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Type:
Task
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Status: Open (View Workflow)
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Priority:
Normal
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Resolution: Unresolved
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Affects Version/s: None
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Fix Version/s: None
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Component/s: None
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Labels:None
As explained in PFS-drp:00454 (https://pfspipe.ipmu.jp/pipermail/reduction/2019/000467.html ) the image rendered by a given fiber is a function of the PSF of the incident light.
This needs to be modeled by the simulator, using an input PSF for a point source, which could possibly apply also to galaxies.
This modeling will help to determine improvements to the 2DDRP extraction kernel - ie., {{FiberTrace}, which presently assumes a uniform fiber illumination.
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DAMD-44 Add galaxy structural parameters to pfsDesign files
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- Open
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