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  1. Data Management
  2. DM-36643

Implement construction of reference flux flats

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    • Improvement
    • Status: To Do
    • Resolution: Unresolved
    • None
    • cp_pipe, ip_isr
    • None

    Description

      After additive effects have been removed from science images, we want to use a reference flux flat to convert it into a fluence image.  This will either be determined from CBP data or from dense starfields in combination with monochromatic dome flats.

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              Unassigned Unassigned
              czw Christopher Waters
              Christopher Waters
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                Updated:

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