- Usage
- Recovering PSF samples from the log
Recovering PSF samples from the log
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.
You may also be interested in...
- The power of temporal 3D (X, Y, t) signal processing (under Tracking is signal preservation)
And all this is just what Tracking does for the deconvolution module.
- SVDecon: Detail Recovery through Spatially Variant Distortion Correction (under Features & Documentation)
It is robust in the presence of severe noise, as well as natural singularities (e.g. over-exposed star cores) in the dataset.
- Bin: Trade Resolution for Noise Reduction (under Features & Documentation)
The Bin module puts you in control over the trade-off between resolution, resolved detail and noise.
- Modes of operation (under Usage)
When multiple star samples are provided, the SVDecon module will operate in the most advanced way.
- Point Spread Functions (PSFs) (under Usage)
All light in your image is spread according to a Point Spread Function (PSF), not just the stars.