Prepare an input file for the profiles.sh code.
% profiles_prep --help usage: profiles_prep a.fits [-v] [-h] [-r 100.0] Additional options: -v = print verbose comments and run in debug mode -h = show a help file and then exit -r = max radius for apertures (rmax=0.0 to use region ds9 region to defibe) EXAMPLES: % ls 20191018T084633.3_acm_sci.fits 20191018T084633.3_acm_sci.reg % profiles_prep 20191018T084633.3_acm_sci.fits % cat 20191018T084633.3_acm_sci.profpars # Output columns from profpars (using midodata.2) Col01 = X center, pixels (from centroid) Col02 = Y center, pixels (from centroid) Col03 = semi-major axis length in pixels Col04 = b/a axis ratio Col05 = position angle (degrees) of major axis Col06 = local background measured in local annulus Col07 = mean bkg (signal per pixel) from BOX regions Col08 = mean error of mean bkg (BOX regions) Col09 = id, line number in regions file # data 413.900 301.950 34.000 1.00000 0.000 482.8040 479.3014 3.0678 1 % profiles_prep 20191018T084633.3_acm_sci.fits -r 43.0 % tail -4 20191018T084633.3_acm_sci.profpars Col08 = mean error of mean bkg (BOX regions) Col09 = id, line number in regions file # data 413.900 301.950 43.000 1.00000 0.000 482.8040 479.3014 3.0678 1 ^^^^^^^^Note that we have used the same regions file in bot cases of the example above. However i the second case we used the "-r" flag to set the macimum radius that will be used for every aperture in our profile run.