2QVO.xds: Difference between revisions

1,481 bytes added ,  9 November 2009
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==XDS data reduction==
==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)]]:
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
  DETECTOR=CCDCHESS        MINIMUM_VALID_PIXEL_VALUE=1    OVERLOAD=65000
  DIRECTION_OF_DETECTOR_X-AXIS= 1.0 0.0 0.0
  DIRECTION_OF_DETECTOR_X-AXIS= 1.0 0.0 0.0
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  POLARIZATION_PLANE_NORMAL= 0.0 1.0 0.0
  POLARIZATION_PLANE_NORMAL= 0.0 1.0 0.0
  SPACE_GROUP_NUMBER=0  !0 for unknown crystals; cell constants are ignored.
  SPACE_GROUP_NUMBER=0  !0 for unknown crystals; cell constants are ignored.
UNIT_CELL_CONSTANTS= 53 53 41  90 90 90
  FRIEDEL'S_LAW=FALSE !Default is TRUE.
  FRIEDEL'S_LAW=FALSE !Default is TRUE.
  NAME_TEMPLATE_OF_DATA_FRAMES=../../g/040707-8_2_2_1.????  ! TIFF
  NAME_TEMPLATE_OF_DATA_FRAMES=../../g/040707-8_2_2_1.????  ! TIFF
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  WFAC1=1.5  !This controls the number of rejected MISFITS in CORRECT; a larger value leads to fewer rejections.
  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
  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 [[Media:Xds_2qvo.tar.bz2.png|here]].
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 [[Media:Xds_2qvo.tar.bz2.png|here]].
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  end
  end
   
   
This writes j_fa.ins, j.hkl, j_fa.hkl . However, we overwrite j.ins now:
This writes j.hkl, j_fa.hkl and j_fa.ins. However, we overwrite j_fa.ins now:
  cat > j_fa.ins <<end
  cat > j_fa.ins <<end
  TITL j_fa.ins SAD in P42
  TITL j_fa.ins SAD in P42
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