/A_wcsf/Run_apr17/local_red/WCS/20180206T105144.7_acm_sci_proc.fits -3.082 0.089 4