Explore Workflows

https://github.com/common-workflow-language/cwl-v1.1.git

Path: tests/record-output-wf.cwl

Branch/Commit ID: 86c46cb397de029e4c91f02cca40fa2b54d22f37

https://github.com/ncbi/pgap.git

Path: task_types/tt_hmmsearch_wnode.cwl

Branch/Commit ID: 1c1f5aa0b0dfe5b07beb8ccb0c0e3c073a9fb592

https://github.com/alpha-unito/Sogei-DevOps-pipeline.git

Path: unito-pipeline/cwl/main-unito.cwl

Branch/Commit ID: d2c960fe089bfe32238cbd6be4961df18b9274a4

Reverse the lines in a document, then sort those lines.

https://github.com/common-workflow-language/cwltool.git

Path: tests/wf/revsort.cwl

Branch/Commit ID: 766d58b47180d92618074679eb9f3c6c30acf638

https://github.com/common-workflow-language/cwl-utils.git

Path: testdata/record-output-wf_v1_0.cwl

Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93

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.

https://github.com/burmist-git/076_cwl.git

Path: uc-120-2.2-optical-throughput-calibration-with-muons.cwl

Branch/Commit ID: a03a36e43b30ada0242d3a67b3e1ad908249acb1

https://github.com/common-workflow-language/cwltool.git

Path: tests/wf/sec-wf-out.cwl

Branch/Commit ID: a8d8d00fd1e4274e1bc16001937db5aae46b0b0d

https://github.com/genome/analysis-workflows.git

Path: qc/workflow_exome.cwl

Branch/Commit ID: d1ee6a2a323cee7e4af00c7e0b926c2192038e1d

https://github.com/genome/analysis-workflows.git

Path: definitions/subworkflows/qc_wgs.cwl

Branch/Commit ID: c235dc6d623879a6c4f5fb307f545c9806eb2d23

https://github.com/CompEpigen/PipelineOlympics.git

Path: CWL/workflows/BAT/BAT_workflow.cwl

Branch/Commit ID: 72ad937a444b6603983f19595ba4a3434557e006