Explore Workflows
View already parsed workflows here or click here to add your own
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binning.cwl
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Path: workflows/binning.cwl Branch/Commit ID: master |
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rw-distr.cwl
run scatter-gather for rw stage |
Path: stage/rw-distr.cwl Branch/Commit ID: master |
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Data2Services CWL workflow to convert CSV/TSV files with statements split, Vincent Emonet <vincent.emonet@gmail.com>
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Path: support/pharmgkb/graphdb-workflow/workflow.cwl Branch/Commit ID: master |
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Optical throughput measurements via muon ring analysis
Upon receiving a new DL0 data product (from either Monte Carlo simulations or observations), DPPS triggers the CalibPipe (ctapipe-process) to process the data using ctapipe, extracting the signal charges and reconstructing muon parameters. The second step involves using the CalibPipe tool to estimate the telescope’s optical throughput using a predefined number of muon events. |
Path: uc-120-2.2-optical-throughput-calibration-with-muons.cwl Branch/Commit ID: master |
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biowardrobe_chipseq_se.cwl
The workflow is used to run CHIP-Seq basic analysis with single-end input FASTQ file. In outputs it returns coordinate sorted BAM file alongside with index BAI file, quality statistics of the input FASTQ file, reads coverage in a form of bigWig file, peaks calling data in a form of narrowPeak or broadPeak files. |
Path: biowardrobe_chipseq_se.cwl Branch/Commit ID: master |
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extract_gencoll_ids
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Path: task_types/tt_extract_gencoll_ids.cwl Branch/Commit ID: e23abd0bc049a2983bd3b12dddca19d3b04506f2 |
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collate_unique_SSU_headers.cwl
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Path: tools/collate_unique_SSU_headers.cwl Branch/Commit ID: ca6ca61 |
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tec_and_amp.cwl
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Path: workflows/linc_target/tec_and_amp.cwl Branch/Commit ID: 7b6185e2e6f9d36b1987274e82842c82ba6f8342 |
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tt_univec_wnode.cwl
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Path: task_types/tt_univec_wnode.cwl Branch/Commit ID: 1ce371c7412debef75edf09e8830d74ac987a668 |
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step-valuefrom-wf.cwl
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Path: v1.0/v1.0/step-valuefrom-wf.cwl Branch/Commit ID: e270bab4f9694da8d46241094341fd0453bfcfc8 |
