Blind foreground subtraction for intensity mapping experiments

David Alonso, Philip Bull, Pedro G. Ferreira, Mário G. Santos

Research output: Contribution to journalArticlepeer-review

Abstract

We make use of a large set of fast simulations of an intensity mapping experiment with characteristics similar to those expected of the Square Kilometre Array in order to study the viability and limits of blind foreground subtraction techniques. In particular, we consider three different approaches: polynomial fitting, principal component analysis (PCA) and independent component analysis (ICA). We review the motivations and algorithms for the three methods, and show that they can all be described, using the same mathematical framework, as different approaches to the blind source separation problem. We study the efficiency of foreground subtraction both in the angular and radial (frequency) directions, as well as the dependence of this efficiency on different instrumental and modelling parameters. For well-behaved foregrounds and instrumental effects, we find that foreground subtraction can be successful to a reasonable level on most scales of interest. We also quantify the effect that the cleaning has on the recovered signal and power spectra. Interestingly, we find that the three methods yield quantitatively similar results, with PCA and ICA being almost equivalent.
Original languageEnglish
Pages (from-to)400-416
Number of pages17
JournalMon. Not. Roy. Astron. Soc.
Volume447
Issue number1
DOIs
Publication statusPublished - 11 Feb 2015

Keywords

  • Methods: statistical
  • Large-scale structure of universe
  • Radio lines: galaxies

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