Explore Workflows

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

Graph Name Retrieved From View
workflow graph prep.cwl

https://git.astron.nl/RD/LINC.git

Path: workflows/linc_target/prep.cwl

Branch/Commit ID: dc7a4f725f6e8dde49b0b1db2e3fbde7fb19990a
workflow graph group-isoforms-batch.cwl

Workflow runs group-isoforms.cwl tool using scatter for isoforms_file input. genes_filename and common_tss_filename inputs are ignored.

https://github.com/Barski-lab/workflows.git

Path: tools/group-isoforms-batch.cwl

Branch/Commit ID: b8e28a017f7b1a2900ec0fd3b3549f123f0c91b4
workflow graph Landsat-8 pan-sharpening

Landsat-8 pan-sharpening

 https://github.com/cwl-for-eo/cwl-101.git

Path: tutorial-3/pan-sharpen.cwl

Branch/Commit ID: f41de311c6c77def3923f7a23f09b2dff46670af

Packed ID: main
workflow graph mut3.cwl

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

Path: tests/wf/mut3.cwl

Branch/Commit ID: a21728aa0e2dd0ffc1be39fdbf9bc76029e90c66
workflow graph Perform camera calibration

Camera calibration data (from telescope-level calibration events) will be recorded alongside science data during and around each observation night by ACADA. Different calibration event types will be recorded to the different streams at this stage. Interleaved flat-field and sky pedestal events are tagged at the telescope level, allowing the data to directly align with the functional decomposition of the CalibPipe and avoid the need of additional event-type filtering. Following this, pixel- and channel-wise camera calibration coefficients are calculated as a function of time. This process includes the computation of aggregated time-series statistics for the calibration events, as well as the detection of non-nominal pixels and time periods (UC-120-2.21). The aggregated statistics are further processed to derive the sky pedestal offsets per waveform sample, flat-fielding coefficients, and pixel timing corrections. Additionally, the CalibPipe calculates the absolute gain for each pixel and gain channel as a function of time. This process will ultimately yield a multiplicative coefficient for the absolute calibration of extracted charge into photoelectrons. To achieve accurate absolute gain and charge calibration, CalibPipe derives telescope-specific systematic corrections (UC-120-2.22) and the conversion factors from digital counts to single photoelectrons (UC-120-2.23).

https://gitlab.cta-observatory.org/cta-computing/dpps/calibrationpipeline/calibpipe.git

Path: workflows/telescope/camera/uc-120-2.20-perform-camera-calibration.cwl

Branch/Commit ID: rc-1.0
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: e413f9b185f0060ffbdd876062133d65daecb7da
workflow graph revsort.cwl

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: 526f36f93655bfb098f766ff020708b5a707513a
workflow graph stdout-wf_v1_2.cwl

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

Path: testdata/stdout-wf_v1_2.cwl

Branch/Commit ID: e413f9b185f0060ffbdd876062133d65daecb7da
workflow graph umi molecular alignment fastq workflow

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

Path: definitions/pipelines/alignment_umi_molecular.cwl

Branch/Commit ID: b9e7392e72506cadd898a6ac4db330baf6535ab6
workflow graph fastq_processing_workflow.cwl

https://github.com/NCI-GDC/gdc-rnaseq-cwl.git

Path: rnaseq-star-align/subworkflows/preprocessing/fastq_processing_workflow.cwl

Branch/Commit ID: 81605548d21d346bce82272dcc00ff456db7ef19