[INSTRM-1081] Predicting stellar flux on AG camera from Gaia magnitudes Created: 02/Oct/20 Updated: 14/Mar/23 Resolved: 14/Mar/23 |
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| Status: | Won't Fix |
| Project: | Instrument control development |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Task | Priority: | Normal |
| Reporter: | naoyuki.tamura | Assignee: | Unassigned |
| Resolution: | Won't Fix | Votes: | 0 |
| Labels: | None | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Issue Links: |
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| Description |
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As we briefly discussed at the ICS/PFI+MCS telecon on Sep 18 2020, if we can predict stellar flux coming onto AG camera detector based on Gaia magnitudes taking into account the WFC, Field Element, and AG filter transmission curves, then we can estimate the sky transparency during field acquisition and auto guiding. |
| Comments |
| Comment by yuki.moritani [ 14/Mar/23 ] |
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Duplicated to |