Determination of Eclipsing Binary Parameters

  • Josef Kallrath
  • Eugene F. Milone


The determination or estimation of physical parameters from eclipsing binary light curves and/or radial velocity curves is an inverse problem and can be formulated as a nonlinear least-squares problem. It is solved by optimizing the agreement between the calculated light and the observed light curve. The parameter vector x corresponding to minimum deviation is the system solution, and the calculated light curve produced from it is said to be the best fit to the data. A measure of the deviation is the weighted sum of the squared residuals.


Inverse Problem Light Curve Light Curf Shot Noise Simplex Algorithm 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.


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Copyright information

© Springer Science+Business Media New York 1999

Authors and Affiliations

  • Josef Kallrath
    • 1
    • 2
  • Eugene F. Milone
    • 3
  1. 1.BASF-AGLudwigshafenGermany
  2. 2.Department of AstronomyUniversity of FloridaGainesvilleUSA
  3. 3.Department of Physics and AstronomyUniversity of CalgaryCalgaryCanada

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