Explore Workflows
View already parsed workflows here or click here to add your own
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pennant_wf.cwl
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Path: beeflow/data/cwl/bee_workflows/pennant/pennant_wf.cwl Branch/Commit ID: ede638569dc3c0a0cd4ccc077a7348df26e1367b |
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tindaisy-vep_annotate.cwl
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Path: cwl/workflows/tindaisy-vep_annotate.cwl Branch/Commit ID: 43330deda32a6ad9e4f8a8cc51a2cf1ba380fff6 |
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tt_kmer_compare_wnode
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Path: task_types/tt_kmer_compare_wnode.cwl Branch/Commit ID: e4d6182d5f7a6a880e5f2b21273cf40d25e187df |
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record-output-wf.cwl
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Path: tests/record-output-wf.cwl Branch/Commit ID: 86c46cb397de029e4c91f02cca40fa2b54d22f37 |
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tt_hmmsearch_wnode.cwl
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Path: task_types/tt_hmmsearch_wnode.cwl Branch/Commit ID: 1c1f5aa0b0dfe5b07beb8ccb0c0e3c073a9fb592 |
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main-unito.cwl
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Path: unito-pipeline/cwl/main-unito.cwl Branch/Commit ID: d2c960fe089bfe32238cbd6be4961df18b9274a4 |
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revsort.cwl
Reverse the lines in a document, then sort those lines. |
Path: tests/wf/revsort.cwl Branch/Commit ID: 766d58b47180d92618074679eb9f3c6c30acf638 |
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record-output-wf_v1_0.cwl
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Path: testdata/record-output-wf_v1_0.cwl Branch/Commit ID: aa13f7bad47e8df2349bdebd163e1830537d7f93 |
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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: a03a36e43b30ada0242d3a67b3e1ad908249acb1 |
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sec-wf-out.cwl
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Path: tests/wf/sec-wf-out.cwl Branch/Commit ID: a8d8d00fd1e4274e1bc16001937db5aae46b0b0d |
