首页 | 本学科首页   官方微博 | 高级检索  
     检索      


An optimal method for the power spectrum measurement
Authors:Yi-Bin Yang Long-Long Feng Jun Pan Xiao-Hu Yang
Institution:[1]Center for Astrophysics, University of Science and Technology of China, Hefei 230026, China [2]Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China [3]Shanghai Astronomical Observatory, the Partner Group of MPA, Nandan Road 80, Shanghai 20030, China
Abstract:An aliasing effect brought up by mass assignment onto Fast Fourier Transformation (FFT) grids may bias measurement of the power spectrum of large scale structures. In this paper, based on the Beylkin's unequally spaced FFT technique, we propose a new precise method to extract the true power spectrum of a large discrete data set. We compare the traditional mass assignment schemes with the new method using the Daub6 and the 3rd-order B-spline scaling functions. Our measurement of Poisson samples and samples of N-body simulations shows that the B-spline scaling function is an optimal choice for mass assignment in the sense that (1) it has a compact support in real space and thus yields an efficient algorithm (2) without any extra corrections. The Fourier space behavior of the 3rd-order B-spline scaling function enables it to be able to accurately recover the true power spectrum with errors less than 5% up to k < kN. It is expected that such a method can be applied to higher order statistics in Fourier space and will enable us to have a precision capture of the non-Gaussian features in the large scale structure of the universe.
Keywords:large scale structure of universe-methods  numerical
本文献已被 维普 万方数据 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号