- Main operation
- Stage two
Stage two
Any removed energy, is collected per pixel and re-distributed across the image in a second pass, giving the user intuitive control, via the 'Grain Dispersion' parameter, over a hard upper size limit beyond which grain is no longer smoothed out.
You may also be interested in...
- F. M., Belgium (under Testimonials)
- Zooming, panning and scaling (under Interface)
Even the way StarTools displays and scales images, has been created specifically for astrophotography.
- Step 7: Final noise reduction, switching Tracking off (under Quick Start)
- Wipe: Gradient Removal, Synthetic Flats and Bias correction (under Features & Documentation)
The Wipe module detects, models and removes source of unwanted light bias, whether introduced in the optical train, camera or by light pollution.
- Sharp: Multi-scale Noise-Aware Structural Detail Enhancement (under Features & Documentation)
StarTools' Detail-aware Wavelet Sharpening allows you to bring out faint structural detail in your images.