Explore Workflows
View already parsed workflows here or click here to add your own
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assemble.cwl
Assemble a set of reads using SKESA |
Path: assemble.cwl Branch/Commit ID: 96dbb414d287f4382e2d477fb1851aeaa5f14f2b |
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Seed Search Compartments
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Path: protein_alignment/wf_seed.cwl Branch/Commit ID: 70f86830b73f7a5de9a234f05d17f8a75af62395 |
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Workflow to run pVACseq from detect_variants and rnaseq pipeline outputs
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Path: definitions/pipelines/pvacseq.cwl Branch/Commit ID: 891c996dbd23d8154ec7609a56da3de841ae124c |
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extract_gencoll_ids
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Path: task_types/tt_extract_gencoll_ids.cwl Branch/Commit ID: 89839cdb0a3216024f5f97af5581ae9753de0496 |
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tt_kmer_compare_wnode
Pairwise comparison |
Path: task_types/tt_kmer_compare_wnode.cwl Branch/Commit ID: 6d5e27ee7c01effb14c40619df9c4f6d321a25bf |
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revsort.cwl
Reverse the lines in a document, then sort those lines. |
Path: tests/wf/revsort.cwl Branch/Commit ID: 58274ef14adbbf7e09dbf6e5170780179669078b |
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CLE gold vcf evaluation workflow
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Path: definitions/subworkflows/vcf_eval_cle_gold.cwl Branch/Commit ID: da335d9963418f7bedd84cb2791a0df1b3165ffe |
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integrity.cwl
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Path: workflows/bamfastq_align/integrity.cwl Branch/Commit ID: f34d3963b33e0a379338cb3cb75b0016f012bf2c |
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Optical throughput measurements via muon ring analysis
Upon receiving a new DL0 data product (from either Monte Carlo simulations or observations), DPPS triggers the CalibPipe (ctapipe-process) to process the data using ctapipe, extracting the signal charges and reconstructing muon parameters. The second step involves using the CalibPipe tool to estimate the telescope’s optical throughput using a predefined number of muon events. |
Path: uc-120-2.2-optical-throughput-calibration-with-muons.cwl Branch/Commit ID: a9d49ac23a6e14f475e277ef11f54f40124ab1ef |
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scatter-wf4.cwl#main
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Path: tests/wf/scatter-wf4.cwl Branch/Commit ID: f8f24046875aa90764cf54736df926363aa326d1 Packed ID: main |
