Explore Workflows
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Cell Ranger Count (RNA+VDJ)
Cell Ranger Count (RNA+VDJ) Quantifies single-cell gene expression, performs V(D)J contigs assembly and clonotype calling of the sequencing data from a single 10x Genomics library in a combined manner. The results of this workflow are primarily used in either “Single-Cell RNA-Seq Filtering Analysis”, “Single-Cell Immune Profiling Analysis”, or “Cell Ranger Aggregate (RNA, RNA+VDJ)” pipelines. |
Path: workflows/cellranger-multi.cwl Branch/Commit ID: 69643d8c15f5357a320aa7e2f6adb2e71302fd20 |
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SetNightSkyBackgroundRate
Derive or calculate night-sky background rate per pixel. |
Path: workflows/SetNightSkyBackgroundRate.cwl Branch/Commit ID: bf4d4a44a543bcc04f4508ce020751c71550acf5 |
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scatter-wf2_v1_0.cwl
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Path: testdata/scatter-wf2_v1_0.cwl Branch/Commit ID: 5759b4275906e6cfe13912c8426de2a2237cb4b0 |
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Workflow that executes the Sounder SIPS end-to-end L1a processing
Cognito credentials to access the U-DS services are retrieved from the AWS Parameter Store with the supplied keys. |
Path: sounder_sips/ssips_L1a_workflow.cwl Branch/Commit ID: bc1cbcea4a36132a801bece4ae69868ee90d4363 |
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conditional_step_no_inputs.cwl
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Path: tests/wf/conditional_step_no_inputs.cwl Branch/Commit ID: dbc4c4c2ad30ed31367b4fbcc3bb4084fdcabaa2 |
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Workflow that executes the Sounder SIPS end-to-end L1b processing
Requires valid AWS credentials as input arguments |
Path: sounder_sips/ssips_L1b_workflow.cwl Branch/Commit ID: bc1cbcea4a36132a801bece4ae69868ee90d4363 |
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ValidateSinglePhotoElectronResponse
Validate single photon electron response. |
Path: workflows/ValidateSinglePhotoElectronResponse.cwl Branch/Commit ID: bf4d4a44a543bcc04f4508ce020751c71550acf5 |
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tt_fscr_calls_pass1
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Path: task_types/tt_fscr_calls_pass1.cwl Branch/Commit ID: c64599f5db2437f9323d41cc3d8d9efb20a2667e |
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ValidateCameraTimeResponse
Validate camera time response. |
Path: workflows/ValidateCameraTimeResponse.cwl Branch/Commit ID: bf4d4a44a543bcc04f4508ce020751c71550acf5 |
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SetTelescopeEfficiency
Derive (or set) an overall efficiency parameter to the telescope throughput due to variations of the optical throughput. Allow for dependencies on off-axis angle and wavelength. |
Path: workflows/SetTelescopeEfficiency.cwl Branch/Commit ID: bf4d4a44a543bcc04f4508ce020751c71550acf5 |
