2QVO.xds

XDS data reduction

This is a pared-down XDS.INP (obtained by egrep -v '^ *!' XDS.INP) based upon XDS-MARCDD.INP from the XDS distribution site - it has only those lines that are not commented out (to arrive here, one takes the steps outlined in Tutorial(First_Steps)):

DETECTOR=CCDCHESS        MINIMUM_VALID_PIXEL_VALUE=1     OVERLOAD=65000
DIRECTION_OF_DETECTOR_X-AXIS= 1.0 0.0 0.0
DIRECTION_OF_DETECTOR_Y-AXIS= 0.0 1.0 0.0
TRUSTED_REGION=0.0 0.99 !Relative radii limiting trusted detector region
MAXIMUM_NUMBER_OF_PROCESSORS=8!<25;ignored by single cpu version of xds
JOB=  XYCORR INIT COLSPOT IDXREF DEFPIX  INTEGRATE CORRECT
ORGX=2000 ORGY=2048  !Detector origin (pixels)! numbers are rough estimates w/ adxv
DETECTOR_DISTANCE= 125.0   !(mm)
ROTATION_AXIS= 1.0 0.0 0.0
OSCILLATION_RANGE=1.0            !degrees (>0)
X-RAY_WAVELENGTH=1.9         !Angstroem
INCIDENT_BEAM_DIRECTION=0.0 0.0 1.0
FRACTION_OF_POLARIZATION=0.95 !default=0.5 for unpolarized beam
POLARIZATION_PLANE_NORMAL= 0.0 1.0 0.0
SPACE_GROUP_NUMBER=0   !0 for unknown crystals; cell constants are ignored.
FRIEDEL'S_LAW=FALSE !Default is TRUE.
NAME_TEMPLATE_OF_DATA_FRAMES=../../g/040707-8_2_2_1.????  ! TIFF
DATA_RANGE=1 360       !Numbers of first and last data image collected
BACKGROUND_RANGE=1 5  !Numbers of first and last data image for background
SPOT_RANGE=1 180       !First and last data image number for finding spots
REFINE(IDXREF)=BEAM AXIS ORIENTATION CELL DISTANCE
REFINE(INTEGRATE)=DISTANCE BEAM ORIENTATION CELL !AXIS
REFINE(CORRECT)=DISTANCE BEAM ORIENTATION CELL AXIS
VALUE_RANGE_FOR_TRUSTED_DETECTOR_PIXELS= 6000 30000 !Used by DEFPIX for excluding shaded parts of the detector.
INCLUDE_RESOLUTION_RANGE=50.0 0 !Angstroem; used by DEFPIX,INTEGRATE,CORRECT
MINIMUM_ZETA=0.1 !Defines width of 'blind region' (XPLAN,INTEGRATE,CORRECT)
WFAC1=1.5  !This controls the number of rejected MISFITS in CORRECT; a larger value leads to fewer rejections.
STRONG_PIXEL=6.0                              !used by: COLSPOT

Using the above as XDS.INP, we run xds_par for the first time. It will stop after the IDXREF step with the usual error message

!!! ERROR !!! INSUFFICIENT PERCENTAGE (< 70%) OF INDEXED REFLECTIONS
AUTOMATIC DATA PROCESSING STOPPED. AS THE CRITERIA FOR A GOOD
SOLUTION ARE RATHER STRICT, YOU MAY CHOOSE TO CONTINUE DATA
PROCESSING AFTER CHANGING THE "JOB="-CARD IN "XDS.INP" TO
"JOB= DEFPIX INTEGRATE CORRECT".
IF THE BEST SOLUTION IS REALLY NONSENSE YOU SHOULD FIRST HAVE
A LOOK AT THE ASCII-FILE "SPOT.XDS". THIS FILE CONTAINS THE
INITIAL SPOT LIST SORTED IN DECREASING SPOT INTENSITY. SPOTS
NEAR THE END OF THE FILE MAY BE ARTEFACTS AND SHOULD BE ERASED.
ALTERNATIVELY YOU MAY TRY DIFFERENT VALUES FOR "INDEX_ORIGIN"
AS SUGGESTED IN THE ABOVE LISTING.
IF THE CRYSTAL HAS SLIPPED AT THE BEGINNING OF DATA COLLECTION
YOU MAY CHOOSE TO SKIP SOME OF THE FIRST FRAMES BY CHANGING
THE "DATA_RANGE=" IN FILE "XDS.INP" AND START ALL OVER AGAIN.

We choose to continue nevertheless and modify XDS.INP to have

JOB=  DEFPIX  INTEGRATE CORRECT

Again we run xds_par. This runs to completion. The automatic spacegroup determination comes up with

SPACE_GROUP_NUMBER=   75
UNIT_CELL_CONSTANTS=    53.10    53.10    40.90  90.000  90.000  90.000

Now we copy these two lines to XDS.INP, replacing the old line SPACE_GROUP_NUMBER=0 . Then we modify the spacegroup number to 77 because we know that the true spacegroup is P4_2. Also, we modify the JOB line once again:

JOB= CORRECT

and run xds_par for the last time.

The resulting output files are XYCORR.LP, INIT.LP, COLSPOT.LP, IDXREF.LP, DEFPIX.LP, INTEGRATE.LP and CORRECT.LP. Data files are XPARM.XDS (from IDXREF), and the XDS_ASCII.HKL file all of which can be downloaded from here.

SHELXC/D/E structure solution

generate XDSCONV.INP (a trick is to use MERGE=TRUE, for some reason the results are better that way) and run xdsconv and shelxc:

 #!/bin/csh -f

cat > XDSCONV.INP <<end
INPUT_FILE=../XDS_ASCII.HKL
OUTPUT_FILE=temp.hkl SHELX
MERGE=TRUE
FRIEDEL'S_LAW=FALSE
end

xdsconv 

shelxc j <<end
SAD   temp.hkl
CELL 53.10 53.10 40.90 90 90 90
SPAG P42
MAXM 2
end

This writes j.hkl, j_fa.hkl and j_fa.ins. However, we overwrite j_fa.ins now:

cat > j_fa.ins <<end
TITL j_fa.ins SAD in P42
CELL  0.98000   53.10   53.10   40.90   90.00   90.00   90.00
LATT  -1
SYMM -Y, X, 1/2+Z
SYMM -X, -Y, Z
SYMM Y, -X, 1/2+Z
SFAC S
UNIT   128
SHEL 999 3.0
FIND 3
NTRY 100
MIND -1.0 2.2
ESEL 1.3
TEST 0 99
SEED 1
PATS
HKLF 3
END
end

shelxd j_fa

This gives best CC All/Weak of 35.61 / 26.03 . Next we run G. Sheldrick's beta-Version of shelxe Version 2009/4:

shelxe.beta -a6 -q j j_fa -h -s0.55 -m20 -b 

Some important lines in the output:

   79 residues left after pruning, divided into chains as follows:
A:  20   B:  22   C:  37

CC for partial structure against native data =  50.42 %
 <wt> = 0.300, Contrast = 0.731, Connect. = 0.817 for dens.mod. cycle 20
 Estimated mean FOM = 0.659   Pseudo-free CC = 68.71 %

clearly indicating that the structure is solved.

For completeness, we run the inverse hand:

shelxe.beta -a6 -q j j_fa -h -s0.55 -m20 -b -i

but of course this gives much worse statistics.