[PIPE2D-650] Apply the SDSS LSF to AMBRE templates Created: 04/Nov/20 Updated: 14/Jul/23 Resolved: 14/Jul/23 |
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| Status: | Done |
| Project: | DRP 2-D Pipeline |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Story | Priority: | Normal |
| Reporter: | Takuji Yamashita | 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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| Epic Link: | flux calibration | ||||||||
| Reviewers: | hassan | ||||||||
| Description |
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Apply the SDSS line spread function (LSF) to the AMBRE model templates in order to accurately compare between an SDSS spectrum and the best fit AMBRE model template. |
| Comments |
| Comment by Masayuki Tanaka [ 14/Jul/23 ] |
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I suspect this ticket was originally intended as a prior task to PIPE2D-651, but LSF convolution is an obvious step in the stellar typing (at least in the current algorithm) and I do not think it deserves a stand-alone ticket. Closing. |