lvmguider 0.4.0b1

🚀 New

• #5 Major refactor of the guider code.
  • Extracted sources are always matched to Gaia DR3 regardless of whether the solution was obtained using astrometry.net or kd-tree. lmag zero points are calculated for each source.
  • Once acquisition is complete the WCS of the individual cameras is determined from the Gaia cross-match, and not by tranlating the reference WCS using the measured offset. This allows each new WCS to also reflect changes in PA.
  • Average zero points and PAs are output.
  • All the metadata is carried out in two dataclasess, CameraSolution and GuiderSolution.
  • The output data model has changed. Former proc- files are now named lvm.{telescope}.guider, and sources are saved as parquet tables. The latter allows to preserve the column types in the presence of missing data.
• #6 Major improvements to co-adding code. QA plots generated during the co-adding process and the results are loaded to the database.
• Implemented guiding in rotation/PA.
• Added script to reprocess all MJDs at LCO and generate co-added products.
• Added file watcher to generate co-adds during the night. Updated the container image to support running the file watcher as a Kubernetes service.

✨ Improved

• Improved the sigma clipping of FWHM outliers.

🏷️ Changed

• Renamed references to "master frame" to "full frame". Coordinates are now referred to as x_ff and y_ff.