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The current code for the RefMaker is going to assume you have exactly one set of parameters for how to choose images that go into a reference.
There would be, however, situations where we may want t…
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A recent version (`3.1.0 (2022-04-01)`) of wsclean has some options that may simplify the solar imaging workflow. To recap, the plan so far has been:
1. Reference calibration / flagging / selfc…
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Stack the residual cutouts to measure the profile further out and to characterize the amount of light in the ICL.
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Seen in tile 68001, here are some spectra showing a step-like trough, often around the blue/red arm transition
 and nodding (large offsets to improve background subtraction). It would be nice if these modes were nativel…
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b-channel spectrum offset bright relative to the other channels.
`akim@cori05:/global/project/projectdirs/desi/spectro/redux/fuji/tiles/pernight/80661/20210101> plot_spectra -i coadd*fits -t 396277…
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It may be useful to add a sky spectrum so that one can check whether or not emission line features of objects are at the wavelengths of strong sky emission lines. This can give some hints about whethe…
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record the 256 point pulse height baseline that the quabo is subtracting from each 256 pixel pulse height image,
so that if we ever want to recover the raw data, perhaps because we developed an impr…
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As I discussed with more people, I feel more confident on this small project.
This is not effected by the dilution effect since we only measure flux related
quantity--mean magnitude. But we need to c…
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There are 57 fiberflatexp files (fiber flat correction per exposure) (from 40 exposures from 12 nights) for which the bug fixed in PR #1642 (and applied in tag 0.51.3) has resulted in an error on the …