Explore Workflows
View already parsed workflows here or click here to add your own
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maw_single.cwl
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Path: cwl/maw_single.cwl Branch/Commit ID: a8b2df3f3918ee400b236c49b34092959293b41b |
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phase VCF
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Path: definitions/subworkflows/phase_vcf.cwl Branch/Commit ID: low-vaf |
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QIIME2 Step 2 (DADA2 option)
QIIME2 DADA2, feature summaries, phylogenetic diversity tree, taxonomic analysis and ancom |
Path: packed/qiime2-step2-dada2-paired.cwl Branch/Commit ID: qiime2-workflow-paired Packed ID: main |
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QIIME2 Step 3
QIIME2 Alpha/beta diversity analysis and Alpha rarefaction plotting |
Path: packed/qiime2-step3-alpha-analysis.cwl Branch/Commit ID: qiime2-workflow Packed ID: main |
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Variant calling workflow for given interval
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Path: WGS-processing/cwl/helper/gatk-wf-with-interval.cwl Branch/Commit ID: main |
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js-expr-req-wf.cwl#wf
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Path: tests/js-expr-req-wf.cwl Branch/Commit ID: master Packed ID: wf |
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bulk scRNA-seq pipeline using Salmon
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Path: bulk-pipeline.cwl Branch/Commit ID: 1af8809 |
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Assess the statistical description of calibration events
When DPPS receives a new DL0 data product, the CalibPipe is triggered to process the calibration events. The CalibPipe performs charge integration and peak time extraction for the entire set of calibration events, and computes aggregated time-series statistics, including the mean, median, and standard deviation. Using these aggregated statistics, the CalibPipe identifies faulty camera pixels, such as those affected by starlight, by applying various outlier detection criteria. Time periods with a significant number of faulty pixels, exceeding a predefined threshold, are flagged as invalid. A refined treatment can then be applied to these time periods to account for the issues. |
Path: workflows/telescope/camera/uc-120-2.21-assess-statistical-description.cwl Branch/Commit ID: rc-1.0 |
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CODEX analysis pipeline using Cytokit
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Path: steps/ometiff_second_stitching.cwl Branch/Commit ID: no-gpu-for-cwl-vis-only |
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Exome QC workflow
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Path: definitions/subworkflows/qc_exome.cwl Branch/Commit ID: master |
