[REDMINE1D-108] [RM-7982] [linemodel] better condition to assess minimal fraction of a line to be measured Created: 13/Jun/23 Updated: 17/Jan/24 |
|
| Status: | Open |
| Project: | 1D Redmine |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Task | Priority: | Normal |
| Reporter: | Redmine-Jira Migtation | Assignee: | Redmine-Jira Migtation |
| Resolution: | Unresolved | Votes: | 0 |
| Labels: | None | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Description |
|
Created on 2023-03-28 10:57:47 by Didier Vibert. % Done: 0 The current condition to include a line in the model, is to asses the fact that at least 30% of half the support (-4sigma, +4sigma) is visible on the extremities of the lambda range.
we should may be ask that at least one sample is close enough to the center ? and require a minimal number of samples and/or a minimal fraction of support covered by the observed samples ? |
| Comments |
| Comment by Redmine-Jira Migtation [ 17/Jan/24 ] |
|
Comment by Vincent Le Brun on 2023-03-28 12:07:40: I would put 50%, even if it is a little more restrictive that the current rule for lines on the border, but on Euclid, 1 pixel might represent the 30% of the 1/2 support, while it will be harder with a global 50% rule |
| Comment by Redmine-Jira Migtation [ 17/Jan/24 ] |
|
Comment by Didier Vibert on 2023-03-28 12:31:08: yes this may be the way to go. But then, currently the amazed library has no knowledge of the sampling, and of the integrated spectral range of one sample. It assumes it is a dirac sampling of a convolved signal where the pixel integration is included in the LSF. Shall we had it as a parameter ? Then, strictly speaking one sample is enough to fit the amplitude if we know the redshift which may be constrained by other lines/features. And the flux variance is supposed to contain the uncertainty due to the number of samples, if the estimated variance on the flux includes the uncertainty on the redshift (and width), which is not the case currently, the estimated flux-variance currently assumes a fixed known width and position... > different conditions could also be set for redshift determination and linemeas. |