# Difference between revisions of "XSCALE ISOCLUSTER"

xscale_isocluster (Linux binary)(Mac binary) is a program that clusters datasets stored in a single unmerged reflection file as written by XSCALE. It implements the method of Brehm and Diederichs (2014) and theory of Diederichs (2017).

The help output (obtained by using the -h option) is

xscale_isocluster KD 2019-05-07. -h option shows options
usage: xscale_isocluster -dmin <lowres> -dmax <highres> -nbin <nbin> -mode <1 or 2> -dim <dim> -clu <#> -cen <#,#,#,...> -<aAisw> XSCALE_FILE_NAME
highres, lowres and nbin (default=1 for low, and 10 for high multiplicity) have the usual meanings.
The default of highres and lowres is the COMMON resolution range of all datasets in XSCALE_FILE.
mode can be 1 (equal volumes of resolution shells) or 2 (increasing volumes; default).
dim is number of dimensions (default 3).
clu (by default 1) is number of clusters.
cen (by default automatically) is a set of cluster centers (up to 9) specified by their ISET.
cen must be specified after clu, and the number of values given must match clu.
-a: use anomalous (instead of isomorphous) signal only (unsuitable for partial datasets)
-A: account for anomalous signal by separating I+ and I- (suitable for partial datasets)
-i: write individual pseudo-PDB files to visualize clusters
-s: scale (default 1) for WEIGHT=1/cos(scale*angle) values written to XSCALE.*.INP file(s)
-w: no weighting of intensities with their sigmas
The XSCALE.?.INP output files have angles [deg] w.r.t. cluster centers


## Usage

For data set analysis, the program uses the method of Brehm and Diederichs (2014) Acta Cryst D70, 101-109 (PDF) whose theoretical background is in Diederichs (2017) Acta Cryst D73, 286-293 (open access). This results in segmentation, i.e. an arrangement of the N datasets represented by N vectors in a low-dimensional space. Typically, the dimension of that space may be chosen as n=2 to 4, but may be higher if N is large.

n=1 would only be suitable if the data sets only differ in their random error (i.e. they are highly isomorphous). One more dimension is required for each additional systematic property which may vary between the data sets, e.g. n=2 is suitable if they only differ in their indexing mode (which then only should have two alternatives!), or in some other systematic property, like the length of a cell axis. Higher values of n (e.g. n=4) are appropriate if e.g. there are 4 indexing possibilities (which is the case in P3x), or more systematic ways in which the data sets may differ (like significant variations in the a, b and c axes), or conformational or compositional differences. In cases where data sets differ e.g. with respect to the composition or conformation of crystallized molecules, it is a priori unknown which value of n should be chosen, so several values need to be tried, and the results inspected (see Xscale_isocluster#Notes).

After segmentation of data sets in n-dimensional space, the program may be used (by specifying the -clu <m> option; default m=1) to try and identify <m> clusters of data sets. The program writes files called XSCALE.1.INP with lines required for scaling the datasets of cluster 1, and similarly XSCALE.2.INP for cluster 2, and so on. Typically, one may want to create directories cluster1 cluster2 ..., and then establish symlinks (called XSCALE.INP) in these to the XSCALE.#.INP files. This enables separate scaling of each cluster.

Furthermore, a file iso.pdb is produced that may be loaded into coot. Then use Show/Cell and Symmetry/Show unit cell (to see the origin, which coot marks with "0"), and visualize the relations between data sets. Systematic differences are related to the angle (with the tip of the angle at the origin) between the vectors that represent the data sets; ideally, in the case of isomorphous data sets all vectors point into the same direction. Random differences are related to the lengths of the vectors (starting at the origin; short vectors correspond to weak/noisy data sets). With the -i option, individual iso.x.pdb files can be written for each cluster. For an example, see SSX.

## Output

The console output gives informational and error messages. Each file XSCALE.x.INP enumerates the contributing INPUT_FILEs in the order of increasing angular distance. Example:

UNIT_CELL_CONSTANTS=  91.490  91.490   68.790   90.000   90.000  120.000
SPACE_GROUP_NUMBER= 145
OUTPUT_FILE=XSCALE.1.HKL
FRIEDEL'S_LAW=FALSE
SAVE_CORRECTION_IMAGES=FALSE
WFAC1=1
INPUT_FILE=../x4/XDS_ASCII.HKL
!new, old ISET=      1      3 strength,dist,cluster=     0.855     0.035      1
!INCLUDE_RESOLUTION_RANGE=00 00
INPUT_FILE=../x3/XDS_ASCII.HKL
!new, old ISET=      2      2 strength,dist,cluster=     0.861     0.045      1
!INCLUDE_RESOLUTION_RANGE=00 00
INPUT_FILE=../x9/XDS_ASCII.HKL
!new, old ISET=      3      7 strength,dist,cluster=     0.852     0.112      1
!INCLUDE_RESOLUTION_RANGE=00 00
INPUT_FILE=../x7/XDS_ASCII.HKL
!new, old ISET=      4      6 strength,dist,cluster=     0.902     0.155      1
!INCLUDE_RESOLUTION_RANGE=00 00
INPUT_FILE=../x1/XDS_ASCII.HKL
!new, old ISET=      5      1 strength,dist,cluster=     0.749     0.173      1
!INCLUDE_RESOLUTION_RANGE=00 00
INPUT_FILE=../x5/XDS_ASCII.HKL
!new, old ISET=      6      4 strength,dist,cluster=     0.678     0.223      1
!INCLUDE_RESOLUTION_RANGE=00 00
INPUT_FILE=../x6/XDS_ASCII.HKL
!new, old ISET=      7      5 strength,dist,cluster=     0.788     0.406      1
!INCLUDE_RESOLUTION_RANGE=00 00


Each INPUT_FILE line is followed by a comment line. In this, the first two numbers (new and old) refer to the numbering of datasets in the resulting XSCALE.#.INP, versus that in the original XSCALE.INP (which produced XSCALE_FILE). Then, dist refers to arccosine of the angle (e.g. a value of 1.57 would mean 90 degrees) to the center of the cluster (the lower the better/closer), strength refers to vector length which is inversely proportional to the random noise in a data set, and cluster, if negative, identifies a dataset that is outside the core of the cluster. To select good datasets and reject bad ones, the user may comment out INPUT_FILE lines which refer to datasets that are far away in angle or outside the core of the cluster. Furthermore, resolution ranges may be specified, possibly based on the output of XDSCC12.

## Notes

• For meaningful results, the number of known values [N*(N-1)/2 is the number of pairwise correlation coefficients] should be (preferrably much) higher than the number of unknowns (1+n*(N-1)). This means that one needs at least 5 data sets if dim=2, and at least 7 if dim=3.
• The clustering of data sets in a low-dimensional space uses the method of Rodriguez and Laio (2014) Science 344, 1492-1496. The clustering result should be checked by the user; one should not rely on this to give sensible results! The main criterion for a cluster should be that all data sets in it are in the same or similar direction, when seen from the origin ("0" in coot) - the length of each vector is not important since it is not related to the amount of non-isomorphism, but to the strength of the data set.
• The eigenvalues are printed out by the program, and can be used to deduce the proper value of the required dimension n. To make use of this, one should run with a high value of dim (e.g. 5), and inspect the list of eigenvalues with the goal of finding a significant drop in magnitude (e.g. a factor of 3 drop between the second and third eigenvalue would point to the third eigenvector being of low importance).
• A different but related program is xds_nonisomorphism.