[DAMD-51] Theoretical spectra for flux calibration: location relative to Butler Created: 13/Apr/19 Updated: 01/Oct/19 |
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| Status: | Open |
| Project: | Data Model |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Story | Priority: | Normal |
| Reporter: | hassan | Assignee: | hassan |
| Resolution: | Unresolved | Votes: | 0 |
| Labels: | None | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Issue Links: |
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| Story Points: | 1 | ||||||||||||||||||||
| Description |
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The location of F-star template spectra with respect to the Butler root, needs to be specified in the ops_pfs PfsMapper.yaml file. It has been proposed by rhl to specify these data as calibrations. |
| Comments |
| Comment by hassan [ 19/Apr/19 ] |
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This ticket requires an new entry for F-star spectra in the PfsMapper.yaml file of the obs_pfs repo. As a complete entry requires knowledge of the data type for the F-star spectra (which is the subject of DAMD-50}}, it is better that DAMD-50 is completed first before this ticket. |