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Type:
Story
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Status: Done (View Workflow)
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Priority:
Normal
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Resolution: Done
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Labels:None
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Story Points:2
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Sprint:2DDRP-2021 A
Masayuki Tanaka points out that for stars we should be tying the spectrophotometry to the psf fluxes rather than the fibre flux. The fibre fluxes are seeing-corrected, but not corrected to a large (ideally infinite) radius, so while they might provide acceptable colours they will not provide acceptable total photometry. Please add psfFlux measurements to the pfsDesign file.