Find changes early
Look for background increases, degraded stars, drift or vibration patterns before committing to a long stack.
A small observatory can produce more frames than a person can inspect manually. A consistent quality-control stage helps identify session changes, isolate questionable data and preserve the reasoning behind every selection.

Analyze compatible datasets locally and keep the review close to the observatory archive.
Look for background increases, degraded stars, drift or vibration patterns before committing to a long stack.
Apply the same review sequence while allowing thresholds to reflect the target, equipment and objective.
Preserve selected frames, rejected frames and the reason for the split when the project requires it.
Analyze a working copy or use a non-destructive workflow. Keep original data and acquisition logs unchanged.
Do not mix targets, filters, exposure regimes or instruments when interpreting relative metrics.
Identify representative good frames and use them to understand normal star shape, background and sharpness for that session.
Inspect the timeline for sudden or progressive changes associated with cloud, focus drift, tracking, wind or vibration.
Automated verdicts should narrow the inspection workload, not eliminate expert review.
Create the stack-ready subset and retain a simple record of criteria, software version and settings.
Describe the camera, FITS volume, review objective and operating systems.