uvmcmcfit
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  • Why Use uvmcmcfit?
  • Installation
  • Input Data Format
  • Examples
    • XMM101: a single, unlensed galaxy
    • ADFS07: A Single, Strongly Lensed Galaxy
    • CDFS_M0: A Complex, Multi-component System
 
uvmcmcfit
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ExamplesΒΆ

This section contains three examples in order of increasing complexity to demonstrate usage of uvmcmcfit.

  • XMM101: a single, unlensed galaxy
    • Preliminary Setup Procedures
      • Inputs
      • Outputs
    • Configuring config.yaml
      • Required keywords
      • Optional keywords
    • Running uvmcmcfit
    • Inspecting the Model Results for XMM101
      • Accessing the Data Directly
      • Testing Convergence
      • Plot the Best-fit Model
      • Plot Several Acceptable Model Fits
      • Plot the Posterior PDFs
      • Plot the Covariance Matrix
  • ADFS07: A Single, Strongly Lensed Galaxy
    • Preliminary Setup Procedures
      • Inputs
      • Outputs
    • Configuring config.yaml
      • Required keywords
      • Optional keywords
    • Running uvmcmcfit
    • Inspecting the Model Results for ADFS07
      • Accessing the Data Directly
      • Testing Convergence
      • Plot the Best-fit Model
      • Plot Several Acceptable Model Fits
      • Plot the Posterior PDFs
      • Plot the Covariance Matrix
  • CDFS_M0: A Complex, Multi-component System
    • 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
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© Copyright 2014, Shane Bussmann. Revision c43b501fb1683a003b44d4b4bc46fa9520ca4806.

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