Any samples you set, are stored in the StarTools.log file and can be restored using the 'LoadPSFs' button.
In the StarTools.log file, you should find entries like these;
PSF samples used (8 PSF sample locations, BASE64 encoded)
VFMAAAgAOAQMA/oDEQHaAoEAIwNeAOQAUwDUAY8AbAI5AdMBMQGkAFAB
If you wish to restore the samples used, put the BASE64 string (starting with VFM... in the example) in a text file. Simply load the the file using the 'LoadPSFs' button.
Pixels that fall inside the masked areas (designated "green" in the mask editor), are used during local PSF model construction.
The Bin module puts you in control over the trade-off between resolution, resolved detail and noise.
When multiple star samples are provided, the SVDecon module will operate in the most advanced way.
It is robust in the presence of severe noise, as well as natural singularities (e.g. over-exposed star cores) in the dataset.
And all this is just what Tracking does for the deconvolution module.
You can convert everything you see to a format you find convenient. Give it a try!