Abstract
It is stressed that poor convergence criteria are often used in light-curve synthesis programs. A large number of iterations (several tens) is needed to arrive at a definite conclusion about convergence. The result is usually that of some parameters little or no knowledge is gained and that the formal error estimates of all parameters are unrealistically small.
References
De Landtsheer, A. C.: 1981,Astrophys. Space Sci. 80, 349.
De Landtsheer, A. C.: 1983,Astron. Astrophys. Suppl. Ser. (in press).
Rafert, J. B. and Twigg, L. W.: 1980,Monthly Notices Roy. Astron. Soc. 193, 79.
Wilson, R. E.: 1983,Astrophys. Space Sci. 92, 229 (this issue).
Wilson, R. E. and Biermann, P.: 1976,Astron. Astrophys. 48,349.
Wilson, R. E. and Devinney, E. J.: 1971,Astrophys. J. 166, 605.
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de Landtsheer, A.C. The accuracy of light curve interpretation programs revisited. Astrophys Space Sci 92, 231–232 (1983). https://doi.org/10.1007/BF00653605
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DOI: https://doi.org/10.1007/BF00653605