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 - Jelic, Vibor
AU - Labropoulos, Panagiotis
AU - Zaroubi, Saleem
AU - Brentjens, Michiel A.
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 smallest spatial scale data is discarded. While it has been shown that LOFAR-EoR image recovery is theoretically possible using image smoothing, we add that wavelet decomposition is an efficient way 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 smallest spatial scale data is discarded. While it has been shown that LOFAR-EoR image recovery is theoretically possible using image smoothing, we add that wavelet decomposition is an efficient way 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 - methods: statistical
KW - cosmology: theory
KW - dark ages, reionization, first stars
KW - diffuse radiation
KW - BLIND SOURCE SEPARATION
KW - 21 CENTIMETER FLUCTUATIONS
KW - FOREGROUND REMOVAL
KW - HIGH-REDSHIFT
KW - INTERGALACTIC MEDIUM
KW - NEUTRAL HYDROGEN
KW - 21-CM EPOCH
KW - TOMOGRAPHY
KW - LOFAR
KW - SIMULATIONS
U2 - 10.1093/mnras/sts333
DO - 10.1093/mnras/sts333
M3 - Article
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 -