Merging: Difference between revisions
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== Merging a set of integration files == | == Merging a set of integration files == | ||
In ''cctbx.xfel'' the per-image scale factors are determined using a ''scaling reference''. This scaling reference is expected to be a previously solved, isomorphous data set. The scale factor is determined by a least-squares fit of the observations to the reference intensities, after applying corrections for polarization<ref>[http://dx.doi.org/10.1107/S0021889882012060 Kahn, R, <i>et al.</i> Macromolecular Crystallography with Synchrotron Radiation: Photographic Data Collection and Polarization Correction. <i>J Appl Cryst</i> <b>15</b>, 330–337 (1982).]</ref>, and a significance filter, which limits the resolution of each diffraction pattern based on the signal-to-noise ratio. Images not conforming to the symmetry of the scaling reference are rejected as outliers, as are images that correlate poorly with the scaling reference and images whose unit cell lies deviates too far from that of the scaling reference. | In ''cctbx.xfel'' the per-image scale factors are determined using a ''scaling reference''. This scaling reference is expected to be a previously solved, isomorphous data set. The scale factor is determined by a least-squares fit of the observations to the reference intensities, after applying corrections for polarization<ref>[http://dx.doi.org/10.1107/S0021889882012060 Kahn, R, <i>et al.</i> Macromolecular Crystallography with Synchrotron Radiation: Photographic Data Collection and Polarization Correction. <i>J Appl Cryst</i> <b>15</b>, 330–337 (1982).]</ref>, and a significance filter, which limits the resolution of each diffraction pattern based on the signal-to-noise ratio. Images not conforming to the symmetry of the scaling reference are rejected as outliers, as are images that correlate poorly with the scaling reference and images whose unit cell lies deviates too far from that of the scaling reference. | ||
''cxi.merge'' may take several passes over the integrated images. In order to speed up processing, ''cxi.merge'' will write the scaled data to a back end database during each pass. Currently three database back ends are implemented. | |||
* <code>FS</code> is the simplest back end. It stores the scaled intensities, their Miller indices, and information about the shots they were observed during in three flat files on the file system. | |||
* The <code>MySQL</code> back end stores data in a MySQL database. The database must be set up beforehand, and credentials to access it must be supplied in the parameters passed to ''cxi.merge''. | |||
* The <code>SQLite</code> back end uses a simple SQLite database, which is written to a single file on the file system. It is easier to use than the <code>MySQL</code> back end and more efficient than the <code>FS</code> backend. Regrettably, the <code>SQLite</code> back end does not appear to work on the Lustre file system. | |||
Compared to indexing and integration, merging is a relatively quick procedure. However, particularly for large datasets, it may significantly strain computational resources. Therefore, it is recommended to merge data on the SLAC's interactive nodes. | Compared to indexing and integration, merging is a relatively quick procedure. However, particularly for large datasets, it may significantly strain computational resources. Therefore, it is recommended to merge data on the SLAC's interactive nodes. | ||
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; backend | ; backend | ||
: Back end database; <code>FS</code> for flat-file ASCII data storage, <code>MySQL</code> and <code>SQLite</code> for the respective proper database back ends. | : Back end database; <code>FS</code> for flat-file ASCII data storage, <code>MySQL</code> and <code>SQLite</code> for the respective proper database back ends. | ||
; d_min | ; d_min | ||
: Limiting resolution for scaling and merging | : Limiting resolution for scaling and merging |
Revision as of 04:14, 4 October 2013
The result of Indexing and integration is a set of Python pickle files, each of which essentially contains a table of Miller indices of the observed reflections, their integrated intensities, and estimated errors. In the general case, these files reflect the measurements from single shots, each exposing different crystals with a unique pulse of X-rays. Merging refers to the procedure applied to unite all these observations into a single data set. During merging, a distinct multiplicative factor, which accounts for the variance in pulse intensity and crystal size, is applied to the observations from a single shot to bring all the observations onto a common scale. The intensities for individual reflections are then summed, and their errors are propagated in quadrature. The result of merging is an mtz file suited for further processing, e.g. molecular replacement.
Merging a set of integration files
In cctbx.xfel the per-image scale factors are determined using a scaling reference. This scaling reference is expected to be a previously solved, isomorphous data set. The scale factor is determined by a least-squares fit of the observations to the reference intensities, after applying corrections for polarization<ref>Kahn, R, et al. Macromolecular Crystallography with Synchrotron Radiation: Photographic Data Collection and Polarization Correction. J Appl Cryst 15, 330–337 (1982).</ref>, and a significance filter, which limits the resolution of each diffraction pattern based on the signal-to-noise ratio. Images not conforming to the symmetry of the scaling reference are rejected as outliers, as are images that correlate poorly with the scaling reference and images whose unit cell lies deviates too far from that of the scaling reference.
cxi.merge may take several passes over the integrated images. In order to speed up processing, cxi.merge will write the scaled data to a back end database during each pass. Currently three database back ends are implemented.
FS
is the simplest back end. It stores the scaled intensities, their Miller indices, and information about the shots they were observed during in three flat files on the file system.
- The
MySQL
back end stores data in a MySQL database. The database must be set up beforehand, and credentials to access it must be supplied in the parameters passed to cxi.merge.
- The
SQLite
back end uses a simple SQLite database, which is written to a single file on the file system. It is easier to use than theMySQL
back end and more efficient than theFS
backend. Regrettably, theSQLite
back end does not appear to work on the Lustre file system.
Compared to indexing and integration, merging is a relatively quick procedure. However, particularly for large datasets, it may significantly strain computational resources. Therefore, it is recommended to merge data on the SLAC's interactive nodes.
$ ssh psanacs.slac.stanford.edu $ cd myrelease
In cctbx.xfel images are merged using the cxi.merge
command.
$ cxi.merge Ls04-lysozyme-merge.phil
Here, Ls04-lysozyme-merge.phil
is a phil-file with the parameters to control the merging procedure. In this tutorial only a subset of the available options are defined.
- backend
- Back end database;
FS
for flat-file ASCII data storage,MySQL
andSQLite
for the respective proper database back ends. - d_min
- Limiting resolution for scaling and merging
- data
- Directory containing integrated data in pickle format. Repeat to specify additional directories.
- merge_anomalous
True
to merge anomalous contributors (i.e. Bijvoet mates),False
to preserve them- min_corr
- Correlation cutoff for rejecting individual frames
- model
- The scaling reference, PDB filename containing atomic coordinates and isomorphous
CRYST1
record - nproc
- Specifies the number of scaling processes cxi.merge may have running at any one time
- output.prefix
- Prefix for all output file names
- rawdata.sdfac_auto
True
to applySDFAC
correction to each image, assuming negative intensities are normally distributed noise- rescale_with_average_cell
- Rescale the images a second time, requiring images to conform to the average unit cell. If set to
True
,set_average_unit_cell
must also be set toTrue
. - set_average_unit_cell
- If
True
set the unit cell of the merged data to the average of the merged images, otherwise use the unit cell of the scaling reference
XXX mention output here, table, rejected images summary
The name of the output file is output.prefix.mtz
.
Calculating the CC1/2 statistic
$ cxi.xmerge
References
<references/>