Plotting the size of extended sources will make the life easier when studying crowded regions (e.g. Galactic plane).
For disk and Gaussian sources the r68 could be used (in this way they are easily comparable). For templates, they could be shown as a point source or better as contours using existing libraries as aplpy.
Plotting the size of extended sources will make the life easier when studying crowded regions (e.g. Galactic plane). For disk and Gaussian sources the r68 could be used (in this way they are easily comparable). For templates, they could be shown as a point source or better as contours using existing libraries as aplpy.
Regards Francesco