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 (same as the number in TEMPFILE.ppm
--> the correlation score for that star, the total number of DN summed over an 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.