Contents

1 Introduction

The vignette 1. Usage of YAPSA describes the general usage of YAPSA as a tool to perform supervised analyses of mutational signatures. Calling of mutational signature in YAPSA is performed with a Non-Negative Least Square (NNLS) algorithm implemented in the function linear combination decomposition (LCD) function based on the function lsei from the package lsei (Wang, Lawson, and Hanson 2015). The function LCD can take signature-specific cutoffs as optional arguments. When choosing optimal cutoffs, this can lead to an increase in sensitivity and specificity as compared to NNLS alone. In such a context, LCD then determines the exposure, i.e., the contribution of signature to the mutational load of a samples, in a three-step computational process:

  1. Find an NNLS solution with all supplied signatures using LCD
  2. Identify those signatures which have a contribution higher than a signature-specific cutoff
  3. Rerun NNLS based on the selected subset of signatures

Mutational signatures as provided by https://cancer.sanger.ac.uk/cosmic/signatures have been extracted by Non-negative Matrix Factorization (NMF). Due to the constraint of non-negativity, these signatures cannot be orthogonal. However, orthogonality is a prerequisite or at least beneficial for least squares algorithms. This lack of orthogonality leads to potential overlapping of the signature in a deconvolution.

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. For YAPSA, we have computed optimal signature cutoffs by a modfied Reciever Operating Characteristic (ROC) analysis on the same data as it had been used for the initial NMF analyses with the extraction of the published mutational signatures ((Alexandrov et al. 2013) and (Alexandrov et al. 2020)). Numeric values for these cutoffs are stored in dataframes accessible after loading the package YAPSA.

In the implementation of the package ROCR (Sing et al. 2005), a modified ROC analysis is parametrized by defining cost terms for punishing false-negative (\(cost_{FN}\)) and false-positive (\(cost_{FP}\)) findings separately. In the following, we will call the ratio between the cost for a false-negative finding divided by the cost for a false positive finding the \(cost_{factor}\) (\(cost_{factor} = cost_{FN}/cost_{FP}\)). Separate ROC analyses were performed for every signature. For every signature, the global minimum of the cost function defines the optimal value for the signature-specific cutoff. However, the shape of the cost function and hence the position of its minimum depend on \(cost_{factor}\). Therefore there is one set of optimal signature-specific cutoffs per chosen value of \(cost_{factor}\) (cf. below).

After having computed the optimal signature-specific cutoffs for a range of values for \(cost_{factor}\), we applied an additional criterion in order to get an optimal value for \(cost_{factor}\): minimization of the overall number of false attributions. Using this criterion, for the Alexandrov COSMIC signatures (AC1 - AC30), the optimal value for \(cost_{factor}\) was determined to be \(6\).

2 Overview of the data

2.1 Signatures

In YAPSA, the patterns of nucleotide exchanges in their triplet context constituting the mutational signatures are stored in data frames which can be loaded as follows (more information provided by the help function, cf.  (1. Usage of YAPSA) for an overview of how these data frames can be re-created from data available online):

data(sigs)
data(sigs_pcawg)

The first command, data(sigs), loads eight dataframes into the workspace. Among these, four contain the patterns of nucleotide exchanges in their triplet context, i.e., the mutational signatures themselves, and the remaining four dataframes contain additional information on the signatures, including a naming and numbering convention, a description of the asserted underlying mutational process and a choice of generic colour coding. In particular, these eight signature dataframes are:

  • Two signature and two additonal information dataframes containing SNV Alexandrov COSMIC signatures (available at https://cancer.sanger.ac.uk/cosmic/signatures_v2, downloaded on January 15th, 2016):
    • AlexCosmicArtif_sig_df and AlexCosmicArtif_sigInd_df,
    • AlexCosmicValid_sig_df and AlexCosmicValid_sigInd_df
  • Two signature and two additonal information dataframes containing SNV Alexadrov Initial signatures (the signatures presented in the initial publication (Alexandrov et al. 2013)):
    • AlexInitialArtif_sig_df and AlexInitialArtif_sigInd_df,
    • AlexInitialValid_sig_df and AlexInitialValid_sigInd_df

Of note, all data provided in YAPSA follows a consistent naming convention:

  • Names containing Valid or Real refer to those subsets of signatures which have been identified by NMF in the respective discovery analyses and validated using orthogonal sequencing technologies.
  • Names containing Artif refer to extended sets of signatures including also those signatures which have later been ascribed to be artifact signatures (reflecting, among others, sequencing errors).

The second command in the above code block, data(sigs_pcawg), loads six additional dataframes into the workspace, three dataframes containing mutational signatures themselves and three dataframes containing additional information on the signatures. In particular, these six dataframes are:

  • Two signature and two additional information dataframes containing SNV Alexandrov PCAWG signatures (available at https://cancer.sanger.ac.uk/cosmic/signatures_v3, downloaded on August 16th, 2018):
    • PCAWG_SP_SBS_sigs_Artif_df and PCAWG_SP_SBS_sigInd_Artif_df,
    • PCAWG_SP_SBS_sigs_Real_df and PCAWG_SP_SBS_sigInd_Real_df
  • One signature and one additional information dataframe containing Indel Alexandrov PCAWG signatures (also available at https://cancer.sanger.ac.uk/cosmic/signatures_v3, downloaded on August 16th, 2018):
    • PCAWG_SP_ID_sigs_df and PCAWG_SP_ID_sigInd_df

As of december 2019 and to our knowledge, it is a unique feature of YAPSA to include PCAWG mutational signatures. Of note, a separate vignette describes the usage of and analysis with Indel signatures.

2.2 Optimal cutoffs

For each of the signature dataframes, corresponding dataframes storing numerical values of the signature-specific cutoffs are available. The cutoff dataframes can be loaded to the workspace analogously to the signatures themselves:

data(cutoffs)
data(cutoffs_pcawg)

The command data(cutoffs) loads cutoff dataframes corresponding to the four Alexandrov COSMIC and Alexandrov initial sets of signatures. In the following, an additional naming convention is introduced:

  • Absolute (abs) signature-specific cutoffs were computed using an ROC analysis performed on absolute exposures as provided by the initial NMF analysis
  • Relative (rel) signature-specific cutoffs were computed using on ROC analysis performed on relative, i.e., normalized exposures as provided by the initial NMF analysis.

This double training has proven to be both useful and necessary in order to account for the heterogeneity of the underlying training data: on one hand, a training with absolute exposures weighs all mutations equally, however a whole genome sequenced (WGS) sample gets a much higher weight due to the high number of mutations detected in it than a whole exome sequenced (WES sample). On the other hand, a training with relative or normalized signature exposures weighs all samples equally, but at the cost of having different weights for mutations originating from samples of different mutation count. Based on these considerations, cutoffs derived from the training with absolute exposures should be used for the supervised analysis of WGS data, whereas cutoffs trained on relative exposures are better suited for the analysis of WES data. The two different sets of cutoffs thus account for the different maximal feature occurrence between WGS and WES data. The correspondence between signatures and cutoffs is as follows:

  • For AlexCosmicValid_sig_df, the corresponding cutoff dataframes are cutoffCOSMICValid_abs_df and cutoffCOSMICValid_rel_df.
  • For AlexCosmicArtif_sig_df, the corresponding cutoff dataframes are cutoffCOSMICArtif_abs_df and cutoffCOSMICArtif_rel_df.

With data(cutoffs_pcawg) the signature-specific cutoff dataframes for the PCAWG signatures are loaded. In this case, only one dataframe with cutoffs per signature dataframe is available. Signature-specific cutoffs are valid for WGS and WES data analysis as differences in the feature occurrence is taken into account during the training procedure.

In the provided dataframes with numerical values for optimal signature-specific cutoffs, the columns correspond to the different signatures of the chosen signature set, whereas the rows encode different values of \(cost_{factor}\) (cf. introduction). For an actual analysis of mutational signatures, only one optimal cutoff value per signature is required, i.e., the user has to choose one row from the chosen cutoff dataframe. As already explained above, optimal values for \(cost_{factor}\) have also been determined. These are listed in the table below. Unless a user has a specific wish to use a different \(cost_{factor}\), it is generally recommended to use these default parameter choices.

(#tab:Table:) Overview of signature specific cutoffs and the cost factor to obtain the optimal cutoffs.
cutoff dataframe optimal cost factor
cutoffInitialValid_abs_df 6
cutoffInitialValid_rel_df 6
cutoffInitialArtif_abs_df 6
cutoffInitialArtif_rel_df 6
cutoffCosmicValid_abs_df 6
cutoffCosmicValid_rel_df 6
cutoffCosmicArtif_abs_df 6
cutoffCosmicArtif_rel_df 6
cutoffPCAWG_SBS_WGSWES_realPid_df 10
cutoffPCAWG_SBS_WGSWES_artiflPid_df 16
cutoffPCAWG_ID_WGS_Pid_df 3

Thus, if a user wants to do an analysis with the Alexandrov COSMIC signatures, discarding the artifact signatures, on WGS data, he/she would use the following code snippet:

data(cutoffs)
current_cutoff_vector <- cutoffCosmicValid_abs_df[6, ]
current_cutoff_vector
##   AC1        AC2        AC3        AC4 AC5         AC6        AC7      AC8
## 6   0 0.01045942 0.08194056 0.01753969   0 0.001548535 0.04013304 0.242755
##         AC9       AC10       AC11      AC12        AC13      AC14       AC15
## 6 0.1151714 0.01008376 0.09924884 0.2106201 0.007876626 0.1443059 0.03796027
##        AC16        AC17      AC18      AC19      AC20      AC21       AC22
## 6 0.3674349 0.002647962 0.3325386 0.1156454 0.1235028 0.1640255 0.03102216
##         AC23       AC24       AC25       AC26        AC27       AC28       AC29
## 6 0.03338659 0.03240176 0.01611908 0.09335221 0.009320062 0.05616434 0.05936213
##         AC30
## 6 0.05915355

3 Application example

The vignette 1. Usage of YAPSA shows how to obtain a mutational catalog (\(V\)) from a vcf file. Here, for the sake of simplicits, we just use an example data set stored in the software package.

data(lymphomaNature2013_mutCat_df)

The mutational catalog \(V\) together with the signatures \(V\) and the corresponding signature-specific cutoffs can be used to determine the signature exposures (corresponding to the matrix \(H\) in the naming convention influenced by NMF) per sample or cohort. This is done by the function LCD_complex_cutoff_combined.

In the examples provided in 1. Usage of YAPSA, signature exposures were determined (i) with a zero cutoff vector, i.e. without signature-specific cutoffs or (ii) with a manually chosen but not necessarily optimal cutoff. In contrast, in the following, we will perform an analysis of mutational signatures using optimal cutoffs and compare the results to an analysis without any cutoffs.

current_sig_df <- AlexCosmicValid_sig_df
current_sigInd_df <- AlexCosmicValid_sigInd_df

3.1 Comparison: analysis without any cutoffs

For the purpose of comparison, we first create a zero cutoff vector:

current_cutoff_vector <- rep(0, dim(AlexCosmicValid_sig_df)[2])

Next, we compute the exposures to the mutational signatures using LCD analysis and this zero cutoff vector:

lymphoma_COSMIC_zero_listsList <-
  LCD_complex_cutoff_combined(
    in_mutation_catalogue_df = lymphomaNature2013_mutCat_df,
    in_cutoff_vector = current_cutoff_vector, 
    in_signatures_df = current_sig_df, 
    in_sig_ind_df = current_sigInd_df)

The function returns an object with the results per cohort, per PID and the consensus between both analyses.

Annotation of a subgroup to each PID allows to group the samples per subgroup upon visualization:

data(lymphoma_PID)
colnames(lymphoma_PID_df) <- "SUBGROUP"
lymphoma_PID_df$PID <- rownames(lymphoma_PID_df)
COSMIC_subgroups_df <- 
  make_subgroups_df(lymphoma_PID_df,
                    lymphoma_COSMIC_zero_listsList$cohort$exposures)

We select the cohort-wide analysis for visualization and make use of the custom plotting function exposures_barplot() in order to display signature exposures as stacked barplots. Note the occurrence of multiple signatures with partially very low exposures.

result_cohort <- lymphoma_COSMIC_zero_listsList$cohort
exposures_barplot(
  in_exposures_df = result_cohort$exposures,
  in_signatures_ind_df = result_cohort$out_sig_ind_df,
  in_subgroups_df = COSMIC_subgroups_df)
Absoute exposures of the COSMIC signatures in the lymphoma mutational catalogs, signature-specific cutoffs with a cost factor of 6 used for the LCD

Figure 1: Absoute exposures of the COSMIC signatures in the lymphoma mutational
catalogs, signature-specific cutoffs with a cost factor of 6 used for the LCD

3.2 Making use of optimal signature-specific cutoffs

The zero-cutoff vector will now be replaced by the signature-specific cutoff vector. After the initial LCD analysis only signatures that contribute higher then their signature specific cutoff value will be considered, leading to a reduction of the overall number of detected signatures.

Based on ?? we know that for the validated COSMIC Signatures the optimal cutoffs are the once computed with a cost factor of six.

current_cutoff_df <- cutoffCosmicValid_abs_df
current_cost_factor <- 6
current_cutoff_vector <- current_cutoff_df[current_cost_factor,]

We again compute signature exposures, but this time using the vector of optimal signature-specific cutoffs:

lymphoma_COSMIC_listsList <-
  LCD_complex_cutoff_combined(
      in_mutation_catalogue_df = lymphomaNature2013_mutCat_df,
      in_cutoff_vector = current_cutoff_vector, 
      in_signatures_df = current_sig_df, 
      in_sig_ind_df = current_sigInd_df)

And again proceeding to a visualization (of note, the sample subgrouping information can be used as in the previous subsection):

result_cohort <- lymphoma_COSMIC_listsList$cohort
exposures_barplot(
  in_exposures_df = result_cohort$exposures,
  in_signatures_ind_df = result_cohort$out_sig_ind_df,
  in_subgroups_df = COSMIC_subgroups_df)
Absolute exposures of the COSMIC signatures in the lymphoma mutational catalogs, signature-specific cutoffs with a cost factor of 6 used for the LCD

Figure 2: Absolute exposures of the COSMIC signatures in the lymphoma mutational
catalogs, signature-specific cutoffs with a cost factor of 6 used for the LCD

We note that the number of identified signatures is smaller. Those signatures which had been identified in the analysis without any cutoffs but not in the analysis with optimal cutoffs can be considered false positive calls.

Reference

Alexandrov, LB, J Kim, NJ Haradhvala, MN Huang, AW Ng, A Boot, KR Covington, et al. 2020. “The Repertoire of Mutational Signatures in Human Cancer.” Nature.
Alexandrov, LB, S Nik-Zainal, DC Wedge, SA Aparicio, S Behjati, AV Biankin, GR Bignell, et al. 2013. “Signatures of Mutational Processes in Cancer.” Nature. Nature Publishing Group.
Sing, Tobias, Oliver Sander, Niko Beerenwinkel, and Thomas Lengauer. 2005. “ROCR: Visualizing Classifier Performance in R.” Bioinfomatics.
Wang, Yong, Charles L. Lawson, and Richard J Hanson. 2015. “Lsei: Solving Least Squares Problems Under Equality/Inequality Constraints.” R-Package Version 1.1-1.