Explore Workflows

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

Path: definitions/subworkflows/strelka_and_post_processing.cwl

Branch/Commit ID: master

https://github.com/eosc-lofar/presto-cwl.git

Path: presto.cwl

Branch/Commit ID: visualise

https://github.com/apaul7/cancer-genomics-workflow.git

Path: definitions/pipelines/bisulfite.cwl

Branch/Commit ID: low-vaf

https://github.com/andurill/ACCESS-Pipeline.git

Path: workflows/marianas/collapsed_fastq_to_bam.cwl

Branch/Commit ID: 0.0.33_dmp

This demonstrates how to wrap a \"real\" tool with a checker workflow that runs both the tool and a tool that performs verification of results

https://github.com/dockstore-testing/md5sum-checker.git

Path: checker-workflow-wrapping-tool.cwl

Branch/Commit ID: develop

https://github.com/RenskeW/cwlprov-provenance.git

Path: prov_data_annotations/example2/wf.cwl

Branch/Commit ID: main

https://git.wur.nl/unlock/cwl.git

Path: cwl/workflows/workflow_demultiplexing.cwl

Branch/Commit ID: master

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

Path: progs/protein_extract.cwl

Branch/Commit ID: test

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-optical-throughput-calibration-with-muons.cwl

Branch/Commit ID: master

https://github.com/MgCoders/of-public.git

Path: 1st-workflow-generated.cwl

Branch/Commit ID: master