[PIPE2D-991] Code to make a synthetic broadband photometry table of AMBRE Created: 28/Feb/22 Updated: 03/Jun/22 Resolved: 03/Jun/22 |
|
| Status: | Done |
| Project: | DRP 2-D Pipeline |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Task | Priority: | Normal |
| Reporter: | Takuji Yamashita | Assignee: | Takuji Yamashita |
| Resolution: | Done | Votes: | 0 |
| Labels: | model-templates | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Epic Link: | flux calibration |
| Reviewers: | hassan |
| Description |
|
A synthetic broadband photometry table of AMBRE model templates is used for broadband SED fitting in flux calibration. This table is generated from the model template set on the user side. I provide a code to make the table in the drp_fstar repository. |
| Comments |
| Comment by Takuji Yamashita [ 03/Jun/22 ] |
|
Because the size of this table is small, we provide it together with an AMBRE model template set. The current model set and the broad-band flux table are provided in PIPE2D-1044. So, I will close this ticket. |
| Comment by Takuji Yamashita [ 03/Jun/22 ] |
|
This work is included in |