Explore Workflows
View already parsed workflows here or click here to add your own
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SSU-from-tablehits.cwl
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Path: tools/SSU-from-tablehits.cwl Branch/Commit ID: 2104dc3 |
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main-wes_chr21_test.cwl
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Path: wes-agha-test/wes_chr21_test-workflow-gcp/main-wes_chr21_test.cwl Branch/Commit ID: master |
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wf_get_reproducible_eclip_peaks.cwl
The main workflow that produces two reproducible peaks via IDR given two eCLIP samples (1 input, 1 IP each). |
Path: cwl/wf_get_reproducible_eclip_peaks.cwl Branch/Commit ID: master |
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predict_tx_features_workflow.cwl
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Path: cwl/predict_tx_features_workflow.cwl Branch/Commit ID: master |
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examplePipeline.cwl
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Path: HCK01_2022_Virtual/Tutorials/GetYourBrainPipelined/CWL-Demo/examplePipeline.cwl Branch/Commit ID: main |
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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-optical-throughput-calibration-with-muons.cwl Branch/Commit ID: master |
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make_search_pair_workflow.cwl
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Path: make_search_pair_workflow.cwl Branch/Commit ID: master |
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RNASelector as a CWL workflow
https://doi.org/10.1007/s12275-011-1213-z |
Path: workflows/rna-selector.cwl Branch/Commit ID: master |
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GRO_run.cwl
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Path: test_workflow_notables_clean/workflow/GRO_run.cwl Branch/Commit ID: master |
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REGENIE workflow
REGENIE workflow |
Path: cwl/regenie_workflow.cwl Branch/Commit ID: master |
