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Generate XDS.INP: Difference between revisions
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→The script: KD 27.4.22 always print out detector serial number
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# revision 1.09 . KD, Feng Yu 7/11/2021 fix detector number BNL E-18-0121 to be E-18-0104 | # revision 1.09 . KD, Feng Yu 7/11/2021 fix detector number BNL E-18-0121 to be E-18-0104 | ||
# revision 1.10 . KD NeXus header for Eiger | # revision 1.10 . KD NeXus header for Eiger | ||
REVISION="1. | # revision 1.11 . KD / Helena Taberman ROTATION_AXIS=-1 0 0 for Eiger .cbf data from Petra P14 | ||
# revision 1.12 . KD / Helena Taberman correct rev 1.11 to be 0 -1 0 | |||
REVISION="1.12 (25-MAR-2022)" | |||
# | # | ||
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# | # | ||
# notes for debugging of the script: | # notes for debugging of the script: | ||
# - add the -x option to | # - add the -x option to #!/bin/bash in first line, to see where an error occurs | ||
# - comment out the removal of tmp1 and tmp2 in the last line | # - comment out the removal of tmp1 and tmp2 in the last line | ||
# | # | ||
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DETECTOR_DISTANCE=`grep ^DISTANCE tmp2 | sed s/DISTANCE=/-/` | DETECTOR_DISTANCE=`grep ^DISTANCE tmp2 | sed s/DISTANCE=/-/` | ||
OSCILLATION_RANGE=`grep OMEGA_DELTA tmp2 | sed s/OMEGA_DELTA=//` | OSCILLATION_RANGE=`grep OMEGA_DELTA tmp2 | sed s/OMEGA_DELTA=//` | ||
DETECTOR_X_AXIS="-1 0 0" | |||
elif [ "$DET" == "experimental-ED" ]; then | elif [ "$DET" == "experimental-ED" ]; then | ||
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fi | fi | ||
# PETRA P14: raw data from Eiger are stored as CBF files so this is treated as Pilatus | # PETRA P14: raw data from Eiger are stored as CBF files so this is treated as Pilatus | ||
if [ "$DET_SN" == "Dectris Eiger 4M, E-08-0107" -o "$DET_SN" == "PILATUS 6M-F, S/N 60-0115-F" ] ; then | if [ "$DET_SN" == "Dectris Eiger 4M, E-08-0107" -o "$DET_SN" == "PILATUS 6M-F, S/N 60-0115-F" \ | ||
-o "$DET_SN" == "Dectris EIGER2 CdTe 16M, E-32-0129" ] ; then | |||
rotation_axis="0 -1 0" | rotation_axis="0 -1 0" | ||
echo ROTATION_AXIS="0 -1 0" at PETRA P14 | echo ROTATION_AXIS="0 -1 0" at PETRA P14 | ||
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DATA_RANGE="1 $nframes" | DATA_RANGE="1 $nframes" | ||
SPOT_RANGE="1 `echo "scale=0; if (${nframes}<2) 1; if (${nframes}>1) ${nframes}/2"|bc -l`" | SPOT_RANGE="1 `echo "scale=0; if (${nframes}<2) 1; if (${nframes}>1) ${nframes}/2"|bc -l`" | ||
SN=`h5dump -d "/entry/instrument/detector/detector_number" $FIRSTFRAME | awk '/\(0\): /{print $2}' | sed s/\"//g` | |||
echo detector serial number is $SN | |||
# find out if HDF5 from Diamond (DLS=1) or Dectris (DLS=0) | # find out if HDF5 from Diamond (DLS=1) or Dectris (DLS=0) | ||
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rotation_axis=`h5dump -a "/entry/sample/transformations/omega/vector" $FIRSTFRAME 2>/dev/null | grep "(0):" | sed -e "s/^.*://; s/,//g"` | rotation_axis=`h5dump -a "/entry/sample/transformations/omega/vector" $FIRSTFRAME 2>/dev/null | grep "(0):" | sed -e "s/^.*://; s/,//g"` | ||
# EIGER2 16M CHESS ID7B2 has S/N E-32-0123 (A. Finke 2020-11-07) v0.99 | # EIGER2 16M CHESS ID7B2 has S/N E-32-0123 (A. Finke 2020-11-07) v0.99 | ||
if [ "$SN" == "E-32-0123" ]; then | if [ "$SN" == "E-32-0123" ]; then | ||
rotation_axis="-1 0 0" | rotation_axis="-1 0 0" | ||
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* Sometimes, the x- and y- values of the primary beam position recorded in the header should be used for ORGY and ORGX (i.e reversed) instead of as ORGX and ORGY. For ADSC, this has been implemented in the script for a number of beamlines. | * Sometimes, the x- and y- values of the primary beam position recorded in the header should be used for ORGY and ORGX (i.e reversed) instead of as ORGX and ORGY. For ADSC, this has been implemented in the script for a number of beamlines. | ||
* there are apparently several flavours of HDF5 files produced at Diamond Light Source. They differ e.g. in the naming of the header items. This means that items like NX, NY, DETECTOR_DISTANCE and number of images cannot always be determined by the [[generate_XDS.INP]] script. Example: The data at /dls/i04-1/data/2021/mx28114-9/processing/Lenye_Diamini/ThiL/ThiL found during the CCP4 2021 online Cape Town workshop. A workaround is to use e.g. xia2 pipeline=3dii to process these files, and - if needed - extract those items from its output files, e.g. from DEFAULT/NATIVE/SWEEP1/index/XDS.INP . | * there are apparently several flavours of HDF5 files produced at Diamond Light Source. They differ e.g. in the naming of the header items. This means that items like NX, NY, DETECTOR_DISTANCE and number of images cannot always be determined by the [[generate_XDS.INP]] script. Example: The data at /dls/i04-1/data/2021/mx28114-9/processing/Lenye_Diamini/ThiL/ThiL found during the CCP4 2021 online Cape Town workshop. A workaround is to use e.g. xia2 pipeline=3dii to process these files, and - if needed - extract those items from its output files, e.g. from DEFAULT/NATIVE/SWEEP1/index/XDS.INP . | ||
== See also == | == See also == | ||