HAR reconstructions for time-series of irregularly pulsating stars

Details HAR reconstructions for time-series of irregularly pulsating stars HAR reconstructions for time-series of irregularly pulsating stars

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..292..347p&link_type=abstract

Interplay of Periodic, Cyclic and Stochastic Variability in Selected Areas of the H-R Diagram. Edited by C. Sterken, ASP Conf. S

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The mathematical properties of the classical AR(tau) processes imply that the latter are in general inadequate for simulating irregular time-series. However, when modified by a subsequent nonlinear m-parameter transformation, the resulting stochastic scheme can provide good reconstructions of the broad features of these series. The method is illustrated by a statistical reconstruction of the V light curve of RU Cam, with tau = 4, m = 6.

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