Abstract
Variation in the enzymatic activity of pharmacogenes is defined by star alleles (haplotypes) comprised of single‐nucleotide variants, small insertion‐deletions, and large structural variants. We recently developed Stargazer, a next‐generation sequencing‐based tool to call star alleles for the clinically important CYP2D6 gene. Here, we present the utility of extending Stargazer to call star alleles for 28 pharmacogenes using whole genome sequencing (WGS) data. We applied Stargazer to WGS data from 70 ethnically diverse samples from the Genetic Testing Reference Materials Coordination Program (GeT‐RM). These reference samples were extensively characterized by GeT‐RM using multiple pharmacogenetic testing assays. In all 28 genes, Stargazer recalled 100% of star alleles (N = 92) present in GeT‐RM's consensus genotypes (N = 1,559). Stargazer also detected star alleles not previously reported by GeT‐RM, including complex structural variants. Our results demonstrate that combining WGS data and Stargazer enables automated, accurate, and comprehensive genotyping of pharmacogenes in the human genome.
Study Highlights.
WHAT IS THE CURRENT KNOWLEDGE ON THE TOPIC?
☑ As the cost of next‐generation sequencing continues to decrease and as the clinical value of whole genome (or targeted panel) sequencing expands, there is an increasing demand for tools to automatically and accurately genotype pharmacogenes from sequence data.
WHAT QUESTION DID THIS STUDY ADDRESS?
☑ Our study compares conventionally obtained genotypes from Genetic Testing Reference Materials Coordination Program with those obtained by interpreting whole genome sequence (WGS) data using an expanded bioinformatics tool known as Stargazer. We also show the utility of WGS and Stargazer to identify additional genetic variants not identified by existing assays.
WHAT DOES THIS STUDY ADD TO OUR KNOWLEDGE?
☑ This study shows that WGS data coupled with Stargazer can provide not only accurate but also a comprehensive platform for pharmacogenetic testing compared with multiple standard approaches.
HOW MIGHT THIS CHANGE CLINICAL PHARMACOLOGY OR TRANSLATIONAL SCIENCE?
☑ By allowing automated, accurate, and comprehensive genotyping of pharmacogenes, the combination between whole genome (or targeted) sequencing and Stargazer offers a feasible path for broad implementation of PGx testing and the optimization of individual drug treatment responses.
Genetic variation contributes significantly to the wide interindividual variability in pharmacological responses and gives rise to differences in systemic drug exposure, safety, and efficacy.1 Not accounting for this genetic variation can lead to severe adverse reactions or a loss of efficacy, due to inappropriate drug choice and/or dosing.2, 3 For example, multiple loss‐of‐function variants in the CYP2C9 gene can greatly diminish drug metabolism by blocking enzyme synthesis or reducing its catalytic function.4, 5 Individuals who are homozygous for these variants are called CYP2C9 poor metabolizers and are at risk of abnormal bleeding if prescribed the average dose of the anticoagulant warfarin.6
Pharmacogenetic (PGx) testing offers the potential for precision drug therapy, through the combination of genetic information and corresponding drug response phenotypes. Optimal pharmacotherapy can be determined by PGx testing to increase the overall efficacy and prevent adverse drug reactions.7 The US Food and Drug Administration provides additional guidance by requiring applicable PGx test information be included in the drug labeling.8 However, to date, broad implementation of PGx testing has met several challenges, and only a few PGx tests are currently routinely used in the clinic.9
A major barrier to broad implementation has been the complexity of many pharmacogenes. Several genes require that PGx testing include a large number of genetic variants to provide accurate predictions of enzymatic activity.10 For example, the clinically important CYP2D6 gene has >100 star alleles (haplotypes) defined by single‐nucleotide variants (SNVs), small insertion‐deletions (indels), and/or large structural variants (SVs).11 These CYP2D6 alleles encode enzymes with normal, decreased, increased, or no function, which translate to inferred clinical phenotypes that range from ultrarapid to poor metabolism.12 Importantly, the frequency of star alleles and phenotypes can vary across different populations,13 highlighting the need for comprehensive variant testing.
Another major challenge has been that a large fraction of existing star alleles cannot be accurately assessed with a single methodology. As stated above, CYP2D6 alleles include SVs, such as deletions, duplications, and complex gene hybrids. Many of these SVs are difficult to detect due to high sequence homology (>95%) with a nearby nonfunctional paralog.14 Thus, several orthogonal genotyping methods, including TaqMan assays, long‐range polymerase chain reaction (PCR), quantitative multiplex PCR, High Resolution Melt analysis, and Sanger sequencing are required to accurately call all SVs in CYP2D6.15 These methods do reliably detect the star alleles needed for clinical application but can be time‐consuming and biased toward the detection of known SVs.
The Centers for Disease Control and Prevention–based Genetic Testing Reference Materials Coordination Program (GeT‐RM) has established genomic DNA reference materials to help the genetic testing community obtain characterized reference materials.16 A GeT‐RM collaborative project recently published genotyping results for 137 ethnically diverse Coriell DNA samples and 28 pharmacogenes.17, 18 These samples were genotyped using several commercial and laboratory‐developed PGx testing assays.17 More recently, GeT‐RM has made whole genome sequencing (WGS) data for 70 of the 137 reference samples publicly available.18
In this study, we utilized the genotyping results from GeT‐RM and the available WGS data to continue the development of a new next‐generation sequencing‐based tool. We extended the SV‐aware algorithm of Stargazer19 to assess star alleles in 28 pharmacogenes (Table 1). Among these genes, CYP2A6, GSTM1, GSTT1, and UGT2B17 are known to display extensive gene‐deletion polymorphisms.20 Additionally, CYP2A6, CYP2B6, and CYP2D6 have been shown to frequently exhibit complex SVs, which include gene hybrids with their paralogs CYP2A7, CYP2B7, and CYP2D7, respectively.21, 22, 23 To evaluate the accuracy of this algorithm, we compared star alleles detected by Stargazer to those previously reported by GeT‐RM. In addition, we provide an in‐depth characterization of the WGS data of these 70 reference samples, which includes the identification of star alleles not tested in previous genotyping efforts. In order to verify Stargazer's SV calls, we explored the Database of Genomic Variants (DGV)24 for variant reports submitted by various studies, including the 1000 Genomes Project (1KGP).25
Table 1.
Gene | Reference allele | Star alleles found in consensus GeT‐RM genotypes (N = 92) | Star alleles only found in nonconsensus GeT‐RM genotypes (N = 31) |
---|---|---|---|
CYP1A1 | *1 | *2, *4, *5 | None |
CYP1A2 | *1A | *1C, *1F, *1L | None |
CYP2A6 | *1 | *2, *4 (del), *9, *17, *20 | *8 |
CYP2B6 | *1 | *2, *6, *7, *18 | *4, *5, *15, *20, *22, *27 |
CYP2C8 | *1 | *2, *3, *4 | None |
CYP2C9 | *1 | *2, *3, *5, *6, *8, *9, *11 | *18 |
CYP2C19 | *1 | *2, *3, *4, *8, *13, *15, *17 | *6, *27 |
CYP2D6 | *1 | *2, *2x2 (dup), *4, *5 (del), *6, *9, *10, *14, *15, *17, *29, *35, *41, *xN (dup) | *21, *36 + *10 (hyb), *40 |
CYP2E1 | *1 | *7 | *4, *5 |
CYP3A4 | *1 | *1B, *2, *3, *22 | *15, *16 |
CYP3A5 | *1 | *3, *6, *7 | None |
CYP4F2 | *1 | *2, *3 | None |
DPYD | *1 | *9 | *4 |
GSTM1 | *A | *B, *0 (del) | None |
GSTP1 | *A | *B, *C, *D | None |
GSTT1 | *A | *0 (del) | *AxN (dup), *B |
NAT1 | *4 | *11, *14, *17 | None |
NAT2 | *4 | *5, *6, *7, *14 | *12, *13 |
SLC15A2 | *1 | *2 | None |
SLC22A2 | *1 | *3, *6, *7 | *2, *K432Q |
SLCO1B1 | *1A | *1B, *5, *14, *15, *17, *21 | None |
SLCO2B1 | *1 | None | *S464F |
TPMT | *1 | *3C, *8 | None |
UGT1A1 | *1 | *6, *28, *60 | *7, *27, *36, *37 |
UGT2B7 | *1 | *2 | *3 |
UGT2B15 | *1 | *2, *5 | *4 |
UGT2B17 | *1 | *2 (del) | None |
VKORC1 | *1 | *2, *3, *4 | None |
Structural variant–defined alleles are indicated by “del” (deletion), “dup” (duplication), and “hyb” (hybrid).
GeT‐RM, Genetic Testing Reference Materials Coordination Program.
Results
Evaluating Stargazer's genotyping accuracy
We applied Stargazer to assess 1,960 genotypes in 28 pharmacogenes in 70 WGS samples from GeT‐RM. To estimate the accuracy of Stargazer, we compared these genotypes with those previously published by GeT‐RM.17 For these samples, GeT‐RM reported a total of 1,559 consensus genotypes comprised of 92 star alleles (Table 1). These consensus genotypes were verified by two or more PGx testing assays.17 In all 28 genes, Stargazer recalled 100% of star alleles present in GeT‐RM's consensus genotypes (Table S1).
WGS confirmation of star alleles present in “non‐consensus” GeT‐RM genotypes
A subset of GeT‐RM genotypes (N = 401) could not be verified by multiple PGx testing assays (Table S1). This is either because certain star alleles were tested by a single method or multiple test results disagreed.17 A total of 31 star alleles were only found in these “nonconsensus” genotypes (Table 1). Stargazer's output confirmed the presence of most of these star alleles with the exception of four alleles: CYP2A6*8, CYP2B6*27, CYP2C9*18, and GSTT1*AxN. These four alleles were not present in the WGS data (Table S2). For example, eight samples were predicted to contain a GSTT1 duplication (GSTT1*AxN) using the Agena Bioscience iPLEX ADME PGx Pro Panel (Agena Bioscience, San Diego, CA). However, Stargazer's output showed that three of these samples had a normal copy number of two, and the remaining five samples had a deletion (GSTT1*0) instead (Figure S1). To provide validation for these deletion events, we searched DGV and found that four of these five samples were also previously shown by 1KGP to have copy number loss in GSTT1 (Table S3).
SV‐defined alleles previously undercalled by GeT‐RM
Stargazer's output showed that three gene deletions (CYP2A6*4, GSTM1*0, and GSTT1*0) and one CYP2D6/CYP2D7 hybrid (CYP2D6*36+*10) were previously under‐reported by GeT‐RM (Figure 1 and Table 2). For example, GeT‐RM tested gene deletions in GSTM1 using the Affymetrix DMET Plus Array (Affymetrix, Santa Clara, CA) and the Agena Bioscience iPLEX ADME PGx Pro Panel. Both assays identified 32 samples with homozygous deletions but found no samples with heterozygous deletions. In contrast, Stargazer detected both heterozygous and homozygous deletions in 21 and 32 samples, respectively. By cross‐referencing to DGV reports from 1KGP, we validated copy number loss in GSTM1 for 13 of the 21 samples with heterozygous deletions (Table S3). Similarly, we used 1KGP's DGV reports to verify Stargazer's genotype calls for samples with CYP2A6*4 (N = 2) and GSTT1*0 (N = 13; Table S3).
Table 2.
Star allele | Assaysa | N of heterozygotes from GeT‐RM | N of homozygotes from GeT‐RM | N of heterozygotes from Stargazer | N of homozygotes from Stargazer |
---|---|---|---|---|---|
CYP2A6*4 | [1, 2] | 4 | 2 | 7 | 2 |
CYP2D6*36 + *10 | [2, 3] | 7 | 0 | 4 | 4 |
GSTM1*0 | [1, 2] | 0 | 32 | 21 | 32 |
GSTT1*0 | [1, 2] | 16 | 18 | 36 | 18 |
GeT‐RM, Genetic Testing Reference Materials Coordination Program.
[1] Affymetrix DMET Plus Array (Affymetrix, Santa Clara, CA); [2] Agena Bioscience iPLEX ADME PGx Pro Panel (Agena Bioscience, San Diego, CA); [3] Agena Bioscience iPLEX ADME CYP2D6 Panel (Agena Bioscience, San Diego, CA).
WGS identification of additional star alleles not previously reported by GeT‐RM
Using the WGS data, Stargazer detected 38 additional star alleles not previously reported by GeT‐RM (Table 3). These alleles were found in 127 of 1,960 genotypes assessed (Table S1). Seven of these alleles contained SVs and were comprised of five gene duplications, one CYP2B6/CYP2B7 hybrid, and one CYP2D6/CYP2D7 hybrid (Figure 2). Of the five duplications, only CYP2A6*1x2, CYP2D6*2x2, and CYP2D6*4x2 are currently listed in existing PGx databases, suggesting that the remaining two, CYP2D6*34x2 and CYP2E1*7x2, may be novel. CYP2D6*34x2 was identified from a single African sample (NA19207), and CYP2E1*7x2 was identified from three African samples (NA19095, NA19226, and NA19908); note that NA19908 was homozygous for CYP2E1*7x2 (Figure 2). DGV reports support the presence of CYP2A6*1x2 in NA18861 (DGV gold standard; copy number gain observed by multiple studies) and the presence of CYP2E1*7x2 in NA19908 (copy number gain observed by 1KGP; Table S3).
Table 3.
Gene | Star alleles (N = 38) |
---|---|
CYP1A1 | *2A, *2B, *13 |
CYP2A6 | *1x2 (dup), *7, *15, *18, *19, *21, *22, *23, *24, *25, *35 |
CYP2B6 | *17, *23, *29 (hyb) |
CYP2C19 | *35 |
CYP2D6 | *4x2 (dup), *34, *34x2 (dup), *39, *46, *68 + *4 (hyb) |
CYP2E1 | *7x2 (dup) |
DPYD | *5, *6 |
GSTM1 | *Ax2 (dup) |
NAT1 | *3, *10, *26 |
SLC22A2 | *4 |
SLCO1B1 | *24, *27, *30, *31, *35 |
TPMT | *16 |
Structural variant‐defined alleles are indicated by “dup” (duplication) and “hyb” (hybrid).
GeT‐RM, Genetic Testing Reference Materials Coordination Program.
Surprisingly, Stargazer detected three gene copies for the CYP3A4, CYP3A5, UGT2B7, and UGT2B15 genes in a single sample (NA18540) (Figure S2). CYP3A4 and CYP3A5 are 77 kbp apart on chromosome 7, whereas UGT2B7 and UGT2B15 are 426 kbp apart on chromosome 4. GeT‐RM did not report any SVs in these genes for this sample or other samples tested.17 Copy number analyses using Stargazer showed no breakpoints in flanking genomic regions (Figure S2), indicating that this sample likely has chromosomal trisomy for chromosomes 4 and 7 (i.e., CYP3A4*1/*1/*1, CYP3A5*1/*1/*3, UGT2B7*1/*1/*2, and UGT2B15*2/*2/*4). This result has been independently confirmed through karyotyping by Redon et al.,26 which has additionally revealed trisomy in chromosomes 9, 14, and 21. This aberrant karyotype most likely arose during cell immortalization.
Statistical phasing of SNVs/indels for star alleles
Using statistical phasing27 with the 1KGP haplotype reference panel,28 Stargazer revised a total of 64 GeT‐RM genotypes (Table S1). For instance, both GeT‐RM and Stargazer found 4 heterozygous SNVs in 14 samples that were indicative of the CYP1A2*1A/*1L or *1C/*1F genotype. GeT‐RM reported both genotypes as equally likely, whereas the phasing algorithm indicated the CYP1A2*1A/*1L genotype to be more likely. In addition, Stargazer revised GeT‐RM genotypes in two related samples, NA12156 (mother) and NA10831 (child), to follow expected inheritance patterns. As an example, GeT‐RM and Stargazer genotyped the mother as UGT1A1*28/*60 and *1/*28, *60, respectively. The mother's correct genotype should be the latter because the child was genotyped as UGT1A1*28, *60/*28, *60 by both GeT‐RM and Stargazer.
Resolving ambiguous CYP2D6 duplications using WGS allelic depth
Both GeT‐RM and Stargazer found seven samples with a gene duplication in the CYP2D6 gene. For four of these samples, GeT‐RM reported genotypes containing gene duplications of an unspecified star allele (CYP2D6*xN), whereas Stargazer resolved these ambiguous duplications using allelic depth of WGS reads (Table S1). For instance, GeT‐RM genotyped the sample NA19819 as CYP2D6*2/*4/*xN because the sample contained three gene copies as well as the CYP2D6*2 (normal function) and *4 (no function) alleles. In contrast, Stargazer called the sample as CYP2D6*2/*4x2, a genotype that was previously independently verified for this sample.19
New star alleles defined with WGS findings
Stargazer identified SNVs, indels, and SVs not present in existing haplotype translation tables. These variants represent 9 new star alleles and were found in a total of 20 Stargazer genotypes in a population‐specific manner (Table 4 and Table S1). More specifically, functional annotation of SNVs/indels added four new star alleles defined by two nonsense variants (CYP2C9*S1 and SLCO1B1*S1), a splice site variant (SLCO1B1*S2), and an in‐frame deletion variant (SLCO2B1*S1). All of these variants have an rsID except for CYP2C9*S1. Concordant with our data, 1KGP previously found SLCO2B1*S1 predominantly in East Asians with allele frequency of 0.105. In addition, 1KGP observed SLCO1B1*S1 and SLCO1B1*S2 exclusively in East Asians and Africans, respectively, which is in agreement with our findings. As shown in Figure 3, copy number analyses with Stargazer also identified three partial gene deletions (SLC22A2*S1, SLC22A2*S2, and UGT2B15*S1), a partial gene duplication (CYP2E1*S1), and a whole gene duplication of CYP2A7 (CYP2A6*1+*S6). To enable automated detection of these SVs, we defined and included five new star alleles as part of the Stargazer algorithm. DGV records confirm the presence of CYP2E1*S1 in NA19143 (copy number gain observed by Wang et al.29) and the presence of SLC22A2*S2 in NA19226 and NA19819 (DGV gold standard; copy number loss observed by multiple studies) (Table S3).
Table 4.
Star allele | Descriptiona | N of African samples | N of East Asian samples | N of European samples |
---|---|---|---|---|
CYP2A6*1 + *S6 | Gene duplication of CYP2A7 (chr19:41358125‐41389907) | 0 | 1 | 0 |
CYP2E1*S1 | Gene duplication in exons 7‐9 (chr10:135350465‐135439323) | 4 | 0 | 0 |
SLC22A2*S1 | Gene deletion in intron 9 (chr6:160649735‐160654861) | 3 | 0 | 0 |
SLC22A2*S2 | Gene deletion affecting 3′‐UTR (chr6:160627751‐160638068) | 2 | 0 | 0 |
UGT2B15*S1 | Gene deletion affecting exons 4‐6 (chr4:69510975‐69528283) | 0 | 0 | 1 |
CYP2C9*S1 | Nonsense (chr10:96741125A>T; no rsID) | 0 | 1 | 0 |
SLCO1B1*S1 | Nonsense (chr12:21349909C>T; rs183501729) | 0 | 1 | 0 |
SLCO1B1*S2 | Splice site (chr12:21329832G>T; rs77271279) | 2 | 0 | 0 |
SLCO2B1*S1 | In‐frame deletion (chr11:74873754GCACAGAAAA>G; rs72408262) | 0 | 4 | 1 |
Genomic coordinates and nucleotide changes are according to Human Genome version 19.
Discussion
Here, we present an extension of the Stargazer algorithm to call star alleles in 28 pharmacogenes from next‐generation sequencing data. Stargazer is one of the first bioinformatics tools that enable systematic identification of star alleles (e.g., Cypiripi,30 Astrolabe,31 PharmCAT,32 and Aldy33). Stargazer is the only tool that uses statistical haplotype phasing,27 which is informed by population haplotype frequencies to call star alleles more accurately. In addition, other tools tend to have difficulties with the detection of complex SVs, such as CYP2D6/CYP2D7 hybrids.30, 31, 32 Lastly, to our knowledge, Stargazer is the most comprehensive tool available and assesses star alleles in more genes than has previously been reported.32, 33
To evaluate the performance of Stargazer, we utilized public WGS data from 70 genotyping reference samples from GeT‐RM. These samples were extensively characterized using multiple standard methods (e.g., allele‐specific PCR, molecular inversion probes, hybridization‐based arrays, and TaqMan assays).17 To verify Stargazer's SV calls, we explored DGV reports from various sources, including 1KGP. In all 28 genes, Stargazer recalled 100% of star alleles present in GeT‐RM's consensus genotypes. Stargazer also identified additional star alleles not previously reported by GeT‐RM, including both known and novel SVs, and correctly found trisomies of the chromosomes 4 and 7 in the sample NA18540. Altogether, these results demonstrate that Stargazer has high sensitivity for the detection of SVs and can accurately assess star alleles in these 28 genes.
With statistical phasing, Stargazer revised star alleles in reference samples that previously had ambiguous or incorrect GeT‐RM genotypes. In the current version of Stargazer, we incorporated the 1KGP haplotype reference panel to increase sample size and improve phase accuracy.34 This approach performed well for our dataset, but we are aware that further applications may be challenged by low‐frequency variants and limited by the magnitude and extent of linkage disequilibrium.35 To ameliorate this issue, we plan to merge multiple large, high‐quality reference panels to obtain additional haplotype information.
CYP2D6 duplications have been reported for normal function, decreased function, and nonfunctional alleles.36, 37, 38 GeT‐RM previously reported ambiguous CYP2D6 genotypes involving duplication of an unspecified allele (CYP2D6*xN). For instance, the sample NA19819 was genotyped as CYP2D6*2/*4/*xN by GeT‐RM where CYP2D6*2 and *4 are normal function and nonfunctional alleles, respectively. Therefore, the sample could tentatively be CYP2D6*2x2/*4 or *2/*4x2, which would predict two completely different phenotypes—normal metabolizer and intermediate metabolizer, respectively. By using allelic depth of WGS reads, Stargazer correctly called the CYP2D6*2/*4x2 genotype for the sample19 and resolved other genotypes with ambiguous CYP2D6 duplications. Furthermore, both GeT‐RM and Stargazer predicted the samples HG00436, NA19109, and NA19226 to be ultrarapid metabolizers (CYP2D6*1/*2x2, *29/*2x2, and *2/*2x2, respectively), which is a major phenotypic consequence of carrying CYP2D6 gene duplications. Collectively, these results highlight that allelic decomposition performed by Stargazer enables accurate phenotype prediction for samples with gene duplications.
We report nine new star alleles defined by variants discovered in WGS data. Although the enzymatic activity of these alleles remains to be functionally characterized, seven alleles likely have an impact on enzyme activity. UGT2B15*S1, for instance, is likely nonfunctional because it includes deletion of the last three exons of the UGT2B15 gene. Another new allele, CYP2A6*1 + *S6, contains a gene duplication in the paralog CYP2A7. The duplication does not directly affect the CYP2A6 sequence, but it could still change CYP2A6 activity because CYP2A7 transcript level has been shown to alter CYP2A6 expression via competition for miRNA binding.39 Conversely, the partial gene deletions in the SLC22A2*S1 and *S2 alleles do not affect the translated region of the SLC22A2 gene and, thus, are unlikely to have a functional consequence.
As of April 2019, there are 359 gene/drug pairs (e.g., CYP2D6/codeine) described by the Clinical Pharmacogenetics Implementation Consortium with accompanying levels of evidence for changing drug choice and dosing decisions.40 The assigned levels (A, B, C, and D) are subject to change, and only levels A and B gene/drug pairs (N = 144) have sufficient evidence for at least one prescribing action to be recommended.40 The 28 pharmacogenes currently targeted by Stargazer include 132 of these gene/drug pairs, 67 of which have level A or B. We plan to further extend Stargazer to additional pharmacogenes, including 26 PGx loci whose consensus genotypes could not be determined in Pratt et al.17 because they were only characterized by one laboratory.
In summary, by leveraging WGS data, we confirmed the consensus results reported by GeT‐RM and expanded the current PGx variation catalogs for the 70 important reference samples. Therefore, our WGS characterization can be added to this public reference resource for other PGx genotyping projects. As sequencing costs continue to decline and as the clinical value of whole genome (or targeted panel) sequencing continues to emerge, there will be an increasing need for systematic and highly efficient analysis algorithms. Our results show that WGS data combined with Stargazer offers a feasible path for accurate PGx testing and the optimization of individual drug treatment responses.
Methods
PGx genotypes and WGS data from GeT‐RM
We accessed PGx genotypes and WGS data for 70 ethnically diverse Coriell DNA samples from GeT‐RM (Tables [Link], [Link]). Both PGx genotypes and WGS data are publically available through the GeT‐RM website.18 GeT‐RM generated consensus and nonconsensus genotypes for 28 pharmacogenes using a variety of testing platforms, as detailed in Pratt et al.17 WGS was performed to a depth of >30X using paired‐end 150‐bp sequence reads on the Illumina HiSeq X (Illumina, San Diego, CA). WGS data were downloaded in the BAM file format, which contains sequence reads aligned to Human Genome version 19 with the program ISAAC.41
Extension of Stargazer to 28 pharmacogenes
The first version of Stargazer (version 1.0.0) included a haplotype translation table for >100 star alleles in the CYP2D6 gene.19 Extension of Stargazer (version 1.0.4) involved construction of 27 additional haplotype translation tables for > 500 star alleles. Star allele information was compiled from several public PGx databases: the Pharmacogene Variation Consortium,42 the Pharmacogenomics Knowledgebase,43 the UGT database,44 the NAT database,45 and the TPMT database.46 Generation of haplotype translation tables involved lifting cDNA coordinates of PGx variants to genomic coordinates from Human Genome version 19. The new version of Stargazer and all haplotype translation tables are available for download: https://stargazer.gs.washington.edu/stargazerweb/.
Description of Stargazer's algorithm
Stargazer's algorithm has been described previously.19 Briefly, for this extended version, SNVs/indels in each gene were assessed from a Variant Call Format (VCF) file generated from BAM files using GATK‐HaplotypeCaller.47 The VCF file was phased using the program Beagle27 with the 1KGP haplotype reference panel.28 Phased SNVs/indels were then matched to star alleles in each gene's haplotype translation table. BAM files were also used to calculate read depth using GATK‐DepthOfCoverage.47 Read depth was converted to copy number by intrasample normalization. Following normalization, SVs were detected by testing pairwise combinations of expected haplotype copy number profiles against the sample's observed copy number profile for both haplotypes. SV results were incorporated to inform the final star allele assignment. Output data of Stargazer included individual genotypes and copy number plots to visually inspect SVs calls (see Figure 1 for examples of these plots).
Assessment of differences in genotype calls between GeT‐RM and Stargazer
Differences in genotype calls between GeT‐RM and Stargazer were carefully evaluated by considering the consistency of star allele assignment across individual PGx testing assays as well as assessment of WGS reads. WGS reads were assessed through visual inspection using Integrative Genomics Viewer,48 as exemplified in Table S2. For validation of Stargazer's results involving SVs, we used existing reports available in DGV. A total of 33 Stargazer genotypes were verified this way (26 samples overlapped with DGV; Table S3).
Assessment of novel variation by Stargazer
Stargazer's output includes a VCF file of detected SNVs/indels not present in existing PGx databases. This VCF file is functionally annotated using SeattleSeq Annotation.49 Functional annotation enables prediction of nonsynonymous variants, which may impact enzyme activity. For samples with SVs that do not match expected copy number profiles, Stargazer performs change point analysis.50 This analysis identifies approximate breakpoints, which are then used to identify subsequent SVs with similar breakpoints in copy number profiles.
Funding
This work was supported by the National Institute of General Medical Sciences (NIGMS) (R24GM115277, P50GM115318, and P01GM116691). S.B.L. is a recipient of Macrogen PhD Fellowship.
Conflict of Interest
The authors declared no competing interests for this work.
Author Contributions
S.B.L., M.M.W., K.E.T., and D.A.N. wrote the manuscript. S.B.L., K.E.T., and D.A.N. designed the research. S.B.L. performed the research. S.B.L. and M.M.W. analyzed the data.
Supporting information
Acknowledgments
The authors acknowledge the Genetic Testing Reference Materials Coordination Program (GeT‐RM) for their generous contribution of pharmacogenetic genotypes and whole genome sequencing data.
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