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  1. DRP 2-D Pipeline
  2. PIPE2D-651

Spectral fitting of SDSS spectra for flux calibration

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    • Type: Story
    • Status: Open (View Workflow)
    • Priority: Normal
    • Resolution: Unresolved
    • Affects Version/s: None
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      Description

      Spectral fitting of SDSS stellar spectra with interpolated AMBRE model templates for flux calibration. This ticket is for a study of the methodology using SDSS F stars in Lee et al. (2011). A target accuracy of fractional residuals is less than 1 percent.

      The SDSS spectra and AMBRE templates should be spectral-whitened in advance in PIPE2D-648. The radial velocities of stars should be estimated in PIPE2D-649

      The probability distributions of broad band stellar typing are used as a prior.

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              • Assignee:
                msyktnk Masayuki Tanaka
                Reporter:
                takuji.yamashita Takuji Yamashita
                Reviewers:
                hassan
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                • Created:
                  Updated: