English

Using inpainting to construct accurate cut-sky CMB estimators

Cosmology and Nongalactic Astrophysics 2017-03-01 v1 Instrumentation and Methods for Astrophysics

Abstract

The direct evaluation of manifestly optimal, cut-sky CMB power spectrum and bispectrum estimators is numerically very costly, due to the presence of inverse-covariance filtering operations. This justifies the investigation of alternative approaches. In this work, we mostly focus on an inpainting algorithm that was introduced in recent CMB analyses to cure cut-sky suboptimalities of bispectrum estimators. First, we show that inpainting can equally be applied to the problem of unbiased estimation of power spectra. We then compare the performance of a novel inpainted CMB temperature power spectrum estimator to the popular apodised pseudo-ClC_l (PCL) method and demonstrate, both numerically and with analytic arguments, that inpainted power spectrum estimates significantly outperform PCL estimates. Finally, we study the case of cut-sky bispectrum estimators, comparing the performance of three different approaches: inpainting, apodisation and a novel low-l leaning scheme. Providing an analytic argument why the local shape is typically most affected we mainly focus on local type non-Gaussianity. Our results show that inpainting allows to achieve optimality also for bispectrum estimation, but interestingly also demonstrate that appropriate apodisation, in conjunction with low-l cleaning, can lead to comparable accuracy.

Keywords

Cite

@article{arxiv.1510.03103,
  title  = {Using inpainting to construct accurate cut-sky CMB estimators},
  author = {H. F. Gruetjen and J. R. Fergusson and M. Liguori and E. P. S. Shellard},
  journal= {arXiv preprint arXiv:1510.03103},
  year   = {2017}
}

Comments

21 pages, 10 figures

R2 v1 2026-06-22T11:17:42.295Z