Explore Workflows
View already parsed workflows here or click here to add your own
Graph | Name | Retrieved From | View |
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schemadef-wf.cwl
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![]() Path: tests/schemadef-wf.cwl Branch/Commit ID: 5f27e234b4ca88ed1280dedf9e3391a01de12912 |
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cache_asnb_entries
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![]() Path: task_types/tt_cache_asnb_entries.cwl Branch/Commit ID: 7b5130d2408bce82ee15c666b37d931ef6f452e3 |
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01-qc-se.cwl
ChIP-seq 01 QC - reads: SE |
![]() Path: v1.0/ChIP-seq_pipeline/01-qc-se.cwl Branch/Commit ID: 33385c6a820a9d4d18cff6fc3a533ec8e3c11c6e |
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RNA-Seq pipeline single-read stranded mitochondrial
Slightly changed original [BioWardrobe's](https://biowardrobe.com) [PubMed ID:26248465](https://www.ncbi.nlm.nih.gov/pubmed/26248465) **RNA-Seq** basic analysis for **strand specific single-read** experiment. An additional steps were added to map data to mitochondrial chromosome only and then merge the output. Experiment files in [FASTQ](http://maq.sourceforge.net/fastq.shtml) format either compressed or not can be used. Current workflow should be used only with single-read strand specific RNA-Seq data. It performs the following steps: 1. `STAR` to align reads from input FASTQ file according to the predefined reference indices; generate unsorted BAM file and alignment statistics file 2. `fastx_quality_stats` to analyze input FASTQ file and generate quality statistics file 3. `samtools sort` to generate coordinate sorted BAM(+BAI) file pair from the unsorted BAM file obtained on the step 1 (after running STAR) 5. Generate BigWig file on the base of sorted BAM file 6. Map input FASTQ file to predefined rRNA reference indices using Bowtie to define the level of rRNA contamination; export resulted statistics to file 7. Calculate isoform expression level for the sorted BAM file and GTF/TAB annotation file using `GEEP` reads-counting utility; export results to file |
![]() Path: workflows/rnaseq-se-dutp-mitochondrial.cwl Branch/Commit ID: bfa3843bcf36125ff258d6314f64b41336f06e6b |
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Telescope Calibration
This workflow performs telescope calibrations and provides camera calibrations, psfs and optical throughputs. |
![]() Path: workflows/calibpipe/TelescopeCalibrations/uc-cp-200.cwl Branch/Commit ID: 76f7c25c0472da23b7e0bfe9f2c18ab6bc369c9d |
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Seed Search Compartments
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![]() Path: protein_alignment/wf_seed.cwl Branch/Commit ID: 91181df8d9ef8eed9d8f40db707b9a4376fecaf5 |
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umi per-lane alignment subworkflow
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![]() Path: definitions/subworkflows/umi_alignment.cwl Branch/Commit ID: d2c2f2eb846ae2e9cdcab46e3bb88e42126cb3f5 |
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Filter Protein Seeds; Find ProSplign Alignments
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![]() Path: protein_alignment/wf_compart_filter_prosplign.cwl Branch/Commit ID: 91181df8d9ef8eed9d8f40db707b9a4376fecaf5 |
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revsort-single-no-docker.cwl
Reverse the lines in a document, then sort those lines. |
![]() Path: input-data/revsort-single-no-docker.cwl Branch/Commit ID: b9e4ce1b42021dec90b645e924eb698261c630ed |
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Atmopsheric Calibration
This workflow performs calibrates atmosphere and produces an atmospheric model and an extinction hypercube. |
![]() Path: workflows/calibpipe/AtmosphericCalibrations/uc-cp-100.cwl Branch/Commit ID: 76f7c25c0472da23b7e0bfe9f2c18ab6bc369c9d |