Observatory workflow

Decide which data deserves processing.

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.

Session quality analysis interface for astronomical FITS data
Local workflow

Analyze compatible datasets locally and keep the review close to the observatory archive.

Operational value

Find changes early

Look for background increases, degraded stars, drift or vibration patterns before committing to a long stack.

Consistency

Use repeatable criteria

Apply the same review sequence while allowing thresholds to reflect the target, equipment and objective.

Traceability

Keep the decision

Preserve selected frames, rejected frames and the reason for the split when the project requires it.

Quality-control protocol

Review the session, not only individual frames.

1. Protect the raw archive

Analyze a working copy or use a non-destructive workflow. Keep original data and acquisition logs unchanged.

2. Group comparable data

Do not mix targets, filters, exposure regimes or instruments when interpreting relative metrics.

3. Establish a baseline

Identify representative good frames and use them to understand normal star shape, background and sharpness for that session.

4. Detect transitions

Inspect the timeline for sudden or progressive changes associated with cloud, focus drift, tracking, wind or vibration.

5. Review borderline frames

Automated verdicts should narrow the inspection workload, not eliminate expert review.

6. Export a project subset

Create the stack-ready subset and retain a simple record of criteria, software version and settings.

Where it fits

Operational and educational use

  • Public observatory imaging sessions.
  • Student telescope projects.
  • Remote or unattended capture review.
  • Archive triage before reprocessing.
Where it stops

Not a universal scientific pipeline

  • It does not replace project-specific calibration.
  • It does not certify scientific suitability.
  • Thresholds must be validated against the intended measurement.
  • Observatory policy remains the controlling standard.