Details
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Type:
Story
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Status: Done
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Resolution: Done
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Fix Version/s: None
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Component/s: None
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Labels:None
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Story Points:10
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Epic Link:
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Sprint:DRP S17-6
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Team:Data Release Production
Description
Augustin Guyonnet [X] has written a prototype data reduction pipeline for the Auxiliary Telescope. Merlin Fisher-Levine should become familiar with how it works, on both a practical ("press button X, Y happens") and theoretical level ("why is Y useful?") level.
This work is likely a close collaboration between Merlin & Augustin. We can most conveniently account for that by double-loading it with SPs (ie, when the two are collaborating, they burn 2 SPs every four hours of work).
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Activity
Hi Merlin,
I have attached the report on the ongoing analysis.
This has also been uploaded with the images at NERSC.
Regarding the Stack :
The first task I would like to discuss/implement would be to find the star from its astrometric coordinates.
Regarding the ongoing analysis :
there is evidence that the dispersing direction drifts from one image to the next (about .1 deg ).
This may potentially be a significant systematic : I shall look into that in more detail.
Merlin has read Augustin's report, in detail, twice. He has made notes on it, he has updated LDM-151 based on it. He says he is now familiar with it. 
I imagine a good way to start this ticket would be for Augustin Guyonnet [X] to upload the document he wrote about this stuff here, and for me to read it.
This should help address both the practical and theoretical aspects, and provide a good way to start the conversation.