K. Yamamoto, G. Nakamura, G. Huetsi, T. Narikawa and T. Sato, “Constraint on the Cosmological f(R) Model from the Multipole Power Spectrum of the SDSS Luminous Red Galaxy Sample and Prospects for a Future Redshift Survey,” Physical Review D, Vol. 81, No. 10, 2010, Article ID: 103517. doi:10.1103/PhysRevD.81.103517

has been cited by the following article:

• TITLE: Window Effect in the Power Spectrum Analysis of a Galaxy Redshift Survey

  AUTHORS: Takahiro Sato, Gert Hütsi, Gen Nakamura, Kazuhiro Yamamoto

  KEYWORDS: Cosmology; Large-Scale Structure of Universe

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.3 No.3, September 3, 2013

  ABSTRACT: We investigate the effect of the window function on the multipole power spectrum in two different ways. First, we consider the convolved power spectrum including the window effect, which is obtained by following the familiar (FKP) method developed by Feldman, Kaiser and Peacock. We show how the convolved multipole power spectrum is related to the original power spectrum, using the multipole moments of the window function. Second, we investigate the deconvolved power spectrum, which is obtained by using the Fourier deconvolution theorem. In the second approach, we measure the multipole power spectrum deconvolved from the window effect. We demonstrate how to deal with the window effect in these two approaches, applying them to the Sloan Digital Sky Survey (SDSS) luminous red galaxy (LRG) sample.