[PIPE2D-368] Fit model stellar templates using whitening Created: 20/Feb/19  Updated: 31/Mar/23  Resolved: 31/Mar/23

Status: Won't Fix
Project: DRP 2-D Pipeline
Component/s: None
Affects Version/s: None
Fix Version/s: None

Type: Task Priority: Normal
Reporter: hassan Assignee: Kiyoto Yabe
Resolution: Won't Fix Votes: 0
Labels: None
Remaining Estimate: Not Specified
Time Spent: Not Specified
Original Estimate: Not Specified

Issue Links:
Blocks
blocks PIPE2D-367 Derive P(Teff, log g, Z) from model t... Open
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.



 Comments   
Comment by Kiyoto Yabe [ 31/Mar/23 ]

I think this is already a part of the current flux calibration, so we can close this ticket.

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