Cctbx.prime: Difference between revisions
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Step-by-step guidelines to post-refine and merge XFEL diffraction images. For more detail and citation, see | Step-by-step guidelines to post-refine and merge XFEL diffraction images. For more detail and citation, see | ||
Enabling X-ray | "Enabling X-ray Free Electron Laser Crystallography for Challenging Biological Systems from a Limited Number of Crystals" | ||
[http://elifesciences.org/content/4/e05421 "DOI: http://dx.doi.org/10.7554/eLife.05421"] | [http://elifesciences.org/content/4/e05421 "DOI: http://dx.doi.org/10.7554/eLife.05421"] | ||
== Step I: Generating input file == | == Step I: Generating input file == |
Revision as of 23:35, 20 May 2015
Prime: post-refinement and merging
Step-by-step guidelines to post-refine and merge XFEL diffraction images. For more detail and citation, see "Enabling X-ray Free Electron Laser Crystallography for Challenging Biological Systems from a Limited Number of Crystals" "DOI: http://dx.doi.org/10.7554/eLife.05421"
Step I: Generating input file
Like most programs developed under cctbx framework, prime reads in input .phil file, which stores all the parameters needed to run post-refinement and merging steps. To generate the template .phil file, do the dry run by calling
$ prime.postrefine
An example of the template .phil file:
data = None run_no = None title = None scale { d_min = 0.1 d_max = 99 sigma_min = 1.5 } ...
You can save the content of the output to any file name - in this tutorial, let's save it to thermolysin.phil.
Step II: Update input parameters
For the first trial, set the required parameters to match with your experiments (you can leave other parameters with their default values - or just delete them from you .phil file). For this tutorial, we use parameters from our thermolysin data set.
data = /path/to/your/integarion/result/pickle_files run_no = 001 title = First trial for thermolysin scale { d_min = 2.1 d_max = 45 sigma_min = 1.5 } postref { scale { d_min = 2.1 d_max = 45 sigma_min = 1.5 partiality_min = 0.1 } crystal_orientation { flag_on = True d_min = 2.1 d_max = 45 sigma_min = 1.5 partiality_min = 0.1 } reflecting_range { flag_on = True d_min = 2.1 d_max = 45 sigma_min = 1.5 partiality_min = 0.1 } unit_cell { flag_on = True d_min = 2.1 d_max = 45 sigma_min = 1.5 partiality_min = 0.1 uc_tolerance = 3 } allparams { flag_on = False d_min = 0.1 d_max = 99 sigma_min = 1.5 partiality_min = 0.1 uc_tolerance = 3 } } merge { d_min = 2.1 d_max = 45 sigma_min = 1.5 partiality_min = 0.1 uc_tolerance = 3 } target_unit_cell = 93.99,93.99,130.87,90,90,120 target_space_group = P 61 2 2 pixel_size_mm = 0.102
Step III: Post-refine and merge
Once you have the input .phil file, you can run prime by calling
prime.postrefine thermolysin.phil
Prime will post-refine and merge for reflection sets using three (default value) macrocycles. At the end of the run, you can obtain merging statistics in the last cycle - all other cycle statistics are also available in log.txt.
An example of merging statistics:
Summary for 001/postref_cycle_1_merge.mtz Bin Resolution Range Completeness <N_obs> |Rsplit CC1/2 N_ind |CCanom N_ind| <I/sigI> <I> ------------------------------------------------------------------------------------------------------------- 02 5.70 - 4.52 100.0 1055 / 1055 65.89 16.02 89.15 1055 0.00 0 20.17 2101.97 03 4.52 - 3.95 100.0 1032 / 1032 61.53 14.48 92.03 1032 0.00 0 20.39 2529.90 04 3.95 - 3.59 100.0 1016 / 1016 54.15 15.61 90.13 1016 0.00 0 16.69 1971.43 05 3.59 - 3.33 100.0 1004 / 1004 42.67 17.66 89.23 1004 0.00 0 14.21 1502.14 06 3.33 - 3.14 100.0 1013 / 1013 32.77 20.40 84.26 1013 0.00 0 11.76 1077.60 07 3.14 - 2.98 100.0 995 / 995 27.36 23.00 78.72 995 0.00 0 11.58 935.37 08 2.98 - 2.85 100.0 1006 / 1006 23.57 22.63 82.26 1006 0.00 0 10.56 722.62 09 2.85 - 2.74 100.0 986 / 986 16.64 28.51 72.90 985 0.00 0 10.01 591.56 10 2.74 - 2.65 99.9 989 / 990 12.41 31.35 72.95 987 0.00 0 9.91 515.07 11 2.65 - 2.56 99.7 979 / 982 9.35 37.14 65.31 970 0.00 0 9.31 438.96 12 2.56 - 2.49 98.0 979 / 999 6.06 45.98 45.37 930 0.00 0 9.45 390.05 13 2.49 - 2.42 95.1 931 / 979 4.46 50.68 34.20 834 0.00 0 8.93 334.80 14 2.42 - 2.37 91.7 896 / 977 3.35 55.66 37.15 729 0.00 0 9.27 320.17 15 2.37 - 2.31 83.9 829 / 988 2.61 56.92 43.21 600 0.00 0 9.60 296.67 16 2.31 - 2.26 72.4 702 / 969 1.97 65.81 26.89 386 0.00 0 10.29 284.39 17 2.26 - 2.22 59.1 582 / 985 1.75 64.72 31.28 275 0.00 0 9.87 284.06 18 2.22 - 2.18 52.9 513 / 970 1.51 71.27 16.86 188 0.00 0 8.93 215.31 19 2.18 - 2.14 35.7 349 / 978 1.32 62.26 68.25 90 0.00 0 8.22 199.09 20 2.14 - 2.10 23.1 227 / 981 1.20 92.14 -9.20 42 0.00 0 8.59 224.44 ------------------------------------------------------------------------------------------------------------- TOTAL 85.9 17224 / 20046 27.11 21.11 92.07 15305 0.00 0 12.87 999.53 ------------------------------------------------------------------------------------------------------------- Summary of refinement and merging No. good frames: 1809 No. bad cc frames: 153 No. bad G frames) : 0 No. bad unit cell frames: 5 No. bad gamma_e frames: 0 No. bad SE: 0 No. observations: 466997
Advance settings
Now that you have your first trial merged data set, you can explore different parameter settings to merge or to obtain the Bijvoet pairs (I+/I-) for your anomalous data set.
Anomalous data:
target_anomalous_flag = True
In the last cycle, prime will output a reflection set with I+ and I-.
Indexing ambiguity
For space groups with indexing ambiguity, use the solutions from cctbx.xfel (see Tutorial for resolving indexing ambiguity) to merge the data set.
indexing_ambiguity { flag_on = True index_basis_in = /path/to/solution/pickle_file.pickle }
Number of micro- and macrocycles
n_postref_cycle = 3 n_postref_sub_cycle = 3
Number of bins for merging statistics
n_bins = 20
Help for input parameters
Most input parameters are self-explained. However, you can run -h switch to view help information for each parameter.
prime.postrefine -h