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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
  • more fiducial markings for geometry
  • better calibrations for motor to positions
  • hardware protection for cameras to avoid changes due to damage (camera replacement, bad-pixels)
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