nemo - a Sunyaev-Zel’dovich effect galaxy cluster and source finder

Contents:

• 1. Installation and Usage
  • 1.1. Current status and previous internal releases
  • 1.2. Software needed
  • 1.3. Installation
  • 1.4. Running Nemo
  • 1.5. Related codes
  • 1.6. Comments, bug reports, help, suggestions etc.
• 2. Quickstart: Cluster Finding in the ACTPol E-D56 Field
  • 2.1. Re-creating the ACTPol two-season cluster catalog
  • 2.2. Downloading ACT maps
  • 2.3. Making a cluster catalog
  • 2.4. Estimating cluster masses
  • 2.5. Calculating completeness
  • 2.6. Generating mock catalogs
• 3. Tutorial: Cluster Finding in Simulated Simons Observatory Maps
  • 3.1. Making multi-component simulated maps
  • 3.2. Making CAR projection maps
  • 3.3. Making beam files
  • 3.4. Running Nemo on small maps
  • 3.5. Extracting the survey mass limit
  • 3.6. Running Nemo on large maps
  • 3.7. Using the input simulation catalogs
• 4. Tutorial: Using the Selection Function for Cluster Cosmology
  • 4.1. Small Maps
  • 4.2. Tiled Maps
• 5. Tutorial: Cluster Finding in TILe-C Compton y-maps
• 6. Advanced Usage
  • 6.1. Forced photometry
  • 6.2. Using the selection function
  • 6.3. Modifying GNFW parameters
  • 6.4. Source injection and flux recovery tests
• 7. Input Formats (Maps and Beams)
• 8. Output
  • 8.1. Directory Structure
  • 8.2. Catalogs
  • 8.3. Filtered Maps
  • 8.4. Selection Function
  • 8.5. Diagnostics
• 9. Configuration File Parameters
• 10. Contributing to Further Development
  • 10.1. Reporting Issues
  • 10.2. Contributing Code
• 11. Testing
• 12. API Reference
  • 12.1. catalogs
  • 12.2. completeness
  • 12.3. filters
  • 12.4. gnfw
  • 12.5. maps
  • 12.6. MockSurvey
  • 12.7. nemoCython
  • 12.8. photometry
  • 12.9. pipelines
  • 12.10. plotSettings
  • 12.11. signals
  • 12.12. startUp

Indices and tables

• Index

• Module Index

• Search Page