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Create FITS for dark-corrected flats #310

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detoma opened this issue Jan 17, 2025 · 1 comment
Open

Create FITS for dark-corrected flats #310

detoma opened this issue Jan 17, 2025 · 1 comment
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@detoma
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detoma commented Jan 17, 2025

Dark-corrected flats are used extensively by scientists to check instrument performance, resolve instrument issues, create new engineering data, etc. The current flat files is hard to work on. I need to create manually dark corrected flats which is not efficient since the pipeline does it already.

Let's create a new directory "flats" where dark-corrected flats are saved with a clear filename:

yyyymmdd.hhmmss.ucomp.wave.flat.fts

This will make a lot easier to analyze flats moving forward.

Notes:

  • make sure to produce these files for flats with either the occulter in or out
@detoma detoma added the enhancement new feature label Jan 17, 2025
@mgalloy mgalloy added this to the UCoMP 1.1 milestone Jan 17, 2025
@detoma
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detoma commented Jan 22, 2025

The special flats with the occulter in will be saved in the new flat directory.

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