MAG Files
Category DART |
Version 1.0 |
Description
MAG files are written by stella. Stella writes out a MAG files for each image in which stella successfully correlates stars. MAG files contain the name of each star in the image, the correlation score, the total number of DN in the image associated with that star, and the star's v magnitude. MAG files live in the MAGFILES directory, which is parallel to LMKFILES, SUMFILES, etc. They are meant to be a shortcut toward a poor man's aperture photometry to assess radiometric response.
Stella names MAG files as PICNAME.REG.
An annotated .MAG file
catno corr sum dn mag --> the columns are the number of the star in the catalog (also shown on TEMPFILE.ppm) --> the correlation score for that star, the total number of DN summed over a circle with radius 150632 0.883 362528 9.500 --> qsize (the final parameter in the stella inputs), and the stellar magnitude. 150692 0.879 285433 9.820 150182 0.905 366901 9.820 151042 0.951 341694 9.910 150068 0.915 203637 10.300 150234 0.912 196155 10.340 151380 0.953 203285 10.350 150010 0.964 188350 10.390 151014 0.933 214639 10.390 150122 0.935 200106 10.410 151432 0.927 190317 10.450 150482 0.947 210444 10.460 150758 0.903 180699 10.460 150154 0.954 159825 10.530 150248 0.858 199390 10.630 150080 0.901 165230 10.790 151240 0.968 165286 10.860 150764 0.842 161857 10.870 150426 0.946 142003 10.880 150522 0.899 187723 10.910 150744 0.920 101989 10.920 150912 0.925 148504 10.960 150940 0.931 141451 10.990 151066 0.870 138391 11.020 150686 0.890 130369 11.110 150350 0.856 108177 11.160 150820 0.960 130938 11.180 150678 0.943 118386 11.190 151216 0.918 106825 11.200 150798 0.928 127300 11.230 150626 0.859 107775 11.260 150514 0.900 114116 11.300 150720 0.901 99973 11.360 151368 0.912 97339 11.420 151224 0.941 116083 11.440 150494 0.933 83160 11.450 150258 0.904 113108 11.460 151284 0.930 95273 11.460 END 1.1400 0.9158 38 --> the PSF used for the Gaussian, the average of the correlations for all the stars, and then the number of stars in the file.