Abstract
We apply the correlated component analysis (CCA) method on simulated data of the Square Kilometre Array, with the aim of accurately cleaning the 21-cm reionization signal from diffuse foreground contamination. The CCA has been developed for the cosmic microwave background, but the application of the Fourier domain implementation of this method to the reionization signal is straightforward. The CCA is a parametric method to estimate the frequency behaviour of the foregrounds from the data by using second-order statistics. We test its performance on foreground simulations of increasing complexity, designed to challenge the parametric models adopted. We also drop the assumption of spectral smoothness that most of the methods rely upon. We are able to clean effectively the simulated data across the explored frequency range (100-200 MHz) for all the foreground simulations. This shows that the CCA method is very promising for epoch of reionization component separation.
Author
Bonaldi, Anna; Brown, Michael L.
Journal
Monthly Notices of the Royal Astronomical Society: Letters
Paper Publication Date
February 2015
Paper Type
Astrostatistics