[PIPE2D-852] Code implementation of broad-band SED fitting for flux calibration Created: 17/Jun/21 Updated: 15/Jul/21 Resolved: 07/Jul/21 |
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| Status: | Done |
| Project: | DRP 2-D Pipeline |
| Component/s: | None |
| Affects Version/s: | None |
| Fix Version/s: | None |
| Type: | Task | Priority: | Normal |
| Reporter: | sogo.mineo | Assignee: | sogo.mineo |
| Resolution: | Done | Votes: | 0 |
| Labels: | flux-calibration | ||
| Remaining Estimate: | Not Specified | ||
| Time Spent: | Not Specified | ||
| Original Estimate: | Not Specified | ||
| Issue Links: |
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| Epic Link: | flux calibration | ||||||||
| Reviewers: | price | ||||||||
| Description |
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Write a code to derive a probability distribution function from broad-band SED fitting of a standard star, and implement it to the flux calibration part in 2DDRP Pipeline. A draft of the code was provided from Takuji Yamashita. |
| Comments |
| Comment by sogo.mineo [ 01/Jul/21 ] |
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I opened two pull requests for this issue: https://github.com/Subaru-PFS/drp_stella/pull/204 Could you review them? FitBroadbandSEDTask introduced by these changes will be a subtask of Yamashita-san's flux calibration. This task is given several fiber fluxes and returns probabilities for various SEDs. Yamashita-san's flux calibration will take these probabilities into account in order to determine the best SED for observed spectra. |
| Comment by sogo.mineo [ 07/Jul/21 ] |
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Thanks for review. Merged to master. |