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Use `IMAGESCL` in Steve's results to compute an updated plate scale.
- [x] plot `IMAGESCL` over the mission
- [x] identify epochs where the plate scale changes
- [x] find a plate scale value for …
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To convert doppler shift to velocity in km/s, shall we use 1074.62 to 1074.70 to compute the conversion factor? This is the same conversion factor used for line width. It is a small difference but sti…
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Enhanced intensity GIF have still problem with "black squares" and interpolation.
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We could use double precision for two areas:
- [x] computations with the data array
- [ ] all computations involving other data such as FITS keywords, constants in configuration files, etc.
Doi…
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Generate an alert (e.g. a single email) that notifies observer when the UCoMP filter temperature is out of nominal range. Email should also go to Boulder team (Giuliana, Mike, Steve, Joan). Can a fla…
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Create a tool that given a date range and config file, produces an image of standard deviations of darks by pixel.
The same image for dark corrected flats would also be useful.
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Are we doing the right thing by promoting keywords across levels and into averaging?
Questions are based on recent processing of the `process.analytic-gaussian` data. Tracking is looking at 2022020…
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Description: Hot pixels are pixels that have an intermittent behavior with regard signal or noise. They are somewhat pathological. Once identified, they can be interpolated over in the Level1 processi…
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There several issues with the raw data as of the 20210222 data:
- [x] `FILTER` keyword for dark data is sometimes "0.000"; it should be either not present or the actual value of the filter wheel po…
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Currently the plate scale for each individual file is computed and stored in `IMAGESCL`. This value should be recorded and plotted nightly.
- [x] record `IMAGESCL` value in the `ucomp_eng` database…