[PIPE2D-367] Derive P(Teff, log g, Z) from model templates Created: 20/Feb/19  Updated: 14/Jul/23

Status: Open
Project: DRP 2-D Pipeline
Component/s: None
Affects Version/s: None
Fix Version/s: None

Type: Task Priority: Normal
Reporter: hassan Assignee: Masayuki Tanaka
Resolution: Unresolved Votes: 0
Labels: flux-calibration, model-spectra-fitting
Remaining Estimate: Not Specified
Time Spent: Not Specified
Original Estimate: Not Specified

Issue Links:
Blocks
blocks PIPE2D-374 Combine P_HSC and P_PFS and construct... Done
is blocked by PIPE2D-836 Stellar typing using the equivalent w... Open
is blocked by PIPE2D-369 Fit stellar model templates using the... Open
is blocked by PIPE2D-368 Fit model stellar templates using whi... Won't Fix
Duplicate
duplicates PIPE2D-305 fluxcalib: P(Teff, log g, Z) from HSC... Won't Fix
duplicates PIPE2D-306 fluxcalib: P(Teff, log g, Z) from PFS... Won't Fix

 Description   

Fit available model templates with HSC photometry and PSF spectroscopy to derive the probability P(Teff, log g, Z), given the input stellar parameters.

There are multiple techniques for performing this work, and these will be the subject of individual tickets. The results of those tickets should be compared in order to determine the best approach.

 Comments   
Comment by Masayuki Tanaka [ 14/Jul/23 ]

We are currently using P(Teff,logg,Z,alpha) from the broad-band photometry and that from the spectral ftting. The broad-band fitting is done, but we are still working on (or improving) the spectral fitting part.

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