[PIPE2D-824] Use data with different pupils to test FRD algorithm Created: 27/Apr/21 Updated: 13/Jan/23 |
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| Status: | Open |
| Project: | DRP 2-D Pipeline |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Task | Priority: | Normal |
| Reporter: | hassan | Assignee: | Brent Belland |
| Resolution: | Unresolved | Votes: | 0 |
| Labels: | None | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Attachments: |
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| Story Points: | 4 | ||||||||
| Sprint: | 2DDRP-2021 A 4, 2DDRP-2021 A5, 2DDRP-2021 A 6, 2DDRP-2021 A 7, 2DDRP-2021 A 8 | ||||||||
| Description |
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Please test the FRD algorithm being developed in PIPE2D-630 against SuNSS data to determine the algorithm's performance. Testing against real data is an effective way to determine how well the algorithm is performing. |
| Comments |
| Comment by ncaplar [ 19/May/21 ] |
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I have generated the post stamp images for dcb data taken with different pupils. I have posted some images of different lines to show the difference. I will upload them to Tiger with instructions soon. |
| Comment by ncaplar [ 19/May/21 ] |
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I am placing post stamp images in /tigress/ncaplar/ReducedData/Data_Jan_21. F/3.3 images in focus have exposure number: F/2.5 images in focus have exposure number: So, to get science post stamp image for spot with number '55', for Argon, taken with F/3.3 pupil, the image name is `/tigress/ncaplar/ReducedData/Data_Jan_21/sci4244023Ar_Stacked.npy`. For variance image, same except substitute sci and var (`/tigress/ncaplar/ReducedData/Data_Jan_21/var4244023Ar_Stacked.npy`) Mask images should be empty, but they are provided at same location, after substituting sci and mask (`/tigress/ncaplar/ReducedData/Data_Jan_21/mask4244023Ar_Stacked.npy`). Brent Belland, get in touch if you find any problems. |