This deep sky astrophotography editing workflow outlines the core post-processing stages used to move from stacked data to a finished image. The process centers on PixInsight, with additional finishing work where needed, and is meant to connect the gallery results with the actual processing decisions behind them.


Slide to see the power of post-processing on the NGC 2245.
Removing light pollution gradients and balancing the stacked data before stretching in PixInsight.
Restoring detail lost to atmospheric blurring so smaller structures remain cleaner and more readable.
Using Spectrophotometric Color Calibration (SPCC) to keep star colors and overall palette grounded in the recorded data.
The goal is not to force detail, but to reveal faint structures cleanly while keeping color, contrast, and star handling consistent with the captured data.
The gallery pages show the source targets and integration details, while the equipment section explains the optics, camera, and filters used to acquire the data.
This section will continue expanding with more step-by-step examples, but it already establishes the processing framework that supports the site's finished astrophotography work.