TY - JOUR
T1 - The scale of the problem
T2 - Recovering images of reionization with generalized morphological component analysis
AU - Chapman, Emma
AU - Abdalla, Filipe B.
AU - Bobin, J.
AU - Starck, J. L.
AU - Harker, Geraint
AU - Jelić, Vibor
AU - Labropoulos, Panagiotis
AU - Brentjens, Michiel A.
AU - Zaroubi, Saleem
AU - de Bruyn, A. G.
AU - Koopmans, L. V.E.
PY - 2013/2/11
Y1 - 2013/2/11
N2 - 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.
AB - 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.
KW - Cosmology: theory
KW - Dark ages
KW - Diffuse radiation.
KW - First stars
KW - Methods: statistical
KW - Reionization
UR - http://www.scopus.com/inward/record.url?scp=84873902656&partnerID=8YFLogxK
U2 - 10.1093/mnras/sts333
DO - 10.1093/mnras/sts333
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AN - SCOPUS:84873902656
SN - 0035-8711
VL - 429
SP - 165
EP - 176
JO - Monthly Notices of the Royal Astronomical Society
JF - Monthly Notices of the Royal Astronomical Society
IS - 1
ER -