CDFS_M0: A Complex, Multi-component System

This example shows how to run uvmcmcfit on a complex system: a strongly lensed galaxy, a weakly lensed galaxy, and a sub-mm bright lens.

• Preliminary Setup Procedures
  • Inputs
  • Outputs
• Configuring config.yaml
  • Required keywords
  • Optional keywords
• Running uvmcmcfit
• Inspecting the Model Results for CDFS_M0
  • Accessing the Data Directly
  • Testing Convergence
  • Plot the Best-fit Model
  • Plot Several Acceptable Model Fits
  • Plot the Posterior PDFs
  • Plot the Covariance Matrix