- Preparing data for the Wipe module
- Edge located dark anomalies
Edge located dark anomalies
Stacking artefacts are the most common dark anomalies located at the edges of your image. Failing to deal with them will lead to a halo effect near the edges of your dataset.
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.
- Usage (under Super Structure)
In this case the Super Structure module can be used to isolate objects in an image and lift them from an otherwise noisy background.
- Mouse controls (under Interface)
As of 1.7, enhanced mouse controls are implemented; Zoom in.
- Zooming, panning and scaling (under Interface)
Even the way StarTools displays and scales images, has been created specifically for astrophotography.
- Step 4: Final global stretch (under Quick Start)
AutoDev will keep solving for a global strecth that best shows the detail in your RoI.