1Y13: Difference between revisions

374 bytes added ,  17 March 2011
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== dataset E1 ==
== dataset E1 ==


Use [[generate_XDS.INP]] and run xds once. Based on R-factors and an inspection of BKGPIX.cbf, I modified the resulting XDS.INP to have
Use [[generate_XDS.INP]] and run xds once. Based on R-factors in the resulting CORRECT.LP, and an inspection of BKGPIX.cbf, I modified XDS.INP to have
  INCLUDE_RESOLUTION_RANGE=50 2.1
  INCLUDE_RESOLUTION_RANGE=40 2.1                      ! too weak beyond 2.1
  VALUE_RANGE_FOR_TRUSTED_DETECTOR_PIXELS=8000. 30000.  
  VALUE_RANGE_FOR_TRUSTED_DETECTOR_PIXELS=8000. 30000. ! raised from 7000 30000 to mask beamstop
and ran xds again. This is the excerpt from CORRECT.LP :
and ran xds again. This is the excerpt from CORRECT.LP :
   
   
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</pre>
</pre>
and
and
<pre>
   Spacegroup        TotProb SysAbsProb    Reindex        Conditions
   Spacegroup        TotProb SysAbsProb    Reindex        Conditions
 
   <P 41 21 2> ( 92)    0.823  0.823                        00l: l=4n, h00: h=2n (zones 1,2)
   <P 41 21 2> ( 92)    0.823  0.823                        00l: l=4n, h00: h=2n (zones 1,2)
   <P 43 21 2> ( 96)    0.823  0.823                        00l: l=4n, h00: h=2n (zones 1,2)
   <P 43 21 2> ( 96)    0.823  0.823                        00l: l=4n, h00: h=2n (zones 1,2)
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     ..........
     ..........
   <P 42 21 2> ( 94)    0.077  0.077                        00l: l=2n, h00: h=2n (zones 1,2)
   <P 42 21 2> ( 94)    0.077  0.077                        00l: l=2n, h00: h=2n (zones 1,2)
 
</pre>
Thus suggesting #92 or #96 - the latter of which agrees with the PDB deposition. Running CORRECT in #96, we obtain:
Thus suggesting #92 or #96 - the latter of which agrees with the PDB deposition. However, running CORRECT in #96 and specifying 103 103 130 90 90 90 as cell parameters, we obtain:


  REFINED PARAMETERS:  DISTANCE BEAM ORIENTATION CELL AXIS                   
  REFINED PARAMETERS:  DISTANCE BEAM ORIENTATION CELL AXIS                   
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  NUMBER OF UNIQUE ACCEPTED REFLECTIONS                79022
  NUMBER OF UNIQUE ACCEPTED REFLECTIONS                79022


so there may be something wrong with the data processing.  
which is much worse than the spacegroup 19 statistics (compare the ISa values - they differ by a factor of 2 !) so there may be something wrong with some assumptions we were making ...


The easiest thing one can do is to inspect INTEGRATE.LP - this lists scale factor, beam divergence and mosaicity for every reflection. There's a [[jiffies|jiffy]] called "scalefactors" which grep's the relevant lines from INTEGRATE.LP
The easiest thing one can do is to inspect INTEGRATE.LP - this lists scale factor, beam divergence and mosaicity for every reflection. There's a [[jiffies|jiffy]] called "scalefactors" which grep's the relevant lines from INTEGRATE.LP. This shows the scale factor (column 3):
[[File:1y13-e1-scales.png]]
2,684

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