A better image starts before processing begins.
Most astrophotography problems are workflow problems: planning, acquisition, frame quality, plate solving, calibration, stacking and processing all affect the final image. This hub explains how the AIT ecosystem connects those decisions.
AIT keeps planning, solving, stacking, analysis, processing and export connected in one working environment.
The decision chain.
Every stage should either improve the data, explain the data or prevent a bad decision from moving forward.
Use sky atlas, planner and mosaic tools to make framing and timing decisions before capture.
Keep sessions readable, with Seestar ingest and file discipline for easier review later.
Use plate solving, FITS/session analysis, tilt checks and quality diagnostics to understand what you captured.
Build the stack from frames that deserve to contribute, with calibration, weighting and rejection logic.
Stretch, correct gradients, separate stars, reduce noise and recover detail with controlled tools.
Prepare clean outputs for web, print, archive, reports, AstroBin or future processing.
Use live stacking as a quality decision.
Live stacking should reveal calibration, rejection and whether the session is still improving.
Before stackingUse Seestar Companion for session decisions.
When the core question is frame quality, FITS diagnostics or whether the session is worth stacking, start there.
After stackingUse AIT for deeper processing.
When the data is ready for stretch, gradients, stars, denoise, detail recovery and export, continue in AIT.