Gd-Lysozyme

In this tutorial, we assume that we are handed an SFX dataset containing Lysozyme diffraction, but are not told anything else. We will have to go through all the data runs, figure out which one is to be used for dark subtraction, and account for untrusted pixels and detector metrology. At this point, we will be prepared to integrate and merge the data. Finally, we will perform simple molecular replacement and ask whether there is any Gd signal in the anomalous difference Fourier.

Discovery of data collection parameters

Log in to pslogin.slac.stanford.edu, and then to psana. Carry through flags so that X-windows will work

ssh -YAC $USER@pslogin.slac.stanford.edu
ssh -YAC psana

Go in to the working directory and source the package manager:

cd ~/myrelease
sit_setup

Create a subdirectory for the 2014 tutorial files if not already done:

mkdir -p cxi84914

List out the Gd-Lysozyme XTC files (this could take time since there are many images):

ls /reg/d/psdm/cxi/cxi84914/xtc/e239
ls /reg/d/psdm/cxi/cxi84914/xtc/e240

Notice that there are numerous runs in the directory. Now we will create composite averages for each run. Grab this configuration file: mkdark_Gd-Lysozyme.cfg and put it in your cxi84914 directory. For one run only from each experiment directory:

cxi.lsf -c ~/myrelease/cxi84914/mkdark_Gd-Lysozyme.cfg \
-o /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e239/ \
-i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq -s -p 8 -x 239 -r 16 -t 0

cxi.lsf -c ~/myrelease/cxi84914/mkdark_Gd-Lysozyme.cfg \
-o /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e240/ \
-i /reg/d/psdm/cxi/cxi84914/xtc/e240 -q psanacsq -s -p 8 -x 240 -r 16 -t 0

Take note:

• -c configuration file
• -o output directory (will be created)
• -i input files (directory containing the XTC streams)
• -q which batch queue to use
• -s funnel all streams for the run into one node (takes longer, but necessary for averaging)
• -p number of cores to use on the node
• -x which experiment number
• -r which run number
• -t which processing trial (auto increments from 0 if not given)

For all the runs in the Gd-Lysozyme data set 239:

kinit
aklog
for m in 27 28 29 30 31; \
 do echo $m; cxi.lsf -c ~/myrelease/cxi84914/mkdark_Gd-Lysozyme.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e239/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq -s -p 8 -x 239 -r ${m} -t 0; done

For all the runs in the Gd-Lysozyme data set 240:

kinit
aklog
for m in 1 2 3 4 5 6 7 8 9 10 12 13 14 16 17 18 19 21 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40; \
 do echo $m; cxi.lsf -c ~/myrelease/cxi84914/mkdark_Gd-Lysozyme.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e240/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e240 -q psanacsq -s -p 8 -x 240 -r ${m} -t 0; done

bjobs lists all your batch jobs; use this form for more information including other-user load:

bjobs -w -u all -q psanacsq
bkill [number] # stops unwanted job

Some runs take up to 2 hrs wall time to average. Find the averages, view the max-composites, and list out header information for each experiment separately and create a table of the results:

ls /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e239/r*/000/out/*.pickle
cctbx.image_viewer `find /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e239/r*/000 -name "max*.pickle"`
for m in `find /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e239/r*/000 -name "max*.pickle"`; 
 do echo $m; cxi.print_pickle $m; echo; done

Let's make a table of the results for experiment 239:

Run	Distance	Wavelength	Diffraction	Comments
27	81.0	1.456964	weak powder
28	81.0	1.456955	strong powder
29	81.0	1.4569557	strong powder
30	81.0	1.4569529	dark
31	81.0	1.456949	strong powder

The next Gd-Lysozyme experiment:

ls /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e240/r*/000/out/*.pickle
cctbx.image_viewer `find /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e240/r*/000 -name "max*.pickle"`
for m in `find /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e240/r*/000 -name "max*.pickle"`; 
 do echo $m; cxi.print_pickle $m; echo; done

Let's make a table of the results for experiment 240:

Run	Distance	Wavelength	Diffraction	Comments
1	156.0	1.145418	dark
2	101.0	1.454165	strong powder
3	81.0	1.454175	strong powder
4	81.0	1.454175	strong powder
5	81.0	1.454175	strong powder
6	81.0	1.454176	strong powder
7	81.0	1.454176	strong powder
8	97.735	1.453730	dark
9	171.0	1.4569401	weak powder
10	81.0	1.456952	strong powder
12	81.0	1.45695	weak powder
13	81.0	1.45815	dark
14	81.0	1.456952	strong powder
16	81.0	1.45697	strong powder
17	81.0	1.457426	weak powder
18	81.0	1.467101	very weak powder
19	81.0	1.456950	strong powder
21	81.0	1.456949	strong powder
24	81.0	1.456950	very weak powder
25	81.0	1.456958	strong powder
26	81.0	1.4569358	strong powder
27	81.0	1.4569524	strong powder
28	81.0	1.456964	very weak powder
29	81.0	1.4570738	strong powder	saturated spots
30	81.0	1.4569528	strong powder	saturated spots
31	81.0	1.4569488	dark
32	81.0	1.456953	strong powder
33	81.0	1.4569476	strong powder
34	81.0	1.4569505	strong powder
35	81.0	1.456966	strong powder
36	81.0	1.456948	strong powder
37	81.0	1.4573264	strong powder
38	81.0	1.4569576	strong powder
39	81.0	1.4569520	strong powder
40	81.0	1.4569505	strong powder

Some conclusions:

• Run 30 was the dark run for experiment 239. We'll use the average and standard deviation for further processing. Tutorial students can take result from the instructor's directory:

/reg/d/psdm/cxi/cxi84914/scratch/tmmclark/initial_dark/e239/r0030/000/out/avg-r0030.pickle
/reg/d/psdm/cxi/cxi84914/scratch/tmmclark/initial_dark/e239/r0030/000/out/stddev-r0030.pickle

• Runs 1, 8, 13 and 31 were dark runs for experiment 240. We will discard runs 1 and 8 since the detector distances are unique and would require separate detector calibration. Either run 13 or 31 will work so we'll use the average and standard deviation of run 31 for further processing of experiment 240. Tutorial students can take result from the instructor's directory:

/reg/d/psdm/cxi/cxi84914/scratch/tmmclark/initial_dark/e240/r0031/000/out/avg-r0031.pickle
/reg/d/psdm/cxi/cxi84914/scratch/tmmclark/initial_dark/e240/r0031/000/out/stddev-r0031.pickle

• We are interested in getting the Gd anomalous signal from lysozyme, runs were collected at the far remote for f” at approximately 8500 eV or 1.457 Angstroms. See the X-ray Anomalous Scattering.

• We'll accept runs 27-29 and 31 ("calibration27") for experiment 239, and in experiment 240 runs 3-7, 10, 11, 14-19, 23-30 and 32-40 ("calibration3"). We'll also discard run 9 of experiment 240 as the diffraction was relatively weak and the unique detector distance would require separate detector calibration.

Prepare to mask out the untrusted pixels

We'll now calculate dark-subtracted averages for experiment 239.

for m in 27 28 29 31; \
 do echo $m; cxi.lsf -c ~/myrelease/cxi84914/mkavg_e239.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e239/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq -s -p 8 -x 239 -r ${m} -t 0; done

This repeats exactly the same averaging calculations as before, except the dark average from run 30 is subtracted. The dark image to be subtracted (along with its std deviation) is defined in the configuration file mkavg_e239.cfg.

Now we'll figure out which pixels are untrusted, and thus should not be integrated. Three criteria will be used:

• Hot pixels--on the average-dark the pixel values exceed 1150 (should be fine tuned by inspecting the dark & using trial and error)
• Hot pixels--on the standard deviation-dark the stddev exceeds 4 and therefore unreliable (also should be fine tuned by trial and error)
• Cold pixels or shadows--on a maximum-composite data image, inspect values and set a minimum threshold value (we choose 15 here)

For more information on masking parameters see creating a mask image

cxi.make_mask -v --maxproj_min 15 --avg_max 1150 --stddev_max 4 --output mask_base.pickle \
 /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e239/r0030/000/out/avg-r0030.pickle \
 /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e239/r0030/000/out/stddev-r0030.pickle \
 /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e239/r0027/000/out/max-r0027.pickle

Inspect the mask:

cctbx.image_viewer mask_base.pickle show_untrusted=true

Non-bonded pixels are masked and untrusted regions of high and low/negative intensity.

Now We need to repeat the procedure above to calculate dark-subtracted averages for experiment 240.

for m in 3 4 5 6 7 10 12 14 16 17 18 19 21 23 24 25 26 27 28 29 20 32 33 34 35 36 37 38 39 40; \
 do echo $m; cxi.lsf -c ~/myrelease/cxi84914/mkavg_e240.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e240/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e240 -q psanacsq -s -p 8 -x 240 -r ${m} -t 0; done

This repeats exactly the same averaging calculations as before, except the dark average from run 31 is subtracted. The dark image to be subtracted (along with its std deviation) is defined in the configuration file mkavg_e240.cfg.

Now we'll figure out which pixels are untrusted, and thus should not be integrated. Three criteria will be used:

• Hot pixels--on the average-dark the pixel values exceed 1250 (should be fine tuned by inspecting the dark & using trial and error)
• Hot pixels--on the standard deviation-dark the stddev exceeds 4 and therefore unreliable (also should be fine tuned by trial and error)
• Cold pixels or shadows--on a maximum-composite data image, inspect values and set a minimum threshold value (we choose 14 here)

For more information on masking parameters see creating a mask image

cxi.make_mask -v --maxproj_min 14 --avg_max 1250 --stddev_max 4 --output mask_base.pickle \
 /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e240/r0031/000/out/avg-r0031.pickle \
 /reg/d/psdm/cxi/cxi84914/scratch/$USER/initial_dark/e240/r0031/000/out/stddev-r0031.pickle \
 /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e240/r0018/000/out/max-r0018.pickle

Inspect the mask:

cctbx.image_viewer mask_base.pickle show_untrusted=true

Non-bonded pixels are masked and untrusted regions of high and low/negative intensity.

Correct the detector metrology

Accurate data integration requires highly precise knowledge of pixel positions in laboratory space (metrology). Gaining this knowledge is especially difficult due to the segmented nature of the CSPAD detector, which is tiled into 64 application-specific integrated circuits (ASICs). The 64 ASICs are arranged in quadrants that are approximately 4-fold rotationally symmetric, with 8 sensors per quadrant and 2 ASICs per sensor. The sensors are field-serviceable, and may therefore change from Run to Run.

We thus need to determine positions and rotations for all 64 tiles, ideally down to an accuracy on order of 10 microns. As a general overview, cctbx takes the following steps:

• Tile placement in physical space is measured by the beamline operators optically using electron microscopy. This is done at the per-sensor level (2 ASICs per sensor). This is already hard-coded; nothing for the user to do.

• Relative positions of the quadrants are determined coarsely by considering powder rings.

• Sensor positions are refined based on Bragg spot diffraction, allowing for whole-pixel translations in x and y.

• ASIC positions are refined to subpixel accuracy based on Bragg diffraction, allow for sub-pixel translations and rotations.

Quadrant positions

The electron microscopy step above determines only the sensor positions relative to the frames of reference of each quadrant; but not the absolute position of each quadrant in space. At the CXI instrument, the forward detector DS1 has rail-mounted quadrants to allow re-sizing of the central hole. The quadrant placement should be assessed for both the forward and back (DS2) detectors.

For lysozyme we examine one of the strong images (maximum composite). Students may use the instructor's files ($USER=tmmclark). We first determine that our image has a timestamp that identifies it within cctbx as being from run 7 (2013):

cxi.print_pickle /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e239/r0028/000/out/max-r0028.pickle 
 > Detector format version: CXI 7.1
cxi.detector_format_versions
cxi.detector_format_versions "CXI 7.1"
cxi.view /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e239/r0028/000/out/max-r0028.pickle \
 distl.detector_format_version="CXI 7.1" viewer.calibrate_unitcell.d_min=10 \
 viewer.calibrate_unitcell.unitcell=79,79,38,90,90,90 viewer.calibrate_unitcell.spacegroup=P43212

The "Settings" GUI panel shows detector distance as well as the hard-coded quadrant positions corresponding to "CXI 7.1", namely [2, -6, 3, -6, -7, 0, -1, -4]. Tile translations have been zeroed out in the code. The settings can be changed in the panel, or alternately given as a separate command line parameter (distl.quad_translations=2,-6,3,-6,-7,0,-1,-4). The object is to align the powder pattern with the predicted rings (red circles) based on the unit cell parameters. It can be seen that the alignment is not quite perfect.

Since we have well-formed powder rings, we can run the automatic quadrant positioning tool:

cspad.quadrants /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e239/r0028/000/out/max-r0028.pickle \
 distl.detector_format_version="CXI 7.1"
> The NEW QUAD translations are: [2, -6, 4, -6, -6, 1, 0, -4]

Try a few different max-composites from runs 27, 29 and 31:

The NEW QUAD translations are: [2, -6, 4, -6, -9, 2, 0, -4] (poor self correlation value approx. 0.06 weak powder diffraction for this run)

The NEW QUAD translations are: [3, -4, 5, -6, -6, 1, 0, -4]

The NEW QUAD translations are: [2, -6, 4, -6, -6, 1, 0, -4]

These can be pasted on to the command line for graphical review:

cxi.view /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e239/r0028/000/out/max-r0028.pickle \
 distl.detector_format_version="CXI 7.1" viewer.calibrate_unitcell.d_min=10 \
 viewer.calibrate_unitcell.unitcell=79,79,38,90,90,90 viewer.calibrate_unitcell.spacegroup=P43212\
 distl.quad_translations=2, -6, 4, -6, -6, 1, 0, -4

This looks slightly better. From the GUI it also appears that distance=81 fits; meaning that the detz_offset for the configuration file of 571 is ok.

Now we need to check e240:

For lysozyme we examine one of the strong images (maximum composite). Students may use the instructor's files ($USER=nksauter). We first determine that our image has a timestamp that identifies it within cctbx as being from run 7 (2013):

cxi.print_pickle /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e240/r0029/000/out/max-r0029.pickle 
 > Detector format version: CXI 7.1
cxi.detector_format_versions
cxi.detector_format_versions "CXI 7.1"
cxi.view /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e240/r0019/000/out/max-r0029.pickle \
 distl.detector_format_version="CXI 7.1" viewer.calibrate_unitcell.d_min=10 \
 viewer.calibrate_unitcell.unitcell=79,79,38,90,90,90 viewer.calibrate_unitcell.spacegroup=P43212

The "Settings" GUI panel shows detector distance as well as the hard-coded quadrant positions corresponding to "CXI 7.1", namely [2, -6, 3, -6, -7, 0, -1, -4]. Tile translations have been zeroed out in the code. The settings can be changed in the panel, or alternately given as a separate command line parameter (distl.quad_translations=2,-6,3,6,-7,0,-1,-4. The object is to align the powder pattern with the predicted rings (red circles) based on the unit cell parameters. It can be seen that the alignment is not quite perfect.

Since we have well-formed powder rings, we can run the automatic quadrant positioning tool:

cspad.quadrants /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e240/r0029/000/out/max-r0029.pickle \
 distl.detector_format_version="CXI 7.1"
> The NEW QUAD translations are:  [2, -6, 4, -6, -6, 1, 0, -4]

Try a few different max-composites from runs 3, 7, 17, 27:

The NEW QUAD translations are: [2, -5, 4, -6, -6, 1, 0, -3]

The NEW QUAD translations are: [2, -5, 4, -6, -6, 1, 0, -4]

The NEW QUAD translations are: [19, -6, 3, -6, -11, 11, 1, -1] (very poor self-correlation coefficient around 0.06 run 17 is weak powder and not a good run to use for the metrology)

The NEW QUAD translations are: [3, -4, 4, -6, -6, 1, 0, -4]

These can be pasted on to the command line for graphical review:

cxi.view /reg/d/psdm/cxi/cxi84914/scratch/$USER/averages/e240/r0029/000/out/max-r0029.pickle \
 distl.detector_format_version="CXI 7.1" viewer.calibrate_unitcell.d_min=10 \
 viewer.calibrate_unitcell.unitcell=79,79,38,90,90,90 viewer.calibrate_unitcell.spacegroup=P43212\
 distl.quad_translations= 2, -6, 4, -6, -6, 1, 0, -4

This looks slightly better. We will continue in the next section to test the distance and find the best value.

Data Discovery Phase

Before we can move forward with metrology on the pixel and sub pixel level, we must test if the data can be indexed and index a test image. Beginning with e239 we will choose run 27 and run hit finding and dump the images for trial 0. The configuration file Gd-Lysozyme-27_discover.cfg (for configuration run 27) names our phil parameter file Gd-Lysozyme-t000.phil (t000 means trial 0)] for trial 0 we comment out the target cell and setting. Modules that are commented out in the config file can be uncommented for indexing once we discover the correct parameters.

 cxi.lsf -c ~/myrelease/cxi84914/e239/Gd-Lysozyme-27_discover.cfg \
 -o /path to home/myrelease/cxi84914/e239/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq -p 8 -x 239 -r 27 -t 0

Nothing can progress until we successfully index an image. The next steps involve adjusting the configuration file so that we can just look the images and find one that should index. First we make a new configuration file that just does a hit find and a raw image dump and examine images to find one with "good" diffraction. We choose the s00 stream as this will give a thin slice of the entire run and we can examine all images from this run using the command:

 cctbx.image_viewer shot-s00-20130315225*

Looking through these images the best is the third image (shot-s00-20130315225354116.pickle). First we check using this image if spot finder has the correct parameters by using the .phil file parameters in image viewer as follows:

 distl.image_viewer distl.minimum_signal_height=5 distal.minimum_spot_height=10 \
 distal.minimum_spot_area=1 shot-s00-20130315225354116.pickle

The spot_finder is finding the spots correctly so it seems there is another issue. In examine the images it is clear that the water rings are not at the expected resolution of approximately 3.5 angstroms but rather around 1.8 angstroms indicating that the detz_offset is incorrect (way off) and indexing is not going to work until this is fixed.

This brings us to trial 1. The detz_offset is incorrect and we aren't in the ball park so first we will try a detz_offset = 591 which puts the detector at 100 mm away to make the water rings be closer to a 3.5 angstrom resolution. To do this we edit Gd-Lysozyme-27_discover.cfg by uncomment the indexing module (also comment out my_ana_pkg.mod_dump:img_thresh, if you don't want to dump the raw images a second time) and change detz_offset to 591. Then run the following command:

  cxi.lsf -c ~/myrelease/cxi84914/e239/Gd-Lysozyme-27_discover.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/USERNAME/results/e239/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq 
 -p 8 -x 239 -r 27 -t 1

Looking at ~/myrelease/cxi84914/e239/r0027/stdout log file s00.out the unit cell found (86.3581, 86.3581, 42.8606, 90, 90, 90) is not the correct one and many images did not index at all. We need to try to get to a value for detz_offset that is in the correct range. For trial 2 we will use a detz_offset of 581, so the detz_offset in Gd-Lysozyme-27_discover.cfg is changed t0 581 and we run the following command:

  cxi.lsf -c ~/myrelease/cxi84914/e239/Gd-Lysozyme-27_discover.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/USERNAME/results/e239/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq -p 8 -x 239 -r 27 -t 2

Checking the log file the indexed unit cell is (78.1073, 78.1073, 39.1608, 90, 90, 90) which is much closer to what we expect and checking how many indexed images are in r0027/002/out

 ls -l |wc -1

counts all files in current directory and we get 188 indexed images out of a total of 303 total images in our image dump of r0027 for trial 0. Before accepting detz_offset of 581 we will try a series of detz_offset values in the range of 575 - 595. Go to your my release in your home directory and create a new directory called diet_trials; cd into it and run this command to create new configuration files with the test detz_offset values.

 for i in `seq 575 595`; do vi -c "%s/581/$i/g" -c "w Gd-Lysozyme-27_discover0$i.cfg" \
 -c q\! ../cxi84914/e239/Gd-Lysozyme-27_discover0.cfg ; done

Here, a vi command is executed repeatedly that searches for the number 581 in your config file and replaces it with a number from 575 to 595, then writes out the new file with an appropriate file name. If this seems like a poor window to search, note that the number was originally 571, and has already been optimized to 581 through earlier trials.

Next, submit indexing jobs for each candidate detz offset from your myrelease folder:

for i in `seq 575 595`; do cxi.lsf -c dist_trials/Gd-Lysozyme-27_discover0$i.cfg \
-o /reg/d/psdm/cxi/cxi84914/scratch/$USER/dist_trials/ -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -r 27 
-q psanacsq -p 8 -t $i; done

When complete, go to your results directory:

cd /reg/d/psdm/cxi/cxi84914/scratch/$USER/dist_trials/r0027

Then determine which detz offset is best:

for i in `ls`; do echo -n "$i "; ls $i/out | wc -l; done

Output for r0027:

detz_offset:        Indexed images:
575                          80
576                          98
577                          120
578                          153
579                          182
580                          185
581                          187
582                          159
583                          154
584                          142
585                          120
586                          116
587                          103
588                          85
589                          81
590                          68
591                          64
592                          58
593                          60
594                          53
595                          50

The detz_offset of 581 gives the most indexed images. So now we move to the next step in the metrology (unit-pixel tile positions). Testing the detz_offset for e240 for the same range of values yields a detz_offset of 580.

Unit-pixel tile positions

We now know the correct detz_offset (581) and we can change the Gd-Lysozyme-t000.phil file by uncommenting the target unit cell and known setting and change the confif file to only do the indexing and integration with a detz_offset=581. Now we will index the data to derive model lattices. The configuration file Gd-Lysozyme-27.cfg (for configuration run 27) names our phil parameter file Gd-Lysozyme-t003.phil (t003 means trial 3)]. We'll then compare model and observation, from which we can deduce better metrology. This will be done for both experiments 239 and 240 separately.

for m in 27 28 29 31; \
 do echo $m; cxi.lsf -c ~/myrelease/cxi84914/e239/Gd-Lysozyme-27.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/$USER/results/e239/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq -p 8 -x 239 -r ${m} -t 3; done

bkill 0 # stop all jobs; wrong file path

Now for e240 with detz_offset of 580 and a different dark path we need a different config file Gd-Lysozyme-3.cfg (for configuration run 3) the .phil file for the two experiments is the same in this trial 1. I have separated the configuration and phil files for each experiment in ~/myrelease/cxi84914 by creating e239 and e240 directories to place the files.

  for m in 3 4 5 6 7 10 12 14 15 16 17 18 19 21 24 25 26 27 28 29 30 32 33 34 35 36 37 38 39 40; \
  do echo $m; cxi.lsf -c ~/myrelease/cxi84914/e240/Gd-Lysozyme-3.cfg   \
 -o /reg/d/psdm/cxi/cxi84914/scratch/tmmclark/results/e240/ -i /reg/d/psdm/cxi/cxi84914/xtc/e240/ \
 -q psanacsq -p 8 -x 240 -r ${m} -t 1; done

A quick command to count how many integration files there are in e239 and e240:

find /reg/d/psdm/cxi/cxi84914/scratch/$USER/results/e239/*/003/integration -name "int*.pickle"|wc -l
find /reg/d/psdm/cxi/cxi84914/scratch/$USER/results/e240/*/001/integration -name "int*.pickle"|wc -l

We have 6427 and 98808 integrated pickles for e239 and e240 respectively.

Determine whole-pixel translations for all sensors on the CSPAD for e239.

cspad.metrology data=/reg/d/psdm/cxi/cxi84914/scratch/$USER/results/e239/r*/003/integration \
bravais_setting_id=9 max_frames=1000 min_count=25 \
detector_format_version="CXI 7.1" ~/myrelease/cxi84914/e239 \
Gd-Lysozyme-t003.phil | tee Gd-27-t003.unit

Determine whole-pixel translations for all sensors on the CSPAD for e240.

cspad.metrology data=/reg/d/psdm/cxi/cxi84914/scratch/$USER/results/e240/r*/001/integration \
bravais_setting_id=9 max_frames=1000 min_count=25 \
detector_format_version="CXI 7.1" ~/myrelease/cxi84914/e240 \
Gd-Lysozyme-t001.phil | tee Gd-27-t001.unit

List out the new unit translations for e239 and e240:

cat Gd-27-t003.unit |grep -A21 "Unit translations"
cat Gd-3-t001.unit |grep -A21 "Unit translations"

Results from three refinement cycles are listed; capture the last one and incorporate it into a new version of the integration phil file, Gd-Lysozyme-t004.phil.

Repeat this process for both experiments, incrementing the trial numbers and creating a new trial phil file each time until the unit pixel translations have converged and the rmsd is less than 1 unit pixel. Once the final unit pixel metrology for experiments e239 and e240 is complete, we have 6669 and 99073 integrated pickle files.

The next step is to incorporate the sub pixel translations and rotations into a new phil file and integrate each experiment once more.

Add sub-pixel corrections

The rmsd is now on the sub pixel level (less than 0.8 or both e239 and e240). We'll leave the unit-translations exactly where they are now. No sub pixel translations were applied to these data, we move to merging, however for this integration round we'll increase our integration limits to 1.8 Angstroms.

Integrate the data

We're ready for the final integration trial. Again edit the configuration file Gd-Lysozyme-27.cfg and Gd-Lysozyme-3.cfg so that they points to the latest phil file, with the converged unit pixel metrologies using .phil files Gd-Lysozyme-27-t007.phil and Gd-Lysozyme-3-t006.phil We use the trials from each experiment where the most images were integrated (only difference was e239 was indexed at 1.8 Angstrom resolution and e240 was indexed at 1.9 Angstrom resolution). Start with merging these indexed images first.

Submit integration jobs:
for m in 27 28 29 31; \
 do echo $m; cxi.lsf -c ~/myrelease/cxi84914/Gd-Lysozyme-27.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/$USER/results/e239/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e239 -q psanacsq -p 8 -x 239 -r ${m} -t 7; done

 for m in 3 4 5 6 7 10 12 14 16 17 18 19 21 24 25 26 27 28 29 30 32 33 34 35 36 37 38 39 40; \
 do echo $m; cxi.lsf -c ~/myrelease/cxi84914/Gd-Lysozyme-3.cfg \
 -o /reg/d/psdm/cxi/cxi84914/scratch/$USER/results/e240/ \
 -i /reg/d/psdm/cxi/cxi84914/xtc/e240 -q psanacsq -p 8 -x 239 -r ${m} -t 6; done

Merge the data

We will merge the data as a new structure see Advanced Merging Tutorial in particular use case 2 (new structure).

back to psana. Get the command file mergeLysozyme.csh. We are merging all the runs from both experiments.

mkdir /reg/d/psdm/cxi/cxi84914/scratch/$USER/merge
cd /reg/d/psdm/cxi/cxi84914/scratch/$USER/merge
./mergeLysozyme.csh trail#e239 trial#e240

Log file

Solve the structure

Some quick commands to evaluate the data. Here the result *.mtz files must be moved back to your $HOME directory and transferred to your laptop to run PHENIX:

cp /reg/d/psdm/cxi/cxi84914/scratch/$USER/merge/e157/thermoanom_2tli_s0_mark0.mtz $HOME
cp /reg/d/psdm/cxi/cxi84914/scratch/$USER/merge/e157/thermonoanom_2tli_s0_mark0.mtz $HOME

Always use the "s0" files; "s1" and "s2" are the semi-datasets used only to calculate CC1/2.

phenix.fetch_pdb --mtz 2tli
phenix.xtriage thermonoanom_2tli_s0_mark0.mtz scaling.input.xray_data.obs_labels=Iobs > triage_noanom.log

Wilson B factor:14.8

phenix.automr 2tli.pdb thermonoanom_2tli_s0_mark0.mtz seq_file=2tli.fa identity=100 copies=1 build=False

The MR-placed model is in ./AutoMR_run_1_/MR.1.pdb.

Obtain the set of R-free-flags used in the Nature Methods paper

wget http://cci.lbl.gov/publications/download/4ow3_original_iobs_flags.mtz

Refine the model

phenix.refine ./AutoMR_run_1_/MR.1.pdb refinement.output.prefix=001 \
 xray_data.file_name=thermonoanom_2tli_s0_mark0.mtz \
 xray_data.r_free_flags.file_name=4ow3_original_iobs_flags.mtz \
 xray_data.r_free_flags.label=R-free-flags \
 main.number_of_macro_cycles=6 optimize_xyz_weight=True \
 optimize_adp_weight=True nproc=20 refinement.input.xray_data.labels=IMEAN \
 ordered_solvent=true ordered_solvent.mode=every_macro_cycle

trial 003: RWORK = 23.1% RFREE = 26.5% out to 2.1 Angstrom

trial 005: RWORK = 22.0% RFREE = 26.3% out to 2.1 Angstrom (taking untrusted pixels into account)

Run an ersatz script (provided by Nat Echols) to measure the peak heights of the anomalous scatterers.

libtbx.python map_height_at_atoms.py \
 001_001.pdb thermoanom_2tli_s0_mark0.mtz \
 input.xray_data.labels=Iobs \
 xray_data.r_free_flags.file_name=4ow3_original_iobs_flags.mtz \
 xray_data.r_free_flags.label=R-free-flags

Promising results for the Zn and one Ca:

pdb="ZN    ZN A 317 " :   5.97 sigma
pdb="CA    CA A 318 " :   0.93 sigma
pdb="CA    CA A 319 " :   2.74 sigma
pdb="CA    CA A 320 " :   1.08 sigma
pdb="CA    CA A 321 " :   0.20 sigma

Better results from trial 005:

pdb="ZN    ZN A 317 " :   7.66 sigma
pdb="CA    CA A 318 " :   1.10 sigma
pdb="CA    CA A 319 " :   2.52 sigma
pdb="CA    CA A 320 " :   1.40 sigma
pdb="CA    CA A 321 " :   1.01 sigma