Explore Workflows
View already parsed workflows here or click here to add your own
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stage_data_workflow.vcf_to_aliquot_maf.cwl
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Path: vcf-to-aliquot-maf/subworkflows/stage_data_workflow.vcf_to_aliquot_maf.cwl Branch/Commit ID: main |
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emblem_textures.cwl
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Path: textures/emblem_textures.cwl Branch/Commit ID: cwl |
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RNA-Seq alignment and transcript/gene abundance workflow
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Path: definitions/pipelines/rnaseq.cwl Branch/Commit ID: low-vaf |
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umi molecular alignment workflow
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Path: definitions/subworkflows/molecular_alignment.cwl Branch/Commit ID: low-vaf |
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bacterial_orthology
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Path: bacterial_orthology/wf_bacterial_orthology.cwl Branch/Commit ID: test |
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abc_step01
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Path: abc_enhancer_gene_prediction/abc-enchancer-gene-prediction-wf.cwl.steps/abc_step01.cwl Branch/Commit ID: main |
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func_summaries.cwl
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Path: workflows/subworkflows/func_summaries.cwl Branch/Commit ID: eosc-life-gos |
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diamond proteinworkflow
\"This workflow performs diamond protein alignment process for predicted protein sequences. It executes 2 processes: diamond index creation and diamond alignment. related CWL file: ./Tools/09_diamond_index.cwl ./Tools/11_diamond_uniprot_alignment.cwl ./Tools/11_diamond_uniprot_filter1.cwl ./Tools/11_diamond_uniprot_filter2.cwl\" |
Path: Workflow/diamond_protein_ssw.cwl Branch/Commit ID: main |
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wf_split_self_and_idr.cwl
This workflow returns the reproducible number of split peaks given a single bam file and its size-matched input pair. This workflow splits the bam file first, but does not do anything to the input. |
Path: cwl/wf_split_self_and_idr.cwl Branch/Commit ID: master |
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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 |
