Abstract
In order to enable a successful application of the realised CB models (presented in the two former articles of the series) in the analysis of the observed light curves, an efficient method unifying the best properties of the gradient method and of the differential-corrections one into a single algorithm (Djurašević, 1991) is proposed. This method is realised by modifying the Marquardt (1963) algorithm. The inverse problem is solved in an iterative cycle of corrections to the model elements based on a nonlinear least-square method.
The interpretation of photometric observations is based on the choice of optimal model parameters yielding the best agreement between an observed light curve and the corresponding synthetic one. Some of these parameters can be determineda priori in an independent way, while the others are found by solving the inverse problem.
The programmes for analysing light curves find the optimal system parameters rapidly, reliably and correctly. The corresponding programme support enables an evident graphic presentation of the results.
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References
Djurašević, G.: 1991,Publ. Obs. Astron. Belgrade, No. 42, 1.
Markover, S. G.: 1956,Astron. Zh. 33, 423.
Marquardt, D. W.: 1963,J. Soc. Ind. Appl. Math. 11, (No. 2), 431.
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Djurašević, G. An analysis of active close binaries (CB) based on photometric measurements. Astrophys Space Sci 197, 17–34 (1992). https://doi.org/10.1007/BF00645069
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DOI: https://doi.org/10.1007/BF00645069