Explore Workflows
View already parsed workflows here or click here to add your own
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rest_parallel.cwl
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Path: Decentralized-FL/CWL_Workflow/rest_parallel.cwl Branch/Commit ID: master |
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step_valuefrom5_wf_with_id_v1_2.cwl
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Path: testdata/step_valuefrom5_wf_with_id_v1_2.cwl Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93 |
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rnaseq-se-dutp.cwl
Runs RNA-Seq dUTP BioWardrobe basic analysis with strand specific single-end data file. |
Path: workflows/rnaseq-se-dutp.cwl Branch/Commit ID: master |
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calculate_contamination_workflow.cwl
GATK4.1.2 Calculate tumor-normal contamination workflow |
Path: subworkflows/calculate_contamination_workflow.cwl Branch/Commit ID: master |
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workflow_input_sf_expr_array.cwl
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Path: testdata/workflow_input_sf_expr_array.cwl Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93 |
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cnv_gridss
CNV GRIDSS calling |
Path: structuralvariants/cwl/subworkflows/cnv_gridss.cwl Branch/Commit ID: 1.0.5 |
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Rapthor imaging subworkflow
This subworkflow performs imaging with direction-dependent corrections. The imaging data are generated (and averaged if possible) and WSClean is used to perform the imaging. Masking and sky model filtering is then done using PyBDSF. |
Path: rapthor_use_case/rapthor-subworkflows-cwl/image_4/subpipeline_parset.cwl Branch/Commit ID: 1b7bcb6e4b5ab4608d74fa36249a2b6644fc4e9a |
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Rapthor imaging workflow
This workflow performs imaging with direction-dependent corrections. The imaging data are generated (and averaged if possible) and WSClean is used to perform the imaging. Masking and sky model filtering is then done using PyBDSF. |
Path: rapthor_use_case/rapthor-subworkflows-cwl/image_4/main.cwl Branch/Commit ID: 1b7bcb6e4b5ab4608d74fa36249a2b6644fc4e9a |
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Rapthor DD calibration workflow
This workflow performs direction-dependent calibration. In general, calibration is done in three steps: (1) a fast phase-only calibration (with core stations constrianed to have the same solutions) to correct for ionospheric effects, (2) a joint slow amplitude calibration (with all stations constrained to have the same solutions) to correct for beam errors, and (3) a further unconstrained slow gain calibration to correct for station-to-station differences. Steps (2) and (3) are skipped if the calibration is phase-only. This calibration scheme works for both HBA and LBA data. The final products of this workflow are solution tables (h5parm files) and plots. |
Path: rapthor_use_case/rapthor-subworkflows-cwl/calibrate_4/main.cwl Branch/Commit ID: 1b7bcb6e4b5ab4608d74fa36249a2b6644fc4e9a |
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pipeline.cwl
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Path: pipeline.cwl Branch/Commit ID: ba1f3f9e0dd74d4f50358f5c95f1d5a3d28e02ae |
