Explore Workflows

View already parsed workflows here or click here to add your own

Graph Name Retrieved From View
workflow graph workflow_input_sf_expr_v1_2.cwl

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

Path: testdata/workflow_input_sf_expr_v1_2.cwl

Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93

workflow graph step_valuefrom5_wf_with_id_v1_2.cwl

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

Path: testdata/step_valuefrom5_wf_with_id_v1_2.cwl

Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93

workflow graph workflow_input_sf_expr_array.cwl

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

Path: testdata/workflow_input_sf_expr_array.cwl

Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93

workflow graph 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.

https://github.com/Bonadux/cwl-workflows-demo.git

Path: rapthor_use_case/rapthor-subworkflows-cwl/image_4/subpipeline_parset.cwl

Branch/Commit ID: 1b7bcb6e4b5ab4608d74fa36249a2b6644fc4e9a

workflow graph 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.

https://github.com/Bonadux/cwl-workflows-demo.git

Path: rapthor_use_case/rapthor-subworkflows-cwl/image_4/main.cwl

Branch/Commit ID: 1b7bcb6e4b5ab4608d74fa36249a2b6644fc4e9a

workflow graph 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.

https://github.com/Bonadux/cwl-workflows-demo.git

Path: rapthor_use_case/rapthor-subworkflows-cwl/calibrate_4/main.cwl

Branch/Commit ID: 1b7bcb6e4b5ab4608d74fa36249a2b6644fc4e9a

workflow graph pipeline.cwl

https://github.com/hubmapconsortium/hra-workflows.git

Path: pipeline.cwl

Branch/Commit ID: ba1f3f9e0dd74d4f50358f5c95f1d5a3d28e02ae

workflow graph cond-single-source-wf-005.1.cwl

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

Path: testdata/cond-single-source-wf-005.1.cwl

Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93

workflow graph md5sum.cwl

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

Path: testdata/md5sum.cwl

Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93

workflow graph 816_wf.cwl

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

Path: tests/wf/816_wf.cwl

Branch/Commit ID: 766d58b47180d92618074679eb9f3c6c30acf638