[PIPE2D-369] Fit stellar model templates using the Cannon-Payne technique Created: 20/Feb/19 Updated: 03/Jul/23 |
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| 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: |
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| Epic Link: | flux calibration | ||||||||
| Description |
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Stellar models (PIPE2D-367) may be fit using the approach used by the "Cannon" (http://adsabs.harvard.edu/abs/2015ApJ...808...16N) and/or "Payne" (https://arxiv.org/pdf/1804.01530.pdf) codes. We should compare these with pre-whitening approaches. |
| Comments |
| Comment by Kiyoto Yabe [ 31/Mar/23 ] |
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Takuji Yamashita Has this been already implemented? |
| Comment by Takuji Yamashita [ 31/Mar/23 ] |
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No, it hasn't. I have no immediate plan to implement this approach. This old ticket will be passed on to Masayuki Tanaka. |