reproject_to_reference
Resample a plate-solved image onto another plate-solved image's pixel grid using astrometric solutions, creating a new reference-aligned view for combining masters across sessions.
Instructions
Resample a plate-solved image onto the pixel grid of another plate-solved image, using the two astrometric solutions (PixInsight's astrometric reprojection): the result has the reference's size and solution and comes from a single interpolation of the source. Use it to bring a master from another telescope or session onto a reference grid; both views need a solution (run_plate_solve). The source is not changed; the result is a new 32-bit float view (output_id, default _reprojected). It reports the size, the time and whether the result is empty (the two fields do not overlap). Registration accuracy is set by the two solutions, so check the star-centroid residual of the result against the reference.
Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| clamp | No | Clamping threshold of the Lanczos and bicubic interpolations, 0 to 1 (default 0.3) | |
| view_id | Yes | Source view to reproject (needs an astrometric solution) | |
| output_id | No | View ID of the result (default <view_id>_reprojected) | |
| reference_id | Yes | View whose size and astrometric solution the result takes (needs an astrometric solution) | |
| interpolation | No | Pixel interpolation (default Lanczos3) |