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m
→‎The script: improve wording
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XDS [http://strucbio.biologie.uni-konstanz.de/~dikay/XDS_html_doc/html_doc/xds_parameters.html#NAME_TEMPLATE_OF_DATA_FRAMES= supports] bzip2-ed frames. Thus, when specifying the frame name parameter of the script, you should leave out any .bz2 extension.
 
XDS [http://strucbio.biologie.uni-konstanz.de/~dikay/XDS_html_doc/html_doc/xds_parameters.html#NAME_TEMPLATE_OF_DATA_FRAMES= 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 ("/").
+
For improved interaction with [[XDSGUI]], it is advantageous to provide an ''absolute'' filename for the data files - one that starts with a slash ("/").
    
== The script ==
 
== The script ==
    
<pre>
 
<pre>
 +
 
#!/bin/bash                                                                   
 
#!/bin/bash                                                                   
 
# purpose: generate XDS.INP                                                   
 
# purpose: generate XDS.INP                                                   
Line 93: Line 94:  
# revision 0.75 . KD 30/08/2017 reversed ORGX and ORGY for marCCD @ BM14 (Indian beamline @ ESRF)
 
# revision 0.75 . KD 30/08/2017 reversed ORGX and ORGY for marCCD @ BM14 (Indian beamline @ ESRF)
 
# revision 0.76 . KD 4/09/2017 include POSITION into REFINE(IDXREF) because latest XDS is more robust. Add comments to keywords.
 
# revision 0.76 . KD 4/09/2017 include POSITION into REFINE(IDXREF) because latest XDS is more robust. Add comments to keywords.
REVISION="0.76 (4-Sep-2017)"
+
# revision 0.77 . KD 19/12/2017 obtain QX QY from CBF header.
 +
# revision 0.78 . KD 21/12/2017 if possible and sensible, provide LIB= line with hardcoded /usr/local/lib64/dectris-neggia.so .
 +
# revision 0.79 . KD 16/01/2018 read OVERLOAD from Pilatus miniCBF header instead of fixing at 1048576
 +
# revision 0.80 . KD 13/02/2018 remove DISTANCE keyword from REFINE() list; remove POSITION from REFINE(IDXREF)
 +
# revision 0.81 . KD 21/02/2018 when encountering CBF files from Eiger (ESRF), treat as Pilatus detector
 +
# revision 0.82 . KD 01/03/2018 STARTING_ANGLE for MarCCD/Pilatus/PHOTON, enabling to use dials.rs_mapper with spot2pdb.
 +
# revision 0.83 . KD 25/06/2018 for ADSC detector #458 at APS BM19, revert the definition of ROTATION_AXIS=-1 0 0. See "Beamline notes" in this wiki.
 +
# revision 0.84 . KD 10/10/2018 implement Pilatus detector with d*TREK header
 +
# revision 0.85 . Jie Nan 09/01/2019 STARTING_ANGLE for Eiger
 +
# revision 0.86 . Keitaro 03/05/2019 Add PILATUS3 6M, S/N 60-0123 at SSRF BL18U-1 with ROTATION_AXIS=-1 0 0
 +
# revision 0.87 . KD 12/10/2019 Add PILATUS XXX, S/N XX-XXX at SSRF BL19U1 and MarCCD detector #43 at BL17B1 with ROTATION_AXIS=-1 0 0
 +
# revision 0.88 . KD 16/10/2019 fixes for SSRF, add "-maxdepth 1" to "find -H ..."
 +
# revision 0.89 . KD 21/10/2019 add ADSC S/N 905 at ALS 8.2.1, S/N 928 at Australian Synchrotron MX2 beamline; final SSRF fixes
 +
# revision 0.90 . KD 25/10/2019 add OLDMAR detector type. Tested w/ SBGrid data set 6. Anomalous signal may have wrong hand!
 +
# revision 0.91 . KD 16/01/2020 Allow negative starting angle for Eiger (found -33 at SLS !).
 +
# revision 0.92 . KD 27/02/2020 read *_master.h5 from Diamond Light Source
 +
# revision 0.93 . KD 13/03/2020 print out 2theta for MarCCD (DETECTOR_*_AXIS can be derived from this)
 +
# revision 0.94 . KD 16/03/2020 bugfix for Bruker-cbf to make bc accept e.g. 3.1e-005 by using awk printf "%.5f" instead of awk print
 +
# revision 0.95 . KD 29/07/2020 fix DLS Eiger HDF5 variant OSCILLATION_RANGE, STARTING_ANGLE. Attention: DLS Eiger variant needs h5dump 1.10 for OVERLOAD!
 +
# revision 0.96 . KD 03/10/2020 make script echo detector serial number if inverted ROTATION_AXIS is detected.
 +
# revision 0.97 . KD 19/10/2020 add UNTRUSTED_RECTANGLEs for Eiger2 (which has a few pixels less than Eiger (thanks to Andreas Förster)
 +
# revision 0.98 . Thomas Hauß (HZB) 06/11/2020 switch Python print syntax to Python3
 +
# revision 0.99 . Aaron Finke (CHESS) 07/11/2020 add ROTATION_AXIS=-1 0 0 for EIGER2 16M detector at MX beamline ID7B2 (CHESS)
 +
# revision 1.00 . Gleb Bourenkov 10/11/2020 add ROTATION_AXIS=0 -1 0 for beamline P14 (EMBL Hamburg) detectors Eiger 16M S/N E-32-0107; previously Eiger 4M S/N E-08-0107 and PILATUS 6M-F, S/N 60-0115-F
 +
# revision 1.01 . KD 07/12/2020 ROTATION_AXIS=0 -1 0 for Pilatus3 2M, S/N 24-0118 at ID23-2 (http://www.globalphasing.com/autoproc/wiki/index.cgi?BeamlineSettings)
 +
# revision 1.02 . KD 11/01/2021 recognize mar555 detector as mar345 (thanks to Thomas Hauß, HZB)
 +
# revision 1.03 . Feng YU 18/7/2021 fix/expand information about Shanghai Synchrotron Radiation Facility (SSRF)
 +
# revision 1.04 . Zhipu Luo 13/08/2021 extract ORGX,ORGY for electron diffraction from SMV header if the wavelength value starts with 0.0
 +
# revision 1.05 . KD specialcase extraction of number of images for BNL detectors E-32-0101 and E-18-0104
 +
# revision 1.06 . KD fix URLs in output. Availability of Apple M1 processor dectris-neggia-Apple-arm64.so . LC_ALL=C .
 +
REVISION="1.06 (15-OCT-2021)"
    
#                                                                                                             
 
#                                                                                                             
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# - for ADSC detectors, there are at least three ways to obtain ORGX and ORGY values from the header (see below);
 
# - 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)  
 
# - 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                             
+
# - on Mac OS X, the Xcode command line tools (from https://developer.apple.com/download/more/) are needed.                           
 
#                                                                                                                 
 
#                                                                                                                 
 
# notes for debugging of the script:                                                                             
 
# notes for debugging of the script:                                                                             
# - add the -v option to the first line, to see where an error occurs                                             
+
# - add the -x option to the 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                                                     
 
#                                                                                                                 
 
#                                                                                                                 
Line 117: Line 148:  
   exit                                                                                                           
 
   exit                                                                                                           
 
fi                                                                                                               
 
fi                                                                                                               
 +
# make sure the locale does not interfere with e.g. awk calculations:
 +
LC_ALL="C";export LC_ALL
 
#                                                                                                                 
 
#                                                                                                                 
 
# defaults:                                                                                                       
 
# defaults:                                                                                                       
#                                                                                                              
+
#      
 +
# conversion radian / degrees:
 +
DEGTOR=57.2957795
 +
                                                                                                       
 
DETECTOR="XXX MINIMUM_VALID_PIXEL_VALUE=XXX OVERLOAD=XXX"                                                         
 
DETECTOR="XXX MINIMUM_VALID_PIXEL_VALUE=XXX OVERLOAD=XXX"                                                         
 
REVERSE_PHI="no"
 
REVERSE_PHI="no"
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# default FRACTION_OF_POLARIZATION
 
# default FRACTION_OF_POLARIZATION
 
pol_frac=0.98
 
pol_frac=0.98
 +
STARTING_ANGLE=0
 +
dtrek_det=""
 +
SEPMIN=7.0
 +
CLUSTER_RADIUS=3.5
 +
REFINE_CORRECT="CELL BEAM ORIENTATION AXIS POSITION ! Default is: refine everything"
    
dname=`echo "$1" | xargs dirname`
 
dname=`echo "$1" | xargs dirname`
Line 149: Line 190:  
# cope with blanks in directory / file name
 
# cope with blanks in directory / file name
 
IFS=$'\n'
 
IFS=$'\n'
find -H $dname -name "$bname" -or -name "${bname}.bz2" -or -name "${bname}.gz" -or -name "${bname}.xz" | egrep -v "_00000.cbf|_000.img" | sort > tmp1
+
find -H $dname -maxdepth 1 -name "$bname" -or -name "${bname}.bz2" -or -name "${bname}.gz" -or -name "${bname}.xz" | egrep -v "_00000.cbf|_000.img" | sort > tmp1
 
if [ ! -s tmp1 ]
 
if [ ! -s tmp1 ]
 
then
 
then
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  data_last=`cut -b $pos1-$pos2 tmp1 | tail -n1 | bc`
 
  data_last=`cut -b $pos1-$pos2 tmp1 | tail -n1 | bc`
 
  DATA_RANGE="$data_first $data_last"
 
  DATA_RANGE="$data_first $data_last"
 +
echo DATA_RANGE=$DATA_RANGE
 
   
 
   
 
  # set SPOT_RANGE to first half of DATA_RANGE
 
  # set SPOT_RANGE to first half of DATA_RANGE
Line 179: Line 221:  
FIRSTFRAME=`head -1 tmp1`
 
FIRSTFRAME=`head -1 tmp1`
 
echo $FIRSTFRAME | grep "\.h5$" && is_h5=1 || is_h5=0
 
echo $FIRSTFRAME | grep "\.h5$" && is_h5=1 || is_h5=0
  −
if [ "$is_h5" == 1 ]; then
  −
# nframes=`h5dump -A -g "/entry/data" $FIRSTFRAME | grep "DATASPACE  SIMPLE" | sed -e "s/,.*//" | awk '{a+=$5}END{print a}'`
  −
nframes=`h5dump -d "/entry/instrument/detector/detectorSpecific/nimages" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
  −
DATA_RANGE="1 $nframes"
  −
SPOT_RANGE="1 `echo "scale=0; ${nframes}/2"|bc -l`"
  −
fi
  −
  −
echo DATA_RANGE=$DATA_RANGE
      
# find out detector type
 
# find out detector type
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  # the reason is that FIRSTFRAME may contain a blank, which makes some commands fail                                                 
 
  # the reason is that FIRSTFRAME may contain a blank, which makes some commands fail                                                 
 
  egrep -qi 'marccd|Corrected' tmp2 && DET=mccd                                 
 
  egrep -qi 'marccd|Corrected' tmp2 && DET=mccd                                 
  grep -q PILATUS tmp2            && DET=pilatus                            
+
  grep -q PILATUS tmp2            && DET=pilatus  
 +
grep -iq Eiger tmp2              && DET=pilatus                           
 
  head -n1 tmp2 | grep -q "^RAXIS" && DET=raxis
 
  head -n1 tmp2 | grep -q "^RAXIS" && DET=raxis
 
  head -n1 tmp2 | grep -q "^R-AXIS" && DET=raxis
 
  head -n1 tmp2 | grep -q "^R-AXIS" && DET=raxis
 
  grep -q "^SOURCE_WAVELENGTH= *1" tmp2 && DET=dtrek
 
  grep -q "^SOURCE_WAVELENGTH= *1" tmp2 && DET=dtrek
 
  grep -q BEAM_CENTER_X tmp2      && DET=adsc                                 
 
  grep -q BEAM_CENTER_X tmp2      && DET=adsc                                 
  grep -q mar345 tmp2 && DET=MAR345    
+
  grep -q mar345 tmp2 && DET=MAR345
 +
# rev. 1.02: in one case, mar555 data could be processed pretending it is mar345, so:
 +
grep -q mar555 tmp2 && DET=MAR345
 
  grep -q BRUKER tmp2 && grep -q CBF tmp2  && DET=Bruker-cbf   
 
  grep -q BRUKER tmp2 && grep -q CBF tmp2  && DET=Bruker-cbf   
  grep -q CMOS1 tmp2 && DET=adsc-CMOS1                  
+
  grep -q CMOS1 tmp2 && DET=adsc-CMOS1  
 +
grep -q MARCONTROL tmp2 && DET=OLDMAR 
 +
grep -q "WAVELENGTH=0.0" tmp2 && DET=experimental-ED                                   
 
else
 
else
 
  h5dump -d "/entry/instrument/detector/description" $FIRSTFRAME | grep -i Eiger > /dev/null && DET=eiger
 
  h5dump -d "/entry/instrument/detector/description" $FIRSTFRAME | grep -i Eiger > /dev/null && DET=eiger
Line 227: Line 265:  
elif [ "$DET" == "mccd" ]; then  
 
elif [ "$DET" == "mccd" ]; then  
 
   echo Data from a MarCCD detector
 
   echo Data from a MarCCD detector
 +
# http://www.sb.fsu.edu/~xray/Manuals/marCCD165header.html has header information
 
                                    
 
                                    
 
   DETECTOR="CCDCHESS MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65500"
 
   DETECTOR="CCDCHESS MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65500"
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   # Check detector serial number and recognize beamline for reversed-phi setting.
 
   # Check detector serial number and recognize beamline for reversed-phi setting.
 
   # Known detectors for reversed-phi in SPring-8: 24: BL26B2 Mar225, 31: BL32XU MX225HE, 38: BL44XU MX225HE, 42: BL44XU MX300HE, 40: BL41XU MX225HE, 106: BL32XU MX225HS
 
   # Known detectors for reversed-phi in SPring-8: 24: BL26B2 Mar225, 31: BL32XU MX225HE, 38: BL44XU MX225HE, 42: BL44XU MX300HE, 40: BL41XU MX225HE, 106: BL32XU MX225HS
 +
  # same for SSRF: BL17B1 rayonix MX300. As on 2019-10-13, this also needs doubling of ORGX and ORGY. But the beamline staff (Wenming) wants to fix the header.
 
   REVERSEPHI_SNs="
 
   REVERSEPHI_SNs="
 
24
 
24
Line 240: Line 280:  
40
 
40
 
42
 
42
 +
43
 
106
 
106
 
"
 
"
Line 246: Line 287:  
   if echo "${DET_SN}${REVERSEPHI_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
   if echo "${DET_SN}${REVERSEPHI_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
     REVERSE_PHI="yes"
 
     REVERSE_PHI="yes"
 +
    echo inverted ROTATION_AXIS since Detector Serial Number is "${DET_SN}"
 
   fi
 
   fi
   Line 260: Line 302:  
   DETECTOR_DISTANCE=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')
 
   DETECTOR_DISTANCE=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')
 
   DETECTOR_DISTANCE=`echo "scale=3; $DETECTOR_DISTANCE/1000" | bc -l`                                     
 
   DETECTOR_DISTANCE=`echo "scale=3; $DETECTOR_DISTANCE/1000" | bc -l`                                     
                                                                                                         
+
 
 +
# Mar 12, 2020 KD
 +
  let SKIP=1724
 +
  TWOTHETA=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')
 +
  TWOTHETA=`echo "scale=3; $TWOTHETA/1000" | bc -l`
 +
  echo 2THETA= $TWOTHETA
 +
 
 +
  let SKIP=1024+256+128+256+44
 +
  STARTING_ANGLE=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')
 +
  STARTING_ANGLE=`echo "scale=2; $STARTING_ANGLE/1000" | bc -l `
 +
  echo STARTING_ANGLE= $STARTING_ANGLE 
 +
                                                                                                     
 
   let SKIP=1024+256+128+256+4                                                                             
 
   let SKIP=1024+256+128+256+4                                                                             
 
   ORGX=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')             
 
   ORGX=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')             
Line 267: Line 320:  
   ORGY=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')             
 
   ORGY=$(od -t dI -j $SKIP -N 4 tmp2 | head -1 | awk '{print $2}')             
 
   ORGY=`echo "scale=2; $ORGY/1000" | bc -l `                                                               
 
   ORGY=`echo "scale=2; $ORGY/1000" | bc -l `                                                               
# FIXME 25.5.2015: reverse ORGX and ORGY for BM14 @ ESRF (no serial number in header)
   
# fixed Aug 30, 2017 after IUCr2017 @ Hyderabad  
 
# fixed Aug 30, 2017 after IUCr2017 @ Hyderabad  
 
   if [ "$DET_SN" == "4" ]; then
 
   if [ "$DET_SN" == "4" ]; then
Line 320: Line 372:  
       BEAM_CENTER_X=`grep BEAM_CENTER_X tmp2 | sed s/BEAM_CENTER_X=//`
 
       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=//`
 
       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="
 
       COMMENT_ORGXY="
 
! Following are possible beam center interpretations for ADSC detectors"
 
! Following are possible beam center interpretations for ADSC detectors"
# at ESRF, PF, ALS 5.0.2 and ... (pls fill in!) the following should be used:         
+
# at ESRF, PF, ALS 5.0.2, AS MX2 and ... (pls fill in!) the following should be used:         
 
       ORGX1=`echo "scale=1; $BEAM_CENTER_Y/$QX" | bc -l`
 
       ORGX1=`echo "scale=1; $BEAM_CENTER_Y/$QX" | bc -l`
 
       ORGY1=`echo "scale=1; $BEAM_CENTER_X/$QX" | bc -l`
 
       ORGY1=`echo "scale=1; $BEAM_CENTER_X/$QX" | bc -l`
       echo - at ESRF, PF, APS Argonne BLs use: ORGX=$ORGX1 ORGY=$ORGY1                     
+
       echo - at ESRF, PF, ALS 8.2.1, APS Argonne BLs use: ORGX=$ORGX1 ORGY=$ORGY1                     
 
       COMMENT_ORGXY="${COMMENT_ORGXY}
 
       COMMENT_ORGXY="${COMMENT_ORGXY}
! ORGX= $ORGX1 ORGY= $ORGY1 ! For ESRF, PF, APS Argonne ..."
+
! ORGX= $ORGX1 ORGY= $ORGY1 ! For ESRF, PF, APS, AS MX2 ..."
 
# this 2nd alternative convention should be used at the following beamlines (pls complete the list): ALS 5.0.3, ...
 
# 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 `
 
       ORGX2=`echo "scale=1; $NX-$BEAM_CENTER_X/$QX" | bc -l `
Line 351: Line 403:  
       # Decision of beam center convention based on detector serial numbers.
 
       # Decision of beam center convention based on detector serial numbers.
 
       DET_SN=`grep DETECTOR_SN tmp2 | sed -e "s/DETECTOR_SN=//"`
 
       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, 923: ALS BL5.0.2 Q315, 933: AichiSR BL2S1 Q315, 916: APS 24 IDE
+
      echo Detector serial number is $DET_SN
 +
       # For convention 1; Known PF detectors = 449: NW12A Q210, 472: NE3A Q270, 474: BL17A Q270, 912: BL5A Q315, 923: ALS BL5.0.2 Q315, 933: AichiSR BL2S1 Q315, 916: APS 24 IDE, 928: AS MX2
 
       ORG1_SNs="
 
       ORG1_SNs="
 
449
 
449
Line 362: Line 415:  
446
 
446
 
916
 
916
 +
905
 +
928
 
"
 
"
 
       ORG4_SNs="
 
       ORG4_SNs="
Line 369: Line 424:  
       ORGX=$ORGX1
 
       ORGX=$ORGX1
 
       ORGY=$ORGY1
 
       ORGY=$ORGY1
 +
      echo the following was chosen based on detector serial number:
 
       elif echo "${DET_SN}${ORG4_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
       elif echo "${DET_SN}${ORG4_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
       ORGX=$ORGX4
 
       ORGX=$ORGX4
 
       ORGY=$ORGY4
 
       ORGY=$ORGY4
 +
      echo the following was chosen based on detector serial number:
 
       else
 
       else
 
       ORGX=$ORGX3
 
       ORGX=$ORGX3
 
       ORGY=$ORGY3
 
       ORGY=$ORGY3
 +
      echo the following default was chosen because the detector serial number was not special-cased:
 
       fi
 
       fi
    
       # Check detector serial number and recognize beamline for reversed-phi setting.
 
       # Check detector serial number and recognize beamline for reversed-phi setting.
 
       # Known detectors for reversed-phi in SPring-8: 915: BL38B1 Q315; APS 19-ID: 458; BM30A: 924
 
       # Known detectors for reversed-phi in SPring-8: 915: BL38B1 Q315; APS 19-ID: 458; BM30A: 924
 +
      # 928 is at Australian Beamline MX2
 +
      # revision 0.83 of this script removes 458 from the list!
 
       REVERSEPHI_SNs="
 
       REVERSEPHI_SNs="
 
915
 
915
458
   
924
 
924
 +
928
 
"
 
"
 
       if echo "${DET_SN}${REVERSEPHI_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
       if echo "${DET_SN}${REVERSEPHI_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
         REVERSE_PHI="yes"
 
         REVERSE_PHI="yes"
 +
        echo inverted ROTATION_AXIS since detector serial number is ${DET_SN}
 
       fi
 
       fi
   Line 408: Line 469:  
   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=//`   
   DIRECTION_OF_DETECTOR_X_AXIS="-1 0 0"                                                                 
+
   DIRECTION_OF_DETECTOR_X_AXIS="-1 0 0"  
 +
                                                                  
 +
elif [ "$DET" == "experimental-ED" ]; then
 +
  DETECTOR="ADSC MINIMUM_VALID_PIXEL_VALUE= 1 OVERLOAD= 65000  ! OVERLOAD is really unknown "
 +
  echo --- Electron diffraction data in SMV format!
 +
  SENSOR_THICKNESS=0.01                                                       
 +
  sed s/\;// tmp2 > tmp1                                                     
 +
  mv tmp1 tmp2                                                               
 +
  X_RAY_WAVELENGTH=`grep WAVELENGTH tmp2 | head -1 | sed s/WAVELENGTH=//`
 +
  NX=`grep SIZE1 tmp2 | tail -1 | sed s/SIZE1=//`
 +
  QX=`grep PIXEL_SIZE tmp2 | sed s/PIXEL_SIZE=//`
 +
  NY=`grep SIZE2 tmp2 | tail -1 | sed s/SIZE2=//`                                           
 +
  QY=$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=//`
 +
  QXY=`echo "scale=1; $QX*($BEAM_CENTER_X+$BEAM_CENTER_Y)" | bc -l`
 +
      if [ "$QXY" "<" "$BEAM_CENTER_X" ] ; then
 +
      ORGX=`echo "scale=2; $BEAM_CENTER_Y/$QX" | bc -l`
 +
      ORGY=`echo "scale=2; $BEAM_CENTER_X/$QX" | bc -l`
 +
      else
 +
      ORGX=`echo "scale=2; $BEAM_CENTER_X/1" | bc -l`
 +
      ORGY=`echo "scale=2; $BEAM_CENTER_Y/1" | bc -l`
 +
      fi
 +
  DETECTOR_DISTANCE=`grep ^DISTANCE tmp2 | sed s/DISTANCE=//`                                                                   
 +
  OSCILLATION_RANGE=`grep OSC_RANGE tmp2 | sed s/OSC_RANGE=//`
 +
  STARTING_ANGLE=`grep OSC_START tmp2 | sed s/OSC_START=//`
 +
  echo --- For TIMEPIX detector, please fix ROTATION_AXIS yourself!
 +
  DIRECTION_OF_DETECTOR_X_AXIS="1 0 0"
 +
  REFINE_CORRECT="ORIENTATION CELL AXIS BEAM ! for ED, no POSITION when CELL is refined"
    
elif [ "$DET" == "pilatus" ]; then
 
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                                         
 
   echo Data from a Pilatus detector                                         
 
   sed s/#// tmp2 > tmp1                                                     
 
   sed s/#// tmp2 > tmp1                                                     
 
   mv tmp1 tmp2                                                               
 
   mv tmp1 tmp2                                                               
 +
  OVERLOAD=1048574
 +
  SEPMIN=4
 +
  CLUSTER_RADIUS=2
 +
  grep -q Count_cutoff tmp2 && OVERLOAD=`awk '/Count_cutoff/{print $2}' tmp2`
 +
  DETECTOR="PILATUS MINIMUM_VALID_PIXEL_VALUE=0 OVERLOAD= $OVERLOAD  !PILATUS"
 +
  QX=0.172 QY=0.172                                                       
 +
# the default above guards against missing Pixel_size line in CBF header
 +
  grep -q Pixel_size tmp2 && QX=`awk '/Pixel_size/{print 1000*$2}' tmp2`
 +
  grep -q Pixel_size tmp2 && QY=`awk '/Pixel_size/{print 1000*$5}' tmp2`                                                   
    
       # find SENSOR_THICKNESS:
 
       # find SENSOR_THICKNESS:
Line 430: Line 526:  
       ORGY=`grep Beam_xy tmp2 | sed -e s/\(// -e s/\)// -e s/\,// | awk '{print $3}'`
 
       ORGY=`grep Beam_xy tmp2 | sed -e s/\(// -e s/\)// -e s/\,// | awk '{print $3}'`
   −
       # find DETECTOR_DISTANCE and OSCILLATION_RANGE:
+
       # find DETECTOR_DISTANCE, OSCILLATION_RANGE, and STARTING_ANGLE:
       DETECTOR_DISTANCE=`awk '/distance/{print $2}' tmp2`
+
       DETECTOR_DISTANCE=`awk '/Detector_distance/{print $2}' tmp2`
 
       DETECTOR_DISTANCE=`echo "$DETECTOR_DISTANCE*1000" | bc -l`
 
       DETECTOR_DISTANCE=`echo "$DETECTOR_DISTANCE*1000" | bc -l`
   −
       OSCILLATION_RANGE=`awk '/Angle/{print $2}' tmp2`
+
       OSCILLATION_RANGE=`awk '/Angle_increment/{print $2}' tmp2`
 +
 
 +
      STARTING_ANGLE=`awk '/Start_angle/{print $2}' tmp2`
 +
      echo STARTING_ANGLE= $STARTING_ANGLE 
    
       # get detector serial number and check if it is included in the list
 
       # get detector serial number and check if it is included in the list
Line 441: Line 540:  
       # Known detectors for reversed-phi at MX2 beamline (Brazilian Synchrotron National Laboratory - LNLS)
 
       # Known detectors for reversed-phi at MX2 beamline (Brazilian Synchrotron National Laboratory - LNLS)
 
       # Known detectors for reversed-phi at CHESS F1 PILATUS3 6M, S/N 60-0127
 
       # Known detectors for reversed-phi at CHESS F1 PILATUS3 6M, S/N 60-0127
 +
      # Known detectors for reversed-phi at SSRF BL18U1 (S/N 60-0123) and BL19U1 (S/N XX-XXX) (!; 2019-10-19: staff will fix this)
 
       DET_SN=`grep "Detector:" tmp2 | sed "s/^.*Detector: *//"`
 
       DET_SN=`grep "Detector:" tmp2 | sed "s/^.*Detector: *//"`
 
       REVERSEPHI_SNs="
 
       REVERSEPHI_SNs="
Line 447: Line 547:  
PILATUS 2M, S/N 24-0109
 
PILATUS 2M, S/N 24-0109
 
PILATUS3 6M, S/N 60-0127
 
PILATUS3 6M, S/N 60-0127
 +
PILATUS3 6M, S/N 60-0123
 
"
 
"
 
       if echo "${DET_SN}${REVERSEPHI_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
       if echo "${DET_SN}${REVERSEPHI_SNs}" | sort | uniq -d | grep [0-9] > /dev/null; then
 
         REVERSE_PHI="yes"
 
         REVERSE_PHI="yes"
 +
        echo inverted ROTATION_AXIS since detector serial number is ${DET_SN}
 +
      fi
 +
      if [ "$DET_SN" == "PILATUS XXX, S/N XX-XXX" ] ; then
 +
        REVERSE_PHI="yes"
 +
        echo inverted rotation axis at SSRF BL19U1
 
       fi
 
       fi
 
        
 
        
Line 456: Line 562:  
         if grep -q "Oscillation_axis X.CW +SLOW" tmp2 ; then
 
         if grep -q "Oscillation_axis X.CW +SLOW" tmp2 ; then
 
           rotation_axis="0 -1 0"
 
           rotation_axis="0 -1 0"
 +
          echo ROTATION_AXIS="0 -1 0" at Diamond I24
 
         fi
 
         fi
 
       fi
 
       fi
# insert similar code for Petra P14 here
+
# PETRA P14: raw data from Eiger are stored as CBF files so this is treated as Pilatus
 +
      if [ "$DET_SN" == "Dectris Eiger 16M, E-32-0107" -o "$DET_SN" == "Dectris Eiger 4M, E-08-0107" -o "$DET_SN" == "PILATUS 6M-F, S/N 60-0115-F" ] ; then
 +
        rotation_axis="0 -1 0"
 +
        echo ROTATION_AXIS="0 -1 0" at PETRA P14
 +
      fi
 +
# ESRF ID23-2:
 +
      if [ "$DET_SN" == "PILATUS3 2M, S/N 24-0118, ESRF ID23" ] ; then
 +
        rotation_axis="0 -1 0"
 +
        echo ROTATION_AXIS="0 -1 0" at ESRF ID23-2
 +
      fi
 +
 
 
elif [ "$DET" == "eiger" ]; then
 
elif [ "$DET" == "eiger" ]; then
   OVERLOAD=`h5dump -d "/entry/instrument/detector/detectorSpecific/countrate_correction_count_cutoff" $FIRSTFRAME | awk '/\(0\):/{print $2}' `
+
nframes=`h5dump -d "/entry/instrument/detector/detectorSpecific/nimages" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
   DETECTOR="EIGER MINIMUM_VALID_PIXEL_VALUE=0 OVERLOAD= $OVERLOAD !EIGER"
+
DATA_RANGE="1 $nframes"
 +
SPOT_RANGE="1 `echo "scale=0; if (${nframes}<2) 1; if (${nframes}>1) ${nframes}/2"|bc -l`"
 +
 +
# find out if HDF5 from Diamond (DLS=1) or Dectris (DLS=0)
 +
  DLS=0
 +
   OVERLOAD=`h5dump -d "/entry/instrument/detector/detectorSpecific/countrate_correction_count_cutoff" $FIRSTFRAME 2>/dev/null` || DLS=1
 +
  if [ "$DLS" == 1 ]; then
 +
    echo Eiger HDF5 from Diamond
 +
# unfortunately h5dump 1.10 is required to get this right for the DLS .h5 files. This version is available at DLS but maybe not elsewhere
 +
    OVERLOAD=`h5dump -d "/entry/instrument/detector/saturation_value" $FIRSTFRAME | awk '/\(0\):/{print $2}'`
 +
  # v0.95: fix the next 2 lines by taking care of negative values with the \- , and stop after first "(0)"
 +
    OSCILLATION_RANGE=`h5dump -d "/entry/data/omega" $FIRSTFRAME | awk '/\(0\): [\-0-9]/{print $3-$2;exit}'`
 +
    STARTING_ANGLE=`h5dump    -d "/entry/data/omega" $FIRSTFRAME | awk '/\(0\): [\-0-9]/{print $2;exit}' | sed -e "s/,//"`
 +
    echo OSCILLATION_RANGE=$OSCILLATION_RANGE STARTING_ANGLE=$STARTING_ANGLE
 +
  # rotation_axis=`h5dump -a "/entry/sample/transformations/omega/vector" $FIRSTFRAME 2>/dev/null | grep "(0):" | sed -e "s/^.*://; s/,//g"`
 +
  # the above gives -1 0 0 for DLS data instead of the correct 1 0 0, so commented out for now
 +
  else
 +
    echo Eiger HDF5 from Dectris
 +
    OVERLOAD=`h5dump -d "/entry/instrument/detector/detectorSpecific/countrate_correction_count_cutoff" $FIRSTFRAME | awk '/\(0\):/{print $2}'`   
 +
    OSCILLATION_RANGE=`h5dump -d "/entry/sample/goniometer/omega_range_average" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
 +
  # STARTING_ANGLE:  the \- was introduced in version 0.91 to allow negative values :
 +
    STARTING_ANGLE=`h5dump -d "/entry/sample/goniometer/omega_start" $FIRSTFRAME | awk '/\(0\): [\-0-9]/{print $2}'`
 +
  # /entry/sample/goniometer/omega_start is missing in some eiger2 detectors (e.g. Eiger2 9M with fw version release-2020.2.1 and SIMPLON API 1.8) (Feng YU 2021-07-18)
 +
    if [ "$STARTING_ANGLE" == "" ]; then
 +
  echo "/entry/sample/goniometer/omega_start not found, try /entry/sample/goniometer/omega"
 +
  STARTING_ANGLE=`h5dump -d /entry/sample/goniometer/omega $FIRSTFRAME | grep "(0):" | head -n 1 | awk '{print $2}' | sed -e "s/,//g"`
 +
    fi
 +
    echo "STARTING_ANGLE=$STARTING_ANGLE"
 +
  # If rotation vector set (NeXus)
 +
    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
 +
    SN=`h5dump -d "/entry/instrument/detector/detector_number" $FIRSTFRAME | awk '/\(0\): /{print $2}' | sed s/\"//g`
 +
    if [ "$SN" == "E-32-0123" ]; then
 +
      rotation_axis="-1 0 0"
 +
      echo CHESS ID7B2 with inverted rotation axis
 +
    fi
 +
  # SSRF BL17U1 and SSRF BL10U2 (Feng YU 2021-07-18)
 +
  # Eiger X 16M (S/N E-32-0111) was installed at SSRF BL17U1 from Oct 2017 to Feb 2021. After Feb 2021, it was moved back to SSRF BL10U2.
 +
# 2021-02-01 00:00:00 CST time stamp is 1612108800
 +
    if [ "$SN" == "E-32-0111" ]; then
 +
      collection_time=`h5dump -d "/entry/instrument/detector/detectorSpecific/data_collection_date" $FIRSTFRAME | grep "(0):" | awk '{print $2}' | sed -e "s/\.\(.*\)/CST/g; s/\"//g"`
 +
      if [ `uname -s` == "Darwin" ]; then
 +
        collection_timestamp=`date -j -f "%Y-%m-%dT%H:%M:%S%Z" $collection_time +%s`
 +
      elif [ `uname -s` == "Linux" ]; then
 +
        collection_timestamp=`date -d $collection_time +%s`
 +
      else
 +
        collection_timestamp=0
 +
      fi
 +
      if [ $collection_timestamp -eq 0 ]; then
 +
        is_rotation_axis_set=1
 +
        rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME 2>/dev/null || is_rotation_axis_set=0`
 +
        if [ "$is_rotation_axis_set" == "1" ]; then
 +
          rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME | grep "(0):" | sed -e "s/^.*://; s/,//g"`
 +
          echo "The rotation axis of SSRF BL10U2 (Eiger X 16M) is $rotation_axis"
 +
        else
 +
          rotation_axis="-1 0 0    ! Cannot determine rotation axis. SSRF BL17U1: -1 0 0; SSRF BL02U1: 0 -1 0"
 +
        fi
 +
      elif [ $collection_timestamp -ge 0 ] && [ $collection_timestamp -le 1612108800 ]; then
 +
        # SSRF BL17U1
 +
        rotation_axis="-1 0 0"
 +
        echo "SSRF BL17U1 (Eiger X 16M) with inverted rotation axis"
 +
      else
 +
        # SSRF BL10U2
 +
        is_rotation_axis_set=1
 +
        rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME 2>/dev/null || is_rotation_axis_set=0`
 +
        if [ "$is_rotation_axis_set" == "1" ]; then
 +
          rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME | grep "(0):" | sed -e "s/^.*://; s/,//g"`
 +
          echo "The rotation axis of SSRF BL10U2 (Eiger X 16M) is $rotation_axis"
 +
        else
 +
          rotation_axis="0 -1 0"
 +
          echo "SSRF BL10U2 (Eiger X 16M) with vertical rotation axis"
 +
        fi
 +
      fi
 +
    fi
 +
  # SSRF BL02U1 (Feng YU 2021-07-18)
 +
  # EIGER2 S 9M SSRF BL02U1 has S/N E-18-0121
 +
    if [ "$SN" == "E-18-0121" ]; then
 +
      is_rotation_axis_set=1
 +
      rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME 2>/dev/null || is_rotation_axis_set=0`
 +
      if [ "$is_rotation_axis_set" == "1" ]; then
 +
        rotation_axis=`h5dump -d "/SSRF/RotationAxis" $FIRSTFRAME | grep "(0):" | sed -e "s/^.*://; s/,//g"`
 +
        echo "The rotation axis of SSRF BL02U1 (Eiger2 S 9M) is $rotation_axis"
 +
      else
 +
        rotation_axis="1 0 0"
 +
        echo "SSRF BL02U1 (Eiger2 S 9M) with horizontal rotation axis"
 +
      fi
 +
    fi
 +
# revision 1.05 specialcase nframes for Eiger detectors at BNL
 +
    if [ "$SN" == "E-18-0121" -o "$SN" == "E-32-0101" ]; then
 +
      echo specialcase nframes for Eiger detectors at BNL:
 +
      nframes=`h5dump -A -g "/entry/data" $FIRSTFRAME | grep "DATASPACE  SIMPLE" | sed -e "s/,.*//" | awk '{a+=$5}END{print a}'`
 +
      DATA_RANGE="1 $nframes"
 +
      SPOT_RANGE="1 `echo "scale=0; if (${nframes}<2) 1; if (${nframes}>1) ${nframes}/2"|bc -l`"
 +
    fi
 +
  fi
 +
  echo DATA_RANGE=$DATA_RANGE
 +
   DETECTOR="EIGER MINIMUM_VALID_PIXEL_VALUE=0 OVERLOAD= $OVERLOAD"
 
   QX=`h5dump -d "/entry/instrument/detector/x_pixel_size" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
 
   QX=`h5dump -d "/entry/instrument/detector/x_pixel_size" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
 
   QY=`h5dump -d "/entry/instrument/detector/y_pixel_size" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
 
   QY=`h5dump -d "/entry/instrument/detector/y_pixel_size" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
   −
   echo Data from a Eiger hdf5
+
   echo OVERLOAD=$OVERLOAD
      SENSOR_THICKNESS=`h5dump -d "/entry/instrument/detector/sensor_thickness" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
+
  SENSOR_THICKNESS=`h5dump -d "/entry/instrument/detector/sensor_thickness" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
      X_RAY_WAVELENGTH=`h5dump -d "/entry/instrument/beam/incident_wavelength" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
+
  X_RAY_WAVELENGTH=`h5dump -d "/entry/instrument/beam/incident_wavelength" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
   −
      NX=`h5dump -d "/entry/instrument/detector/detectorSpecific/x_pixels_in_detector" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
+
  NX=`h5dump -d "/entry/instrument/detector/detectorSpecific/x_pixels_in_detector" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
      NY=`h5dump -d "/entry/instrument/detector/detectorSpecific/y_pixels_in_detector" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
+
  NY=`h5dump -d "/entry/instrument/detector/detectorSpecific/y_pixels_in_detector" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
   −
      # find ORGX and ORGY:
+
  # find ORGX and ORGY:
      ORGX=`h5dump -d "/entry/instrument/detector/beam_center_x" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
+
  ORGX=`h5dump -d "/entry/instrument/detector/beam_center_x" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
      ORGY=`h5dump -d "/entry/instrument/detector/beam_center_y" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
+
  ORGY=`h5dump -d "/entry/instrument/detector/beam_center_y" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
 +
 
 +
  # find DETECTOR_DISTANCE :
 +
  DETECTOR_DISTANCE=`h5dump -d "/entry/instrument/detector/detector_distance" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'` 
   −
      # find DETECTOR_DISTANCE and OSCILLATION_RANGE:
+
  SEPMIN=4
      DETECTOR_DISTANCE=`h5dump -d "/entry/instrument/detector/detector_distance" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2*1000}'`
+
  CLUSTER_RADIUS=2
      OSCILLATION_RANGE=`h5dump -d "/entry/sample/goniometer/omega_range_average" $FIRSTFRAME | awk '/\(0\): [0-9]/{print $2}'`
     −
      # If rotation vector set (NeXus)
  −
      rotation_axis=`h5dump -a "/entry/sample/transformations/omega/vector" $FIRSTFRAME 2>/dev/null | grep "(0):" | sed -e "s/^.*://; s/,//g"`
  −
 
   
elif [ "$DET" == "raxis" ]; then
 
elif [ "$DET" == "raxis" ]; then
 
   echo Data from a RAXIS detector
 
   echo Data from a RAXIS detector
Line 489: Line 701:  
   #let SKIP=768
 
   #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=$(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("'$FIRSTFRAME'","rb");f.seek(768);print "%.4d"%struct.unpack(">i",f.read(4))')
+
!  NX=$(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("'$FIRSTFRAME'","rb");f.seek(772);print "%.4d"%struct.unpack(">i",f.read(4))')
+
!  NY=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(772);print "%.4d"%struct.unpack(">i",f.read(4))')
 +
   NX=$(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("'$FIRSTFRAME'","rb");f.seek(344);print "-%.4f"%struct.unpack(">f",f.read(4))')
+
!  DETECTOR_DISTANCE=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(344);print "-%.4f"%struct.unpack(">f",f.read(4))')
 +
   DETECTOR_DISTANCE=$(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("'$FIRSTFRAME'","rb");f.seek(540);print "%.4f"%struct.unpack(">f",f.read(4))')
+
!  ORGX=$(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("'$FIRSTFRAME'","rb");f.seek(544);print "%.4f"%struct.unpack(">f",f.read(4))')
+
!  ORGY=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(544);print "%.4f"%struct.unpack(">f",f.read(4))')
 +
   ORGX=$(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("'$FIRSTFRAME'","rb");f.seek(524);phis,phie=struct.unpack(">ff",f.read(8));print "%.4f"%(phie-phis)')
+
!  OSCILLATION_RANGE=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(524);phis,phie=struct.unpack(">ff",f.read(8));print "%.4f"%(phie-phis)')
 +
   OSCILLATION_RANGE=$(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("'$FIRSTFRAME'","rb");f.seek(776);print "%.6f"%struct.unpack(">f",f.read(4))')
+
!  QX=$(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("'$FIRSTFRAME'","rb");f.seek(780);print "%.6f"%struct.unpack(">f",f.read(4))')
+
!  QY=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(780);print "%.6f"%struct.unpack(">f",f.read(4))')
 +
   QX=$(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("'$FIRSTFRAME'","rb");f.seek(292);print "%.6f"%struct.unpack(">f",f.read(4))')
+
!  X_RAY_WAVELENGTH=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(292);print "%.6f"%struct.unpack(">f",f.read(4))')
 +
   X_RAY_WAVELENGTH=$(python -c 'import struct; f=open("'$FIRSTFRAME'","rb");f.seek(292);print("%.6f"%struct.unpack(">f",f.read(4)))')
    
elif [ "$DET" == "dtrek" ]; then
 
elif [ "$DET" == "dtrek" ]; then
   echo "Data from a RAXIS or Saturn detector with dTREK format"
+
   echo "Data from a RAXIS or Saturn or Pilatus detector with dTREK format"
    
   sed s/\;// tmp2 > tmp1
 
   sed s/\;// tmp2 > tmp1
Line 511: Line 732:     
   dname=`grep "DETECTOR_NAMES=" tmp2 | sed -e "s/.*=//"`
 
   dname=`grep "DETECTOR_NAMES=" tmp2 | sed -e "s/.*=//"`
 
+
  flip=1
 
   if [ "$dname" == "CCD_" ]; then
 
   if [ "$dname" == "CCD_" ]; then
 
     DETECTOR="SATURN MINIMUM_VALID_PIXEL_VALUE=1"
 
     DETECTOR="SATURN MINIMUM_VALID_PIXEL_VALUE=1"
Line 528: Line 749:  
     echo ""
 
     echo ""
 
   fi
 
   fi
   else # should be RX_
+
   elif [ "$dname" == "PILT_" ]; then
 +
    DETECTOR="PILATUS MINIMUM_VALID_PIXEL_VALUE=0"
 +
    dtrek_det="pilatus"
 +
    SEPMIN=3
 +
    CLUSTER_RADIUS=1.5
 +
    rotation_axis="0 1 0"  # TODO: read from header
 +
    flip=-1
 +
    SENSOR_THICKNESS=0.45  # TODO: read from header
 +
# 2theta
 +
    TWOTHETA=`awk '/PILT_GONIO_VALUES=/{print $2}' tmp2`
 +
    echo TWOTHETA=$TWOTHETA
 +
    R1=`echo "scale=7;  c($TWOTHETA/$DEGTOR)" | bc -l`
 +
    R3=`echo "scale=7; -s($TWOTHETA/$DEGTOR)" | bc -l`
 +
    DIRECTION_OF_DETECTOR_X_AXIS="$R1 0 $R3"
 +
  elif [ "$dname" == "RX_" ]; then
 
     DETECTOR="RAXIS MINIMUM_VALID_PIXEL_VALUE=0"
 
     DETECTOR="RAXIS MINIMUM_VALID_PIXEL_VALUE=0"
 
     dtrek_det="raxis"
 
     dtrek_det="raxis"
 +
  else
 +
    DETECTOR="XXX MINIMUM_VALID_PIXEL_VALUE=XXX"
 +
    dtrek_det="unknown"
 
   fi
 
   fi
   
   # find OVERLOAD
 
   # find OVERLOAD
 
   SATURATED_VALUE=`grep SATURATED_VALUE tmp2 | head -1 | sed s/SATURATED_VALUE=//`
 
   SATURATED_VALUE=`grep SATURATED_VALUE tmp2 | head -1 | sed s/SATURATED_VALUE=//`
Line 562: Line 799:  
   idx=$((i-1))
 
   idx=$((i-1))
 
   if [ "${GONIO_NAMES[$idx]}" == "Distance" ]; then
 
   if [ "${GONIO_NAMES[$idx]}" == "Distance" ]; then
 +
    DETECTOR_DISTANCE="${GONIO_VALUES[$idx]}"
 +
    # TODO: Check unit!! - ${GONIO_UNITS[$idx]}
 +
  fi
 +
  if [ $flip -gt 0 ]; then
 
     DETECTOR_DISTANCE="-${GONIO_VALUES[$idx]}"
 
     DETECTOR_DISTANCE="-${GONIO_VALUES[$idx]}"
 
     # TODO: Check unit!! - ${GONIO_UNITS[$idx]}
 
     # TODO: Check unit!! - ${GONIO_UNITS[$idx]}
 +
    echo "using distance <0"
 
   fi
 
   fi
 
   done
 
   done
Line 576: Line 818:  
  DETECTOR="MAR345  MINIMUM_VALID_PIXEL_VALUE=0  OVERLOAD=130000"
 
  DETECTOR="MAR345  MINIMUM_VALID_PIXEL_VALUE=0  OVERLOAD=130000"
 
  NX=`awk '/FORMAT/{print $2}' tmp2`
 
  NX=`awk '/FORMAT/{print $2}' tmp2`
  NY=$NX
+
# next line is rev 1.02 (previously NY= $NX):
 +
  NY=`awk -v NX=$NX '/FORMAT/{print $4/NX}' tmp2`
 
  QX=`awk '/PIXEL/{print $3/1000.}' tmp2`
 
  QX=`awk '/PIXEL/{print $3/1000.}' tmp2`
 
  QY=`awk '/PIXEL/{print $5/1000.}' tmp2`
 
  QY=`awk '/PIXEL/{print $5/1000.}' tmp2`
Line 591: Line 834:  
  X_RAY_WAVELENGTH=`grep 'WAVELENGTH' tmp2 | awk '{print $2}'`  
 
  X_RAY_WAVELENGTH=`grep 'WAVELENGTH' tmp2 | awk '{print $2}'`  
 
  OSCILLATION_RANGE=`grep 'PHI' tmp2 | awk '{print $5-$3}'`     
 
  OSCILLATION_RANGE=`grep 'PHI' tmp2 | awk '{print $5-$3}'`     
  TRUSTED_REGION="0 0.99"         
+
  TRUSTED_REGION="0 0.99"  
 +
 
 +
elif [ "$DET" == "OLDMAR" ]; then
 +
 
 +
echo  "Data from old type MAR image plate detector"
 +
DETECTOR="MAR  MINIMUM_VALID_PIXEL_VALUE=0  OVERLOAD=130000"
 +
NX=`awk 'NR==2 {print $2}' tmp2`
 +
NY=$NX
 +
QX=`awk 'NR==2 {print $15}' tmp2`
 +
QY=$QX
 +
ORGX=`awk 'NR==2 {print $19}' tmp2`
 +
ORGY=`awk 'NR==2 {print $20}' tmp2`
 +
DETECTOR_DISTANCE=`awk 'NR==2 {print $22}' tmp2`             
 +
X_RAY_WAVELENGTH=`awk 'NR==2 {print $21}' tmp2`
 +
OSCILLATION_RANGE=`awk 'NR==2 {print $24-$23}' tmp2`   
 +
TRUSTED_REGION="0 0.99" 
 +
rotation_axis="0 1 0" 
 +
echo unsure if sign of anomalous signal is correct - please verify or try both hands!
 +
        
 
elif [ "$DET" == "Bruker-cbf" ]; then
 
elif [ "$DET" == "Bruker-cbf" ]; then
 
    
 
    
 
  echo  "Data from a Bruker-cbf detector"
 
  echo  "Data from a Bruker-cbf detector"
# conversion radian / degrees:
  −
DEGTOR=57.2957795
   
# MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT:
 
# MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT:
 
  MNOPIAS=6  
 
  MNOPIAS=6  
Line 622: Line 881:     
  X_RAY_WAVELENGTH=`awk '/diffrn_radiation_wavelength.wavelength/{print $2}' tmp2`  
 
  X_RAY_WAVELENGTH=`awk '/diffrn_radiation_wavelength.wavelength/{print $2}' tmp2`  
  OMEGA=`awk '/OMEGA \? \? \?/{print $5}' tmp2`
+
# fix 16.3.20: instead of print, use printf "%.5f", because bc does not accept e.g. 3.1e-005
  DELTAOMEGA=`awk '/OMEGA \? \? \?/{print $6}' tmp2`
+
  OMEGA=`awk '/OMEGA \? \? \?/{printf "%.5f",$5}' tmp2`
  PHI=`awk '/PHI \? \? \?/{print $5}' tmp2`
+
  DELTAOMEGA=`awk '/OMEGA \? \? \?/{printf "%.5f",$6}' tmp2`
  DELTAPHI=`awk '/PHI \? \? \?/{printf "%5.4f",$6}' tmp2`
+
  PHI=`awk '/PHI \? \? \?/{printf "%.5f",$5}' tmp2`
  KAPPA=`awk '/CHI \? \? \?/{print $5}' tmp2`
+
  DELTAPHI=`awk '/PHI \? \? \?/{printf "%.5f",$6}' tmp2`
echo OMEGA DELTAOMEGA PHI DELTAPHI KAPPA= $OMEGA $DELTAOMEGA $PHI $DELTAPHI $KAPPA
+
  KAPPA=`awk '/CHI \? \? \?/{printf "%.5f",$5}' tmp2`
 +
# echo OMEGA DELTAOMEGA PHI DELTAPHI KAPPA= $OMEGA $DELTAOMEGA $PHI $DELTAPHI $KAPPA
 +
 
 
# test whether the absolute value of deltaphi is > absolute value of deltaomega
 
# test whether the absolute value of deltaphi is > absolute value of deltaomega
 
  if (( $(echo "${DELTAPHI}^2 > ${DELTAOMEGA}^2"|bc -l) )); then
 
  if (( $(echo "${DELTAPHI}^2 > ${DELTAOMEGA}^2"|bc -l) )); then
Line 636: Line 897:  
     rotation_axis="$R1 $R2 $R3"
 
     rotation_axis="$R1 $R2 $R3"
 
     OSCILLATION_RANGE=${DELTAPHI}
 
     OSCILLATION_RANGE=${DELTAPHI}
 +
    STARTING_ANGLE=${PHI}
 
# here we could check if DELTAPHI is <0, and if so, negate it and rotation_axis
 
# here we could check if DELTAPHI is <0, and if so, negate it and rotation_axis
 
  else
 
  else
Line 641: Line 903:  
     rotation_axis="0 -1 0"
 
     rotation_axis="0 -1 0"
 
     OSCILLATION_RANGE=${DELTAOMEGA}
 
     OSCILLATION_RANGE=${DELTAOMEGA}
 +
    STARTING_ANGLE=${OMEGA}
 
# here we could check if DELTAOMEGA is <0, and if so, negate it and rotation_axis
 
# here we could check if DELTAOMEGA is <0, and if so, negate it and rotation_axis
 
  fi
 
  fi
 +
echo STARTING_ANGLE= $STARTING_ANGLE        ! only read by IDXREF               
 +
 
# 2theta
 
# 2theta
 
   TWOTHETA=`awk '/TWOTHETA \? \? \?/{print $5}' tmp2`
 
   TWOTHETA=`awk '/TWOTHETA \? \? \?/{print $5}' tmp2`
Line 657: Line 922:  
echo ORGX= $ORGX ORGY= $ORGY - check these values with adxv !
 
echo ORGX= $ORGX ORGY= $ORGY - check these values with adxv !
 
echo DETECTOR_DISTANCE= $DETECTOR_DISTANCE  ! only read by XYCORR, IDXREF                     
 
echo DETECTOR_DISTANCE= $DETECTOR_DISTANCE  ! only read by XYCORR, IDXREF                     
echo OSCILLATION_RANGE= $OSCILLATION_RANGE  ! only read by IDXREF                
+
echo OSCILLATION_RANGE= $OSCILLATION_RANGE  ! only read by IDXREF  
 
echo X-RAY_WAVELENGTH= $X_RAY_WAVELENGTH    ! only read by IDXREF                   
 
echo X-RAY_WAVELENGTH= $X_RAY_WAVELENGTH    ! only read by IDXREF                   
   Line 668: Line 933:  
$COMMENT_ORGXY
 
$COMMENT_ORGXY
 
DETECTOR_DISTANCE= $DETECTOR_DISTANCE !read by XYCORR, IDXREF. Negative if detector normal points to crystal.               
 
DETECTOR_DISTANCE= $DETECTOR_DISTANCE !read by XYCORR, IDXREF. Negative if detector normal points to crystal.               
OSCILLATION_RANGE= $OSCILLATION_RANGE                  
+
OSCILLATION_RANGE= $OSCILLATION_RANGE  
 +
STARTING_ANGLE= $STARTING_ANGLE               
 
X-RAY_WAVELENGTH= $X_RAY_WAVELENGTH                       
 
X-RAY_WAVELENGTH= $X_RAY_WAVELENGTH                       
 
NAME_TEMPLATE_OF_DATA_FRAMES=$NAME_TEMPLATE_OF_DATA_FRAMES
 
NAME_TEMPLATE_OF_DATA_FRAMES=$NAME_TEMPLATE_OF_DATA_FRAMES
Line 700: Line 966:  
STRONG_PIXEL=4          ! COLSPOT: only use strong reflections (default is 3)
 
STRONG_PIXEL=4          ! COLSPOT: only use strong reflections (default is 3)
 
MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT=$MNOPIAS ! default of 6 is sometimes too high
 
MINIMUM_NUMBER_OF_PIXELS_IN_A_SPOT=$MNOPIAS ! default of 6 is sometimes too high
! close spots/long cell axis: reduce SEPMIN and CLUSTER_RADIUS from their defaults of 6 and 3
+
! close spots/long cell axis: reduce SEPMIN and CLUSTER_RADIUS from their defaults of 7 and 3.5
! SEPMIN=4 CLUSTER_RADIUS=2 ! should be default for Pilatus and other detectors with low PSF
+
SEPMIN=$SEPMIN CLUSTER_RADIUS=$CLUSTER_RADIUS ! 4 and 2 for Pixel Array Detectors
! since XDS 01-MAR-2015, POSITION supersedes DISTANCE. DISTANCE only for compatibility w/ old XDS.
+
! since XDS 01-MAR-2015, POSITION supersedes DISTANCE.
! nowadays headers are usually correct so refine DISTANCE/POSITION in INTEGRATE but not IDXREF
+
! nowadays headers are usually correct so refine POSITION in INTEGRATE but not IDXREF if low to medium resolution
REFINE(IDXREF)=CELL BEAM ORIENTATION AXIS POSITION ! works best with XDS >= BUILT=20170720
+
! however, if the spots from COLSPOT extend to 2A then POSITION could, and if 1.5A POSITION should be refined
REFINE(INTEGRATE)= DISTANCE POSITION BEAM ORIENTATION ! AXIS CELL
+
REFINE(IDXREF)=CELL BEAM ORIENTATION AXIS  ! add POSITION if high resolution, or DETECTOR_DISTANCE inaccurate
! REFINE(CORRECT)=CELL BEAM ORIENTATION AXIS DISTANCE POSITION ! Default is: refine everything
+
REFINE(INTEGRATE)= POSITION BEAM ORIENTATION ! AXIS CELL . If 1.5A or higher it is ok to refine CELL (unless electron diffraction)
 
+
REFINE(CORRECT)= $REFINE_CORRECT
 
! parameters specifically for this detector and beamline:
 
! parameters specifically for this detector and beamline:
 
DETECTOR= $DETECTOR
 
DETECTOR= $DETECTOR
Line 717: Line 983:     
eof
 
eof
 +
 +
if [ "$DET" == "eiger" ] && [ "$is_h5" == 1 ]; then
 +
  if [ "$DLS" == 0 ] ; then
 +
    if [ -e /usr/local/lib64/dectris-neggia.so ]; then
 +
      echo LIB=/usr/local/lib64/dectris-neggia.so >> XDS.INP
 +
      echo LIB= line was written to XDS.INP . For Apple ARM64 processors, you must modify the name.
 +
    else
 +
      echo !LIB=/usr/local/lib64/dectris-neggia.so >> XDS.INP
 +
      echo /usr/local/lib64/dectris-neggia.so was not found - specify location manually!
 +
    fi
 +
  else
 +
    if [ -e /usr/local/lib64/durin-plugin.so ]; then
 +
      echo LIB=/usr/local/lib64/durin-plugin.so >> XDS.INP
 +
      echo LIB= line was written to XDS.INP
 +
    else
 +
      echo !LIB=/usr/local/lib64/durin-plugin.so >> XDS.INP
 +
      echo /usr/local/lib64/durin-plugin.so was not found - specify location manually!
 +
    fi
 +
  fi
 +
fi
 +
 
if [ "$DET" == "raxis" -o "$dtrek_det" == "raxis" ]; then
 
if [ "$DET" == "raxis" -o "$dtrek_det" == "raxis" ]; then
 
  cat >> XDS.INP << eof
 
  cat >> XDS.INP << eof
Line 730: Line 1,017:  
   echo "ROTATION_AXIS= $rotation_axis  ! only read by IDXREF" >> XDS.INP
 
   echo "ROTATION_AXIS= $rotation_axis  ! only read by IDXREF" >> XDS.INP
 
  elif [ "$REVERSE_PHI" == "no" ]; then
 
  elif [ "$REVERSE_PHI" == "no" ]; then
   echo 'ROTATION_AXIS=1 0 0  ! Australian Synchrotron, SERCAT ID-22 (?), APS 19-ID (?), ESRF BM30A, SPring-8, SSRF BL17U need -1 0 0. Diamond ID24 needs 0 -1 0' >> XDS.INP
+
   echo 'ROTATION_AXIS=1 0 0  ! Australian Synchrotron, SERCAT ID-22 (?), APS 19-ID (?), ESRF BM30A, SPring-8, SSRF need -1 0 0. Diamond ID24 needs 0 -1 0' >> XDS.INP
 
  else
 
  else
 
   echo 'ROTATION_AXIS=-1 0 0  ! if this is wrong, please contact author.' >> XDS.INP
 
   echo 'ROTATION_AXIS=-1 0 0  ! if this is wrong, please contact author.' >> XDS.INP
Line 774: Line 1,061:  
elif [ "$DET" == "pilatus" -o "$DET" == "eiger" ]; then
 
elif [ "$DET" == "pilatus" -o "$DET" == "eiger" ]; then
 
cat >> XDS.INP << eof
 
cat >> XDS.INP << eof
SEPMIN=4 CLUSTER_RADIUS=2
   
NUMBER_OF_PROFILE_GRID_POINTS_ALONG_ALPHA/BETA=13 ! Default is 9 - Increasing may improve data  
 
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,  
 
NUMBER_OF_PROFILE_GRID_POINTS_ALONG_GAMMA=13      ! accuracy, particularly if finely-sliced on phi,  
 
!                                                  and does not seem to have any downsides.  
 
!                                                  and does not seem to have any downsides.  
 
eof
 
eof
   if [ $NX == "1475" ]; then
+
   if [ "$NX" == "1028"  -a "$NY" == "1062" ]; then
 +
# Eiger2 1M ; v0.97 numbers from Andreas Förster
 +
    cat >> XDS.INP << eof
 +
UNTRUSTED_RECTANGLE=    0 1029    512  551
 +
eof
 +
  elif [ "$NX" == "1475" ]; then
 
     if ! grep -q Flat_field tmp2 ; then
 
     if ! grep -q Flat_field tmp2 ; then
 
     cat >> XDS.INP << eof
 
     cat >> XDS.INP << eof
Line 812: Line 1,103:  
eof
 
eof
 
     fi
 
     fi
   elif [ $NX == "2463" ]; then
+
   elif [ "$NX" == "2068"  -a "$NY" == "2162" ]; then
 +
# Eiger2 4M ; v0.97 numbers from Andreas Förster
 +
    cat >> XDS.INP << eof
 +
!EXCLUSION OF VERTICAL DEAD AREAS OF THE EIGER2 4M DETECTOR
 +
UNTRUSTED_RECTANGLE= 1028 1041      0 2163
 +
!EXCLUSION OF HORIZONTAL DEAD AREAS OF THE EIGER 4M DETECTOR
 +
UNTRUSTED_RECTANGLE=    0 2069    512  551
 +
UNTRUSTED_RECTANGLE=    0 2069  1062 1101
 +
UNTRUSTED_RECTANGLE=    0 2069  1612 1651
 +
eof
 +
  elif [ "$NX" == "2463" ]; then
 
# Pilatus 6M
 
# Pilatus 6M
 
# FIXME: here we could test if a Flat_field correction was applied like we do for 2M
 
# FIXME: here we could test if a Flat_field correction was applied like we do for 2M
Line 832: Line 1,133:  
UNTRUSTED_RECTANGLE=  0 2464  2315 2333
 
UNTRUSTED_RECTANGLE=  0 2464  2315 2333
 
eof
 
eof
   elif [ $NX == "3110"  -a $NY == "3269" ]; then
+
   elif [ "$NX" == "3110"  -a "$NY" == "3269" ]; then
 
# Eiger 9M
 
# Eiger 9M
 
     cat >> XDS.INP << eof
 
     cat >> XDS.INP << eof
Line 845: Line 1,146:  
UNTRUSTED_RECTANGLE= 0 3110 2717 2757
 
UNTRUSTED_RECTANGLE= 0 3110 2717 2757
 
eof
 
eof
   elif [ $NX == "4150" -a $NY == "4371" ]; then
+
   elif [ "$NX" == "3108"  -a "$NY" == "3262" ]; then
 +
# Eiger2 9M ; v0.97 numbers from Andreas Förster
 +
    cat >> XDS.INP << eof
 +
!EXCLUSION OF VERTICAL DEAD AREAS OF THE EIGER2 9M DETECTOR
 +
UNTRUSTED_RECTANGLE= 1028 1041      0 3262
 +
UNTRUSTED_RECTANGLE= 2068 2081      0 3263
 +
!EXCLUSION OF HORIZONTAL DEAD AREAS OF THE EIGER2 9M DETECTOR
 +
UNTRUSTED_RECTANGLE=    0 3109    512  551
 +
UNTRUSTED_RECTANGLE=    0 3109  1062 1101
 +
UNTRUSTED_RECTANGLE=    0 3109  1612 1651
 +
UNTRUSTED_RECTANGLE=    0 3109  2162 2201
 +
UNTRUSTED_RECTANGLE=    0 3109  2712 2751
 +
eof
 +
  elif [ "$NX" == "4150" -a "$NY" == "4371" ]; then
 
# Eiger 16M
 
# Eiger 16M
 
     cat >> XDS.INP << eof
 
     cat >> XDS.INP << eof
Line 860: Line 1,174:  
  UNTRUSTED_RECTANGLE= 2069 2082      0 4371  
 
  UNTRUSTED_RECTANGLE= 2069 2082      0 4371  
 
  UNTRUSTED_RECTANGLE= 3109 3122      0 4371
 
  UNTRUSTED_RECTANGLE= 3109 3122      0 4371
 +
eof
 +
  elif [ "$NX" == "4148" -a "$NY" == "4362" ]; then
 +
# Eiger2 16M ; v0.97 numbers from Andreas Förster
 +
    cat >> XDS.INP << eof
 +
!EXCLUSION OF HORIZONTAL DEAD AREAS OF THE EIGER2 16M DETECTOR
 +
UNTRUSTED_RECTANGLE= 1028 1041      0 4363
 +
UNTRUSTED_RECTANGLE= 2068 2081      0 4363
 +
UNTRUSTED_RECTANGLE= 3108 3121      0 4363
 +
!EXCLUSION OF VERTICAL DEAD AREAS OF THE EIGER2 16M DETECTOR
 +
UNTRUSTED_RECTANGLE=    0 4149    512  551
 +
UNTRUSTED_RECTANGLE=    0 4149  1062 1101
 +
UNTRUSTED_RECTANGLE=    0 4149  1612 1651
 +
UNTRUSTED_RECTANGLE=    0 4149  2162 2201
 +
UNTRUSTED_RECTANGLE=    0 4149  2712 2751
 +
UNTRUSTED_RECTANGLE=    0 4149  3262 3301
 +
UNTRUSTED_RECTANGLE=    0 4149  3812 3851
 
eof
 
eof
 
   fi
 
   fi
 
fi
 
fi
 
echo XDS.INP is ready for use. The file has only the most important keywords.
 
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 Full documentation, including complete detector templates, at xds.mr.mpg.de .
echo http://www.mpimf-heidelberg.mpg.de/~kabsch/xds . More documentation in XDSwiki
+
echo More documentation in strucbio.biologie.uni-konstanz.de/xdswiki/index.php .
echo After running xds, inspect, using XDS-Viewer, at least the beamstop mask in
+
echo After running xds, inspect at least the agreement of predicted and observed  
echo BKGPIX.cbf, and the agreement of predicted and observed spots in FRAME.cbf!
+
echo spots in FRAME.cbf!
 
rm -f tmp1 tmp2
 
rm -f tmp1 tmp2
# end of generate_XDS.INP
+
 
 
</pre>
 
</pre>
   Line 882: Line 1,212:  
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.
 
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.
   −
On Mac OS X, installation of the "Command Line Tools" (from http://developer.apple.com/downloads; requires Apple ID) is required. These are also part of the (larger, but also free) [http://developer.apple.com/tools/xcode Xcode] package. This package comes with a license that has to be accepted by the user when running a Command Line Tool for the first time.
+
See also [[Generate_XDS.INP#Dependencies]] below, and the [[Installation]] article.
   −
See also the [[Installation]] article.
+
== Copying generate_XDS.INP from XDSwiki webserver ==
 +
On Linux:
 +
wget https://strucbio.biologie.uni-konstanz.de/pub/linux_bin/generate_XDS.INP
 +
chmod a+x generate_XDS.INP
 +
On Mac:
 +
curl -o generate_XDS.INP https://strucbio.biologie.uni-konstanz.de/pub/linux_bin/generate_XDS.INP
 +
chmod a+x generate_XDS.INP
 +
See also [[Installation]].
    
== Obtaining generate_XDS.INP from this webpage ==
 
== Obtaining generate_XDS.INP from this webpage ==
Line 920: Line 1,257:  
The script makes use of many GNU commands, like <code>ls, grep, egrep, awk, cut, cat, echo, wc, bc, head, sed, tail, cp, od, python</code>. Some of them (like <code>od</code> and <code>python</code>) are only used in case of specific detectors (MarCCD and RAXIS, respectively).  
 
The script makes use of many GNU commands, like <code>ls, grep, egrep, awk, cut, cat, echo, wc, bc, head, sed, tail, cp, od, python</code>. Some of them (like <code>od</code> and <code>python</code>) are only used in case of specific detectors (MarCCD and RAXIS, respectively).  
 
The script will only work if all the required commands are available. They reside in either the <code>coreutils</code> RPM, or specific RPMs (<code>gawk, sed, bc, grep, python</code> ...). Please note that to get the <code>strings</code> command on some Linux distributions (e.g. FC23) you need to install the <code>binutils</code> RPM package.
 
The script will only work if all the required commands are available. They reside in either the <code>coreutils</code> RPM, or specific RPMs (<code>gawk, sed, bc, grep, python</code> ...). Please note that to get the <code>strings</code> command on some Linux distributions (e.g. FC23) you need to install the <code>binutils</code> RPM package.
For Eiger data processing, the <code>h5dump</code> program must be installed. This is part of <code>hdf5-tools</code> (Ubuntu) or <code>hdf5</code> (RHEL).
+
For Eiger data processing, the <code>h5dump</code> program must be installed. This is part of <code>hdf5-tools</code> (Ubuntu) or <code>hdf5</code> (RHEL). The .h5 files collected at Diamond Light Source require a very new version of h5dump (namely h5dump 1.10) to extract the OVERLOAD parameter from the .h5 file; this version is available by default in Ubuntu 20.04 and RHEL/CentOS 8.
 +
 
 +
On Mac OS X, installation of the "Command Line Tools" (from http://developer.apple.com/downloads; requires Apple ID) is required (open a terminal and type <code>xcode-select --install</code>). These are also part of the (larger, but also free) [http://developer.apple.com/tools/xcode Xcode] package. This package comes with a license that has to be accepted by the user when running a Command Line Tool (e.g. <code>strings</code>) for the first time.
   −
An easy way to check for missing programs is
+
One way to check for missing programs is
  which ls grep egrep awk cut cat echo wc bc head sed tail cp od python strings h5dump
+
  #!/bin/bash
 +
for i in  ls grep egrep awk cut cat echo wc bc head sed tail cp od python strings h5dump ; do
 +
    if [ ! -x /bin/$i ] && [ ! -x /usr/bin/$i ]; then
 +
      echo $i not found
 +
    fi
 +
done
    
A command that should go a long way in providing all these tools for RedHat-derived distros is (as root)
 
A command that should go a long way in providing all these tools for RedHat-derived distros is (as root)
Line 929: Line 1,273:  
and for Ubuntu this would be (untested!)
 
and for Ubuntu this would be (untested!)
 
  sudo apt-get install coreutils binutils gawk sed bc grep python hdf5-tools
 
  sudo apt-get install coreutils binutils gawk sed bc grep python hdf5-tools
 +
 +
See also [[Installation]].
    
== Limitations ==
 
== Limitations ==
   −
* The script tries to interpret the header of the frames, so is currently limited to Dectris (Pilatus, Eiger), ADSC (Quantum), Rigaku (several types), MAR (CCD and image plate) detectors, and one Bruker detector. Other detectors need some values to be manually filled into XDS.INP - the relevant places are marked with XXX. These are detector properties (type, pixel size and number, min and max counts in a pixel), and experimental parameters like oscillation range, wavelength, distance, and direct beam position (or rather: point of detector that is closest to the crystal). For fine-tuning of detector parameters, see the [http://xds.mpimf-heidelberg.mpg.de/html_doc/xds_prepare.html detector-specific templates].
+
* The script tries to interpret the header of the frames, so is currently limited to Dectris (Pilatus, Eiger), ADSC (Quantum), Rigaku (several types), MAR (CCD and image plate) detectors, and one Bruker detector. Other detectors need some values to be manually filled into XDS.INP - the relevant places are marked with XXX. These are detector properties (type, pixel size and number, min and max counts in a pixel), and experimental parameters like ROTATION_AXIS, OSCILLATION_RANGE, X-RAY_WAVELENGTH, DETECTOR_DISTANCE, and XORG, YORG. For fine-tuning of detector parameters, see the [http://xds.mpimf-heidelberg.mpg.de/html_doc/xds_prepare.html detector-specific templates].
* The authors have made a "best effort" to provide a XDS.INP that results in the correct sign of the anomalous signal. In the case of one detector type (internally called Rigaku SMV) this requires reversal of one detector axis, and a negative DETECTOR_DISTANCE, as is found in some of the [http://xds.mpimf-heidelberg.mpg.de/html_doc/xds_prepare.html detector-specific templates]. '''For an unusual or unknown detector setup, the correct sign of the anomalous signal needs to be established and verified e.g. with a good dataset from a test crystal that has a anomalous signal.''' The authors do not take any responsibility for problems arising from incorrect sign of the anomalous signal, nor - obviously! - for any other mischief arising in or from data processing.
+
* The authors have made a "best effort" to provide a XDS.INP that results in the correct sign of the anomalous signal. In the case of one detector type (internally called Rigaku SMV) this requires reversal of one detector axis, and a negative DETECTOR_DISTANCE, as is found in some of the [http://xds.mpimf-heidelberg.mpg.de/html_doc/xds_prepare.html detector-specific templates]. '''For an unusual or unknown detector setup, the correct sign of the anomalous signal needs to be established and verified e.g. with a good dataset from a test crystal that has an anomalous signal.''' The authors do not take any responsibility for problems arising from incorrect sign of the anomalous signal, nor - obviously! - for any other mischief arising in or from data processing.
* At some beamlines, the ROTATION_AXIS should be -1 0 0 ("backwards") instead of the usual 1 0 0 ("horizontal"), or even 0 1 0 ("vertical") like at one of the PETRA Hamburg BLs. We have only just started the article [[Beamline notes]], and the frame headers do not have this information, so the default chosen by [[generate_XDS.INP]] may be wrong and need manual correction.
+
* At some beamlines, the ROTATION_AXIS should be -1 0 0 ("backwards") instead of the usual 1 0 0 ("horizontal"), or even 0 1 0 ("vertical") like at one of the PETRA Hamburg BLs. The frame headers do not have this information, so the default chosen by [[generate_XDS.INP]] may be wrong and need manual correction. Pls also see the article [[Beamline notes]].
* 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. A beamline that is also known to have reversed X and Y is BM14 (ESRF; Mar CCD, as of April 2014) but the script does not currently implement the reversal.
+
* 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 be found 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 ==
Line 941: Line 1,288:  
* GlobalPhasing's list of beamlines and their settings is at http://www.globalphasing.com/autoproc/wiki/index.cgi?BeamlineSettings .
 
* GlobalPhasing's list of beamlines and their settings is at http://www.globalphasing.com/autoproc/wiki/index.cgi?BeamlineSettings .
 
* [[Beamline notes]] to collect information about specific settings
 
* [[Beamline notes]] to collect information about specific settings
 +
* [[spot2pdb]] for visualizing reciprocal space
2,461

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