2VB1: Difference between revisions

1,215 bytes added ,  11 March 2011
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  INCLUDE_RESOLUTION_RANGE=30 0.65
  INCLUDE_RESOLUTION_RANGE=30 0.65


=== XSCALE.LP main table ===
=== XSCALE.LP tables ===
 
The error model is adjusted by XSCALE:
    a        b          ISa    ISa0  INPUT DATA SET
7.094E+00  1.294E-04  33.00  38.03 ../a/XDS_ASCII.HKL                               
7.476E+00  1.170E-04  33.81  38.95 ../b/XDS_ASCII.HKL                               
7.453E+00  1.598E-04  28.98  38.00 ../c/XDS_ASCII.HKL                               
6.539E+00  1.640E-04  30.54  39.08 ../d/XDS_ASCII.HKL                               
7.304E+00  1.342E-04  31.94  37.69 ../e/XDS_ASCII.HKL                               
8.201E+00  1.574E-04  27.83  35.58 ../f/XDS_ASCII.HKL                               
8.182E+00  1.759E-04  26.36  27.60 ../g/XDS_ASCII.HKL                               
7.717E+00  3.694E-04  18.73  21.93 ../h/XDS_ASCII.HKL                               
and there are about 1500 rejected reflections.


  SUBSET OF INTENSITY DATA WITH SIGNAL/NOISE >= -3.0 AS FUNCTION OF RESOLUTION
  SUBSET OF INTENSITY DATA WITH SIGNAL/NOISE >= -3.0 AS FUNCTION OF RESOLUTION
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     total    1435805  190032    191232      99.4%      3.1%      3.3%  1434290  33.42    3.3%    3.1%    3%  0.801  170264
     total    1435805  190032    191232      99.4%      3.1%      3.3%  1434290  33.42    3.3%    3.1%    3%  0.801  170264


 
If two more resolution shells are added, they look like -
    0.64      23276    7411      9155      81.0%      35.0%    40.6%    22324    2.90    41.7%    47.9%    3%  0.683    3204
    0.63      18044    6488      9647      67.3%      42.2%    49.7%    16630    2.22    50.7%    60.9%    -5%  0.643    2437
So there is still useful signal beyond 0.65 A.


Remark: The first frames of sweeps g and h show a shadow in one corner of the detector. Nothing was done by me to exclude this shadow from processing (but one should do so if the resolution should be expanded beyond 0.65 A which the XSCALE statistics suggest to be possible). There is however no facility in XDS to exclude bad areas of specific frames in a dataset; one would need to chop the dataset into two parts.
Remark: The first frames of sweeps g and h show a shadow in one corner of the detector. Nothing was done by me to exclude this shadow from processing (but one should do so if the resolution should be expanded beyond 0.65 A which the XSCALE statistics suggest to be possible). There is however no facility in XDS to exclude bad areas of specific frames in a dataset; one would need to chop the dataset into two parts.
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