library(BiocStyle)
The concept of mutational signatures was introduced in a series of papers by Ludmil Alexandrov et al. (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013) and (Alexandrov, Nik-Zainal, Wedge, Campbell, et al. 2013). A computational framework was published (Alexandrov 2012) with the purpose to detect a limited number of mutational processes which then describe the whole set of SNVs (single nucleotide variants) in a cohort of cancer samples. The general approach (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013) is as follows:
Note that the NMF itself solves the above problem for a given number of signatures \(l\). In order to achieve a reduction in complexity, the number of signatures has to be smaller than the number of features ($l < $n), as indicated in the above figure. The framework of Ludmil Alexandrov et al. (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013) performs not only the NMF decomposition itself, but also identifies the appropriate number of signatures by an iterative procedure.
Another software, the Bioconductor package SomaticSignatures to perform analyses of mutational signatures, is available (Gehring et al. 2015). It allows the matrix decomposition to be performed by NMF and alternatively by PCA (principal component analysis). Both methods have in common that they can be used for discovery, i.e. for the extraction of new signatures. However, they only work well if the analyzed data set has sufficient statistical power, i.e. a sufficient number of samples and sufficient numbers of counts per feature per sample.
The package YAPSA introduced here is complementary to these existing software packages. It is designed for a supervised analysis of mutational signatures, i.e. an analysis with already known signatures \(W\), and with much lower requirements on statistical power of the input data.
In a context where mutational signatures \(W\) are already known (because they were decribed and published as in (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013) or they are available in a database as under http://cancer.sanger.ac.uk/cosmic/signatures), we might want to just find the exposures \(H\) for these known signatures in the mutational catalogue \(V\) of a given cohort. Mathematically, this is a different and potentially simpler task.
The YAPSA-package (Yet Another Package for Signature Analysis) presented
here provides the function LCD
(linear combination decomposition)
to perform this task. The advantage of this method is that there are no
constraints on the cohort size, so LCD
can be run for as little as one
sample and thus be used e.g. for signature analysis in personalized oncology.
In contrast to NMF, LCD
is very fast and requires very little computational
resources. YAPSA has some other unique functionalities, which are briefly
mentioned below and described in detail in separate vignettes.
In the following, we will denote the columns of \(V\) by \(V_{(\cdot j)}\), which
corresponds to the mutational catalogue of sample \(j\). Analogously we denote
the columns of \(H\) by \(H_{(\cdot j)}\), which is the exposure vector of sample
\(j\). Then LCD
is designed to solve the optimization problem:
Remember that \(j\) is the index over samples, \(m\) is the number of samples,
\(i\) is the index over signatures and \(l\) is the number of signatures. LCD
uses a non-negative least squares (NNLS) algorithm (from the R package
nnls ) to solve this optimization problem. Note that the
optimization procedure is carried out for every \(V_{(\cdot j)}\), i.e. for every
column of \(V\) separately. Of course \(W\) is constant, i.e. the same for every
\(V_{(\cdot j)}\).
This procedure is highly sensitive: as soon as a signature has a contribution
or an exposure in at least one sample of a cohort, it will be reported (within
the floating point precision of the operating system). This might blur the
picture and counteracts the initial purpose of complexity reduction. Therefore
there is a function LCD_complex_cutoff
. This function takes as a second
argument a cutoff (a value between zero and one). In the analysis, it will keep
only those signatures which have a cumulative (over the cohort) normalized
exposure greater than this cutoff. In fact it runs the LCD-procedure twice:
once to find initial exposures, summing over the cohort and excluding the ones
with too low a contribution as described just above, and a second time doing
the analysis only with the signatures left over. Beside the exposures \(H\)
corresponding to this reduced set of signatures, the function
LCD_complex_cutoff
also returns the reduced set of signatures itself.
Another R package for the supervised analysis of mutational signatures is
available: deconstructSigs (Rosenthal et al. 2016). One difference
between LCD_complex_cutoff
as described here in YAPSA
and the corresponding
function whichSignatures
in deconstructSigs is that
LCD_complex_cutoff
accepts different cutoffs and signature-specific cutoffs
(accounting for potentially different detectability of different signatures),
whereas in whichSignatures
in deconstructSigs a general fixed
cutoff is set to be 0.06. In the following, we briefly mention other features
of the software package YAPSA and refer to the corresponding vignettes for
detailed descriptions.
One special characteristic of YAPSA is that it provides the opportunity to perform analyses of mutational signtures with signature-specific cutoffs. Different signatures have different detectability. Those with high detectability will occur as false positive calls more often. In order to account for the different detectability, we introduced the concept of signature-specific cutoffs: a signature which leads to many false positive calls has to cross a higher threshold than a signature which rarely leads to false positive calls. While this vignette introduces how to work with signature-specific cutoffs in general, optimal signature-specific cutoffs are presented in 2. Signature-specific cutoffs.
In order to evaluate the confidence of computed exposures to mutational signatures, YAPSA provides 95% confidence intervals (CIs). The computation relies on the concept of profile likelihood (Raue et al. 2009). Details can be found in 3. Confidence Intervals.
For some questions it is useful to assign the SNVs detected in the samples of a cohort to categories. We call an analysis of mutational signatures which takes into account these strata a stratified analysis, which has the potential to reveal enrichment and depletion patterns. Of note, this is different from performing completely separate and independent NNLS analyses of mutational signatures on the different strata. Instead, the results of the unstratified analysis are used as input for a constrained analysis for the strata. Details can be found in 4. Stratified Analysis of Mutational Signatures
Recently a new and extended set of mutational signatures was published by the Pan Cancer Analysis of Whole Genomes (PCAWG) consortium (Alexandrov et al. 2020). In addition to an extended set of SNV mutational signatures, that analysis for the first time had sufficient statistical power to also extract 17 Indel signatures, based on a classification of Indels into 83 categories or features. YAPSA also offers functionality to perform supervised analyses of mutational signatures on these Indel signatures, details can be found in 5. Indel signature analysis
We will now apply some functions of the YAPSA package to Whole Genome Sequencing datasets published in Alexandrov et al. (2013). First we have to load this data and get an overview (first subsection). Then we will load data on published signatures (second subsection). Only in the third subsection we will actually start using the YAPSA functions.
library(YAPSA)
library(knitr)
opts_chunk$set(echo=TRUE)
opts_chunk$set(fig.show='asis')
In the following, we will load and get an overview of the data used in the analysis by Alexandrov et al. (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013)
data("lymphoma_Nature2013_raw")
This creates a dataframe with 128639 rows. It is equivalent to executing the R code
lymphoma_Nature2013_ftp_path <- paste0(
"ftp://ftp.sanger.ac.uk/pub/cancer/AlexandrovEtAl/",
"somatic_mutation_data/Lymphoma B-cell/",
"Lymphoma B-cell_clean_somatic_mutations_",
"for_signature_analysis.txt")
lymphoma_Nature2013_raw_df <- read.csv(file=lymphoma_Nature2013_ftp_path,
header=FALSE,sep="\t")
The format is inspired by the vcf format with one line per called variant. Note that the files provided at that URL have no header information, therefore we have to add some. We will also slightly adapt the data structure:
names(lymphoma_Nature2013_raw_df) <- c("PID","TYPE","CHROM","START",
"STOP","REF","ALT","FLAG")
lymphoma_Nature2013_df <- subset(lymphoma_Nature2013_raw_df,TYPE=="subs",
select=c(CHROM,START,REF,ALT,PID))
names(lymphoma_Nature2013_df)[2] <- "POS"
kable(head(lymphoma_Nature2013_df),
caption = "First rows of the file containing the SNV variant calls.")
CHROM | POS | REF | ALT | PID |
---|---|---|---|---|
1 | 183502381 | G | A | 07-35482 |
18 | 60985506 | T | A | 07-35482 |
18 | 60985748 | G | T | 07-35482 |
18 | 60985799 | T | C | 07-35482 |
2 | 242077457 | A | G | 07-35482 |
6 | 13470412 | C | T | 07-35482 |
Here, we have selected only the variants characterized as subs
(those are the
SNVs we are interested in for the mutational signatures
analysis, small indels are filtered out by this step), so we are left with
128212 variants or rows. Note that there are
48 different samples:
unique(lymphoma_Nature2013_df$PID)
## [1] 07-35482 1060 1061 1065 1093
## [6] 1096 1102 4101316 4105105 4108101
## [11] 4112512 4116738 4119027 4121361 4125240
## [16] 4133511 4135350 4142267 4158726 4159170
## [21] 4163639 4175837 4177856 4182393 4189200
## [26] 4189998 4190495 4193278 4194218 4194891
## [31] 515 DLBCL-PatientA DLBCL-PatientB DLBCL-PatientC DLBCL-PatientD
## [36] DLBCL-PatientE DLBCL-PatientF DLBCL-PatientG DLBCL-PatientH DLBCL-PatientI
## [41] DLBCL-PatientJ DLBCL-PatientK DLBCL-PatientL DLBCL-PatientM EB2
## [46] FL009 FL-PatientA G1
## 48 Levels: 07-35482 1060 1061 1065 1093 1096 1102 4101316 4105105 ... G1
For convenience later on, we annotate subgroup information to every variant (indirectly through the sample it occurs in). For reasons of simplicity, we also restrict the analysis to the Whole Genome Sequencing (WGS) datasets:
lymphoma_Nature2013_df$SUBGROUP <- "unknown"
DLBCL_ind <- grep("^DLBCL.*",lymphoma_Nature2013_df$PID)
lymphoma_Nature2013_df$SUBGROUP[DLBCL_ind] <- "DLBCL_other"
MMML_ind <- grep("^41[0-9]+$",lymphoma_Nature2013_df$PID)
lymphoma_Nature2013_df <- lymphoma_Nature2013_df[MMML_ind,]
data(lymphoma_PID)
for(my_PID in rownames(lymphoma_PID_df)) {
PID_ind <- which(as.character(lymphoma_Nature2013_df$PID)==my_PID)
lymphoma_Nature2013_df$SUBGROUP[PID_ind] <-
lymphoma_PID_df$subgroup[which(rownames(lymphoma_PID_df)==my_PID)]
}
lymphoma_Nature2013_df$SUBGROUP <- factor(lymphoma_Nature2013_df$SUBGROUP)
unique(lymphoma_Nature2013_df$SUBGROUP)
## [1] WGS_D WGS_F WGS_B WGS_I
## Levels: WGS_B WGS_D WGS_F WGS_I
Rainfall plots provide a quick overview of the mutational load of a sample. To this end we have to compute the intermutational distances. But first we still do some reformatting…
lymphoma_Nature2013_df <- translate_to_hg19(lymphoma_Nature2013_df,"CHROM")
lymphoma_Nature2013_df$change <-
attribute_nucleotide_exchanges(lymphoma_Nature2013_df)
lymphoma_Nature2013_df <-
lymphoma_Nature2013_df[order(lymphoma_Nature2013_df$PID,
lymphoma_Nature2013_df$CHROM,
lymphoma_Nature2013_df$POS),]
lymphoma_Nature2013_df <- annotate_intermut_dist_cohort(lymphoma_Nature2013_df,
in_PID.field="PID")
data("exchange_colour_vector")
lymphoma_Nature2013_df$col <-
exchange_colour_vector[lymphoma_Nature2013_df$change]
Now we can select one sample and make the rainfall plot. The plot function used here relies on the package gtrellis by Zuguang Gu (Gu, Eils, and Schlesner 2016).
choice_PID <- "4121361"
PID_df <- subset(lymphoma_Nature2013_df,PID==choice_PID)
#trellis_rainfall_plot(PID_df,in_point_size=unit(0.5,"mm"))
This shows a rainfall plot typical for a lymphoma sample with clusters of increased mutation density e.g. at the immunoglobulin loci.
As stated above, one of the functions in the YAPSA package (LCD
) is
designed to do mutational signatures analysis with known signatures. There are
(at least) two possible sources for signature data: i) the ones published
initially by Alexandrov et al. (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013), and ii) an updated and curated
current set of mutational signatures is maintained by Ludmil Alexandrov at
http://cancer.sanger.ac.uk/cosmic/signatures. The following three subsections
describe how you can load the data from these resources. Alternatively, you can
bypass the three following subsections because the signature datasets are also
included in this package:
data(sigs)
We first load the (older) set of signatures as published in Alexandrov et al. (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013):
Alex_signatures_path <- paste0("ftp://ftp.sanger.ac.uk/pub/cancer/",
"AlexandrovEtAl/signatures.txt")
AlexInitialArtif_sig_df <- read.csv(Alex_signatures_path,header=TRUE,sep="\t")
kable(AlexInitialArtif_sig_df[c(1:9),c(1:4)])
Substitution.Type | Trinucleotide | Somatic.Mutation.Type | Signature.1A |
---|---|---|---|
C>A | ACA | A[C>A]A | 0.0112 |
C>A | ACC | A[C>A]C | 0.0092 |
C>A | ACG | A[C>A]G | 0.0015 |
C>A | ACT | A[C>A]T | 0.0063 |
C>A | CCA | C[C>A]A | 0.0067 |
C>A | CCC | C[C>A]C | 0.0074 |
C>A | CCG | C[C>A]G | 0.0009 |
C>A | CCT | C[C>A]T | 0.0073 |
C>A | GCA | G[C>A]A | 0.0083 |
We will now reformat the dataframe:
Alex_rownames <- paste(AlexInitialArtif_sig_df[,1],
AlexInitialArtif_sig_df[,2],sep=" ")
select_ind <- grep("Signature",names(AlexInitialArtif_sig_df))
AlexInitialArtif_sig_df <- AlexInitialArtif_sig_df[,select_ind]
number_of_Alex_sigs <- dim(AlexInitialArtif_sig_df)[2]
names(AlexInitialArtif_sig_df) <- gsub("Signature\\.","A",
names(AlexInitialArtif_sig_df))
rownames(AlexInitialArtif_sig_df) <- Alex_rownames
kable(AlexInitialArtif_sig_df[c(1:9),c(1:6)],
caption="Exemplary data from the initial Alexandrov signatures.")
A1A | A1B | A2 | A3 | A4 | A5 | |
---|---|---|---|---|---|---|
C>A ACA | 0.0112 | 0.0104 | 0.0105 | 0.0240 | 0.0365 | 0.0149 |
C>A ACC | 0.0092 | 0.0093 | 0.0061 | 0.0197 | 0.0309 | 0.0089 |
C>A ACG | 0.0015 | 0.0016 | 0.0013 | 0.0019 | 0.0183 | 0.0022 |
C>A ACT | 0.0063 | 0.0067 | 0.0037 | 0.0172 | 0.0243 | 0.0092 |
C>A CCA | 0.0067 | 0.0090 | 0.0061 | 0.0194 | 0.0461 | 0.0097 |
C>A CCC | 0.0074 | 0.0047 | 0.0012 | 0.0161 | 0.0614 | 0.0050 |
C>A CCG | 0.0009 | 0.0013 | 0.0006 | 0.0018 | 0.0088 | 0.0028 |
C>A CCT | 0.0073 | 0.0098 | 0.0011 | 0.0157 | 0.0432 | 0.0111 |
C>A GCA | 0.0083 | 0.0169 | 0.0093 | 0.0107 | 0.0376 | 0.0119 |
This results in a dataframe for signatures, containing 27 signatures as column vectors. It is worth noting that in the initial publication, only a subset of these 27 signatures were validated by an orthogonal sequencing technology. So we can filter down:
AlexInitialValid_sig_df <- AlexInitialArtif_sig_df[,grep("^A[0-9]+",
names(AlexInitialArtif_sig_df))]
number_of_Alex_validated_sigs <- dim(AlexInitialValid_sig_df)[2]
We are left with 22 signatures.
An updated and curated set of mutational signatures is maintained by Ludmil Alexandrov at http://cancer.sanger.ac.uk/cosmic/signatures. We will use this set for the following analysis:
Alex_COSMIC_signatures_path <-
paste0("http://cancer.sanger.ac.uk/cancergenome/",
"assets/signatures_probabilities.txt")
AlexCosmicValid_sig_df <- read.csv(Alex_COSMIC_signatures_path,
header=TRUE,sep="\t")
Alex_COSMIC_rownames <- paste(AlexCosmicValid_sig_df[,1],
AlexCosmicValid_sig_df[,2],sep=" ")
COSMIC_select_ind <- grep("Signature",names(AlexCosmicValid_sig_df))
AlexCosmicValid_sig_df <- AlexCosmicValid_sig_df[,COSMIC_select_ind]
number_of_Alex_COSMIC_sigs <- dim(AlexCosmicValid_sig_df)[2]
names(AlexCosmicValid_sig_df) <- gsub("Signature\\.","AC",
names(AlexCosmicValid_sig_df))
rownames(AlexCosmicValid_sig_df) <- Alex_COSMIC_rownames
kable(AlexCosmicValid_sig_df[c(1:9),c(1:6)],
caption="Exemplary data from the updated Alexandrov signatures.")
AC1 | AC2 | AC3 | AC4 | AC5 | AC6 | |
---|---|---|---|---|---|---|
C>A ACA | 0.0110983 | 0.0006827 | 0.0221723 | 0.0365 | 0.0149415 | 0.0017 |
C>A ACC | 0.0091493 | 0.0006191 | 0.0178717 | 0.0309 | 0.0089609 | 0.0028 |
C>A ACG | 0.0014901 | 0.0000993 | 0.0021383 | 0.0183 | 0.0022078 | 0.0005 |
C>A ACT | 0.0062339 | 0.0003239 | 0.0162651 | 0.0243 | 0.0092069 | 0.0019 |
C>G ACA | 0.0018011 | 0.0002635 | 0.0240026 | 0.0097 | 0.0116710 | 0.0013 |
C>G ACC | 0.0025809 | 0.0002699 | 0.0121603 | 0.0054 | 0.0072921 | 0.0012 |
C>G ACG | 0.0005925 | 0.0002192 | 0.0052754 | 0.0031 | 0.0023038 | 0.0000 |
C>G ACT | 0.0029640 | 0.0006110 | 0.0232777 | 0.0054 | 0.0116962 | 0.0018 |
C>T ACA | 0.0295145 | 0.0074416 | 0.0178722 | 0.0120 | 0.0218392 | 0.0312 |
This results in a dataframe containing 30 signatures as column vectors. For reasons of convenience and comparability with the initial signatures, we reorder the features. To this end, we adhere to the convention chosen in the initial publication by Alexandrov et al. (Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013) for the initial signatures.
COSMIC_order_ind <- match(Alex_rownames,Alex_COSMIC_rownames)
AlexCosmicValid_sig_df <- AlexCosmicValid_sig_df[COSMIC_order_ind,]
kable(AlexCosmicValid_sig_df[c(1:9),c(1:6)],
caption=paste0("Exemplary data from the updated Alexandrov ",
"signatures, rows reordered."))
AC1 | AC2 | AC3 | AC4 | AC5 | AC6 | |
---|---|---|---|---|---|---|
C>A ACA | 0.0110983 | 0.0006827 | 0.0221723 | 0.0365 | 0.0149415 | 0.0017 |
C>A ACC | 0.0091493 | 0.0006191 | 0.0178717 | 0.0309 | 0.0089609 | 0.0028 |
C>A ACG | 0.0014901 | 0.0000993 | 0.0021383 | 0.0183 | 0.0022078 | 0.0005 |
C>A ACT | 0.0062339 | 0.0003239 | 0.0162651 | 0.0243 | 0.0092069 | 0.0019 |
C>A CCA | 0.0065959 | 0.0006774 | 0.0187817 | 0.0461 | 0.0096749 | 0.0101 |
C>A CCC | 0.0073424 | 0.0002137 | 0.0157605 | 0.0614 | 0.0049523 | 0.0241 |
C>A CCG | 0.0008928 | 0.0000068 | 0.0019634 | 0.0088 | 0.0028006 | 0.0091 |
C>A CCT | 0.0071866 | 0.0004163 | 0.0147229 | 0.0432 | 0.0110135 | 0.0571 |
C>A GCA | 0.0082326 | 0.0003520 | 0.0096965 | 0.0376 | 0.0118922 | 0.0024 |
Note that the order of the features, i.e. nucleotide exchanges in their trinucleotide content, is changed from the fifth line on as indicated by the row names.
For every set of signatures, the functions in the YAPSA package require an
additional dataframe containing meta information about the signatures. In that
dataframe you can specify the order in which the signatures are going to be
plotted and the colours asserted to the different signatures. In the following
subsection we will set up such a dataframe. However, the respective dataframes
are also stored in the package. If loaded by data(sigs)
the following
code block can be bypassed.
signature_colour_vector <- c("darkgreen","green","pink","goldenrod",
"lightblue","blue","orangered","yellow",
"orange","brown","purple","red",
"darkblue","magenta","maroon","yellowgreen",
"violet","lightgreen","sienna4","deeppink",
"darkorchid","seagreen","grey10","grey30",
"grey50","grey70","grey90")
bio_process_vector <- c("spontaneous deamination","spontaneous deamination",
"APOBEC","BRCA1_2","Smoking","unknown",
"defect DNA MMR","UV light exposure","unknown",
"IG hypermutation","POL E mutations","temozolomide",
"unknown","APOBEC","unknown","unknown","unknown",
"unknown","unknown","unknown","unknown","unknown",
"nonvalidated","nonvalidated","nonvalidated",
"nonvalidated","nonvalidated")
AlexInitialArtif_sigInd_df <- data.frame(sig=colnames(AlexInitialArtif_sig_df))
AlexInitialArtif_sigInd_df$index <- seq_len(dim(AlexInitialArtif_sigInd_df)[1])
AlexInitialArtif_sigInd_df$colour <- signature_colour_vector
AlexInitialArtif_sigInd_df$process <- bio_process_vector
COSMIC_signature_colour_vector <- c("green","pink","goldenrod",
"lightblue","blue","orangered","yellow",
"orange","brown","purple","red",
"darkblue","magenta","maroon",
"yellowgreen","violet","lightgreen",
"sienna4","deeppink","darkorchid",
"seagreen","grey","darkgrey",
"black","yellow4","coral2","chocolate2",
"navyblue","plum","springgreen")
COSMIC_bio_process_vector <- c("spontaneous deamination","APOBEC",
"defect DNA DSB repair hom. recomb.",
"tobacco mutatgens, benzo(a)pyrene",
"unknown",
"defect DNA MMR, found in MSI tumors",
"UV light exposure","unknown","POL eta and SHM",
"altered POL E",
"alkylating agents, temozolomide",
"unknown","APOBEC","unknown",
"defect DNA MMR","unknown","unknown",
"unknown","unknown",
"associated w. small indels at repeats",
"unknown","aristocholic acid","unknown",
"aflatoxin","unknown","defect DNA MMR",
"unknown","unknown","tobacco chewing","unknown")
AlexCosmicValid_sigInd_df <- data.frame(sig=colnames(AlexCosmicValid_sig_df))
AlexCosmicValid_sigInd_df$index <- seq_len(dim(AlexCosmicValid_sigInd_df)[1])
AlexCosmicValid_sigInd_df$colour <- COSMIC_signature_colour_vector
AlexCosmicValid_sigInd_df$process <- COSMIC_bio_process_vector
YAPSA can also perform analyses based on other sets of mutational signatures. Details can be found in additional vignettes on signature-specific cutoffs and Indel signatures.
Now we can start using the functions from the YAPSA package. We will start with
a mutational signatures analysis using known signatures (the ones we loaded in
the above paragraph). For this, we will use the functions LCD
and
LCD_complex_cutoff
.
This section uses functions which are to a large extent wrappers for functions in the package SomaticSignatures by Julian Gehring (Gehring et al. 2015).
library(BSgenome.Hsapiens.UCSC.hg19)
word_length <- 3
lymphomaNature2013_mutCat_list <-
create_mutation_catalogue_from_df(
lymphoma_Nature2013_df,
this_seqnames.field = "CHROM", this_start.field = "POS",
this_end.field = "POS", this_PID.field = "PID",
this_subgroup.field = "SUBGROUP",
this_refGenome = BSgenome.Hsapiens.UCSC.hg19,
this_wordLength = word_length)
The function create_mutation_catalogue_from_df
returns a list object with
several entries. We will use the one called matrix
.
names(lymphomaNature2013_mutCat_list)
## [1] "matrix" "frame"
lymphomaNature2013_mutCat_df <- as.data.frame(
lymphomaNature2013_mutCat_list$matrix)
kable(lymphomaNature2013_mutCat_df[c(1:9),c(5:10)])
4116738 | 4119027 | 4121361 | 4125240 | 4133511 | 4135350 | |
---|---|---|---|---|---|---|
C>A ACA | 127 | 31 | 72 | 34 | 49 | 75 |
C>A ACC | 104 | 36 | 39 | 19 | 36 | 80 |
C>A ACG | 13 | 2 | 2 | 1 | 6 | 8 |
C>A ACT | 102 | 33 | 48 | 22 | 47 | 56 |
C>A CCA | 139 | 43 | 47 | 29 | 51 | 70 |
C>A CCC | 66 | 34 | 35 | 7 | 25 | 42 |
C>A CCG | 9 | 7 | 6 | 3 | 7 | 11 |
C>A CCT | 167 | 47 | 50 | 32 | 58 | 84 |
C>A GCA | 90 | 47 | 66 | 29 | 45 | 66 |
The LCD
function performs the decomposition of a mutational catalogue into a
priori known signatures and the respective exposures to these signatures as
described in the second section of this vignette. We use the signatures from
(Alexandrov, Nik-Zainal, Wedge, Aparicio, et al. 2013) from the COSMIC website
(https://cancer.sanger.ac.uk/cosmic/signatures_v2).
current_sig_df <- AlexCosmicValid_sig_df
current_sigInd_df <- AlexCosmicValid_sigInd_df
lymphomaNature2013_COSMICExposures_df <-
LCD(lymphomaNature2013_mutCat_df,current_sig_df)
Some adaptation (extracting and reformatting the information which sample belongs to which subgroup):
COSMIC_subgroups_df <-
make_subgroups_df(lymphoma_Nature2013_df,
lymphomaNature2013_COSMICExposures_df)
The resulting signature exposures can be plotted using custom plotting functions. First as absolute exposures:
exposures_barplot(
in_exposures_df = lymphomaNature2013_COSMICExposures_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
Here, as no colour information was given to the plotting function
exposures_barplot
, the identified signatures are coloured in a rainbow
palette. If you want to assign colours to the signatures, this is possible via
a data structure of type sigInd_df
.
exposures_barplot(
in_exposures_df = lymphomaNature2013_COSMICExposures_df,
in_signatures_ind_df = current_sigInd_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
This figure has a colour coding which suits our needs, but there is one slight inconsistency: colour codes are assigned to all 30 provided signatures, even though some of them might not have any contributions in this cohort:
rowSums(lymphomaNature2013_COSMICExposures_df)
## AC1 AC2 AC3 AC4 AC5 AC6
## 7600.27742 6876.08962 7532.33628 0.00000 11400.47725 165.58975
## AC7 AC8 AC9 AC10 AC11 AC12
## 1360.82451 10792.42576 40780.45251 750.23999 2330.47206 1416.84002
## AC13 AC14 AC15 AC16 AC17 AC18
## 1278.21673 972.57536 1277.88738 1616.08615 10715.25907 1345.94448
## AC19 AC20 AC21 AC22 AC23 AC24
## 1269.86003 231.99919 909.70554 48.66650 61.22061 0.00000
## AC25 AC26 AC27 AC28 AC29 AC30
## 639.25443 258.02212 382.52388 4768.13630 76.81403 4745.16264
This can be overcome by using LCD_complex_cutoff
. It requires an additional
parameter: in_cutoff_vector
; this is already the more general framework which
will be explained in more detail in the following section.
zero_cutoff_vector <- rep(0,dim(current_sig_df)[2])
CosmicValid_cutoffZero_LCDlist <- LCD_complex_cutoff(
in_mutation_catalogue_df = lymphomaNature2013_mutCat_df,
in_signatures_df = current_sig_df,
in_cutoff_vector = zero_cutoff_vector,
in_sig_ind_df = current_sigInd_df)
We can re-create the subgroup information (even though this is identical to the already determined one):
COSMIC_subgroups_df <-
make_subgroups_df(lymphoma_Nature2013_df,
CosmicValid_cutoffZero_LCDlist$exposures)
And if we plot this, we obtain:
exposures_barplot(
in_exposures_df = CosmicValid_cutoffZero_LCDlist$exposures,
in_signatures_ind_df = CosmicValid_cutoffZero_LCDlist$out_sig_ind_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
Note that this time, only the 28 signatures which actually have a contribution to this cohort are displayed in the legend.
Of course, also relative exposures may be plotted:
exposures_barplot(
in_exposures_df = CosmicValid_cutoffZero_LCDlist$norm_exposures,
in_signatures_ind_df = CosmicValid_cutoffZero_LCDlist$out_sig_ind_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
Now let’s rerun the analysis with a cutoff to discard signatures with insufficient cohort-wide contribution.
my_cutoff <- 0.06
The cutoff of 0.06 means that a signature is kept if it’s exposure
represents at least 6% of all SNVs in the cohort. We will use
the function LCD_complex_cutoff
instead of LCD
.
general_cutoff_vector <- rep(my_cutoff,dim(current_sig_df)[2])
CosmicValid_cutoffGen_LCDlist <- LCD_complex_cutoff(
in_mutation_catalogue_df = lymphomaNature2013_mutCat_df,
in_signatures_df = current_sig_df,
in_cutoff_vector = general_cutoff_vector,
in_sig_ind_df = current_sigInd_df)
At the chosen cutoff of 0.06, we are left with 6 signatures. We can look at these signatures in detail and their attributed biological processes:
kable(CosmicValid_cutoffGen_LCDlist$out_sig_ind_df, row.names=FALSE,
caption=paste0("Signatures with cohort-wide exposures > ",my_cutoff))
sig | index | colour | process |
---|---|---|---|
AC1 | 1 | green | spontaneous deamination |
AC3 | 3 | goldenrod | defect DNA DSB repair hom. recomb. |
AC5 | 5 | blue | unknown |
AC8 | 8 | orange | unknown |
AC9 | 9 | brown | POL eta and SHM |
AC17 | 17 | lightgreen | unknown |
Again we can plot absolute exposures:
exposures_barplot(
in_exposures_df = CosmicValid_cutoffGen_LCDlist$exposures,
in_signatures_ind_df = CosmicValid_cutoffGen_LCDlist$out_sig_ind_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
And relative exposures:
exposures_barplot(
in_exposures_df = CosmicValid_cutoffGen_LCDlist$norm_exposures,
in_signatures_ind_df = CosmicValid_cutoffGen_LCDlist$out_sig_ind_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
When using LCD_complex_cutoff
, we have to supply a vector of cutoffs with as
many entries as there are signatures. In the analysis carried out above, these
were all equal, but this is not a necessary condition. Indeed it may make sense
to provide different cutoffs for different signatures.
specific_cutoff_vector <- general_cutoff_vector
specific_cutoff_vector[c(1,5)] <- 0
specific_cutoff_vector
## [1] 0.00 0.06 0.06 0.06 0.00 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06
## [16] 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06 0.06
In this example, the cutoff for signatures AC1 and AC5 is thus set to 0,
whereas the cutoffs for all other signatures remains at 0.06. Running the
function LCD_complex_cutoff
is completely analogous:
CosmicValid_cutoffSpec_LCDlist <- LCD_complex_cutoff(
in_mutation_catalogue_df = lymphomaNature2013_mutCat_df,
in_signatures_df = current_sig_df,
in_cutoff_vector = specific_cutoff_vector,
in_sig_ind_df = current_sigInd_df)
Plotting absolute exposures for visualization:
exposures_barplot(
in_exposures_df = CosmicValid_cutoffSpec_LCDlist$exposures,
in_signatures_ind_df = CosmicValid_cutoffSpec_LCDlist$out_sig_ind_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
And relative exposures:
exposures_barplot(
in_exposures_df = CosmicValid_cutoffSpec_LCDlist$norm_exposures,
in_signatures_ind_df = CosmicValid_cutoffSpec_LCDlist$out_sig_ind_df,
in_subgroups_df = COSMIC_subgroups_df)
## Warning: `offset` is deprecated, use `location` instead.
Note that the signatures extracted with the signature-specific cutoffs are the same in the example displayed here. Depending on the analyzed cohort and the choice of cutoffs, the extracted signatures may vary considerably. A unique feature of YAPSA is that it also provides optimal signature-specific cutoffs, a topic explained in a separate vignette.
To identify groups of samples which were exposed to similar mutational
processes, the exposure vectors of the samples can be compared. The YAPSA
package provides a custom function for this task: complex_heatmap_exposures
,
which uses the package ComplexHeatmap by Zuguang Gu
(???). It produces output as follows:
complex_heatmap_exposures(CosmicValid_cutoffGen_LCDlist$norm_exposures,
COSMIC_subgroups_df,
CosmicValid_cutoffGen_LCDlist$out_sig_ind_df,
in_data_type="norm exposures",
in_subgroup_colour_column="col",
in_method="manhattan",
in_subgroup_column="subgroup")
## Warning: The input is a data frame, convert it to the matrix.
If you are interested only in the clustering and not in the heatmap
information, you could also use hclust_exposures
:
hclust_list <-
hclust_exposures(CosmicValid_cutoffGen_LCDlist$norm_exposures,
COSMIC_subgroups_df,
in_method="manhattan",
in_subgroup_column="subgroup")
The dendrogram produced by either the function complex_heatmap_exposures
or
the function hclust_exposures
can be cut to yield signature exposures specific
to subgroups of PIDs.
cluster_vector <- cutree(hclust_list$hclust,k=4)
COSMIC_subgroups_df$cluster <- cluster_vector
subgroup_colour_vector <- rainbow(length(unique(COSMIC_subgroups_df$cluster)))
COSMIC_subgroups_df$cluster_col <-
subgroup_colour_vector[factor(COSMIC_subgroups_df$cluster)]
complex_heatmap_exposures(CosmicValid_cutoffGen_LCDlist$norm_exposures,
COSMIC_subgroups_df,
CosmicValid_cutoffGen_LCDlist$out_sig_ind_df,
in_data_type="norm exposures",
in_subgroup_colour_column="cluster_col",
in_method="manhattan",
in_subgroup_column="cluster")
## Warning: The input is a data frame, convert it to the matrix.
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