Explore Workflows
View already parsed workflows here or click here to add your own
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scatter-wf3.cwl#main
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Path: cwltool/schemas/v1.0/v1.0/scatter-wf3.cwl Branch/Commit ID: 7ec307b01442936fad9b1149f4500496557505ff Packed ID: main |
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scatter-wf4.cwl#main
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Path: tests/wf/scatter-wf4.cwl Branch/Commit ID: 0184e647cde1bc44279107d6df31b3ebb138769c Packed ID: main |
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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: eb6a98289850791cd1891c89e5209180c35c7858 |
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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: eb6a98289850791cd1891c89e5209180c35c7858 |
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scatter-wf3_v1_2.cwl#main
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Path: testdata/scatter-wf3_v1_2.cwl Branch/Commit ID: 0ab1d42d10f7311bb4032956c4a6f3d2730d9507 Packed ID: main |
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Seed Protein Alignments
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Path: protein_alignment/wf_seed_seqids.cwl Branch/Commit ID: 2afb5ebafd1353ba063cc74ee9a7eaf347afce5c |
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search.cwl#main
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Path: tests/search.cwl Branch/Commit ID: 1f3ef888d9ef2306c828065c460c1800604f0de4 Packed ID: main |
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js-expr-req-wf.cwl#wf
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Path: cwltool/schemas/v1.0/v1.0/js-expr-req-wf.cwl Branch/Commit ID: 7ec307b01442936fad9b1149f4500496557505ff Packed ID: wf |
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Create Genomic Collection for Bacterial Pipeline
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Path: genomic_source/wf_genomic_source.cwl Branch/Commit ID: 8ea3637b0f11eac1ea5599c41d74e00d85fb778d |
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RNA-Seq pipeline paired-end strand specific
The original [BioWardrobe's](https://biowardrobe.com) [PubMed ID:26248465](https://www.ncbi.nlm.nih.gov/pubmed/26248465) **RNA-Seq** basic analysis for a **paired-end** experiment. A corresponded input [FASTQ](http://maq.sourceforge.net/fastq.shtml) file has to be provided. Current workflow should be used only with the paired-end RNA-Seq data. It performs the following steps: 1. Use STAR to align reads from input FASTQ files according to the predefined reference indices; generate unsorted BAM file and alignment statistics file 2. Use fastx_quality_stats to analyze input FASTQ files and generate quality statistics files 3. Use samtools sort to generate coordinate sorted BAM(+BAI) file pair from the unsorted BAM file obtained on the step 1 (after running STAR) 4. Generate BigWig file on the base of sorted BAM file 5. Map input FASTQ files to predefined rRNA reference indices using Bowtie to define the level of rRNA contamination; export resulted statistics to file 6. 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-pe-dutp.cwl Branch/Commit ID: 4a80f5b8f86c83af39494ecc309b789aeda77964 |
