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# edit [[XDS.INP]] and change/add the following: | # edit [[XDS.INP]] and change/add the following: | ||
ORGX=3130 ORGY=3040 ! for ADSC, header values are subject to interpretation; these values from visual inspection | ORGX=3130 ORGY=3040 ! for ADSC, header values are subject to interpretation; these values from visual inspection | ||
UNTRUSTED_RECTANGLE= | ! the following is for masking the beamstop shadow in sweeps c-d | ||
UNTRUSTED_RECTANGLE=0 3189 2960 3087 ! use XDS-viewer of ADXV to find the values | |||
! the following is for sweeps e-h | |||
UNTRUSTED_RECTANGLE=1 3160 3000 3070 | |||
TRUSTED_REGION=0 1.5 ! we want the whole detector area | TRUSTED_REGION=0 1.5 ! we want the whole detector area | ||
ROTATION_AXIS=-1 0 0 ! at this beamline the spindle goes backwards! | ROTATION_AXIS=-1 0 0 ! at this beamline the spindle goes backwards! | ||
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! significant for hi-res data; 34.812736=32*(value for silicon as printed to CORRECT.LP if SILICON= not given) | ! significant for hi-res data; 34.812736=32*(value for silicon as printed to CORRECT.LP if SILICON= not given) | ||
MAXIMUM_NUMBER_OF_PROCESSORS=4 ! for fast processing on a machine with many cores (e.g. for 16 cores) | MAXIMUM_NUMBER_OF_PROCESSORS=4 ! for fast processing on a machine with many cores (e.g. for 16 cores) | ||
MAXIMUM_NUMBER_OF_JOBS=6 ! "overcommit" the available cores but on the whole this produces results faster | MAXIMUM_NUMBER_OF_JOBS=6 ! "overcommit" the available cores but on the whole this produces results faster | ||
SPACE_GROUP_NUMBER=1 ! this is known | SPACE_GROUP_NUMBER=1 ! this is known | ||
UNIT_CELL_CONSTANTS= 27.07 31.25 33.76 87.98 108.00 112.11 ! from 2vb1 | UNIT_CELL_CONSTANTS= 27.07 31.25 33.76 87.98 108.00 112.11 ! from 2vb1 | ||
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INCLUDE_RESOLUTION_RANGE=30 0.65 | INCLUDE_RESOLUTION_RANGE=30 0.65 | ||
=== XSCALE.LP | === 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. It is reassuring to note that the error model works well; the ISa goes down toward sweep h probably because the crystal degrades. But see also the "a posterior remarks" below - sweep h is the one that is most affected by a shadow on the detector. | |||
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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LIMIT OBSERVED UNIQUE POSSIBLE OF DATA observed expected Corr | LIMIT OBSERVED UNIQUE POSSIBLE OF DATA observed expected Corr | ||
2.91 | 2.91 16170 2112 2147 98.4% 2.2% 2.4% 16157 78.96 2.5% 1.1% -12% 0.741 2023 | ||
2.06 | 2.06 40349 3831 3856 99.4% 2.4% 2.7% 40345 84.89 2.6% 0.9% -9% 0.764 3803 | ||
1.68 | 1.68 65329 5068 5087 99.6% 3.1% 3.2% 65321 83.77 3.3% 1.0% 0% 0.847 5020 | ||
1.45 | 1.45 73373 6147 6163 99.7% 3.2% 3.5% 73371 78.02 3.4% 1.0% 2% 0.842 6053 | ||
1.30 | 1.30 71196 6651 6657 99.9% 3.2% 3.5% 71196 71.07 3.4% 1.1% 4% 0.857 6503 | ||
1.19 | 1.19 74542 7287 7298 99.8% 3.2% 3.4% 74534 67.06 3.3% 1.2% 5% 0.854 7060 | ||
1.10 | 1.10 84918 8269 8278 99.9% 3.4% 3.7% 84891 63.24 3.6% 1.3% 7% 0.853 7988 | ||
1.03 | 1.03 87890 8584 8603 99.8% 4.1% 4.4% 87855 56.26 4.4% 1.5% 5% 0.818 8231 | ||
0.97 | 0.97 92917 9460 9465 99.9% 5.2% 5.6% 92894 48.90 5.5% 1.7% 4% 0.795 9010 | ||
0.92 | 0.92 83994 9911 9927 99.8% 5.7% 6.3% 83969 41.67 6.0% 2.0% 6% 0.787 9358 | ||
0.88 | 0.88 74100 9620 9621 100.0% 6.3% 7.1% 74082 35.74 6.7% 2.5% 4% 0.772 9040 | ||
0.84 | 0.84 81322 11511 11518 99.9% 6.9% 7.7% 81300 30.43 7.3% 3.3% 1% 0.760 10609 | ||
0.81 | 0.81 67539 10239 10247 99.9% 7.1% 7.7% 67518 25.96 7.7% 4.2% 2% 0.779 9364 | ||
0.78 | 0.78 73980 11807 11817 99.9% 7.1% 7.3% 73951 22.34 7.7% 5.3% 2% 0.799 10699 | ||
0.75 | 0.75 86111 13831 13839 99.9% 8.4% 8.6% 86076 18.77 9.2% 6.8% 2% 0.809 12496 | ||
0.73 | 0.73 64554 10481 10488 99.9% 10.3% 10.4% 64525 15.73 11.3% 8.2% 3% 0.815 9384 | ||
0.71 | 0.71 71891 11727 11741 99.9% 12.8% 13.0% 71844 12.95 14.0% 10.6% 3% 0.810 10436 | ||
0.69 | 0.69 80168 13157 13163 100.0% 16.6% 16.9% 80065 10.16 18.2% 14.1% 2% 0.799 11662 | ||
0.67 | 0.67 84431 14747 14766 99.9% 22.2% 22.7% 84231 7.44 24.4% 19.7% 3% 0.798 12520 | ||
0.65 | 0.65 61031 15592 16551 94.2% 27.6% 30.6% 60165 4.36 31.8% 33.1% 1% 0.723 9005 | ||
total | 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. | |||
== Some ''a posteriori'' remarks == | |||
* For sweeps e-h one should use TRUSTED_REGION= 0 1.2 since that already gives 0.626 A in the corners. | |||
* The first and last 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 at least if the resolution should be expanded beyond 0.65 A which the XSCALE statistics suggest to be possible). <br> One could experiment with MINIMUM_VALID_PIXEL_VALUE= 40 (or so) instead of 1 - I'd probably try that, but of course one does not want to exclude valid pixels so the result has to be carefully checked. <br> Anyway, there is no general facility in XDS to exclude bad areas of ''specific'' frames in a dataset; one needs to chop the dataset into parts and deal with each shadow separately. | |||
== Comparison of data processing: published (2006) ''vs'' XDS results == | == Comparison of data processing: published (2006) ''vs'' XDS results == | ||
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<tr><b> | <tr><b> | ||
<td> published(2006) </td> | <td> published (2006) </td> | ||
<td> 30-0.65Å (0.67-0.65Å) </td> | <td> 30-0.65Å (0.67-0.65Å) </td> | ||
<td> 1331953 (12764) </td> | <td> 1331953 (12764) </td> | ||
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<tr><b> | <tr><b> | ||
<td> XDS </td> | <td> XDS Version Dec 06, 2010 </td> | ||
<td> 30-0.65Å (0.67-0.65Å) </td> | <td> 30-0.65Å (0.67-0.65Å) </td> | ||
<td> | <td> 1435805 (61031) </td> | ||
<td> | <td> 190032 (15592) </td> | ||
<td> 7.5 (3.9) </td> | <td> 7.5 (3.9) </td> | ||
<td> 99.4 (94. | <td> 99.4 (94.2) </td> | ||
<td> 3. | <td> 3.1 (27.6) </td> | ||
<td> 33. | <td> 33.4 (4.4) </td> | ||
</b></tr> | </b></tr> | ||
</table> | </table> | ||
== Availability of data from XDS processing == | |||
I changed XSCALE.INP to have | |||
!FRIEDEL'S_LAW=TRUE ! by commenting it out XSCALE will use FRIEDEL'S_LAW=FALSE | |||
! since this is how the data were processed | |||
RESOLUTION_SHELLS=2.91 2.06 1.68 1.45 1.30 1.19 1.10 1.03 0.97 0.92 0.88 0.84 0.80 0.76 0.73 0.70 0.67 0.65 0.64 0.63 | |||
and ran XSCALE again, to get a file with reflections to 0.63 A. | |||
Conversion to other program systems is performed with XDSCONV. XDSCONV.INP for producing a MTZ file with intensities and anomalous signal is: | |||
INPUT_FILE= lys-xds.ahkl | |||
OUTPUT_FILE=temp.hkl CCP4_I | |||
After running xdsconv, I cut-and-paste the screen output: | |||
f2mtz HKLOUT temp.mtz<F2MTZ.INP | |||
cad HKLIN1 temp.mtz HKLOUT output_file_name.mtz<<EOF | |||
LABIN FILE 1 ALL | |||
END | |||
EOF | |||
and obtain output_file_name.mtz which I mv to [https://{{SERVERNAME}}/pub/xds-datared/2vb1/xds-hewl-I.mtz xds-hewl-I.mtz]. SFCHECK statistics for this file are [https://{{SERVERNAME}}/pub/xds-datared/2vb1/sfcheck_XXXX.pdf here]. | |||
Similarly, using OUTPUT_FILE=temp.hkl CCP4 I obtained a file with amplitudes, [https://{{SERVERNAME}}/pub/xds-datared/2vb1/xds-hewl-F.mtz xds-hewl-F.mtz] | |||