[PIPE2D-367] Derive P(Teff, log g, Z) from model templates - PFS-JIRA

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Details

Type: Task
Status: Open (View Workflow)
Priority: Normal
Resolution: Unresolved
Affects Version/s: None
Fix Version/s: None
Component/s: None
Labels:
- flux-calibration
- model-spectra-fitting

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.

Attachments

Issue Links

blocks

PIPE2D-374 Combine P_HSC and P_PFS and construct the best-fit spectrum

Done

duplicates

PIPE2D-305 fluxcalib: P(Teff, log g, Z) from HSC photometry

Won't Fix

PIPE2D-306 fluxcalib: P(Teff, log g, Z) from PFS spectra

Won't Fix

is blocked by

PIPE2D-836 Stellar typing using the equivalent width

Open

PIPE2D-369 Fit stellar model templates using the Cannon-Payne technique

Open

PIPE2D-368 Fit model stellar templates using whitening

Won't Fix

(1 is blocked by)

Activity

People

Assignee:

Masayuki Tanaka

Reporter:

hassan

Votes:

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Watchers:

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Dates

Created:

19/Feb/19 5:53 PM

Updated:

14/Jul/23 6:26 AM