Generate XDS.INP
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This script generates XDS.INP based on a list of frame names supplied on the commandline. It currently works for MarCCD, ADSC and Pilatus detectors; since this is just a bash script, extension to other detectors is very easy.
On Mac OS X, installation of the "Command Line Tools" (from http://developer.apple.com/downloads; requires Apple ID) is required (I think). These are a part of the (larger, but also free) Xcode package.
Usage
Usage is just (don't forget the quotation marks!):
generate_XDS.INP "/home/myname/frms/mydata_1_???.img"
XDS supports bzip2-ed frames. Thus, when specifying the frame name parameter of the script, you should leave out any .bz2 extension.
For improved interaction with XDSGUI, it is advantageous to use an absolute filename - one that starts with a slash ("/").
The script
#!/bin/bash
# purpose: generate XDS.INP
#
# tested with some datasets from ALS, SSRL, SLS, ESRF, BESSY, SPring-8 and PF; only MARCCD, ADSC/SMV, PILATUS, RAXIS (in-house) detectors;
# for other detectors, values marked with XXX must be manually filled in.
#
# revision 0.03 . Kay Diederichs 2/2010
# revision 0.04 . Kay Diederichs 4/2010 - include alternative ORGX, ORGY calculations for ADSC
# revision 0.05 . Kay Diederichs 5/2010 - grep for "Corrected" in addition to "marccd"; needed for BESSY
# revision 0.06 . KD 6/2010 - add UNTRUSTED_RECTANGLE and UNTRUSTED_ELLIPSE; use `whereis catmar` and so on
# revision 0.07 . KD 6/2010 - decide about ORGX/Y info in MAR header being pixels or mm; other fixes
# revision 0.08 . KD 6/2010 - fixes for Pilatus 6M
# revision 0.09 . KD 6/2010 - get rid of requirement for mccd_xdsparams.pl and/or catmar; rather use "od"
# revision 0.10 . Tim Gruene 7/2010 - set link 'images' to image directory if path exceeds 72 characters
# revision 0.11 . KD 7/2010 - for MarCCD: look for distance info at different byte position
# revision 0.12 . KD 7/2010 - fix for negative PHISTART
# revision 0.13 . KD 8/2010 - store correct NX NY QX QY in XDS.INP
# revision 0.14 . KD 1/2011 - SENSOR_THICKNESS for Pilatus; MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT=3
# revision 0.15 . KD 2/2011 - add comment for -ive sign of APS 19-ID and Australian Synchrotron rotation axis
# revision 0.16 . KD 3/2011 - SENSOR_THICKNESS=0.01 for ADSC and MarCCD. Add comment about SILICON=
# revision 0.17 . KD 3/2011 - make it work for .bz2 frames; improve screen output
# revision 0.18 . KD 4/2011 - faster by doing "strings" only once; revert "images/${1##/*/}" "correction"
# revision 0.19 . KD 6/2011 - bugfix for 0.18
# revision 0.20 . KD 7/2011 - redirect stderr of /bin/ls to /dev/null
# revision 0.21 . KD 11/2011 - SEPMIN, CLUSTER_RADIUS hints; read NX NY from header (for Pilatus 2M)
# revision 0.22 . KD 12/2011 - Pilatus 2M UNTRUSTED_RECTANGLE lines, SENSOR_THICKNESS from header
# revision 0.23 . KD 1/2012 - add UNTRUSTED_QUADRILATERAL, remove MINIMUM_ZETA (0.05 is default now)
# revision 0.24 . KD 3/2012 - remove revision 0.10 since XDS now takes much longer paths
# revision 0.25 . KD 3/2012 - remove revision 0.22 for PSI Pilatus 2M; see http://www.globalphasing.com/autoproc/wiki/index.cgi?TroubleShootingKnownIssues
# revision 0.26 . KD 7/2012 - Mac-compatibility: replace od flags --skip-bytes= and --read-bytes= with -j and -N (thanks to Oliver Clarke for working this out!)
# revision 0.27 . KD 11/2012 - EXCLUDE_RESOLUTION_RANGE lines and generic Pilatus Flat_field test
# revision 0.28 . Keitaro 11/2012 - for MarCCD: read oscillation range from the position 1024+736 (fix for omega rotation)
# revision 0.29 . KD 1/2013 - include UNTRUSTED_RECTANGLEs for Pilatus 6M; never hurts but needed if the beamline software does not mark them with -2 or such
# revision 0.30 . Keitaro 3/2013 - for ADSC: write all possible beam center conventions in XDS.INP as comments
# revision 0.31 . Keitaro 3/2013 - add comment for reversed phi for SPring-8
# revision 0.32 . Keitaro 3/2013 - add RAXIS support. only tested with RAXIS IV++ and VII.
# revision 0.33 . Keitaro 5/2013 - automatically set ROTATION_AXIS=-1 0 0 for SPring-8 BL32XU/41XU/44XU beamlines based on detector serial numbers.
# revision 0.34 . Keitaro 5/2013 - recognize ADSC detectors in Photon Factory and choose correct beam center convention based on detector serial numbers.
# revision 0.35 . KD 6/2013 - reduce 7000 to 6000 for shadow detection; insert comment about *_RESOLUTION_RANGE lines
# revision 0.36 . KD 6/2013 - insert NUMBER_OF_PROFILE_GRID* lines for Pilatus (suggested by C.Vonrhein)
# revision 0.37 . Keitaro 10/2013 - fix for MX225HS detector on SPring-8 BL32XU (Ignore case when matching marccd in header); but cannot decide reverse-phi because of missing detector S/N
REVISION="0.37 (31-October-2013)"
#
# usage: e.g. generate_XDS.INP "frms/mydata_1_???.img"
# make sure to have the two quotation marks !
# the ? are wildcards for the frame numbers.
#
# limitations:
# - frame numbers are assumed to start with 1 and run consecutively
#
# known problems:
# - for ADSC detectors, there are at least three ways to obtain ORGX and ORGY values from the header (see below);
# - the same might be a problem for MAR headers, too (not sure about this)
# - on Mac OS X, Xcode (from http://developer.apple.com/tools/xcode) might be needed - not sure about this
#
# notes for debugging of the script:
# - add the -v option to the first line, to see where an error occurs
# - comment out the removal of tmp1 and tmp2 in the last line
#
# ====== Start of script ======
echo generate_XDS.INP version $REVISION . Obtain the latest version from
echo http://strucbio.biologie.uni-konstanz.de/xdswiki/index.php/generate_XDS.INP
if [ "$1" == "help" ] || [ "$1" == "-help" ] || [ "$1" == "-h" ]; then
echo usage: generate_XDS.INP \"frms/mydata_1_???.img\" \(_with_ the quotation marks!\)
echo if the frames are compressed with bzip2, leave out the .bz2 extension!
exit
fi
#
# defaults:
#
DETECTOR="XXX MINIMUM_VALID_PIXEL_VALUE=XXX OVERLOAD=XXX"
REVERSE_PHI="no"
ORGX=XXX
ORGY=XXX
DETECTOR_DISTANCE=XXX
OSCILLATION_RANGE=XXX
X_RAY_WAVELENGTH=XXX
QX=XXX
QY=XXX
NX=XXX
NY=XXX
SENSOR_THICKNESS=0
# see how we are called:
NAME_TEMPLATE_OF_DATA_FRAMES="$1"
# list frames matching the wildcards in NAME_TEMPLATE_OF_DATA_FRAMES
# don't accept the "direct beam" shot at SLS/Pilatus PX-I and PX-II
/bin/ls -C1 $1 $1.bz2 2>/dev/null | egrep -v "_00000.cbf|_000.img" > tmp1 || exit 1
# we can continue - the frames are found
# set upper limit of DATA_RANGE to number of frames (see "limitations" above)
DATA_RANGE=`wc -l tmp1 | awk '{print $1}'`
# set upper limit of SPOT_RANGE to half of DATA_RANGE, but not less than 1
SPOT_RANGE=`echo "scale=0; $DATA_RANGE/2" | bc -l`
SPOT_RANGE=`echo "if ($SPOT_RANGE<1) 1;if ($SPOT_RANGE>1) $SPOT_RANGE" | bc -l`
echo DATA_RANGE=1 $DATA_RANGE
# find out detector type
DET=XXX
FIRSTFRAME=`head -1 tmp1`
echo $FIRSTFRAME | grep -q bz2 && bzcat $FIRSTFRAME > tmp1 && FIRSTFRAME=tmp1
strings $FIRSTFRAME > tmp2
egrep -qi 'marccd|Corrected' tmp2 && DET=mccd
grep -q PILATUS tmp2 && DET=pilatus
grep -q BEAM_CENTER_X tmp2 && DET=adsc
head -n1 tmp2 | grep -q "^RAXIS" && DET=raxis
# identify other detector types in the same way (MAR IP would be straightforward)
# parse ASCII header of first frame
if [ "$DET" == "XXX" ]; then
echo "this is not a MAR, ADSC/SMV or PILATUS detector - fill in XXX values manually!"
DETECTOR="XXX MINIMUM_VALID_PIXEL_VALUE=XXX OVERLOAD=XXX"
# find parameters of first frame
elif [ "$DET" == "mccd" ]; then
echo Data from a MarCCD detector
DETECTOR="CCDCHESS MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65500"
SENSOR_THICKNESS=0.01
# use first frame of dataset to obtain parameters
# Check detector serial number and recognize beamline for reversed-phi setting.
# Known detectors for reversed-phi in SPring-8: 31: BL32XU MX225HE, 38: BL44XU MX225HE, 42: BL44XU MX300HE, 40: BL41XU MX225HE
REVERSEPHI_SNs="
31
38
40
42
"
# get detector serial number and check if it is included in the list
DET_SN=`grep "Detector Serial Number =" tmp2 | sed "s/Detector Serial Number = //"`
if echo "${DET_SN}${REVERSEPHI_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
REVERSE_PHI="yes"
fi
# offsets are documented; values can be found in mccd_xdsparams.pl script
let SKIP=1024+80
NX=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
let SKIP=$SKIP+4
NY=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
let SKIP=1720
DETECTOR_DISTANCE=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
DETECTOR_DISTANCE=`echo "scale=3; $DETECTOR_DISTANCE/1000" | bc -l`
let SKIP=1024+256+128+256+4
ORGX=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
ORGX=`echo "scale=2; $ORGX/1000" | bc -l `
let SKIP=$SKIP+4
ORGY=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
ORGY=`echo "scale=2; $ORGY/1000" | bc -l `
let SKIP=1024+736
OSCILLATION_RANGE=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
OSCILLATION_RANGE=`echo "scale=3; $OSCILLATION_RANGE/1000" | bc -l`
let SKIP=1024+256+128+256+128+4
QX=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
QX=`echo "scale=10; $QX/1000000" |bc -l `
let SKIP=$SKIP+4
QY=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
QY=`echo "scale=10; $QY/1000000" |bc -l `
let SKIP=1024+256+128+256+128+128+12
X_RAY_WAVELENGTH=$(od -t dI -j $SKIP -N 4 $FIRSTFRAME | head -1 | awk '{print $2}')
X_RAY_WAVELENGTH=`echo "scale=5; $X_RAY_WAVELENGTH/100000" | bc -l`
# at most BLs, ORGX and ORGY are in pixels, but sometimes in mm ... guess:
NXBYFOUR=`echo "scale=0; $NX/4" | bc -l `
ORGXINT=`echo "scale=0; $ORGX/1" | bc -l `
if [ $ORGXINT -lt $NXBYFOUR ]; then
ORGX=`echo "scale=1; $ORGX/$QX" | bc -l`
ORGY=`echo "scale=1; $ORGY/$QY" | bc -l`
echo MARCCD detector: header ORGX, ORGY seem to be in mm ... converting to pixels
else
echo MARCCD detector: header ORGX, ORGY seem to be in pixel units
fi
elif [ "$DET" == "adsc" ]; then
DETECTOR="ADSC MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65000"
echo Data from ADSC detector. Obtaining ORGX, ORGY depends on beamline setup:
SENSOR_THICKNESS=0.01
sed s/\;// tmp2 > tmp1
mv tmp1 tmp2
# find X_RAY_WAVELENGTH:
X_RAY_WAVELENGTH=`grep WAVELENGTH tmp2 | head -1 | sed s/WAVELENGTH=//`
# find NX, QX, ORGX and ORGY:
NX=`grep SIZE1 tmp2 | tail -1 | sed s/SIZE1=//`
QX=`grep PIXEL_SIZE tmp2 | sed s/PIXEL_SIZE=//`
# FIXME - next 2 lines should be done properly, from header
NY=$NX
QY=$QX
BEAM_CENTER_X=`grep BEAM_CENTER_X tmp2 | sed s/BEAM_CENTER_X=//`
BEAM_CENTER_Y=`grep BEAM_CENTER_Y tmp2 | sed s/BEAM_CENTER_Y=//`
# fix 2010-04-26 - tell user about possible ORGX, ORGY alternatives -
COMMENT_ORGXY="
! Following are possible beam center interpretations for ADSC detectors"
# at ESRF, PF, and ... (pls fill in!) the following should be used:
ORGX1=`echo "scale=1; $BEAM_CENTER_Y/$QX" | bc -l`
ORGY1=`echo "scale=1; $BEAM_CENTER_X/$QX" | bc -l`
echo - at ESRF,PF BLs use: ORGX=$ORGX1 ORGY=$ORGY1
COMMENT_ORGXY="${COMMENT_ORGXY}
! ORGX= $ORGX1 ORGY= $ORGY1 ! For ESRF,PF,..."
# this 2nd alternative convention should be used at the following beamlines (pls complete the list): ALS 5.0.3, ...
ORGX2=`echo "scale=1; $NX-$BEAM_CENTER_X/$QX" | bc -l `
ORGY2=`echo "scale=1; $BEAM_CENTER_Y/$QX" | bc -l `
echo - at e.g. ALS 5.0.3 use: ORGX=$ORGX2 ORGY=$ORGY2
COMMENT_ORGXY="${COMMENT_ORGXY}
! ORGX= $ORGX2 ORGY= $ORGY2 ! For ALS 5.0.3,.."
# this 3rd alternative convention should be used at the following beamlines (pls complete the list): ALS 8.2.2, ...
ORGX3=`echo "scale=1; $BEAM_CENTER_X/$QX" | bc -l `
ORGY3=`echo "scale=1; $NX-$BEAM_CENTER_Y/$QX" | bc -l `
echo - at e.g. ALS 8.2.2 use: ORGX=$ORGX3 ORGY=$ORGY3 - this is written to XDS.INP
COMMENT_ORGXY="${COMMENT_ORGXY}
! ORGX= $ORGX3 ORGY= $ORGY3 ! For ALS 8.2.2,.."
# the latter alternative is written into the generated XDS.INP ! You have to correct this manually in XDS.INP, or adjust this script.
# Decision of beam center convention based on detector serial numbers.
DET_SN=`grep DETECTOR_SN tmp2 | sed -e "s/DETECTOR_SN=//"`
# For convention 1; Known PF detectors = 449: NW12A Q210, 472: NE3A Q270, 474: BL17A Q270, 912: BL5A Q315
ORG1_SNs="
449
472
474
912
"
if echo "${DET_SN}${ORG1_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
ORGX=$ORGX1
ORGY=$ORGY1
else
ORGX=$ORGX3
ORGY=$ORGY3
fi
# find DETECTOR_DISTANCE and OSCILLATION_RANGE:
DETECTOR_DISTANCE=`grep DISTANCE tmp2 | sed s/DISTANCE=//`
OSCILLATION_RANGE=`grep OSC_RANGE tmp2 | sed s/OSC_RANGE=//`
elif [ "$DET" == "pilatus" ]; then
DETECTOR="PILATUS MINIMUM_VALID_PIXEL_VALUE=0 OVERLOAD= 1048576 !PILATUS"
QX=0.172 QY=0.172
echo Data from a Pilatus detector
sed s/#// tmp2 > tmp1
mv tmp1 tmp2
# find SENSOR_THICKNESS:
SENSOR_THICKNESS=`grep thickness tmp2 | sed -e s/'Silicon sensor, thickness'// | awk '{print $1*1000}'`
# find X_RAY_WAVELENGTH:
X_RAY_WAVELENGTH=`grep Wavelength tmp2 | sed -e s/Wavelength// -e s/A// | awk '{print $1}'`
# find NX and NY; 2463/2527 is 6M, 1475/1679 is 2M
NX=`grep X-Binary-Size-Fastest-Dimension tmp2 | awk '{print $2}'`
NY=`grep X-Binary-Size-Second-Dimension tmp2 | awk '{print $2}'`
# find ORGX and ORGY:
ORGX=`grep Beam_xy tmp2 | sed -e s/\(// -e s/\)// -e s/\,// | awk '{print $2}'`
ORGY=`grep Beam_xy tmp2 | sed -e s/\(// -e s/\)// -e s/\,// | awk '{print $3}'`
# find DETECTOR_DISTANCE and OSCILLATION_RANGE:
DETECTOR_DISTANCE=`awk '/distance/{print $2}' tmp2`
DETECTOR_DISTANCE=`echo "$DETECTOR_DISTANCE*1000" | bc -l`
OSCILLATION_RANGE=`awk '/Angle/{print $2}' tmp2`
elif [ "$DET" == "raxis" ]; then
echo Data from a RAXIS detector
DETECTOR="RAXIS MINIMUM_VALID_PIXEL_VALUE=0 OVERLOAD=2000000"
#let SKIP=768
#NX=$(od -t x -j $SKIP -N 4 $FIRSTFRAME |awk 'NR==1{print toupper($2)}'|perl -nle '@array= $_ =~/.{2}/g; print "ibase=16;obase=A;".join("",reverse @array)'|bc)
NX=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(768);print "%.4d"%struct.unpack(">i",f.read(4))')
NY=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(772);print "%.4d"%struct.unpack(">i",f.read(4))')
DETECTOR_DISTANCE=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(344);print "-%.4f"%struct.unpack(">f",f.read(4))')
ORGX=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(540);print "%.4f"%struct.unpack(">f",f.read(4))')
ORGY=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(544);print "%.4f"%struct.unpack(">f",f.read(4))')
OSCILLATION_RANGE=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(524);phis,phie=struct.unpack(">ff",f.read(8));print "%.4f"%(phie-phis)')
QX=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(776);print "%.6f"%struct.unpack(">f",f.read(4))')
QY=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(780);print "%.6f"%struct.unpack(">f",f.read(4))')
X_RAY_WAVELENGTH=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(292);print "%.6f"%struct.unpack(">f",f.read(4))')
else
echo should never come here
exit 1
fi
echo ORGX= $ORGX ORGY= $ORGY - check these values with adxv !
echo DETECTOR_DISTANCE= $DETECTOR_DISTANCE
echo OSCILLATION_RANGE= $OSCILLATION_RANGE
echo X-RAY_WAVELENGTH= $X_RAY_WAVELENGTH
# now we know everything that is required to generate XDS.INP
cat > XDS.INP << eof
! written by generate_XDS.INP version $REVISION
JOB= XYCORR INIT COLSPOT IDXREF DEFPIX INTEGRATE CORRECT
ORGX= $ORGX ORGY= $ORGY ! check these values with adxv !\
$COMMENT_ORGXY
DETECTOR_DISTANCE= $DETECTOR_DISTANCE
OSCILLATION_RANGE= $OSCILLATION_RANGE
X-RAY_WAVELENGTH= $X_RAY_WAVELENGTH
NAME_TEMPLATE_OF_DATA_FRAMES=$NAME_TEMPLATE_OF_DATA_FRAMES
! REFERENCE_DATA_SET=xxx/XDS_ASCII.HKL ! e.g. to ensure consistent indexing
DATA_RANGE=1 $DATA_RANGE
SPOT_RANGE=1 $SPOT_RANGE
! BACKGROUND_RANGE=1 10 ! rather use defaults (first 5 degree of rotation)
SPACE_GROUP_NUMBER=0 ! 0 if unknown
UNIT_CELL_CONSTANTS= 70 80 90 90 90 90 ! put correct values if known
INCLUDE_RESOLUTION_RANGE=50 0 ! after CORRECT, insert high resol limit; re-run CORRECT
! IDXREF now obeys INCLUDE_RESOLUTION_RANGE and EXCLUDE_RESOLUTION_RANGE to exclude ice-rings
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
! UNTRUSTED_QUADRILATERAL= x1 y1 x2 y2 x3 y3 x4 y4 ! see documentation
!
! parameters with changes wrt default values:
TRUSTED_REGION=0.00 1.2 ! partially use corners of detectors; 1.41421=full use
VALUE_RANGE_FOR_TRUSTED_DETECTOR_PIXELS=6000. 30000. ! often 7000 or 8000 is ok
STRONG_PIXEL=4 ! COLSPOT: only use strong reflections (default is 3)
MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT=3 ! default of 6 is sometimes too high
! close spots: reduce SEPMIN and CLUSTER_RADIUS from their defaults of 6 and 3, e.g. to 4 and 2
! for bad or low resolution data remove the "!" in the following line:
! REFINE(IDXREF)=CELL BEAM ORIENTATION AXIS ! DISTANCE
REFINE(INTEGRATE)=CELL BEAM ORIENTATION ! AXIS DISTANCE
! REFINE(CORRECT)=CELL BEAM ORIENTATION AXIS DISTANCE ! Default is: refine everything
! parameters specifically for this detector and beamline:
DETECTOR= $DETECTOR
SENSOR_THICKNESS= $SENSOR_THICKNESS
! attention CCD detectors: for very high resolution (better than 1A) make sure to specify SILICON
! as about 32* what CORRECT.LP suggests (absorption of phosphor is much higher than that of silicon)
NX= $NX NY= $NY QX= $QX QY= $QY ! to make CORRECT happy if frames are unavailable
eof
if [ "$DET" == "raxis" ]; then
cat >> XDS.INP << eof
DIRECTION_OF_DETECTOR_X-AXIS=1 0 0
DIRECTION_OF_DETECTOR_Y-AXIS=0 -1 0
INCIDENT_BEAM_DIRECTION=0 0 1
ROTATION_AXIS=0 1 0
!FRACTION_OF_POLARIZATION=0.98 ! uncomment if synchrotron
POLARIZATION_PLANE_NORMAL=1 0 0
eof
else
if [ "$REVERSE_PHI" == "no" ]; then
echo 'ROTATION_AXIS=1 0 0 ! at e.g. Australian Synchrotron, SERCAT ID-22 (?), APS 19-ID (?), ESRF BM30A, SPring-8 this needs to be -1 0 0' >> XDS.INP
else
echo 'ROTATION_AXIS=-1 0 0 ! if this is wrong, please contact author.' >> XDS.INP
fi
cat >> XDS.INP << eof
DIRECTION_OF_DETECTOR_X-AXIS=1 0 0
DIRECTION_OF_DETECTOR_Y-AXIS=0 1 0
INCIDENT_BEAM_DIRECTION=0 0 1
FRACTION_OF_POLARIZATION=0.98 ! better value is provided by beamline staff!
POLARIZATION_PLANE_NORMAL=0 1 0
eof
fi
cat >> XDS.INP << eof
!used by DEFPIX and CORRECT to exclude ice-reflections / ice rings - uncomment if necessary
!EXCLUDE_RESOLUTION_RANGE= 3.93 3.87 !ice-ring at 3.897 Angstrom
!EXCLUDE_RESOLUTION_RANGE= 3.70 3.64 !ice-ring at 3.669 Angstrom
!EXCLUDE_RESOLUTION_RANGE= 3.47 3.41 !ice-ring at 3.441 Angstrom
!EXCLUDE_RESOLUTION_RANGE= 2.70 2.64 !ice-ring at 2.671 Angstrom
!EXCLUDE_RESOLUTION_RANGE= 2.28 2.22 !ice-ring at 2.249 Angstrom
!EXCLUDE_RESOLUTION_RANGE= 2.102 2.042 !ice-ring at 2.072 Angstrom - strong
!EXCLUDE_RESOLUTION_RANGE= 1.978 1.918 !ice-ring at 1.948 Angstrom - weak
!EXCLUDE_RESOLUTION_RANGE= 1.948 1.888 !ice-ring at 1.918 Angstrom - strong
!EXCLUDE_RESOLUTION_RANGE= 1.913 1.853 !ice-ring at 1.883 Angstrom - weak
!EXCLUDE_RESOLUTION_RANGE= 1.751 1.691 !ice-ring at 1.721 Angstrom - weak
eof
if [ "$DET" == "pilatus" ]; then
cat >> XDS.INP << eof
NUMBER_OF_PROFILE_GRID_POINTS_ALONG_ALPHA/BETA=13 ! Default is 9 - Increasing may improve data
NUMBER_OF_PROFILE_GRID_POINTS_ALONG_GAMMA=13 ! accuracy, particularly if finely-sliced on phi,
! and does not seem to have any downsides.
eof
if [ $NX == "1475" ]; then
if ! grep -q Flat_field tmp2 ; then
cat >> XDS.INP << eof
! the following specifications are for a detector _without_ proper
! flat_field correction; they cut away one additional pixel adjacent
! to each UNTRUSTED_RECTANGLE
!EXCLUSION OF VERTICAL DEAD AREAS OF THE PILATUS 2M DETECTOR
UNTRUSTED_RECTANGLE= 486 496 0 1680
UNTRUSTED_RECTANGLE= 980 990 0 1680
!EXCLUSION OF HORIZONTAL DEAD AREAS OF THE PILATUS 2M DETECTOR
UNTRUSTED_RECTANGLE= 0 1476 194 214
UNTRUSTED_RECTANGLE= 0 1476 406 426
UNTRUSTED_RECTANGLE= 0 1476 618 638
UNTRUSTED_RECTANGLE= 0 1476 830 850
UNTRUSTED_RECTANGLE= 0 1476 1042 1062
UNTRUSTED_RECTANGLE= 0 1476 1254 1274
UNTRUSTED_RECTANGLE= 0 1476 1466 1486
eof
else
cat >> XDS.INP << eof
!EXCLUSION OF VERTICAL DEAD AREAS OF THE PILATUS 2M DETECTOR
UNTRUSTED_RECTANGLE= 487 495 0 1680
UNTRUSTED_RECTANGLE= 981 989 0 1680
!EXCLUSION OF HORIZONTAL DEAD AREAS OF THE PILATUS 2M DETECTOR
UNTRUSTED_RECTANGLE= 0 1476 195 213
UNTRUSTED_RECTANGLE= 0 1476 407 425
UNTRUSTED_RECTANGLE= 0 1476 619 637
UNTRUSTED_RECTANGLE= 0 1476 831 849
UNTRUSTED_RECTANGLE= 0 1476 1043 1061
UNTRUSTED_RECTANGLE= 0 1476 1255 1273
UNTRUSTED_RECTANGLE= 0 1476 1467 1485
eof
fi
elif [ $NX == "2463" ]; then
# Pilatus 6M
# FIXME: here we could test if a Flat_field correction was applied like we do for 2M
cat >> XDS.INP << eof
UNTRUSTED_RECTANGLE= 487 495 0 2528
UNTRUSTED_RECTANGLE= 981 989 0 2528
UNTRUSTED_RECTANGLE=1475 1483 0 2528
UNTRUSTED_RECTANGLE=1969 1977 0 2528
UNTRUSTED_RECTANGLE= 0 2464 195 213
UNTRUSTED_RECTANGLE= 0 2464 407 425
UNTRUSTED_RECTANGLE= 0 2464 619 637
UNTRUSTED_RECTANGLE= 0 2464 831 849
UNTRUSTED_RECTANGLE= 0 2464 1043 1061
UNTRUSTED_RECTANGLE= 0 2464 1255 1273
UNTRUSTED_RECTANGLE= 0 2464 1467 1485
UNTRUSTED_RECTANGLE= 0 2464 1679 1697
UNTRUSTED_RECTANGLE= 0 2464 1891 1909
UNTRUSTED_RECTANGLE= 0 2464 2103 2121
UNTRUSTED_RECTANGLE= 0 2464 2315 2333
eof
fi
fi
echo XDS.INP is ready for use. The file has only the most important keywords.
echo Full documentation, including complete detector templates, is at
echo http://www.mpimf-heidelberg.mpg.de/~kabsch/xds . More documentation in XDSwiki
echo After running xds, inspect, using XDS-Viewer, at least the beamstop mask in
echo BKGPIX.cbf, and the agreement of predicted and observed spots in FRAME.cbf!
rm -f tmp1 tmp2
# end of generate_XDS.INP
System-wide or personal installation
Ask your system adminstrator to cut-and-paste the script into e.g. /usr/local/bin/generate_XDS.INP, and to make it "executable".
But you may also cut-and-paste the script from this webpage into a file in e.g. your home directory; the filename should be generate_XDS.INP. After creating the file, make it executable - e.g. if it's in your $HOME, use:
chmod +x ~/generate_XDS.INP
After that, you can just run it in a similar way as if it were installed in your $PATH:
~/generate_XDS.INP "frms/mydata_1_???.img"
By using your own file, you can easily update to the latest revision, or even change the script, without having to bother the system administrator.
Generating generate_XDS.INP from this webpage
Instead of cutting-and-pasting the lines of the script, you (or the system administrator) could just cut-and-paste the following four lines
wget http://strucbio.biologie.uni-konstanz.de/xdswiki/index.php/generate_XDS.INP -O - | \ sed -e s/\ \;/\ /g -e s/\>\;/\>/g -e s/\<\;/\</g -e s/amp\;//g -e s/\"\;/\"/g -e s/\&\#\1\6\0\;/\ /g | \ sed '/# end of generate_XDS.INP/,$d' | awk '/^#/,/rm -f tmp1 tmp2/' > generate_XDS.INP chmod +x generate_XDS.INP
to copy the script from this website into an executable file generate_XDS.INP in your current directory.