[INSTRM-927] Model sky contribution from AG image Created: 20/Mar/20 Updated: 18/Feb/22 Resolved: 18/Feb/22 |
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| Status: | Done |
| Project: | Instrument control development |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Task | Priority: | Normal |
| Reporter: | hassan | Assignee: | chyan |
| Resolution: | Done | Votes: | 0 |
| Labels: | EngRun | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Issue Links: |
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| Story Points: | 4 | ||||||||||||||||
| Sprint: | PreEngRun05 A, PreEngRun05 B, PreEngRun05 C | ||||||||||||||||
| Reviewers: | hassan | ||||||||||||||||
| Description |
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Construct a model for the sky. This will be subsequently used for sky subtraction |
| Comments |
| Comment by rhl [ 21/Mar/20 ] |
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The "model" will presumably be very simple, the number of photons/second/arcsec^2 on the AG should be sufficient. It'd probably be good enough to report DN/second/pixel as we can probably calibrate the flux measured by the AG to the sky fibres directly. |
| Comment by chyan [ 18/Feb/22 ] |
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This is related to |