Application of the Kalman Filter to Light Curves of Eclipsing Binaries

Details Application of the Kalman Filter to Light Curves of Eclipsing Binaries Application of the Kalman Filter to Light Curves of Eclipsing Binaries

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ap%26ss..44...63j&link_type=abstract

Astrophysics and Space Science, Volume 44, Issue 1, pp.63-83

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

Recently Kopal (1975a, b, c, d) initiated a new approach to the analysis of the light curves of eclipsing binary systems in which the solution is based on transforming the problem from the conventional time-domain into the frequency-domain. Irrespective of the type of eclipse, the present formulation of the frequency approach requires that a set of quantitiesA 2m, called moments, be determined from the observations. It is the purpose of the present paper to describe a data interpolation and smoothing technique based on a version of the Kalman filter to pre-process observations and to determine the quantitiesA 2m in an optimal sense.

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