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Titlebook: Astronomical Time Series; Proceedings of The F Dan Maoz,Amiel Sternberg,Elia M. Leibowitz Conference proceedings 1997 Springer Science+Busi

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Radial Velocity Detections of Extra-Solar Planetsar planets will improve dramatically our understanding of the formation of planets and planetary systems, which was based till the last decade on the sole example of the solar system. Nevertheless, no extra-solar planet was convincingly detected until recently. This is so because planets are very fa
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Tests of Irregularly Sampled Stochastic Time Series for AGN collected by the AGN WATCH, using more data, to obtain reverberation results for more objects, one will have to rely on irregularly sampled lightcurves. Previous analyses of irregularly sampled observations suggest that it is possible to obtain results from such data sets. To evaluate the statistic
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Wavelet Transforms of Flickering Light Curves in Cataclysmic Variabless up to more than an entire magnitude in others. This phenomenon is known as flickering. Phenomenologically, it appears as a continuous series of overlapping flares in the light curves. For a comprehensive review, see Bruch (1992). As an example, Fig. 1 shows a light curve of the novalike variable V
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Fast Computation of Trigonometric Sums with Applications to the Frequency Analysis of Astronomical D..., . and for the full grid .., ., . = 0,..., . − 1 of frequencies. The similar approach is known from radio astronomy in the context of synthesis imaging. However, when the so-called “gridding” is method to obtain relatively crude interpolations from unequally spaced two dimensional measurements (
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