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This reports processing of triclinic hen egg-white lysozyme data @ 0.65Å resolution (PDB id [ | This reports processing of triclinic hen egg-white lysozyme data @ 0.65Å resolution (PDB id [http://www.rcsb.org/pdb/explore/explore.do?structureId=2VB1 2VB1]). Data (sweeps a to h, each comprising 60 to 360 frames of 72MB) were collected by Zbigniew Dauter at APS 19-ID and are available from [http://bl831.als.lbl.gov/example_data_sets/APS/19-ID/2vb1/ here]. Details of data collection, processing and refinement are [http://journals.iucr.org/d/issues/2007/12/00/be5097/index.html published]. | ||
== XDS processing == | == XDS processing == | ||
# use [[generate_XDS.INP]] to obtain a good starting point | # use [[generate_XDS.INP]] to obtain a good starting point | ||
# edit [[XDS.INP]] and change the following: | # edit [[XDS.INP]] and change/add the following: | ||
ORGX=3130 ORGY=3040 ! for ADSC, header values are subject to interpretation; | ORGX=3130 ORGY=3040 ! for ADSC, header values are subject to interpretation; these values from visual inspection | ||
UNTRUSTED_RECTANGLE=1 3160 3000 3070 ! <xmin xmax ymin ymax> to mask shadow of beamstop; XDS-viewer to find out | |||
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! | ||
SILICON=34.812736 ! account for theta-dependant absorption in the CCD's phosphor. The correction is only | |||
! 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, use (e.g. for 16 cores) | |||
MAXIMUM_NUMBER_OF_JOBS=6 ! This "overcommits" the available cores but on the whole this produces results faster (see below). | |||
SPACE_GROUP_NUMBER=1 ! this is known | |||
UNIT_CELL_CONSTANTS= 27.07 31.25 33.76 87.98 108.00 112.11 ! from 2vb1 | |||
FRIEDEL'S_LAW=TRUE ! we're not concerned with the anomalous signal | |||
Then, run "xds_par". It completes after about 5 minutes on a fast machine, and we may inspect (at least) IDXREF.LP and CORRECT.LP (see below), and use "XDS-viewer FRAME.cbf" to get a visual impression of the integration as it applies to the last frame. | |||
By inspecting IDXREF.LP, one should make sure that everything works as it should, i.e. that a large percentage of reflections was actually indexed nicely, e.g.: | |||
... | ... | ||
Line 25: | Line 31: | ||
STANDARD DEVIATION OF SPINDLE POSITION (DEGREES) 0.12 | STANDARD DEVIATION OF SPINDLE POSITION (DEGREES) 0.12 | ||
=== Optimization === | === Optimization === | ||
The main target of optimization is the | The main target of optimization is the asymptotic (i.e. best) I/sigma (ISa) (Diederichs (2010) [http://dx.doi.org/10.1107/S0907444910014836 Acta Cryst. D 66, 733-40]) as printed out by CORRECT (and XSCALE). A higher ISa should mean better data. | ||
However: ISa also rises if more reflections are thrown out as outliers ("misfits") so it is not considered to be optimization if just WFAC1 is reduced. Please note that the default WFAC1 is 1; this should result in the rejection of about 1% of observations. If you feel that 1% is too much then just increase WFAC1, to, say, 1.5 - that should result in rejection of less than 0.1%. This will slightly increase completeness, but will reduce I/sigma and ISa, and increase R-factors. | However: ISa also rises if more reflections are thrown out as outliers ("misfits") so it is not considered to be optimization if just WFAC1 is reduced. Please note that the default WFAC1 is 1; this should result in the rejection of about 1% of observations. If you feel that 1% is too much then just increase WFAC1, to, say, 1.5 - that should result in rejection of less than (say) 0.1%. This will slightly increase completeness, but will reduce I/sigma and ISa, and increase R-factors. | ||
The following quantities may be tested for their influence on ISa: | The following quantities may be tested for their influence on ISa: | ||
Line 43: | Line 43: | ||
REFLECTING_RANGE= 0.669 REFLECTING_RANGE_E.S.D.= 0.096 | REFLECTING_RANGE= 0.669 REFLECTING_RANGE_E.S.D.= 0.096 | ||
copy these two lines into XDS.INP | copy these two lines into XDS.INP | ||
* prevent refinement in INTEGRATE: REFINE(INTEGRATE)= ! | |||
== Example: sweep e == | == Example: sweep e == | ||
=== [[XDS.INP]]; as generated by [[generate_XDS.INP]] === | === [[XDS.INP]]; as generated by [[generate_XDS.INP]] === | ||
... | generate_XDS.INP "../../APS/19-ID/2vb1/p1lyso_e.0???.img" | ||
Then include the changes detailed above, resulting in: | |||
<pre> | <pre> | ||
JOB= XYCORR INIT COLSPOT IDXREF DEFPIX INTEGRATE CORRECT | JOB= XYCORR INIT COLSPOT IDXREF DEFPIX INTEGRATE CORRECT | ||
MAXIMUM_NUMBER_OF_PROCESSORS= | MAXIMUM_NUMBER_OF_PROCESSORS=4 | ||
MAXIMUM_NUMBER_OF_JOBS= | MAXIMUM_NUMBER_OF_JOBS=6 | ||
ORGX= 3130 ORGY= 3040 ! check these values with adxv ! | ORGX= 3130 ORGY= 3040 ! check these values with adxv ! | ||
UNTRUSTED_RECTANGLE=1 3160 3000 3070 ! <xmin xmax ymin ymax> to mask shadow of beamstop; XDS-viewer to find out | |||
DETECTOR_DISTANCE= 99.9954 | DETECTOR_DISTANCE= 99.9954 | ||
OSCILLATION_RANGE= 0.500 | OSCILLATION_RANGE= 0.500 | ||
Line 64: | Line 67: | ||
! BACKGROUND_RANGE=1 10 ! rather use defaults (first 5 degree of rotation) | ! BACKGROUND_RANGE=1 10 ! rather use defaults (first 5 degree of rotation) | ||
SPACE_GROUP_NUMBER= | SPACE_GROUP_NUMBER=1 ! 0 if unknown | ||
UNIT_CELL_CONSTANTS= | UNIT_CELL_CONSTANTS= 27.07 31.25 33.76 87.98 108.00 112.11 ! PDB 2vb1 | ||
INCLUDE_RESOLUTION_RANGE=50 0 ! after CORRECT, insert high resol limit; re-run CORRECT | INCLUDE_RESOLUTION_RANGE=50 0 ! after CORRECT, insert high resol limit; re-run CORRECT | ||
FRIEDEL'S_LAW=FALSE ! This acts only on the CORRECT step | !FRIEDEL'S_LAW=FALSE ! This acts only on the CORRECT step | ||
! If the anom signal turns out to be, or is known to be, very low or absent, | ! If the anom signal turns out to be, or is known to be, very low or absent, | ||
! use FRIEDEL'S_LAW=TRUE instead (or comment out the line); re-run CORRECT | ! use FRIEDEL'S_LAW=TRUE instead (or comment out the line); re-run CORRECT | ||
Line 92: | Line 95: | ||
! parameters specifically for this detector and beamline: | ! parameters specifically for this detector and beamline: | ||
DETECTOR= ADSC MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65000 | DETECTOR= ADSC MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65000 | ||
SENSOR_THICKNESS=0.01 SILICON=34.812736 | |||
NX= 6144 NY= 6144 QX= 0.051294 QY= 0.051294 ! to make CORRECT happy if frames are unavailable | NX= 6144 NY= 6144 QX= 0.051294 QY= 0.051294 ! to make CORRECT happy if frames are unavailable | ||
DIRECTION_OF_DETECTOR_X-AXIS=1 0 0 | DIRECTION_OF_DETECTOR_X-AXIS=1 0 0 | ||
Line 102: | Line 106: | ||
</pre> | </pre> | ||
=== [[CORRECT.LP]] | === [[CORRECT.LP]] 1st pass === | ||
STANDARD DEVIATION OF SPOT POSITION (PIXELS) 0.87 | |||
STANDARD DEVIATION OF SPINDLE POSITION (DEGREES) 0.10 | |||
CRYSTAL MOSAICITY (DEGREES) 0.126 | |||
... | |||
a b ISa | |||
6.630E+00 1.091E-04 37.18 | |||
... | |||
SUBSET OF INTENSITY DATA WITH SIGNAL/NOISE >= -3.0 AS FUNCTION OF RESOLUTION | |||
RESOLUTION NUMBER OF REFLECTIONS COMPLETENESS R-FACTOR R-FACTOR COMPARED I/SIGMA R-meas Rmrgd-F Anomal SigAno Nano | |||
LIMIT OBSERVED UNIQUE POSSIBLE OF DATA observed expected Corr | |||
1.77 9195 4841 9501 51.0% 1.5% 1.5% 8708 48.74 2.1% 1.6% 0% 0.000 0 | |||
1.26 29991 15327 16721 91.7% 1.5% 1.6% 29328 45.26 2.1% 1.7% 0% 0.000 0 | |||
1.03 38643 19731 21636 91.2% 1.7% 1.7% 37824 38.67 2.5% 2.1% 0% 0.000 0 | |||
0.89 46156 23404 25561 91.6% 2.3% 2.4% 45504 27.56 3.3% 3.4% 0% 0.000 0 | |||
0.80 51509 26034 28868 90.2% 4.0% 4.0% 50950 17.55 5.6% 7.0% 0% 0.000 0 | |||
0.73 55989 28253 32034 88.2% 7.0% 6.8% 55472 10.98 9.8% 13.2% 0% 0.000 0 | |||
0.68 59733 30115 34776 86.6% 13.1% 13.0% 59236 6.08 18.6% 26.0% 0% 0.000 0 | |||
0.63 35385 18436 37367 49.3% 25.6% 26.9% 33898 2.99 36.3% 52.1% 0% 0.000 0 | |||
0.60 8991 4972 39725 12.5% 51.2% 56.9% 8038 1.34 72.4% 105.0% 0% 0.000 0 | |||
total 335592 171113 246189 69.5% 2.3% 2.4% 328958 19.58 3.3% 7.4% 0% 0.000 0 | |||
NUMBER OF REFLECTIONS IN SELECTED SUBSET OF IMAGES 343716 | |||
NUMBER OF REJECTED MISFITS 8112 | |||
NUMBER OF SYSTEMATIC ABSENT REFLECTIONS 0 | |||
NUMBER OF ACCEPTED OBSERVATIONS 335604 | |||
NUMBER OF UNIQUE ACCEPTED REFLECTIONS 171119 | |||
The number of "misfits" (rejections) is higher than expected (1 %). Either one considers the anomalous signal (of the 6 sulfurs) to be significant, or one simply increases WFAC1 from its default of 1, to (say) 1.2 . | |||
=== [[XDS.INP]]; optimized === | |||
Using the output of "grep _E INTEGRATE.LP|tail -2" edit XDS.INP to have | |||
JOB= INTEGRATE CORRECT | |||
BEAM_DIVERGENCE= 0.428 BEAM_DIVERGENCE_E.S.D.= 0.043 | |||
REFLECTING_RANGE= 0.880 REFLECTING_RANGE_E.S.D.= 0.126 | |||
... | |||
REFINE(INTEGRATE)= ! | |||
Then "cp GXPARM.XDS XPARM.XDS", and then another round of "xds_par". Five minutes later, we get: | |||
=== [[CORRECT.LP]] optimization pass === | |||
This looks a little bit better - less standard deviation, higher ISa, better R-factors, less misfits: | |||
= | STANDARD DEVIATION OF SPOT POSITION (PIXELS) 0.83 | ||
STANDARD DEVIATION OF SPINDLE POSITION (DEGREES) 0.08 | |||
CRYSTAL MOSAICITY (DEGREES) 0.096 | |||
a b ISa | |||
6.439E+00 1.076E-04 37.98 | |||
... | |||
SUBSET OF INTENSITY DATA WITH SIGNAL/NOISE >= -3.0 AS FUNCTION OF RESOLUTION | |||
RESOLUTION NUMBER OF REFLECTIONS COMPLETENESS R-FACTOR R-FACTOR COMPARED I/SIGMA R-meas Rmrgd-F Anomal SigAno Nano | |||
LIMIT OBSERVED UNIQUE POSSIBLE OF DATA observed expected Corr | |||
1.77 9149 4817 9501 50.7% 1.5% 1.5% 8664 49.75 2.1% 1.5% 0% 0.000 0 | |||
1.26 30049 15348 16723 91.8% 1.5% 1.6% 29402 46.26 2.1% 1.6% 0% 0.000 0 | |||
1.03 38920 19863 21637 91.8% 1.7% 1.7% 38114 39.61 2.4% 2.0% 0% 0.000 0 | |||
0.89 46381 23508 25562 92.0% 2.2% 2.3% 45746 28.39 3.1% 3.2% 0% 0.000 0 | |||
0.80 51605 26071 28868 90.3% 3.8% 3.8% 51068 18.21 5.3% 6.5% 0% 0.000 0 | |||
0.73 56126 28314 32041 88.4% 6.6% 6.4% 55624 11.45 9.3% 12.3% 0% 0.000 0 | |||
0.68 59735 30093 34771 86.5% 12.6% 12.3% 59284 6.34 17.8% 24.8% 0% 0.000 0 | |||
0.63 35754 18620 37370 49.8% 24.1% 25.5% 34268 3.11 34.1% 48.9% 0% 0.000 0 | |||
0.60 9180 5075 39730 12.8% 48.6% 54.3% 8210 1.40 68.7% 100.5% 0% 0.000 0 | |||
total 336899 171709 246203 69.7% 2.2% 2.3% 330380 20.14 3.2% 6.9% 0% 0.000 0 | |||
NUMBER OF REFLECTIONS IN SELECTED SUBSET OF IMAGES 344751 | |||
NUMBER OF REJECTED MISFITS 7842 | |||
NUMBER OF SYSTEMATIC ABSENT REFLECTIONS 0 | |||
NUMBER OF ACCEPTED OBSERVATIONS 336909 | |||
NUMBER OF UNIQUE ACCEPTED REFLECTIONS 171714 | |||
Revision as of 16:38, 11 March 2011
This reports processing of triclinic hen egg-white lysozyme data @ 0.65Å resolution (PDB id 2VB1). Data (sweeps a to h, each comprising 60 to 360 frames of 72MB) were collected by Zbigniew Dauter at APS 19-ID and are available from here. Details of data collection, processing and refinement are published.
XDS processing
- use generate_XDS.INP to obtain a good starting point
- 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 UNTRUSTED_RECTANGLE=1 3160 3000 3070 ! <xmin xmax ymin ymax> to mask shadow of beamstop; XDS-viewer to find out TRUSTED_REGION=0 1.5 ! we want the whole detector area ROTATION_AXIS=-1 0 0 ! at this beamline the spindle goes backwards! SILICON=34.812736 ! account for theta-dependant absorption in the CCD's phosphor. The correction is only ! 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, use (e.g. for 16 cores) MAXIMUM_NUMBER_OF_JOBS=6 ! This "overcommits" the available cores but on the whole this produces results faster (see below). SPACE_GROUP_NUMBER=1 ! this is known UNIT_CELL_CONSTANTS= 27.07 31.25 33.76 87.98 108.00 112.11 ! from 2vb1 FRIEDEL'S_LAW=TRUE ! we're not concerned with the anomalous signal
Then, run "xds_par". It completes after about 5 minutes on a fast machine, and we may inspect (at least) IDXREF.LP and CORRECT.LP (see below), and use "XDS-viewer FRAME.cbf" to get a visual impression of the integration as it applies to the last frame. By inspecting IDXREF.LP, one should make sure that everything works as it should, i.e. that a large percentage of reflections was actually indexed nicely, e.g.:
... 63879 OUT OF 72321 SPOTS INDEXED. ... ***** DIFFRACTION PARAMETERS USED AT START OF INTEGRATION ***** REFINED VALUES OF DIFFRACTION PARAMETERS DERIVED FROM 63879 INDEXED SPOTS REFINED PARAMETERS: DISTANCE BEAM AXIS CELL ORIENTATION STANDARD DEVIATION OF SPOT POSITION (PIXELS) 0.53 STANDARD DEVIATION OF SPINDLE POSITION (DEGREES) 0.12
Optimization
The main target of optimization is the asymptotic (i.e. best) I/sigma (ISa) (Diederichs (2010) Acta Cryst. D 66, 733-40) as printed out by CORRECT (and XSCALE). A higher ISa should mean better data.
However: ISa also rises if more reflections are thrown out as outliers ("misfits") so it is not considered to be optimization if just WFAC1 is reduced. Please note that the default WFAC1 is 1; this should result in the rejection of about 1% of observations. If you feel that 1% is too much then just increase WFAC1, to, say, 1.5 - that should result in rejection of less than (say) 0.1%. This will slightly increase completeness, but will reduce I/sigma and ISa, and increase R-factors.
The following quantities may be tested for their influence on ISa:
- copying GXPARM.XDS to XPARM.XDS
- including the information from the first integration pass into XDS.INP - just do "grep _E INTEGRATE.LP|tail -2" and get e.g.
BEAM_DIVERGENCE= 0.386 BEAM_DIVERGENCE_E.S.D.= 0.039 REFLECTING_RANGE= 0.669 REFLECTING_RANGE_E.S.D.= 0.096
copy these two lines into XDS.INP
- prevent refinement in INTEGRATE: REFINE(INTEGRATE)= !
Example: sweep e
XDS.INP; as generated by generate_XDS.INP
generate_XDS.INP "../../APS/19-ID/2vb1/p1lyso_e.0???.img"
Then include the changes detailed above, resulting in:
JOB= XYCORR INIT COLSPOT IDXREF DEFPIX INTEGRATE CORRECT MAXIMUM_NUMBER_OF_PROCESSORS=4 MAXIMUM_NUMBER_OF_JOBS=6 ORGX= 3130 ORGY= 3040 ! check these values with adxv ! UNTRUSTED_RECTANGLE=1 3160 3000 3070 ! <xmin xmax ymin ymax> to mask shadow of beamstop; XDS-viewer to find out DETECTOR_DISTANCE= 99.9954 OSCILLATION_RANGE= 0.500 X-RAY_WAVELENGTH= 0.6525486 NAME_TEMPLATE_OF_DATA_FRAMES=../../APS/19-ID/2vb1/p1lyso_e.0???.img ! REFERENCE_DATA_SET=xxx/XDS_ASCII.HKL ! e.g. to ensure consistent indexing DATA_RANGE=1 360 SPOT_RANGE=1 180 ! BACKGROUND_RANGE=1 10 ! rather use defaults (first 5 degree of rotation) SPACE_GROUP_NUMBER=1 ! 0 if unknown UNIT_CELL_CONSTANTS= 27.07 31.25 33.76 87.98 108.00 112.11 ! PDB 2vb1 INCLUDE_RESOLUTION_RANGE=50 0 ! after CORRECT, insert high resol limit; re-run CORRECT !FRIEDEL'S_LAW=FALSE ! This acts only on the CORRECT step ! If the anom signal turns out to be, or is known to be, very low or absent, ! use FRIEDEL'S_LAW=TRUE instead (or comment out the line); re-run CORRECT ! remove the "!" in the following line: ! STRICT_ABSORPTION_CORRECTION=TRUE ! if the anomalous signal is strong: in that case, in CORRECT.LP the three ! "CHI^2-VALUE OF FIT OF CORRECTION FACTORS" values are significantly> 1, e.g. 1.5 ! ! exclude (mask) untrusted areas of detector, e.g. beamstop shadow : ! UNTRUSTED_RECTANGLE= 1800 1950 2100 2150 ! x-min x-max y-min y-max ! repeat ! UNTRUSTED_ELLIPSE= 2034 2070 1850 2240 ! x-min x-max y-min y-max ! if needed ! ! parameters with changes wrt default values: TRUSTED_REGION=0.00 1.5 ! partially use corners of detectors; 1.41421=full use VALUE_RANGE_FOR_TRUSTED_DETECTOR_PIXELS=7000. 30000. ! often 8000 is ok MINIMUM_ZETA=0.05 ! integrate close to the Lorentz zone; 0.15 is default STRONG_PIXEL=6 ! COLSPOT: only use strong reflections (default is 3) MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT=3 ! default of 6 is sometimes too high REFINE(INTEGRATE)=CELL BEAM ORIENTATION ! AXIS DISTANCE ! parameters specifically for this detector and beamline: DETECTOR= ADSC MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65000 SENSOR_THICKNESS=0.01 SILICON=34.812736 NX= 6144 NY= 6144 QX= 0.051294 QY= 0.051294 ! to make CORRECT happy if frames are unavailable DIRECTION_OF_DETECTOR_X-AXIS=1 0 0 DIRECTION_OF_DETECTOR_Y-AXIS=0 1 0 INCIDENT_BEAM_DIRECTION=0 0 1 ROTATION_AXIS=-1 0 0 ! at e.g. SERCAT ID-22 this needs to be -1 0 0 FRACTION_OF_POLARIZATION=0.98 ! better value is provided by beamline staff! POLARIZATION_PLANE_NORMAL=0 1 0
CORRECT.LP 1st pass
STANDARD DEVIATION OF SPOT POSITION (PIXELS) 0.87 STANDARD DEVIATION OF SPINDLE POSITION (DEGREES) 0.10 CRYSTAL MOSAICITY (DEGREES) 0.126 ... a b ISa 6.630E+00 1.091E-04 37.18 ... SUBSET OF INTENSITY DATA WITH SIGNAL/NOISE >= -3.0 AS FUNCTION OF RESOLUTION RESOLUTION NUMBER OF REFLECTIONS COMPLETENESS R-FACTOR R-FACTOR COMPARED I/SIGMA R-meas Rmrgd-F Anomal SigAno Nano LIMIT OBSERVED UNIQUE POSSIBLE OF DATA observed expected Corr 1.77 9195 4841 9501 51.0% 1.5% 1.5% 8708 48.74 2.1% 1.6% 0% 0.000 0 1.26 29991 15327 16721 91.7% 1.5% 1.6% 29328 45.26 2.1% 1.7% 0% 0.000 0 1.03 38643 19731 21636 91.2% 1.7% 1.7% 37824 38.67 2.5% 2.1% 0% 0.000 0 0.89 46156 23404 25561 91.6% 2.3% 2.4% 45504 27.56 3.3% 3.4% 0% 0.000 0 0.80 51509 26034 28868 90.2% 4.0% 4.0% 50950 17.55 5.6% 7.0% 0% 0.000 0 0.73 55989 28253 32034 88.2% 7.0% 6.8% 55472 10.98 9.8% 13.2% 0% 0.000 0 0.68 59733 30115 34776 86.6% 13.1% 13.0% 59236 6.08 18.6% 26.0% 0% 0.000 0 0.63 35385 18436 37367 49.3% 25.6% 26.9% 33898 2.99 36.3% 52.1% 0% 0.000 0 0.60 8991 4972 39725 12.5% 51.2% 56.9% 8038 1.34 72.4% 105.0% 0% 0.000 0 total 335592 171113 246189 69.5% 2.3% 2.4% 328958 19.58 3.3% 7.4% 0% 0.000 0 NUMBER OF REFLECTIONS IN SELECTED SUBSET OF IMAGES 343716 NUMBER OF REJECTED MISFITS 8112 NUMBER OF SYSTEMATIC ABSENT REFLECTIONS 0 NUMBER OF ACCEPTED OBSERVATIONS 335604 NUMBER OF UNIQUE ACCEPTED REFLECTIONS 171119
The number of "misfits" (rejections) is higher than expected (1 %). Either one considers the anomalous signal (of the 6 sulfurs) to be significant, or one simply increases WFAC1 from its default of 1, to (say) 1.2 .
XDS.INP; optimized
Using the output of "grep _E INTEGRATE.LP|tail -2" edit XDS.INP to have
JOB= INTEGRATE CORRECT BEAM_DIVERGENCE= 0.428 BEAM_DIVERGENCE_E.S.D.= 0.043 REFLECTING_RANGE= 0.880 REFLECTING_RANGE_E.S.D.= 0.126 ... REFINE(INTEGRATE)= !
Then "cp GXPARM.XDS XPARM.XDS", and then another round of "xds_par". Five minutes later, we get:
CORRECT.LP optimization pass
This looks a little bit better - less standard deviation, higher ISa, better R-factors, less misfits:
STANDARD DEVIATION OF SPOT POSITION (PIXELS) 0.83 STANDARD DEVIATION OF SPINDLE POSITION (DEGREES) 0.08 CRYSTAL MOSAICITY (DEGREES) 0.096 a b ISa 6.439E+00 1.076E-04 37.98 ... SUBSET OF INTENSITY DATA WITH SIGNAL/NOISE >= -3.0 AS FUNCTION OF RESOLUTION RESOLUTION NUMBER OF REFLECTIONS COMPLETENESS R-FACTOR R-FACTOR COMPARED I/SIGMA R-meas Rmrgd-F Anomal SigAno Nano LIMIT OBSERVED UNIQUE POSSIBLE OF DATA observed expected Corr 1.77 9149 4817 9501 50.7% 1.5% 1.5% 8664 49.75 2.1% 1.5% 0% 0.000 0 1.26 30049 15348 16723 91.8% 1.5% 1.6% 29402 46.26 2.1% 1.6% 0% 0.000 0 1.03 38920 19863 21637 91.8% 1.7% 1.7% 38114 39.61 2.4% 2.0% 0% 0.000 0 0.89 46381 23508 25562 92.0% 2.2% 2.3% 45746 28.39 3.1% 3.2% 0% 0.000 0 0.80 51605 26071 28868 90.3% 3.8% 3.8% 51068 18.21 5.3% 6.5% 0% 0.000 0 0.73 56126 28314 32041 88.4% 6.6% 6.4% 55624 11.45 9.3% 12.3% 0% 0.000 0 0.68 59735 30093 34771 86.5% 12.6% 12.3% 59284 6.34 17.8% 24.8% 0% 0.000 0 0.63 35754 18620 37370 49.8% 24.1% 25.5% 34268 3.11 34.1% 48.9% 0% 0.000 0 0.60 9180 5075 39730 12.8% 48.6% 54.3% 8210 1.40 68.7% 100.5% 0% 0.000 0 total 336899 171709 246203 69.7% 2.2% 2.3% 330380 20.14 3.2% 6.9% 0% 0.000 0 NUMBER OF REFLECTIONS IN SELECTED SUBSET OF IMAGES 344751 NUMBER OF REJECTED MISFITS 7842 NUMBER OF SYSTEMATIC ABSENT REFLECTIONS 0 NUMBER OF ACCEPTED OBSERVATIONS 336909 NUMBER OF UNIQUE ACCEPTED REFLECTIONS 171714
XSCALE results
a few sweeps were optimized by copying the two lines containing mosaicity and beam divergence values from INTEGRATE.LP to XDS.INP
main table
SUBSET OF INTENSITY DATA WITH SIGNAL/NOISE >= -3.0 AS FUNCTION OF RESOLUTION RESOLUTION NUMBER OF REFLECTIONS COMPLETENESS R-FACTOR R-FACTOR COMPARED I/SIGMA R-meas Rmrgd-F Anomal SigAno Nano LIMIT OBSERVED UNIQUE POSSIBLE OF DATA observed expected Corr 2.91 15799 2114 2147 98.5% 2.3% 2.5% 15787 73.42 2.6% 1.1% -15% 0.705 1969 2.06 39607 3830 3856 99.3% 2.5% 2.8% 39602 81.49 2.6% 0.9% -11% 0.750 3794 1.68 64423 5068 5087 99.6% 3.1% 3.3% 64415 82.27 3.3% 1.0% -3% 0.843 5018 1.45 72869 6147 6163 99.7% 3.2% 3.5% 72867 77.43 3.4% 1.0% 0% 0.833 6055 1.30 71079 6652 6657 99.9% 3.3% 3.5% 71079 70.69 3.4% 1.1% 8% 0.865 6506 1.19 74584 7287 7298 99.8% 3.2% 3.4% 74575 66.78 3.4% 1.2% 5% 0.870 7060 1.10 84893 8268 8278 99.9% 3.5% 3.7% 84865 62.98 3.6% 1.3% 5% 0.858 7983 1.03 87893 8585 8603 99.8% 4.2% 4.4% 87859 56.04 4.4% 1.5% 4% 0.828 8238 0.97 92833 9457 9465 99.9% 5.2% 5.6% 92810 48.70 5.5% 1.7% 6% 0.802 9010 0.92 83981 9911 9927 99.8% 5.7% 6.3% 83954 41.48 6.0% 2.1% 5% 0.785 9362 0.88 74101 9620 9621 100.0% 6.3% 7.2% 74083 35.53 6.7% 2.6% 5% 0.785 9041 0.84 81383 11511 11518 99.9% 6.8% 7.7% 81361 30.26 7.3% 3.3% 1% 0.760 10616 0.81 67616 10240 10247 99.9% 7.1% 7.8% 67596 25.84 7.7% 4.2% 1% 0.782 9368 0.78 74077 11807 11817 99.9% 7.2% 7.3% 74049 22.26 7.8% 5.2% 1% 0.797 10697 0.75 86236 13831 13839 99.9% 8.5% 8.7% 86206 18.77 9.3% 6.7% 2% 0.809 12497 0.73 64601 10481 10488 99.9% 10.4% 10.5% 64573 15.77 11.3% 8.2% 2% 0.810 9375 0.71 71886 11727 11741 99.9% 12.8% 13.0% 71835 13.05 14.0% 10.6% 2% 0.800 10420 0.69 80233 13156 13163 99.9% 16.5% 16.9% 80130 10.32 18.1% 13.7% 1% 0.796 11661 0.67 84259 14746 14766 99.9% 22.0% 22.5% 84056 7.61 24.1% 19.6% 3% 0.789 12468 0.65 60775 15579 16551 94.1% 27.5% 30.3% 59893 4.49 31.7% 32.3% 1% 0.723 8936 total 1433128 190017 191232 99.4% 3.3% 3.5% 1431595 33.18 3.5% 3.5% 2% 0.801 170074
Comparison of data processing: published (2006) vs XDS results
resolution (highest resolution range) | observations | unique reflections | Multiplicity | Completeness (%) | R merge (%) | mean I/sigma | |
published(2006) | 30-0.65Å (0.67-0.65Å) | 1331953 (12764) | 187165 (6353) | 7.1 (2.7) | 97.6 (67.3) | 4.5 (18.4) | 36.2 (4.2) |
XDS | 30-0.65Å (0.67-0.65Å) | 1433128 (60775) | 190017 (15579) | 7.5 (3.9) | 99.4 (94.1) | 3.3 (27.5) | 33.2 (4.5) |
timings for processing sweep "e" as a function of MAXIMUM_NUMBER_OF_PROCESSORS and MAXIMUM_NUMBER_OF_JOBS
The following is going to be rather technical! If you are only interested in crystallography, skip this.
Using
MAXIMUM_NUMBER_OF_PROCESSORS=2 MAXIMUM_NUMBER_OF_JOBS=8
we observe for the INTEGRATE step:
total cpu time used 2063.6 sec total elapsed wall-clock time 296.1 sec
Using
MAXIMUM_NUMBER_OF_PROCESSORS=1 MAXIMUM_NUMBER_OF_JOBS=16
the times are
total cpu time used 2077.1 sec total elapsed wall-clock time 408.2 sec
Using
MAXIMUM_NUMBER_OF_PROCESSORS=4 MAXIMUM_NUMBER_OF_JOBS=4
the times are
total cpu time used 2102.8 sec total elapsed wall-clock time 315.6 sec
Using
MAXIMUM_NUMBER_OF_PROCESSORS=16 ! the default for xds_par on a 16-core machine MAXIMUM_NUMBER_OF_JOBS=1 ! the default
the times are
total cpu time used 2833.4 sec total elapsed wall-clock time 566.5 sec
but please note that this actually only uses 10 processors, since the default DELPHI=5 and the OSCILLATION_RANGE is 0.5°.
Using
MAXIMUM_NUMBER_OF_PROCESSORS=4 MAXIMUM_NUMBER_OF_JOBS=8
(thus overcommitting the available cores by a factor of 2) the times are
total cpu time used 2263.5 sec total elapsed wall-clock time 320.8 sec
Using
MAXIMUM_NUMBER_OF_PROCESSORS=4 MAXIMUM_NUMBER_OF_JOBS=6
(thus overcommitting the available cores, but less severely) the times are
total cpu time used 2367.6 sec total elapsed wall-clock time 267.2 sec
Thus,
MAXIMUM_NUMBER_OF_PROCESSORS=4 MAXIMUM_NUMBER_OF_JOBS=6
performs best for a 2-Xeon X5570 (HT enabled, thus 16 cores) machine with 24GB of memory and a RAID1 consisting of 2 1TB SATA disks. It should be noted that the dataset has 27GB, and in 296 seconds this means 92 MB/s continuous reading. The processing time is thus limited by the disk access, not by the CPU. And no, the data are not simply read from RAM (tested by "echo 3 > /proc/sys/vm/drop_caches" before the XDS run).