2002/07/30 by D. C. Srivastava, S. K. Sahay
Physics and Astronomy · #gr-qc #astro-ph
paper · pdf · doi:10.1046/j.1365-8711.2002.05915.x
published as Mon.Not.Roy.Astron.Soc. 337 (2002) 315-321 · Accepted in MNRAS, 14 pages, 4 figures
arxiv created 2002/07/30 · arxiv updated 2009/11/30
In this paper we obtain the Fourier Transform of a continuous gravitational wave. We have analysed the data set for (i) one year observation time and (ii) arbitrary observation time, for arbitrary location of detector and source taking into account the effects arising due to rotational as well as orbital motion of the earth. As an application of the transform we considered spin down and N-component signal analysis.