The majority of life on Earth is non-diploid and represented by prokaryotes, viruses, and their derivatives, such as our own mitochondria or plant’s chloroplasts. In non-diploid systems, allele frequencies can range anywhere between 0 and 100% and there could be multiple (not just two) alleles per locus. The main challenge associated with non-diploid variant calling is the difficulty in distinguishing between the sequencing noise (abundant in all NGS platforms) and true low frequency variants. Some of the early attempts to do this well have been accomplished on human mitochondrial DNA although the same approaches will work equally good on viral and bacterial genomes (Rebolledo-Jaramillo et al. 2014, Li et al. 2015).

As an example of non-diploid systems, we will be using human mitochondrial genome. However, this approach will also work for most bacterial and viral genomes.

There are two ways one can call variants:

1. By comparing reads against an existing genome assembly
2. By assembling a genome first and then mapping against that assembly

Open image in new tab

In this tutorial we will take the first path, in which we map reads against an existing assembly. Later in the course, after we learn about assembly approaches, we will try the second approach as well.

The goal of this example is to detect heteroplasmies - variants within mitochondrial DNA. Mitochondria are transmitted maternally, and heteroplasmy frequencies may change dramatically and unpredictably during the transmission due to a germ-line bottleneck (Cree et al. 2008). As we mentioned above, the procedure for finding variants in bacterial or viral genomes will be essentially the same.

Datasets representing a child and a mother are available in Zenodo. These datasets were obtained by paired-end Illumina sequencing of human genomic DNA enriched for mitochondria. The enrichment was performed using long-range PCR with two primer pairs that amplify the entire mitochondrial genome. Samples will therefore still contain a lot of DNA from the nuclear genome, which, in this case, is a contaminant.

Agenda

In this tutorial, we will cover:

1. Importing data
   1. Checking data quality
2. Mapping reads to a reference
3. Postprocessing mapped reads
   1. Merging BAM datasets
   2. Removing duplicates
   3. Left-aligning indels
   4. Filtering reads
4. Calling non-diploid variants
   1. Filtering variants
5. Examining the results
   1. Visualising with VCF.IOBIO
   2. Visualising with IGV
   3. Comparing frequencies
6. Conclusion

Importing data

For this tutorial we have prepared a subset of data previously by our group (Rebolledo-Jaramillo et al. 2014). Let’s import these data into Galaxy. They are available from this Galaxy Library or via Zenodo

Hands On: Get the data

1. Create a new history for this tutorial and give it a meaningful name

   Tip: Creating a new history

   To create a new history simply click the new-history icon at the top of the history panel:

   

   Tip: Renaming a history

   1. Click on galaxy-pencil (Edit) next to the history name (which by default is “Unnamed history”)
   2. Type the new name
   3. Click on Save
   4. To cancel renaming, click the galaxy-undo “Cancel” button

   If you do not have the galaxy-pencil (Edit) next to the history name (which can be the case if you are using an older version of Galaxy) do the following:

   1. Click on Unnamed history (or the current name of the history) (Click to rename history) at the top of your history panel
   2. Type the new name
   3. Press Enter

2. Import files from Zenodo:

   https://zenodo.org/record/1251112/files/raw_child-ds-1.fq
   https://zenodo.org/record/1251112/files/raw_child-ds-2.fq
   https://zenodo.org/record/1251112/files/raw_mother-ds-1.fq
   https://zenodo.org/record/1251112/files/raw_mother-ds-2.fq
   

3. Check that all newly created datasets in your history are assigned datatype fastqsanger, and fix any missing or wrong datatype assignment

   Tip: Changing the datatype

   • Click on the galaxy-pencil pencil icon for the dataset to edit its attributes
   • In the central panel, click galaxy-chart-select-data Datatypes tab on the top
   • In the galaxy-chart-select-data Assign Datatype, select fastqsanger from “New type” dropdown
     • Tip: you can start typing the datatype into the field to filter the dropdown menu
   • Click the Save button

Checking data quality

Before proceeding with the analysis, we need to find out how good the data actually is. For this will use FastQC.

Hands On: Assess quality of data

1. Run FastQC ( Galaxy version 0.72+galaxy1) on each of the four FASTQ datasets with the following parameters:
   • param-files “Short read data from your current history”: all 4 FASTQ datasets selected with Multiple datasets

   Tip: Select multiple datasets

   1. Click on param-files Multiple datasets
   2. Select several files by keeping the Ctrl (or COMMAND) key pressed and clicking on the files of interest

Once the FastQC jobs runs, you will be able to look at the HTML reports generated by this tool. The data have generally high quality in this example:

Open image in new tab

Mapping reads to a reference

Our reads are long (250 bp) so we will use BWA-MEM (Li 2013) to align them against the reference genome as it has good mapping performance for longer reads (100bp and up).

Hands On: Map reads

1. Use Map with BWA-MEM ( Galaxy version 0.7.17.1) to map the reads to the reference genome with the following parameters:
   • “Will you select a reference genome from your history or use a built-in index?”: Use a built-in genome index
     • “Using reference genome”: Human: hg38 (or a similarly named option)
   • “Single or Paired-end reads”: Paired
     • param-files “Select first set of reads”: select both -1 datasets selected with Multiple datasets
     • param-files “Select second set of reads”: select both -2 datasets selected with Multiple datasets
   • “Set read groups information?”: Set read groups (SAM/BAM specification)
     • “Auto-assign”: Yes
     • “Auto-assign”: Yes
     • “Platform/technology used to produce the reads (PL)”: ILLUMINA
     • “Auto-assign”: Yes

Comment: More about selecting datasets

By selecting datasets 1 and 3 as Select the first set of reads and datasets 2 and 4 as Select the second set of reads, Galaxy will automatically launch two BWA-MEM jobs using datasets 1,2 and 3,4 generating two resulting BAM files. By setting Set read groups information to Set read groups (SAM/BAM specifications) and clicking Auto-assign we will ensure that the reads in the resulting BAM dataset are properly set.

Postprocessing mapped reads

Merging BAM datasets

Because we have set read groups, we can now merge the two BAM dataset into one. This is because read groups label each read as belonging to either mother or child.

Hands On: Merge multiple datasets into one

1. Use MergeSAMFiles ( Galaxy version 2.18.2.1) to merge the BAM datasets with the following parameters:
   • param-files “Select SAM/BAM dataset or dataset collection”: select both BAM datasets produced by BWA-MEM tool
   • “Select validation stringency”: Lenient

Removing duplicates

Preparation of sequencing libraries (at least at the time of writing) for technologies such as Illumina (used in this example) involves PCR amplification. It is required to generate sufficient number of sequencing templates so that a reliable detection can be performed by base callers. PCR has its own biases which are especially profound in cases of multi-template PCR used for construction of sequencing libraries (Kanagawa 2003).

Duplicates can be identified based on their outer alignment coordinates or using sequence-based clustering. One of the common ways for identification of duplicate reads is the MarkDuplicates utility from Picard package which is designed to identify both PCR and optical duplicates.

Details: More about MarkDuplicates

Duplicates are identified as read pairs having identical 5’ positions (coordinate and strand) for both reads in a mate pair (and optionally, matching unique molecular identifier reads; see BARCODE_TAG option). Optical, or more broadly sequencing, duplicates are duplicates that appear clustered together spatially during sequencing and can arise from optical/imagine-processing artifacts or from biochemical processes during clonal amplification and sequencing; they are identified using the READ_NAME_REGEX and the OPTICAL_DUPLICATE_PIXEL_DISTANCE options. The tool’s main output is a new SAM or BAM file in which duplicates have been identified in the SAM flags field, or optionally removed (see REMOVE_DUPLICATE and REMOVE_SEQUENCING_DUPLICATES), and optionally marked with a duplicate type in the ‘DT’ optional attribute. In addition, it also outputs a metrics file containing the numbers of READ_PAIRS_EXAMINED, SECONDARY_OR_SUPPLEMENTARY_RDS, UNMAPPED_READS, UNPAIRED_READS, UNPAIRED_READ DUPLICATES, READ_PAIR_DUPLICATES, and READ_PAIR_OPTICAL_DUPLICATES.

Usage example: java -jar picard.jar MarkDuplicates I=input.bam O=marked_duplicates.bam M=marked_dup_metrics.txt

Hands On: De-duplicate mapped data

1. Use MarkDuplicates ( Galaxy version 2.18.2.2) to de-duplicate the merged BAM datasets with the following parameters:
   • param-file “Select SAM/BAM dataset or dataset collection”: select the merged BAM dataset produced by MergeSAMFiles tool
   • “The scoring strategy for choosing the non-duplicate among candidates”: SUM_OF_BASE_QUALITIES
   • “The maximum offset between two duplicate clusters in order to consider them optical duplicates”: 100
   • “Select validation stringency”: Lenient

MarkDuplicates produces a BAM dataset with duplicates removed and also a metrics file. Let’s take a look at the metrics data:

raw_child-ds-	55	27551	849	55	50	1658	1	0.06103	219750
raw_mother-ds-	95	54973	1951	95	89	4712	2	0.08645	302188

Column headers are:

• LIBRARY (read group in our case)
• UNPAIRED_READS_EXAMINED
• READ_PAIRS_EXAMINED-
• SECONDARY_OR_SUPPLEMENTARY_RDS
• UNMAPPED_READS
• UNPAIRED_READ_DUPLICATES
• READ_PAIR_DUPLICATES
• READ_PAIR_OPTICAL_DUPLICATES
• PERCENT_DUPLICATION
• ESTIMATED_LIBRARY_SIZE

Question

1. What percent of read duplication are found in each read group (child and mother)?

Solution

1. The two datasets have ~6% and ~9% duplicates for child and mother, respectively.

Left-aligning indels

Left aligning of indels (a variant of re-aligning) is extremely important for obtaining accurate variant calls. For illustrating how left-aligning works, we expanded on an example provided by Tan et al. 2015. Suppose you have a reference sequence and a sequencing read:

Reference GGGCACACACAGGG
Read      GGGCACACAGGG

If you look carefully you will see that the read is simply missing a CA repeat. But it is not apparent to a mapper, so some of possible alignments and corresponding variant calls include:

Alignment                 Variant Call

GGGCACACACAGGG            Ref: CAC
GGGCAC--ACAGGG            Alt: C

GGGCACACACAGGG            Ref: ACA
GGGCA--CACAGGG            Alt: A

GGGCACACACAGGG            Ref: GCA
GGG--CACACAGGG            Alt: G

The last of these is left-aligned. In this case gaps (represented by dashes) are moved as far left as possible. For a formal definition of left-alignment and variant normalization, see Tan et al. 2015.

Hands On: Left-align indels

1. Use BamLeftAlign ( Galaxy version 1.3.1) to perform left alignment with the following parameters:
   • “Choose the source for the reference genome”: Locally cached
   • param-file “Select alignment file in BAM format”: select the BAM dataset produced by MarkDuplicates tool
   • “Using reference genome”: hg38
   • “Maximum number of iterations’: 5

Filtering reads

Remember that we are trying to call variants in mitochondrial genome. Let focus only on the reads derived from mitochondria genome by filtering everything else out.

Hands On: Filter BAM data

1. Use Filter BAM datasets on a variety of attributes ( Galaxy version 2.4.1) with the following parameters:
   • param-file “BAM dataset(s) to filter”: select the BAM dataset produced by BamLeftAlign tool
   • In “Condition”:
     • In “1: Condition”:
       • In “Filter”:
         • In “1: Filter”:
           • “Select BAM property to filter on”: mapQuality
           • “Filter on read mapping quality (phred scale)”: >=20
         • In “2: Filter”:
           • “Select BAM property to filter on”: isPaired
           • “Selected mapped reads”: Yes
         • Click on “Insert Filter”
         • In “3: Filter”:
           • “Select BAM property to filter on”: isProperPair
           • “Select reads with mapped mate”: Yes
         • Click on “Insert Filter”
         • In “4: Filter”:
           • “Select BAM property to filter on”: reference
           • “Select reads with mapped mate”: chrM

   Comment: Filtering reads

   Further explanation of the filters used:

   • mapQuality is set to ≥20. Mapping quality reflects the probability that the read is placed incorrectly using phred scale. Thus 20 is 1/100 or 1% chance that the read is incorrectly mapped. By setting this parameter to ≥20, we will keep all reads that have 1% or less probability of being mapped incorrectly.
   • isPaired will eliminate singleton (unpaired) reads.
   • isProperPair will only keep reads that map to the same chromosome and are properly placed.
   • reference is set to the mitochondrial chromosome, chrM.

Calling non-diploid variants

FreeBayes is widely used for calling variants in diploid systems. However, it can also be used for calling variants in pooled samples where the number of samples is not known. This is the exact scenario we have here: in our sample we have multiple mitochondrial (or bacterial or viral) genomes, but we do not know exactly how many. Thus we will use the --pooled-continuous option of FreeBayes to generate frequency-based variant calls as well as some other options highlighted below.

Hands On: Calling variants

1. Use FreeBayes ( Galaxy version 1.3.1) to call variants with the following parameters:
   • “Choose the source for the reference genome”: Locally cached
   • “Run in batch mode?”: Run individually
   • param-file “BAM dataset”: select the BAM dataset produced by last Filter tool step
   • “Using reference genome”: hg38
   • “Limit variant calling to a set of regions?”: Limit to region
     • “Region Chromosome”: chrM
     • “Region Start”: 1
     • “Region End”: 16000
   • “Choose parameter selection level”: 5: Full list of options
     • “Population model options”: Set population model options
       • “The expected mutation rate or pairwise nucleotide diversity among the population under analysis”: 0.001
       • “Set ploidy for the analysis”: 1
       • “Assume that samples result from pooled sequencing”: Yes
       • “Output all alleles which pass input filters, regardless of genotyping outcome or model”: Yes

   Comment: Population model options

   The “Population model options” are one of the most important parameter choices to make when calling variants in non-diploid systems.

   • “Allelic scope options”: Set allelic scope options
     • “Ignore SNP alleles”: No
     • “Ignore indels alleles”: No
     • “Ignore multi-nucleotide polymorphisms, MNPs”: Yes
     • “Ignore complex events (composites of other classes)”: Yes

   Comment: Allelic scope options

   Mitochondria has a number of low complexity regions (mononucleotide repeats). Setting the allelic scope parameters as described above will decrease noise from these regions.

   • “Input filters”: Set input filters
     • “Exclude alignments from analysis if they have a mapping quality less than”: 20
     • “Exclude alleles from analysis if their supporting base quality less than”: 30

   Comment: Filter options

   Setting Exclude alignments from analysis if they have a mapping quality less than to 20 (phred score of 20) will make FreeBayes only consider reliably aligned reads. Setting Exclude alleles from analysis if their supporting base quality less than to 30 (phred score of 30) will make FreeBayes only consider high quality bases.

FreeBayes will produce a VCF dataset similar to what is shown below (you may need to scroll sideways to see it in full). It lists 25 sites of interest. For brevity, the header lines have been removed:

#CHROM	POS	ID	REF	ALT	QUAL	FILTER	INFO	FORMAT	raw_child-ds-	raw_mother-ds-
chrM	73	.	A	G	30438.6	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=949;CIGAR=1X;DP=950;DPB=950;DPRA=0;EPP=144.879;EPPR=5.18177;GTI=0;LEN=1;MEANALT=1;MQM=55.8314;MQMR=60;NS=2;NUMALT=1;ODDS=2187.64;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=34948;QR=37;RO=1;RPL=322;RPP=215.867;RPPR=5.18177;RPR=627;RUN=1;SAF=421;SAP=29.2075;SAR=528;SRF=0;SRP=5.18177;SRR=1;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:226:0,226:0:0:226:8314:-739.462,0	1:724:1,723:1:37:723:26634:-2346.86,0
chrM	263	.	A	G	11603.3	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=364;CIGAR=1X;DP=364;DPB=364;DPRA=0;EPP=16.755;EPPR=0;GTI=0;LEN=1;MEANALT=1;MQM=60;MQMR=0;NS=2;NUMALT=1;ODDS=982.556;PAIRED=1;PAIREDR=0;PAO=0;PQA=0;PQR=0;PRO=0;QA=13201;QR=0;RO=0;RPL=276;RPP=213.858;RPPR=0;RPR=88;RUN=1;SAF=172;SAP=5.39653;SAR=192;SRF=0;SRP=0;SRR=0;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:108:0,108:0:0:108:3896:-350.812,0	1:256:0,256:0:0:256:9305:-837.344,0
chrM	310	.	TCC	CCC	4471	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=150;CIGAR=1X2M;DP=171;DPB=180.333;DPRA=0;EPP=7.70068;EPPR=4.45795;GTI=0;LEN=1;MEANALT=2.5;MQM=59.88;MQMR=60;NS=2;NUMALT=1;ODDS=407.373;PAIRED=1;PAIREDR=1;PAO=11;PQA=237;PQR=0;PRO=0;QA=5147;QR=194;RO=6;RPL=113;RPP=86.6265;RPPR=8.80089;RPR=37;RUN=1;SAF=35;SAP=95.6598;SAR=115;SRF=1;SRP=8.80089;SRR=5;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:54:0,49:0:0:49:1645:-150.867,0	1:117:6,101:6:194:101:3502:-315.963,0
chrM	513	.	GCACACACACAC	GCACACACACACAC	2095.84	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=109;CIGAR=1M2I11M;DP=150;DPB=172.167;DPRA=0;EPP=109.173;EPPR=6.05036;GTI=0;LEN=2;MEANALT=3.5;MQM=60;MQMR=60;NS=2;NUMALT=1;ODDS=225.991;PAIRED=1;PAIREDR=1;PAO=5;PQA=101.5;PQR=101.5;PRO=5;QA=3824;QR=1196;RO=35;RPL=19;RPP=103.436;RPPR=4.56135;RPR=90;RUN=1;SAF=80;SAP=54.8268;SAR=29;SRF=24;SRP=13.4954;SRR=11;TYPE=ins;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:34:5,28:5:163:28:996:-74.9521,0	1:116:30,81:30:1033:81:2828:-161.475,0
chrM	750	.	A	G	47254.6	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1459;CIGAR=1X;DP=1459;DPB=1459;DPRA=0;EPP=48.5904;EPPR=0;GTI=0;LEN=1;MEANALT=1;MQM=59.8705;MQMR=0;NS=2;NUMALT=1;ODDS=3230.11;PAIRED=1;PAIREDR=0;PAO=0;PQA=0;PQR=0;PRO=0;QA=53335;QR=0;RO=0;RPL=594;RPP=112.315;RPPR=0;RPR=865;RUN=1;SAF=1007;SAP=461.453;SAR=452;SRF=0;SRP=0;SRR=0;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:331:0,331:0:0:331:11988:-1073.7,0	1:1128:0,1128:0:0:1128:41347:-3719.34,0
chrM	1438	.	A	G	75374.8	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=2237;CIGAR=1X;DP=2238;DPB=2238;DPRA=0;EPP=47.8812;EPPR=5.18177;GTI=0;LEN=1;MEANALT=1;MQM=59.8605;MQMR=60;NS=2;NUMALT=1;ODDS=5003.07;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=84494;QR=37;RO=1;RPL=1397;RPP=304.171;RPPR=5.18177;RPR=840;RUN=1;SAF=925;SAP=148.392;SAR=1312;SRF=0;SRP=5.18177;SRR=1;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:488:0,488:0:0:488:18416:-1656.39,0	1:1750:1,1749:1:37:1749:66078:-5935.03,0
chrM	2706	.	A	G	39098.5	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1222;CIGAR=1X;DP=1235;DPB=1235;DPRA=0;EPP=3.188;EPPR=3.17734;GTI=0;LEN=1;MEANALT=1;MQM=59.9926;MQMR=60;NS=2;NUMALT=1;ODDS=2496.46;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=45333;QR=474;RO=13;RPL=507;RPP=79.8897;RPPR=3.17734;RPR=715;RUN=1;SAF=225;SAP=1062.06;SAR=997;SRF=5;SRP=4.51363;SRR=8;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:246:1,245:1:32:245:9136:-818.843,0	1:989:12,977:12:442:977:36197:-3215.79,0
chrM	3197	.	T	C	130583	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=3879;CIGAR=1X;DP=3892;DPB=3892;DPRA=0;EPP=59.2643;EPPR=3.17734;GTI=0;LEN=1;MEANALT=1;MQM=59.9938;MQMR=60;NS=2;NUMALT=1;ODDS=12192.8;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=146498;QR=463;RO=13;RPL=2190;RPP=143.521;RPPR=7.18621;RPR=1689;RUN=1;SAF=1459;SAP=519.999;SAR=2420;SRF=7;SRP=3.17734;SRR=6;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:1358:4,1354:4:150:1354:50893:-4563.63,0	1:2534:9,2525:9:313:2525:95605:-8569.92,0
chrM	3243	.	A	G	10397.4	.	AB=0;ABP=0;AC=1;AF=0.5;AN=2;AO=1365;CIGAR=1X;DP=3092;DPB=3092;DPRA=0;EPP=116.418;EPPR=46.9792;GTI=0;LEN=1;MEANALT=1;MQM=59.956;MQMR=59.8917;NS=2;NUMALT=1;ODDS=2394.09;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=49004;QR=63273;RO=1727;RPL=849;RPP=179.415;RPPR=105.14;RPR=516;RUN=1;SAF=443;SAP=368.01;SAR=922;SRF=637;SRP=261.033;SRR=1090;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:1035:341,694:341:12439:694:24871:-1118.32,0	0:2057:1386,671:1386:50834:671:24133:0,-2399.65
chrM	4769	.	A	G	48890.4	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1545;CIGAR=1X;DP=1545;DPB=1545;DPRA=0;EPP=162.63;EPPR=0;GTI=0;LEN=1;MEANALT=1;MQM=51.4796;MQMR=0;NS=2;NUMALT=1;ODDS=4468.76;PAIRED=1;PAIREDR=0;PAO=0;PQA=0;PQR=0;PRO=0;QA=57939;QR=0;RO=0;RPL=463;RPP=541.537;RPPR=0;RPR=1082;RUN=1;SAF=890;SAP=80.6281;SAR=655;SRF=0;SRP=0;SRR=0;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:517:0,517:0:0:517:19209:-1665.33,0	1:1028:0,1028:0:0:1028:38730:-3308.01,0
chrM	5539	.	A	G	3281.62	.	AB=0;ABP=0;AC=1;AF=0.5;AN=2;AO=379;CIGAR=1X;DP=787;DPB=787;DPRA=0;EPP=216.428;EPPR=224.5;GTI=0;LEN=1;MEANALT=1;MQM=54.1504;MQMR=53.777;NS=2;NUMALT=1;ODDS=755.62;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=13803;QR=15250;RO=408;RPL=74;RPP=308.741;RPPR=351.808;RPR=305;RUN=1;SAF=286;SAP=216.428;SAR=93;SRF=318;SRP=279.681;SRR=90;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	0:299:221,78:221:8252:78:2824:0,-485.016	1:488:187,301:187:6998:301:10979:-358.012,0
chrM	7028	.	C	T	70453.4	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=2109;CIGAR=1X;DP=2114;DPB=2114;DPRA=0;EPP=63.8084;EPPR=3.44459;GTI=0;LEN=1;MEANALT=1;MQM=55.9113;MQMR=59.2;NS=2;NUMALT=1;ODDS=6416.42;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=78988;QR=192;RO=5;RPL=1123;RPP=22.3353;RPPR=3.44459;RPR=986;RUN=1;SAF=969;SAP=33.1175;SAR=1140;SRF=3;SRP=3.44459;SRR=2;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:708:1,707:1:39:707:26465:-2367.64,0	1:1406:4,1402:4:153:1402:52523:-4692.5,0
chrM	7269	.	G	A	59443.2	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1773;CIGAR=1X;DP=1773;DPB=1773;DPRA=0;EPP=129.209;EPPR=0;GTI=0;LEN=1;MEANALT=1;MQM=58.3328;MQMR=0;NS=2;NUMALT=1;ODDS=5563.82;PAIRED=1;PAIREDR=0;PAO=0;PQA=0;PQR=0;PRO=0;QA=66393;QR=0;RO=0;RPL=929;RPP=11.8591;RPPR=0;RPR=844;RUN=1;SAF=848;SAP=10.2718;SAR=925;SRF=0;SRP=0;SRR=0;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:619:0,619:0:0:619:23040:-2069.26,0	1:1154:0,1154:0:0:1154:43353:-3894.52,0
chrM	8860	.	A	G	48674.5	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1552;CIGAR=1X;DP=1556;DPB=1556;DPRA=0;EPP=36.1924;EPPR=5.18177;GTI=0;LEN=1;MEANALT=1;MQM=46.5528;MQMR=58.25;NS=2;NUMALT=1;ODDS=4986.6;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=56983;QR=146;RO=4;RPL=845;RPP=29.6556;RPPR=5.18177;RPR=707;RUN=1;SAF=844;SAP=28.8889;SAR=708;SRF=2;SRP=3.0103;SRR=2;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:598:0,598:0:0:598:21921:-1876.69,0	1:958:4,954:4:146:954:35062:-3002.8,0
chrM	9477	.	G	A	31596.7	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=944;CIGAR=1X;DP=946;DPB=946;DPRA=0;EPP=58.9901;EPPR=3.0103;GTI=0;LEN=1;MEANALT=1;MQM=59.3178;MQMR=60;NS=2;NUMALT=1;ODDS=2909.29;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=35363;QR=67;RO=2;RPL=521;RPP=25.1023;RPPR=7.35324;RPR=423;RUN=1;SAF=469;SAP=3.09311;SAR=475;SRF=1;SRP=3.0103;SRR=1;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:329:2,327:2:67:327:12108:-1080.66,0	1:617:0,617:0:0:617:23255:-2090.4,0
chrM	9548	.	G	A	23689.1	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=729;CIGAR=1X;DP=730;DPB=730;DPRA=0;EPP=65.6375;EPPR=5.18177;GTI=0;LEN=1;MEANALT=1;MQM=59.7133;MQMR=60;NS=2;NUMALT=1;ODDS=2252;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=26539;QR=38;RO=1;RPL=394;RPP=13.3792;RPPR=5.18177;RPR=335;RUN=1;SAF=339;SAP=10.7579;SAR=390;SRF=1;SRP=5.18177;SRR=0;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:261:1,260:1:38:260:9395:-838.704,0	1:469:0,469:0:0:469:17144:-1542,0
chrM	11467	.	A	G	157655	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=4755;CIGAR=1X;DP=4759;DPB=4759;DPRA=0;EPP=620.69;EPPR=3.0103;GTI=0;LEN=1;MEANALT=1;MQM=59.9394;MQMR=42.5;NS=2;NUMALT=1;ODDS=15848.9;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=179486;QR=151;RO=4;RPL=3558;RPP=2548.64;RPPR=3.0103;RPR=1197;RUN=1;SAF=1995;SAP=270.266;SAR=2760;SRF=2;SRP=3.0103;SRR=2;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:1820:0,1820:0:0:1820:68685:-6177.29,0	1:2939:4,2935:4:151:2935:110801:-9948.16,0
chrM	11719	.	G	A	86257.7	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=2676;CIGAR=1X;DP=2687;DPB=2687;DPRA=0;EPP=15.4873;EPPR=12.6832;GTI=0;LEN=1;MEANALT=1;MQM=59.6039;MQMR=60;NS=2;NUMALT=1;ODDS=6603.9;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=96531;QR=397;RO=11;RPL=1384;RPP=9.87851;RPPR=4.78696;RPR=1292;RUN=1;SAF=1292;SAP=9.87851;SAR=1384;SRF=2;SRP=12.6832;SRR=9;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:714:3,711:3:109:711:25643:-2282.19,0	1:1973:8,1965:8:288:1965:70888:-6347.71,0
chrM	12308	.	A	G	63434.1	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1900;CIGAR=1X;DP=1905;DPB=1905;DPRA=0;EPP=73.302;EPPR=3.44459;GTI=0;LEN=1;MEANALT=1;MQM=59.9621;MQMR=60;NS=2;NUMALT=1;ODDS=5056.51;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=71094;QR=184;RO=5;RPL=1169;RPP=222.265;RPPR=3.44459;RPR=731;RUN=1;SAF=907;SAP=11.463;SAR=993;SRF=3;SRP=3.44459;SRR=2;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:547:5,542:5:184:542:20196:-1799.85,0	1:1358:0,1358:0:0:1358:50898:-4577.25,0
chrM	12372	.	G	A	58077.1	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1737;CIGAR=1X;DP=1741;DPB=1741;DPRA=0;EPP=74.4189;EPPR=5.18177;GTI=0;LEN=1;MEANALT=1;MQM=60;MQMR=60;NS=2;NUMALT=1;ODDS=4910.27;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=64920;QR=149;RO=4;RPL=775;RPP=46.726;RPPR=3.0103;RPR=962;RUN=1;SAF=941;SAP=29.2942;SAR=796;SRF=3;SRP=5.18177;SRR=1;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:539:3,536:3:112:536:19922:-1781.72,0	1:1202:1,1201:1:37:1201:44998:-4043.68,0
chrM	13617	.	T	C	27663.7	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=846;CIGAR=1X;DP=848;DPB=848;DPRA=0;EPP=303.228;EPPR=3.0103;GTI=0;LEN=1;MEANALT=1;MQM=59.8972;MQMR=60;NS=2;NUMALT=1;ODDS=2549.91;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=31932;QR=78;RO=2;RPL=638;RPP=477.603;RPPR=7.35324;RPR=208;RUN=1;SAF=314;SAP=124.993;SAR=532;SRF=1;SRP=3.0103;SRR=1;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:284:0,284:0:0:284:10656:-956.335,0	1:564:2,562:2:78:562:21276:-1906.39,0
chrM	14766	.	C	T	54363.3	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1633;CIGAR=1X;DP=1633;DPB=1633;DPRA=0;EPP=21.2132;EPPR=0;GTI=0;LEN=1;MEANALT=1;MQM=59.9853;MQMR=0;NS=2;NUMALT=1;ODDS=4408.47;PAIRED=1;PAIREDR=0;PAO=0;PQA=0;PQR=0;PRO=0;QA=61054;QR=0;RO=0;RPL=852;RPP=9.71354;RPPR=0;RPR=781;RUN=1;SAF=1113;SAP=470.614;SAR=520;SRF=0;SRP=0;SRR=0;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:473:0,473:0:0:473:17508:-1575.01,0	1:1160:0,1160:0:0:1160:43546:-3916.74,0
chrM	14793	.	A	G	52354.7	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=1605;CIGAR=1X;DP=1605;DPB=1605;DPRA=0;EPP=123.965;EPPR=0;GTI=0;LEN=1;MEANALT=1;MQM=59.9688;MQMR=0;NS=2;NUMALT=1;ODDS=4357.82;PAIRED=1;PAIREDR=0;PAO=0;PQA=0;PQR=0;PRO=0;QA=58638;QR=0;RO=0;RPL=950;RPP=120.75;RPPR=0;RPR=655;RUN=1;SAF=940;SAP=105.327;SAR=665;SRF=0;SRP=0;SRR=0;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:475:0,475:0:0:475:17313:-1557.59,0	1:1130:0,1130:0:0:1130:41325:-3717.26,0
chrM	15301	.	G	A	67202.5	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=2029;CIGAR=1X;DP=2036;DPB=2036;DPRA=0;EPP=73.6971;EPPR=4.45795;GTI=0;LEN=1;MEANALT=1.5;MQM=60;MQMR=60;NS=2;NUMALT=1;ODDS=5288.64;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=75132;QR=224;RO=6;RPL=962;RPP=14.8095;RPPR=3.0103;RPR=1067;RUN=1;SAF=1129;SAP=59.1336;SAR=900;SRF=1;SRP=8.80089;SRR=5;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:563:2,561:2:75:561:20714:-1856.3,0	1:1473:4,1468:4:149:1468:54418:-4880.92,0
chrM	15326	.	A	G	73749.6	.	AB=0;ABP=0;AC=2;AF=1;AN=2;AO=2200;CIGAR=1X;DP=2201;DPB=2201;DPRA=0;EPP=68.7112;EPPR=5.18177;GTI=0;LEN=1;MEANALT=1;MQM=60;MQMR=60;NS=2;NUMALT=1;ODDS=5718.37;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=82190;QR=38;RO=1;RPL=1013;RPP=32.8937;RPPR=5.18177;RPR=1187;RUN=1;SAF=1088;SAP=3.57883;SAR=1112;SRF=0;SRP=5.18177;SRR=1;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:597:1,596:1:38:596:22276:-2000.05,0	1:1604:0,1604:0:0:1604:59914:-5388.94,0

Filtering variants

After filtering the data with stringent input parameters (restricting base quality to a minimum of 30 and mapping quality to a minimum of 20) a considerable amount of variants due to read-alignment bias exists. Erik Garrison has a beautiful illustration of various biases potentially affecting called variants and making a locus sequence-able.

Open image in new tab

A robust tool set for processing VCF data is provided by vcflib developed by Erik Garrison, the author of FreeBayes. One way to filter VCF is using INFO fields of the VCF dataset. If you look at the VCF dataset shown above you will see all comment lines beginning with ##INFO. These are INFO fields. Each VCF record contains a list of INFO tags describing a wide range of properties for each VCF record. You will see that FreeBayes and NVC differ significantly in the number and types of INFO fields each of these caller generates. This why the two require different filtering strategies.

Among numerous types of data generated by FreeBayes let’s consider the following variant properties:

• ##INFO=<ID=DP,Number=1,Type=Integer,Description="Total read depth at the locus"> - This is the number of reads covering a given site.
• ##INFO=<ID=SRP,Number=1,Type=Float,Description="Strand balance probability for the reference allele: Phred-scaled upper-bounds estimate of the probability of observing the deviation between SRF and SRR given E(SRF/SRR) ~ 0.5, derived using Hoeffding's inequality"> - The higher this quantity the better the site as it diminishes the chance of the site having significant strand bias.
• ##INFO=<ID=SAP,Number=A,Type=Float,Description="Strand balance probability for the alternate allele: Phred-scaled upper-bounds estimate of the probability of observing the deviation between SAF and SAR given E(SAF/SAR) ~ 0.5, derived using Hoeffding's inequality"> - The higher this quantity the better the site as it diminishes the chance of the site having significant strand bias (also see this discussion on the freebayes forum).
• ##INFO=<ID=EPP,Number=A,Type=Float,Description="End Placement Probability: Phred-scaled upper-bounds estimate of the probability of observing the deviation between EL and ER given E(EL/ER) ~ 0.5, derived using Hoeffding's inequality"> - The higher this number the lower the chance of having significant placement bias.
• QUAL - phred scaled variant quality.

Hands On: Filtering VCF data

1. Use VCFfilter ( Galaxy version 1.0.0_rc1+galaxy3) to filter the variants with the following parameters:
   • param-file “VCF dataset to filter”: select the VCF dataset produced by FreeBayes tool
   • In “more filters”:
     • In “1: more filters”:
       • “Select the filter type”: Info filter (-f)
       • “Specify filtering value”: SRP > 20
     • Insert more filters:
     • In “2: more filters”:
       • “Select the filter type”: Info filter (-f)
       • “Specify filtering value”: SAP > 20
     • Insert more filters:
     • In “3: more filters”:
       • “Select the filter type”: Info filter (-f)
       • “Specify filtering value”: EPP > 20
     • Insert more filters:
     • In “4: more filters”:
       • “Select the filter type”: Info filter (-f)
       • “Specify filtering value”: QUAL > 20
     • Insert more filters:
     • In “5: more filters”:
       • “Select the filter type”: Info filter (-f)
       • “Specify filtering value”: DP > 20

   Comment: VCF filter options

   Filtering FreeBayes VCF for strand bias (SPR and SAP), placement bias (EPP), variant quality (QUAL), and depth of coverage (DP).

Question

1. How many variants remain after filtering the VCF?

Solution

1. Two variants remain after filtering the VCF (your results might be different depending on the input and references you use):

   #CHROM	POS	ID	REF	ALT	QUAL	FILTER	INFO	FORMAT	raw_child-ds-	raw_mother-ds-
   chrM	3243	.	A	G	10397.4	.	AB=0;ABP=0;AC=1;AF=0.5;AN=2;AO=1365;CIGAR=1X;DP=3092;DPB=3092;DPRA=0;EPP=116.418;EPPR=46.9792;GTI=0;LEN=1;MEANALT=1;MQM=59.956;MQMR=59.8917;NS=2;NUMALT=1;ODDS=2394.09;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=49004;QR=63273;RO=1727;RPL=849;RPP=179.415;RPPR=105.14;RPR=516;RUN=1;SAF=443;SAP=368.01;SAR=922;SRF=637;SRP=261.033;SRR=1090;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	1:1035:341,694:341:12439:694:24871:-1118.32,0	0:2057:1386,671:1386:50834:671:24133:0,-2399.65
   chrM	5539	.	A	G	3281.62	.	AB=0;ABP=0;AC=1;AF=0.5;AN=2;AO=379;CIGAR=1X;DP=787;DPB=787;DPRA=0;EPP=216.428;EPPR=224.5;GTI=0;LEN=1;MEANALT=1;MQM=54.1504;MQMR=53.777;NS=2;NUMALT=1;ODDS=755.62;PAIRED=1;PAIREDR=1;PAO=0;PQA=0;PQR=0;PRO=0;QA=13803;QR=15250;RO=408;RPL=74;RPP=308.741;RPPR=351.808;RPR=305;RUN=1;SAF=286;SAP=216.428;SAR=93;SRF=318;SRP=279.681;SRR=90;TYPE=snp;technology.ILLUMINA=1	GT:DP:AD:RO:QR:AO:QA:GL	0:299:221,78:221:8252:78:2824:0,-485.016	1:488:187,301:187:6998:301:10979:-358.012,0
   

Examining the results

For visualizing VCFs Galaxy has two external tool options. The first is called VCF.IOBIO developed by Gabor Marth’s group at the University of Utah. The second is called IGV developed by Broad Institute.

Visualising with VCF.IOBIO

VCF.IOBIO can be invoked by expanding a VCF dataset in Galaxy’s history by clicking on it:

Hands On: Display data in VCF.IOBIO

Open image in new tab

Open image in new tab

Visualising with IGV

Similarly to VCF.IOBIO expanding a history item representing a VCF dataset will reveal an IGV link:

Hands On: Display data in IGV

Open image in new tab

The difference between ‘local’ and ‘Human hg38’ links is explained in the following video:

Visualizing our FreeBayes dataset will produce this:

Open image in new tab

Comparing frequencies

Visualizing VCF datasets is a good way to get an overall idea of the data, but it does not tell a lot of details. For example, above we have visualized site 3243 using IGV. It is interesting but we need to find out more. One thing we can do is to convert VCF dataset into a tab-delimited representation and with it play a bit more.

Hands On: Convert VCF to tab-delimited data

1. Use VCFtoTab-delimited ( Galaxy version 1.0.0_rc1+galaxy0) to filter the variants with the following parameters:
   • param-file “Select VCF dataset to convert”: select the VCF dataset produced by VCFfilter tool
   • “Report data per sample”: Yes
   • “Fill empty fields with”: Nothing

Question

1. Why are there four rows in the VCFtoTab-delimited tool output when the input VCF had only two rows?
2. How many columns are in the VCFtoTab-delimited tool output?

Solution

1. Since “Report data per sample” was set to Yes, VCFtoTab-delimited tool produced two rows for each of the two variants, one row per sample (child and mother).
2. There are 62 (!) columns in the output of VCFtoTab-delimited tool.

Open image in new tab

Let’s restrict ourselves to a few key columns:

• 2 POS - position along mitochondrial genome
• 4 REF - reference allele
• 5 ALT - alternative allele
• 52 SAMPLE - name of the sample
• 54 AO - number of alternative observations (how many times do we see the alternative allele at this position in this sample)
• 55 DP - depth of coverage at this site for this sample

Hands On: Cut columns from a file

1. Use Cut columns from a table to select specific columns with the following parameters:
   • “Cut columns”: c2,c4,c5,c52,c54,c55
   • “Delimited by”: Tab
   • param-file “From”: select the tabular dataset produced by VCFtoTab-delimited tool

Running Cut will generate the following dataset:

POS  REF ALT     SAMPLE       AO    DP
--------------------------------------
3243	A	G	raw_child-ds-	694	1035
3243	A	G	raw_mother-ds-	671	2057
5539	A	G	raw_child-ds-	78	299
5539	A	G	raw_mother-ds-	301	488

Let’s look at position 3243. At this site, the mother sample has 671 Gs (since G is the alternative allele) and 2057-671=1386 As. The child sample has 694 Gs and 1035-694=341 As:

Allele     A     G
-------------------
Mother  1386   691
Child   341    694

Question

1. What do you notice about the relative frequencies of the A and G alleles between mother and child?

Solution

1. The major allele in the mother (A) becomes the minor allele in the child – a remarkable frequency change due to mitochondrial bottleneck!

Conclusion

This entire analysis is available as a Galaxy history that you can import into your Galaxy account and play with.

Now you know how to call variants in non-diploid system, so try it on bacteria, viruses, etc.

You've Finished the Tutorial

Please also consider filling out the Feedback Form as well!

Key points

• Variation in human mitochondria is a proxy for other haploid systems.

• Nucleotide variants in haploid systems may have any frequency between 0 and 1.

• Distinguishing true variants from noise is not easy and requires accounting
  for strand bias and read placement bias.

• FreeBayes can be effectively used to call variants in haploid systems.

Frequently Asked Questions

• Tutorial FAQs
• Topic FAQs
• Galaxy FAQs
• GTN Matrix Chat
• Galaxy Help Forum

Useful literature

Further information, including links to documentation and original publications, regarding the tools, analysis techniques and the interpretation of results described in this tutorial can be found here.

References

1. Kanagawa, T., 2003 Bias and artifacts in multitemplate polymerase chain reactions (PCR). Journal of Bioscience and Bioengineering 96: 317–323. https://doi.org/10.1016/S1389-1723(03)90130-7 http://www.sciencedirect.com/science/article/pii/S1389172303901307
2. Cree, L. M., D. C. Samuels, S. C. de Sousa Lopes, H. K. Rajasimha, P. Wonnapinij et al., 2008 A reduction of mitochondrial DNA molecules during embryogenesis explains the rapid segregation of genotypes. Nature Genetics 40: 249–254. 10.1038/ng.2007.63
3. Li, H., 2013 Aligning sequence reads, clone sequences and assembly contigs with BWA-MEM.
4. Rebolledo-Jaramillo, B., M. S.-W. Su, N. Stoler, J. A. McElhoe, B. Dickins et al., 2014 Maternal age effect and severe germ-line bottleneck in the inheritance of human mitochondrial DNA. Proceedings of the National Academy of Sciences 111: 15474–15479. 10.1073/pnas.1409328111 https://www.pnas.org/content/111/43/15474
5. Li, W., J. Köster, H. Xu, C.-H. Chen, T. Xiao et al., 2015 Quality control, modeling, and visualization of CRISPR screens with MAGeCK-VISPR. 16: 10.1186/s13059-015-0843-6
6. Olson, N. D., S. P. Lund, R. E. Colman, J. T. Foster, J. W. Sahl et al., 2015 Best practices for evaluating single nucleotide variant calling methods for microbial genomics. Frontiers in Genetics 6: 235. 10.3389/fgene.2015.00235
7. Tan, A., G. R. Abecasis, and H. M. Kang, 2015 Unified representation of genetic variants. Bioinformatics 31: 2202–2204. 10.1093/bioinformatics/btv112

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Citing this Tutorial

1. Anton Nekrutenko, Alex Ostrovsky, Calling variants in non-diploid systems (Galaxy Training Materials). https://training.galaxyproject.org/training-material/topics/variant-analysis/tutorials/non-dip/tutorial.html Online; accessed TODAY
2. Hiltemann, Saskia, Rasche, Helena et al., 2023 Galaxy Training: A Powerful Framework for Teaching! PLOS Computational Biology 10.1371/journal.pcbi.1010752
3. Batut et al., 2018 Community-Driven Data Analysis Training for Biology Cell Systems 10.1016/j.cels.2018.05.012

BibTeX

@misc{variant-analysis-non-dip,
author = "Anton Nekrutenko and Alex Ostrovsky",
	title = "Calling variants in non-diploid systems (Galaxy Training Materials)",
	year = "",
	month = "",
	day = "",
	url = "\url{https://training.galaxyproject.org/training-material/topics/variant-analysis/tutorials/non-dip/tutorial.html}",
	note = "[Online; accessed TODAY]"
}
@article{Hiltemann_2023,
	doi = {10.1371/journal.pcbi.1010752},
	url = {https://doi.org/10.1371%2Fjournal.pcbi.1010752},
	year = 2023,
	month = {jan},
	publisher = {Public Library of Science ({PLoS})},
	volume = {19},
	number = {1},
	pages = {e1010752},
	author = {Saskia Hiltemann and Helena Rasche and Simon Gladman and Hans-Rudolf Hotz and Delphine Larivi{\`{e}}re and Daniel Blankenberg and Pratik D. Jagtap and Thomas Wollmann and Anthony Bretaudeau and Nadia Gou{\'{e}} and Timothy J. Griffin and Coline Royaux and Yvan Le Bras and Subina Mehta and Anna Syme and Frederik Coppens and Bert Droesbeke and Nicola Soranzo and Wendi Bacon and Fotis Psomopoulos and Crist{\'{o}}bal Gallardo-Alba and John Davis and Melanie Christine Föll and Matthias Fahrner and Maria A. Doyle and Beatriz Serrano-Solano and Anne Claire Fouilloux and Peter van Heusden and Wolfgang Maier and Dave Clements and Florian Heyl and Björn Grüning and B{\'{e}}r{\'{e}}nice Batut and},
	editor = {Francis Ouellette},
	title = {Galaxy Training: A powerful framework for teaching!},
	journal = {PLoS Comput Biol}
}

                   

Galaxy Administrators: Install the missing tools

You can use Ephemeris's shed-tools install command to install the tools used in this tutorial.

shed-tools install [-g GALAXY] [-a API_KEY] -t <(curl https://training.galaxyproject.org/training-material/api/topics/variant-analysis/tutorials/non-dip/tutorial.json | jq .admin_install_yaml -r)

Alternatively you can copy and paste the following YAML

---
install_tool_dependencies: true
install_repository_dependencies: true
install_resolver_dependencies: true
tools:
- name: bamtools_filter
  owner: devteam
  revisions: cb20f99fd45b
  tool_panel_section_label: SAM/BAM
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: bwa
  owner: devteam
  revisions: 3fe632431b68
  tool_panel_section_label: Mapping
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: fastqc
  owner: devteam
  revisions: e7b2202befea
  tool_panel_section_label: FASTA/FASTQ
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: freebayes
  owner: devteam
  revisions: 156b60c1530f
  tool_panel_section_label: Variant Calling
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: freebayes
  owner: devteam
  revisions: 57def2d7c093
  tool_panel_section_label: Variant Calling
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: freebayes
  owner: devteam
  revisions: 156b60c1530f
  tool_panel_section_label: Variant Calling
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: freebayes
  owner: devteam
  revisions: ef2c525bd8cd
  tool_panel_section_label: Variant Calling
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: picard
  owner: devteam
  revisions: a1f0b3f4b781
  tool_panel_section_label: Picard
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: picard
  owner: devteam
  revisions: f9242e01365a
  tool_panel_section_label: Picard
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: vcf2tsv
  owner: devteam
  revisions: e92b3c0f9224
  tool_panel_section_label: Variant Calling
  tool_shed_url: https://toolshed.g2.bx.psu.edu/
- name: vcffilter
  owner: devteam
  revisions: 81972652519c
  tool_panel_section_label: Variant Calling
  tool_shed_url: https://toolshed.g2.bx.psu.edu/

Feedback

t{ hist[0] | to_stars }}	1
t{ hist[0] | to_stars }}	1
t{ hist[0] | to_stars }}	1
t{ hist[0] | to_stars }}	1

November 2018

• 2 stars: Liked: I like the idea Disliked: After running the FreeBayes I ended up with 2 variants instead of 30. And so got stuck there. Also it's not clear why the filtering and subsequent steps would be done on the markduplicates output, rather than the left align output. Why do the leftalign if we don't use that output again? I did both and got the same results. Overall I am finding the galaxy experience to be rather frustrating. I'm trying to decide whether to incorporate these tutorials in my class, but often I can't find the necessary input data, get unexplained errors, or get output different from the tutorial