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  1. DRP 2-D Pipeline
  2. PIPE2D-1182

Add some outputs for debugging of flux calibration

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    • Type: Task
    • Status: Done (View Workflow)
    • Priority: Normal
    • Resolution: Done
    • Affects Version/s: None
    • Fix Version/s: None
    • Component/s: None

      Description

      For the sake of quick debugging analyses, we will add the following optional outputs:

      1. Reduced chi-squares of prior, posterior, and likelihood probabilities
      2. The best-fit model template of each standard, which is LSF-convolved and scaled with broad-bands
      3. Whitened model templates of #2
      4. Galactic extinction A(lambda) and E(B-V) of each standard
      5. Attenuated #2 model templates by Galactic extinction

      These are made with --debug

      Each of #1 will be included in each existing output of probabilities. #2,3,5 will be in a new output together with #4. 

      EDIT
      What we really want, as a substitute for 2-5, is the whitened model flux that is being compared to the whitened observed flux while chi^2 is constructed. We can already output the latter (whitened observed flux), so we want the former (whitened model flux) now.

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            • Assignee:
              sogo.mineo sogo.mineo
              Reporter:
              takuji.yamashita Takuji Yamashita
              Reviewers:
              price
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