run_plate_solve
Plate solve an open image against the local Gaia DR3 catalog to add an astrometric solution, enabling downstream processes like photometry and color calibration.
Instructions
Plate solve an open image with ImageSolver against the local Gaia DR3/SP database (offline). Adds the astrometric solution needed by run_spfc, run_mgc and run_spcc. Needs an approximate position (ra_deg, dec_deg; within a fraction of the field is enough) and scale (pixel_scale in arcsec/px, or focal_length_mm + pixel_size_um) unless the image keywords already carry RA, DEC and FOCALLEN/XPIXSZ. The scale seed may be off by about 2x. Observation time is read from DATE-OBS/DATE, else today.
Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| ra_deg | No | Approximate center RA in degrees | |
| dec_deg | No | Approximate center Dec in degrees | |
| view_id | Yes | View ID to plate solve | |
| pixel_scale | No | Approximate pixel scale in arcsec/pixel | |
| pixel_size_um | No | Pixel size in microns | |
| observation_jd | No | Julian date of the observation (only if no DATE-OBS/DATE keyword) | |
| focal_length_mm | No | Focal length in mm (use with pixel_size_um instead of pixel_scale) |