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  1. DRP 2-D Pipeline
  2. PIPE2D-837

Regrid stellar parameters for combined P_HSC and P_PFS

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      In order to derive the best fit stellar model based on the combined probability function of P_photometry and P_spectrum, we re-grid the stellar parameters. The best fit spectrum is extracted from the RBF model (PIPE2D-460). 

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          Task - A task that needs to be done. PIPE2D-374 Combine P_HSC and P_PFS and construct the best-fit spectrum

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              • Assignee:
                takuji.yamashita Takuji Yamashita
                Reporter:
                takuji.yamashita Takuji Yamashita
                Reviewers:
                hassan
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