Problems

From XDSwiki
Revision as of 10:52, 18 July 2013 by Kay (talk | contribs) (Indexing failures)

This is a collection of problems and their solutions.

XDS crashes

XDS should never crash (if it terminates with an error message, this does not count as crash). If it does, it is either a bug in the program which should be brought to the attention of Wolfgang Kabsch or Kay Diederichs, and will be fixed, or it is a problem with your computer.

If it crashes for the second reason, these are the things to try/consider:

huge frames leading to overflow of the shell's stack limit

Increase the stack limit of your shell, e.g. (if using csh or tcsh) with

limit stacksize 102400 

or (in case of bash)

ulimit -s 102400 

The numbers above mean a 10-fold increase over the default, and should be enough. I've found this to be necessary for unusually large frames (32 MB). xds_par in this case also might need an increase of the environment variable OMP_STACKSIZE (e.g. "setenv OMP_STACKSIZE 128M").

memory consumption exceeding the 4GB barrier when using the 32bit binary

As pointed out by James Holton, the memory consumed by huge frames in combination with many threads may be larger than 32 bits allow. Execution then stops with

forrtl: severe (41): insufficient virtual memory 

The workaround is to limit the MAXIMUM_NUMBER_OF_PROCESSORS, or to use XDS instead of XDS_PAR. An even better solution is to switch to the 64bit binary, but that of course requires a 64bit operating system.

Problems with OpenMP

If the "xds_par" binary crashed, try "xds". xds_par uses OpenMP for parallelization, which adds complexity. If it works with xds, but not with xds_par, then there is a chance that some environment variable needs to be set/changed. In any case the XDS developers would like to learn about this.

limitation of the parallel 32bit binary

The 32bit OpenMP binary may not be able to allocate enough storage when using many threads (e.g. >10). The error message might be something like:

OMP: Error #34: System unable to allocate necessary resources for OMP thread:
OMP: System error #11: Resource temporarily unavailable

64bit binary on a 32 bit operating system

If the error message is e.g.

xds: Exec format error. Wrong Architecture.

or

-bash: /usr/local/bin/xds: cannot execute binary file

make sure to use the 32bit version of XDS instead - you try to run the 64bit version on a 32bit operating system; this won't work.

CPU without SSE2 support

If the error message is

forrtl: severe (168): Program Exception - illegal instruction
Image              PC        Routine            Line        Source
xds                08055250  Unknown               Unknown  Unknown
xds                0804B3F6  Unknown               Unknown  Unknown

this means that unfortunately the CPU of your machine is too old to be supported by XDS (which in this respect is compiled with the default options of the ifort compiler). This may happen e.g. with old AMD CPUs that don't support SSE2 (on Linux check the flags field of /proc/cpuinfo for the presence of the sse2 flag).

According to [1] the following Intel-compatible CPUs did not implement SSE2 after SSE2 was introduced (2001):

  • AMD CPUs prior to Athlon 64, including all Socket A-based CPUs
  • Intel CPUs prior to Pentium 4
  • VIA C3
  • Transmeta Crusoe

ASSERT VIOLATION

If you get e.g.

!!! ERROR !!! ASSERT VIOLATION IN "RESTHKL"

this indicates that an internal error has occurred, i.e. some situation was hit that the program is not prepared to handle. There must be something very special about your dataset - maybe a very small number of reflections, maybe only negative intensities, maybe something else - which triggers the bug. If this happens then get in touch with the XDS developers - they will most likely ask to make your XDS.INP and data frames available to them, to fix the program.

Indexing failures

In case of IDXREF problems, you should definitively inspect, using XDS-viewer or adxv, the FRAME.cbf file which is written by COLSPOT. This file shows the first frame of the SPOT_RANGE, together with strong pixels that COLSPOT found on this frame, marked with white pixels. IDXREF will use those spot positions which have at least as many strong pixels as MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT specifies.

You will only be able to look at this file if you prevent XDS from running INTEGRATE. This can be achieved e.g. by

JOB= XYCORR INIT COLSPOT IDXREF DEFPIX ! INTEGRATE CORRECT

since FRAME.cbf is overwritten by INTEGRATE. When FRAME.cbf is written by INTEGRATE, it shows the last frame of the DATA_RANGE, and you should make sure that the predictions (circles) match the observed reflections.

To look at all spot positions found by COLSPOT, you could try

echo "set yrange [] reverse ; plot 'SPOT.XDS' us 1:2 w dots" | gnuplot -persist

This may also help to find shaded regions on the detector.

IDXREF ends with !!! ERROR !!! message

These messages should really be called !!! WARNING !!!. The two types occuring most often are:

 !!! ERROR !!! SOLUTION IS INACCURATE

This message is printed if the "STANDARD DEVIATION OF SPOT POSITION (PIXELS)" is larger than the MAXIMUM_ERROR_OF_SPOT_POSITION= (default of 3).

or

!!! ERROR !!! INSUFFICIENT PERCENTAGE (< 50%) OF INDEXED REFLECTIONS

This message is printed if less than the given percentage of reflections that COLSPOT found was actually indexed. If this occurs, it is clearly a warning sign.

The message continues in both cases:

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.

This is printed out for you to actually read, and take action accordingly. In most cases you just change the JOBS - line in XDS.INP to read

JOB= DEFPIX INTEGRATE CORRECT

and then continue to run XDS. In other cases you may want to change SPOT.XDS, or other keywords in XDS.INP (see also below). But in any case this is an important alert that should make you check the correctness of the parameters that describe the data collection (X-RAY_WAVELENGTH, DETECTOR_DISTANCE, ORGX, ORGY, OSCILLATION_RANGE, NAME_TEMPLATE_OF_DATA_FRAMES).

IDXREF.LP does not show the expected lattice

By specifying the spacegroup and unitcell, you tell XDS that it should index based on those reflections that match that spacegroup and unitcell. In a sense, you _force_ that spacegroup and cell. This will discard other (spurious?) reflections, and usually leads to a clean list of Bravais lattice possibilities.

If the data reduction fails nevertheless (in terms of bad R-factors and ISa in the CORRECT step), then chances are that you specified some parameter wrongly, or not accurate enough (ORGY and ORGY are the most likely candidates), or that the crystal does not match your idea about its spacegroup and unit cell. Actually the latter happens pretty frequently (which is why it is always the safest way to collect 180° of spindle rotation unless you know your crystals very well; this is also a good strategy in other respects).

If you tell XDS that you do not to know the spacegroup (SPACE_GROUP_NUMBER= 0), then IDXREF takes all observed reflections into account. By design, the spacegroup decision is then postponed until the CORRECT step, or rather to a run of pointless after CORRECT, and it may be not vital to closely inspect IDXREF.LP, because CORRECT.LP has basically the same information, plus more.

none of the lattices in IDXREF.LP (except aP) has a good QUALITY OF FIT

It is a good idea to use many frames for the SPOT_RANGE, (e.g. the first half of the DATA_RANGE, as does the generate_XDS.INP script) for the COLSPOT and IDXREF steps.

It is entirely possible to run COLSPOT for the complete DATA_RANGE (in that case the parameters of SPOT_RANGE are the same as for the DATA_RANGE), and to try smaller SPOT_RANGEs in IDXREF - this means COLSPOT has to be run only once, and the JOBS= line has e.g.

JOBS= IDXREF 

only. Maybe some SPOT_RANGE sub-range gives a clear answer. In that case it may be useful to use

REFINE(INTEGRATE)=! AXIS BEAM ORIENTATION CELL DISTANCE

because otherwise the spurious reflections in the other ranges will probably disturb the on-the-fly refinement of parameters.

I've seen datasets where each reflection had a satellite associated with the main reflection, but separate from it. This is well visible in FRAME.cbf written by COLSPOT. In such a case it helps to use

MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT= 12 ! re-run COLSPOT after changing the parameter !

thus doubling (w.r.t. the default of 6) the required spotsize that makes a reflection be used for indexing. In the latest case this made it possible to index cleanly on a single frame (which is actually not uncommon).

A final possibility: your crystal may really be triclinic - hopefully you collected 180° of data, or even a bit more than that.

See also

XDS.INP#What can go wrong with this file?

Low dose data