[PIPE2D-983] Reflect the uncertainties of the extinction correction to classification errors Created: 21/Feb/22 Updated: 26/Apr/23 Due: 18/Mar/22 Resolved: 26/Apr/23 |
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| Status: | Done |
| Project: | DRP 2-D Pipeline |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Task | Priority: | Normal |
| Reporter: | ishigaki | Assignee: | ishigaki |
| Resolution: | Done | Votes: | 0 |
| Labels: | f-star-selection, flux-calibration | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Issue Links: |
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| Reviewers: | Masayuki Tanaka | ||||||||||||||||||||
| Description |
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We adopt the estimated extinction correction uncertainties to a training/validation data to re-evaluate classification errors. |
| Comments |
| Comment by ishigaki [ 24/Mar/23 ] |
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This task has been done along with the ticket |
| Comment by Masayuki Tanaka [ 26/Apr/23 ] |
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The Galactic extinction is a fitting parameter in brutus and is marginalized over in the derived stellar parameters. Closing this ticket. |