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  1. DRP 2-D Pipeline
  2. PIPE2D-368

Fit model stellar templates using whitening

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    • Type: Task
    • Status: Won't Fix (View Workflow)
    • Priority: Normal
    • Resolution: Won't Fix
    • Affects Version/s: None
    • Fix Version/s: None
    • Component/s: None
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    • Story Points:
      5

      Description

      One way to implement PIPE2D-367 are the following steps proposed by Masayuki Tanaka:

      • whiten the spectra
      • fit the whitened spectra with the templates to derive P(Teff,log g,Z)

      Implement this.

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          Task - A task that needs to be done. PIPE2D-367 Derive P(Teff, log g, Z) from model templates

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              • Assignee:
                kiyoto.yabe Kiyoto Yabe
                Reporter:
                hassan hassan
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                • Created:
                  Updated:
                  Resolved: