Stellar Occultation Reduction Analysis

Details:

  • Overview
  • Using and Citing SORA
  • Installation
  • Releases
  • About Us

Code:

  • Modules
  • Getting Started
  • Examples
  • Video Tutorials
  • Jupyter-Notebook Guidelines
    • Body Class
    • Star Class
    • prediction() function and the PredictionTable Class
    • Observer and Spacecraft Classes
    • LightCurve Class
    • Occultation Class
    • ChiSquare Class
  • Known Issues
Stellar Occultation Reduction Analysis
  • Jupyter-Notebook Guidelines
  • View page source

SORA: Stellar Occultation Reduction and Analysis


Jupyter-Notebook Guidelines

All the Jupyter-Notebooks can be downloaded here

  • Body Class
    • 0. Index
    • 1. Instantiating a Body object
    • 2. Body Physical Attributes
    • 3. Ephemeris
    • 4. Pole Position Angle and Aperture Angle
    • 5. Apparent Magnitude
    • 6. The Ephemeris Classes
    • 7. The frame attribute
    • 8. The shape attribute
  • Star Class
    • 0. Index
    • 1. Instantiating Star Object
    • 2. Changing or including magnitudes
    • 3. Propagated positions
    • 4. Adding offsets
    • 5. The Apparent Diameter of the star
  • prediction() function and the PredictionTable Class
    • 0. Index
    • 1. Predicting stellar occultation
    • 2. The PredictionTable
    • 3. Using PredictionTable
    • 4. Plotting occultation maps
    • 5. Occultation parameters
  • Observer and Spacecraft Classes
    • 0. Index
    • 1. Instantiating an Observer or Spacecraft Object
    • 2. Setting and/or modifing parameters
    • 3. Apparent Sidereal Time
    • 4. Ksi and Eta projection
    • 5. MPC observatories
  • LightCurve Class
    • 0. Index
    • 1. Instantiating a LightCurve Object
    • 2. Set and/or modifing model parameters
    • 3. Preparing the LightCurve
    • 4. Automatic detection of Occultations
    • 5. Complete occultation light curve model and fitting
    • 6. Viewing and saving the results
  • Occultation Class
    • 0. Index
    • 1. Instantiating an Occultation Object and adding observations
    • 2. Projecting the times in the sky plane and the Chords
    • 3. Ellipse fit
    • 4. Viewing and saving the results
  • ChiSquare Class
    • 0. Index
    • 1. Instantiating a ChiSquare Object
    • 2. Viewing the results
    • 3. Saving the results and plots
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