run_plate_solve
Plate solve an open image offline against Gaia DR3/SP to obtain the astrometric solution required by SPFC, MGC, and SPCC. Provide approximate RA/Dec and scale, or use existing image keywords.
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) |