[PIPE2D-361] Select F-star candidates from the HSC data Created: 19/Feb/19 Updated: 14/Jul/23 Resolved: 14/Jul/23 |
|
| Status: | Done |
| Project: | DRP 2-D Pipeline |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Story | Priority: | Normal |
| Reporter: | hassan | Assignee: | Masayuki Tanaka |
| Resolution: | Done | Votes: | 0 |
| Labels: | f-star-selection, flux-calibration | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Issue Links: |
|
||||||||||||||||||||||||
| Story Points: | 6 | ||||||||||||||||||||||||
| Epic Link: | flux calibration | ||||||||||||||||||||||||
| Sprint: | 2DDRP-2019 C, 2DDRP-2019 E, 2DDRP-2019 G | ||||||||||||||||||||||||
| Description |
|
From existing HSC data, select F-star candidates for use in PFS flux calibration. The selection criteria should be documented, and a list of those candidates should be written to a location determined by INFRA-242 . I propose the list to be in CSV format, but that can be for discussion. |
| Comments |
| Comment by Kiyoto Yabe [ 03/Jul/23 ] |
|
This may be a task of ishigaki ? |
| Comment by Masayuki Tanaka [ 14/Jul/23 ] |
|
For FLUXSTD, we need bright stars (e.g., g<~20). They are bright enough that they can be securely selected from PS1+Gaia. HSC covers a small fraction of the sky and stars brighter than ~18th magnitudes are often saturated. So, we'd better use PS1+Gaia. I am closing this ticket but please reopen if I am missing the point of the ticket. |