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Title: Small Angular Scale Simulations of the Microwave Sky

Authors: D. Sáez (1), E. Holtmann (2), G. F. Smoot (2) ((1) Departamento de Astronomía y Astrofísica, Universidad de Valencia, Burjassot, Valencia, Spain, (2) Lawrence Berkeley Laboratory, Space Science Laboratory, CfPA, University of California, Berkeley CA)
Abstract: We describe and compare two types of microwave sky simulations which are good for small angular scales. The first type uses expansions in spherical harmonics, and the second one is based on plane waves and the Fast Fourier Transform. The angular power spectrum is extracted from maps corresponding to both types of simulations, and the resulting spectra are appropriately compared. In this way, the features and usefulness of Fourier simulations are pointed out. For $\ell \geq 100$, all the simulations lead to similar accuracies; however, the CPU cost of Fourier simulations is $\sim 10$ times smaller than that for spherical harmonic simulations. For $\ell \leq 100$, the simulations based on spherical harmonics seem to be preferable.
Comments: 16 pages (LATEX), 2 postcript figures. Accepted in ApJ
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:astro-ph/9606164v1

Submission history

From: Diego Saez [view email]
[v1] Wed, 26 Jun 1996 10:28:17 GMT (442kb)