Big-Picture To-do:
- implement algorithms (FPGA/GPU/Phi)
- implement supporting infrastructure (beam-center finding)
- validate effect of reduction on physics
- data transport
- ami support for setting drp parameters
Hutch Spreadsheets Showing Algorithms Used in 2015/2016
- amo/sxr (sioan)
- xpp/xcs (silke)
- DRP (cpo)
Possible Users To Contact
amo/sxr:
- nora berrah
- dan higley
- mankowsky
- urs staub (elsa abreu)
- marcus kubin (slow andor)
- emmanuel jal
- sam vinko
- christoph bostedt
xpp/xcs:
- timbvd
- mike kozina
- reis / mariano
- henrik
- ulvestad
- marco
SPI:
- Henry Chapman (Anton Barty, Kartik Ayyer, Andrew Morgan)
- Janos Hajdu (Filipe Maia)
- John Spence (Rick Kirian)
- Abbas Ourmazd (Peter Schwander)
- Veit Elser (Duane Loh, Ti-yen Lan)
- Jamie Sethian (Peter Zwart, Jeffrey Donatelli)
Crystallography:
- Ilme Schlichting (Thomas Barends, Lutz Foucar)
- Nick Sauter (Aaron Brewster)
- Henry Chapman (Anton Barty, Thomas White)
- Axel Brunger (Artem Lyubimov, Monarin Uervirojnangkoorn)
- Petra Fromme (Nadia Zatsepin)
- James Holton
Possible Simplifying Requirements
- don't change geometry
- if you do change geometry have a way to get new geometry info in a standard way
- stable beam-center (um, jets 50um). standard way to get beam center
- stable jets
- make jets/beam comparable unless you need stable to a pixel-size
- stable experimental setup
- don't switch between sparse/dense photon cases for spectrometer, and/or understand in advance
- measure detector tilts
- avoid double-beam-focus seen in SPI
- smaller pixels would mean photons don't occupy single-pixels, and we would get fooled less by hot-pixels
- gravity sensors on cameras
Overview
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