Explore Workflows
View already parsed workflows here or click here to add your own
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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 |
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tt_hmmsearch_wnode.cwl
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Path: task_types/tt_hmmsearch_wnode.cwl Branch/Commit ID: 45d134ce3d436c53637a2d83755e9b4613267e9f |
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kmer_seq_entry_extract_wnode
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Path: task_types/tt_kmer_seq_entry_extract_wnode.cwl Branch/Commit ID: 6d5e27ee7c01effb14c40619df9c4f6d321a25bf |
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tinyrna_wf.cwl
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Path: tiny/cwl/workflows/tinyrna_wf.cwl Branch/Commit ID: 943cb16fc421f0a37df3619086cbd0330c78174e |
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kmer_cache_retrieve
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Path: task_types/tt_kmer_cache_retrieve.cwl Branch/Commit ID: 6d5e27ee7c01effb14c40619df9c4f6d321a25bf |
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concatenate-flag.cwl
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Path: workflows/concatenate-flag.cwl Branch/Commit ID: a5a91f3bee1603874715f612adc3f56cc64e55f3 |
