[PIPE2D-366] Identify absorption features Created: 20/Feb/19 Updated: 23/Dec/22 Resolved: 23/Dec/22 |
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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: | hassan | Assignee: | Masayuki Tanaka |
| Resolution: | Done | Votes: | 0 |
| Labels: | flux-calibration, model-templates | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Issue Links: |
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| Story Points: | 6 | ||||||||
| Description |
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Identify which absorption features are sensitive to stellar atmosphere parameters for F-stars. A short report of the features to be used and how they were determined should be provided. The absorption features should be written to a persistent file that can be subsequently loaded into the 2D DRP pipeline for flux calibration. The format needs to be decided. The location would be determined by Kiyoto Yabe. |
| Comments |
| Comment by rhl [ 08/Mar/19 ] |
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The location of this file isn't important as it'll be loaded as a butler object. We do need to get it into the datamodel, and come up with a way of storing it "permanently" away from the live code/data, and potentially versioning it. Using git seems reasonable here, but we still have to sort out the details – and I agree that Kiyoto Yabe would be a good person. |
| Comment by Masayuki Tanaka [ 23/Dec/22 ] |
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This ticket is obsolete and superseded by |