Explore Workflows
View already parsed workflows here or click here to add your own
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Dockstore.cwl
Testing: align sequences with bwa mem, then convert ot BAM |
Path: Dockstore.cwl Branch/Commit ID: master |
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bam to trimmed fastqs and HISAT alignments
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Path: definitions/subworkflows/bam_to_trimmed_fastq_and_hisat_alignments.cwl Branch/Commit ID: downsample_and_recall |
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bulk scRNA-seq pipeline using Salmon
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Path: bulk-pipeline.cwl Branch/Commit ID: b9c8e26 |
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rRNA_selection.cwl
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Path: tools/rRNA_selection.cwl Branch/Commit ID: 56dafa4 |
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sc_atac_seq_initial_analysis.cwl
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Path: sc-atac-seq-pipeline/steps/sc_atac_seq_initial_analysis.cwl Branch/Commit ID: 68e0cc1 |
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Varscan Workflow
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Path: definitions/subworkflows/varscan_germline.cwl Branch/Commit ID: downsample_and_recall |
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upload_results_workflow.cwl
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Path: workflows/subworkflows/upload_results_workflow.cwl Branch/Commit ID: master |
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Alignment without BQSR
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Path: definitions/subworkflows/sequence_to_bqsr_mouse.cwl Branch/Commit ID: downsample_and_recall |
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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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validate_interleaved_fq.cwl
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Path: cwls/validate_interleaved_fq.cwl Branch/Commit ID: 0.3.2 |
