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Description
To further reduce write-to-disk size, we can save photometric fluxes for specific targets. Ideally this should not reduce frame rates, so threading might be useful. Or a queue system.
Requires #5 to be implemented potentially, or simply do this across whole image. Similar input format as #5 .
It would require flat fielding first. Or maybe that can be done in post-processing if the thumbnails are also saved. But let's not assume thumbnails are stored for this and require the user to point to a suitable flat field image: flat_field_image
Steps for each target would be:
- centroid on expected position
- measure and record fwhm (need later for aperture correction)
- aperture photometry given
aperture_sizeandsky_radiussky_annnulus_width
Fine to store as raw fluxes.
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