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Scripts and interfaces: Difference between revisions
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== autoxds == | == autoxds == | ||
script | 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) | |||