Abstract
The accurate and precise removal of 21-cm foregrounds from Epoch of Reionization (EoR) redshifted 21-cm emission data is essential if we are to gain insight into an unexplored cosmological era.We apply a non-parametric technique, Generalized Morphological Component Analysis (GMCA), to simulated Low Frequency Array (LOFAR)-EoR data and show that it has the ability to clean the foregrounds with high accuracy. We recover the 21-cm 1D, 2D and 3D power spectra with high accuracy across an impressive range of frequencies and scales. We show that GMCA preserves the 21-cm phase information, especially when the smallestspatial scale data is discarded. While it has been shown that LOFAR-EoR image recovery istheoretically possible using image smoothing, we add thatwavelet decomposition is an efficientway of recovering 21-cm signal maps to the same or greater order of accuracy with more flexibility. By comparing the GMCA output residual maps (equal to the noise, 21-cm signal and any foreground fitting errors) with the 21-cm maps at one frequency and discarding the smaller wavelet scale information, we find a correlation coefficient of 0.689, compared to 0.588 for the equivalently smoothed image. Considering only the pixels in a central patch covering 50 per cent of the total map area, these coefficients improve to 0.905 and 0.605, respectively, and we conclude that wavelet decomposition is a significantly more powerful method to denoise reconstructed 21-cm maps than smoothing.
Original language | English |
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Pages (from-to) | 165-176 |
Number of pages | 12 |
Journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY |
Volume | 429 |
Issue number | 1 |
DOIs | |
State | Published - 11 Feb 2013 |
Externally published | Yes |
Keywords
- Cosmology: theory
- Dark ages
- Diffuse radiation.
- First stars
- Methods: statistical
- Reionization
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science