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Revision as of 21:00, 27 February 2010
, 21:00, 27 February 2010→autoxds
== autoxds ==
== autoxds ==
script developed by Michel Fodje at Canadian Macromolecular Crystallography Facility (Saskatoon) and in use e.g. at SSRL (Stanford) . See [A Quick XDS Tutorial for SSRL http://smb.slac.stanford.edu/facilities/software/xds/]. Download: http://smb.slac.stanford.edu/templates/xds/autoxds ; download http://smb.slac.stanford.edu/templates/xds/mccd_xdsparams.pl , too!
script in use at SSRL (Stanford) . See [A Quick XDS Tutorial for SSRL http://smb.slac.stanford.edu/facilities/software/xds/]. Download: http://smb.slac.stanford.edu/templates/xds/autoxds ; download http://smb.slac.stanford.edu/templates/xds/mccd_xdsparams.pl , too!
== autoXDS ==
script developed by Michel Fodje at Canadian Macromolecular Crystallography Facility (Saskatoon)
== xdsme ==
by Pierre Legrand at SOLEIL (French synchrotron): web address: http://code.google.com/p/xdsme/
Here's a short description of the program:
xdsme is a collection of python scripts made to simplify the processing of crystal
diffraction images with the XDS Program Package. Provided that the diffraction
parameters are well recorded in the diffraction image headers, XDS data processing
can be started with a simple command line like:
$ xdsme pos1_1_???.img
Supported detector image format include: ADSC, MARCCD, MAR345 + experimental
for PILATUS, SATURN, RAXIS and MAR555.
* xdsme (XDS.py), xscale.py and xdsconv.py for data processing, scaling and file conversion.
* XOalign.py for the goniometer setting calculation (to work with different type of goniometer including Kappa, mini-Kappa, Euler...).
* xds2mos.py or xds2dnz.py ... (for conversion of orientation matrices)
